Input: [1] Can Dogma Develop? [0]

Output: Tracts


Input: [1] Another way to explain the doctrine of Transubstantiation [0]

Output: Video


Input: [1] Proving Inspiration [0]

Output: Tracts


Input: [1] Can the souls in purgatory pray for us? [0]

Output: Video


Input: [1] Biblical evidence for the Real Presence [0]

Output: Video


Input: [1] Which Church teachings have been declared infallible? [0]

Output: Quick Questions


Input: [1] Is purgatory a physical place? [0]

Output: Video


Input: [1] Is there any verse in the Bible wherein Jesus himself said that he is God? [0]

Output: Quick Questions


Input: [1] Nicene Credence [0]

Output: Magazine Articles


Input: [1] Did the Church change the number of the sacraments? [0]

Output: Quick Questions


Input: [1] Does "consubstantiation" have anything to do with Jesus having two natures? [0]

Output: Quick Questions


Input: [1] A Trip Down Heresy Lane [0]

Output: Magazine Articles


Input: [1] Why Mary? [2] 5/11/2012 7pm ET [0]

Output: Radio Shows


Input: [1] Where can I find original documents defining Church teachings? [0]

Output: Quick Questions


Input: [1] When did the Church come up with the doctrine that each species (bread and wine) contains both the body and the blood of Christ? [0]

Output: Quick Questions


Input: [1] I believe everything the creed says, but why must I also believe in papal infallibility? [0]

Output: Quick Questions


Input: [1] How to Read the Bible [2] 6/25/2010 6pm ET [0]

Output: Radio Shows


Input: [1] Dogma, Doctrine, Discipline [2] 2/8/2013 6pm ET [0]

Output: Radio Shows


Input: [0] 1 [Views] 522 [Item title]

Output: Joint coupling variability can likely indicate lower extremity injury occurrence


Input: [0] 2 [Views] 401 [Item title]

Output: Are anthropometric, flexibility, muscular strength, and endurance variables related to clubhead velocity in low and high handicap golfers?


Input: [0] 3 [Views] 387 [Item title]

Output: Effect of biological movement variability on the performance of the golf swing in high and low handicapped players


Input: [0] 4 [Views] 373 [Item title]

Output: Does successful unanticipated turning ability lead to successful unanticipated straight sprint ability in netballers?


Input: [0] 5 [Views] 359 [Item title]

Output: Ground reaction forces and loading rates associated with Parkour and traditional drop landing techniques


Input: [0] 6 [Views] 333 [Item title]

Output: Effectiveness of foot orthoses for treatment and prevention of lower limb injuries


Input: [0] 7 [Views] 332 [Item title]

Output: Kinematic alterations due to different loading schemes in early acceleration sprint performance from starting blocks


Input: [0] 8 [Views] 326 [Item title]

Output: Effects of caffeine and carbohydrate mouth rinses on repeated sprint performance


Input: [0] 9 [Views] 316 [Item title]

Output: Dominant limb asymmetry greater than 10% during unanticipated agility performance is associated with prospective injury occurrence


Input: [0] 10 [Views] 308 [Item title]

Output: Core-training using the Bodywall™ training system versus a conventional gym-based approach: Effects on core endurance


Input: [... so try these instead] FamilySearch Product Support [FamilySearch Wiki is not a...]

Output: FamilySearch products directory

FamilySearch Wiki:Try another wiki | Learn | FamilySearch.org


Input: [... so try these instead] Familypedia, GenerationStation, WeRelate.org, WikiTree, 1000Memories FamilySearch [FamilySearch Wiki is not a...]

Output: Place for ancestor information

FamilySearch Wiki:Try another wiki | Learn | FamilySearch.org


Input: [FamilySearch Wiki is not a...]

Output: Advertising site

FamilySearch Wiki:Try another wiki | Learn | FamilySearch.org


Input: [... so try these instead] ProductWiki [FamilySearch Wiki is not a...]

Output: Collection of product reviews

FamilySearch Wiki:Try another wiki | Learn | FamilySearch.org


Input: [... so try these instead] Religion-wiki, Mormon Wiki [FamilySearch Wiki is not a...]

Output: Place for religious doctrine or practices

FamilySearch Wiki:Try another wiki | Learn | FamilySearch.org


Input: [... so try these instead] LDS Temples [FamilySearch Wiki is not a...]

Output: Place for image of LDS temples

FamilySearch Wiki:Try another wiki | Learn | FamilySearch.org


Input: [... so try these instead] Wikipedia [FamilySearch Wiki is not a...]

Output: Encyclopedia of other things

FamilySearch Wiki:Try another wiki | Learn | FamilySearch.org


Input: [... so try these instead] Wikipedia, nationalarchives.gov.uk, Families in British India [FamilySearch Wiki is not a...]

Output: Place for detailed historical information

FamilySearch Wiki:Try another wiki | Learn | FamilySearch.org


Input: [... so try these instead] USGenWeb; We Relate.org which allows GEDCOM uploads; 1000Memories; WikiTree; Family History Library (offline); Genealogical Societies—Online directories include: daddezio; Federation of Genealogical Societies; Other places: scribd which accepts PDF's of your files. Be sure to add links to your files from appropriate places in this Wiki. [FamilySearch Wiki is not a...]

Output: Places to post biographies, data sets and genealogical records

FamilySearch Wiki:Try another wiki | Learn | FamilySearch.org


Input: [C/N] C & N [MATERIAL_2] Hair [C/N_3] N [MATERIAL]

Output: Bedding,herbivorous


Input: [C/N] N [MATERIAL_2] Hay [C/N_3] C [MATERIAL]

Output: Blood meal


Input: [C/N] N [MATERIAL_2] Lake weeds [C/N_3] N [MATERIAL]

Output: Bone meal


Input: [C/N] N [MATERIAL_2] Leaves [C/N_3] C [MATERIAL]

Output: Coffee grounds


Input: [C/N] O,alkalizer [MATERIAL_2] Lint [C/N_3] N [MATERIAL]

Output: Crushed egg shells


Input: [C/N] N [MATERIAL_2] Manure [C/N_3] N [MATERIAL]

Output: Feathers


Input: [C/N] N [MATERIAL_2] Paper(non-recyclable) [C/N_3] C [MATERIAL]

Output: Fruit


Input: [C/N] N [MATERIAL_2] Peanut shells [C/N_3] C [MATERIAL]

Output: Fruit peels and rinds


Input: [C/N] C [MATERIAL_2] Straw [C/N_3] C [MATERIAL]

Output: Garden debris, dried


Input: [C/N] C & N [MATERIAL_2] Pumpkins [C/N_3] N [MATERIAL]

Output: Garden debris, fresh


Input: [C/N] C [MATERIAL_2] Vegetable scraps [C/N_3] N [MATERIAL]

Output: Grass clippings, dried


Input: [C/N] N [MATERIAL_2] Tea grounds and leaves [C/N_3] N [MATERIAL]

Output: Grass clippings, fresh


Input: [Bar code #] 830095 [Sponsor] Cook [Comment] allows utilities to have too much control over commission [Description]

Output: changes qualifications for PUC commissioners

Public Citzen's Guide to Amending the PUC Sunset Bill - TexasVox: The Voice of Public Citizen in Texas


Input: [Bar code #] 830100 [Sponsor] Gonzalez [Comment] shouldn’t apply to just one company [Description]

Output: gives PUC citing authority over a new plant in the El Paso area

Public Citzen's Guide to Amending the PUC Sunset Bill - TexasVox: The Voice of Public Citizen in Texas


Input: [Bar code #] 830085 [Sponsor] Krause [Comment] jeopardizes reliability [Description]

Output: eliminates the PUC’s ability to issue a cease and desist order

Public Citzen's Guide to Amending the PUC Sunset Bill - TexasVox: The Voice of Public Citizen in Texas


Input: [Bar code #] 830105 [Sponsor] Laubenberg [Comment] jeopardizes reliability [Description]

Output: eliminates the PUC’s ability to issue a cease and desist order

Public Citzen's Guide to Amending the PUC Sunset Bill - TexasVox: The Voice of Public Citizen in Texas


Input: [Bar code #] 830091 [Sponsor] Phillips [Comment] could jeopardize reliability and create inefficiencies [Description]

Output: interferes with reliability must run plans

Public Citzen's Guide to Amending the PUC Sunset Bill - TexasVox: The Voice of Public Citizen in Texas


Input: [Bar code #] 830092 [Sponsor] Phillips [Comment] significantly increases electric consumers’ costs [Description]

Output: requires CREZ lines to be buried in a specific municipality

Public Citzen's Guide to Amending the PUC Sunset Bill - TexasVox: The Voice of Public Citizen in Texas


Input: [Bar code #] 830093 [Sponsor] Stanford [Comment] prevents the PUC from stopping abusive behavior and protecting reliability of the electric grid [Description]

Output: eliminates cease and desist orders for retail customers

Public Citzen's Guide to Amending the PUC Sunset Bill - TexasVox: The Voice of Public Citizen in Texas


Input: [Bar code #] 830094 [Sponsor] Sheets [Comment] two commissioners could meet without following open meeting requirements [Description]

Output: creates a 5 member Public Utility Commission

Public Citzen's Guide to Amending the PUC Sunset Bill - TexasVox: The Voice of Public Citizen in Texas


Input: [Bar code #] 830079 [Sponsor] Simpson [Comment] jeopardizes reliability [Description]

Output: eliminates the PUC’s ability to issue a cease and desist order

Public Citzen's Guide to Amending the PUC Sunset Bill - TexasVox: The Voice of Public Citizen in Texas


Input: [Bar code #] 830080 [Sponsor] Simpson [Comment] prevents the PUC from preventing abusive behavior and protecting reliability of the electric grid [Description]

Output: eliminates cease and desist orders for retail customers

Public Citzen's Guide to Amending the PUC Sunset Bill - TexasVox: The Voice of Public Citizen in Texas


Input: [Bar code #] 830081 [Sponsor] Simpson [Comment] puts unfair cost burden on customers [Description]

Output: shifts cost of opting out of advanced metering to other customers

Public Citzen's Guide to Amending the PUC Sunset Bill - TexasVox: The Voice of Public Citizen in Texas


Input: [Bar code #] 830074 [Sponsor] S Turner [Comment] opens door to even more industry influence over regulators through campaign contributions [Description]

Output: changes to single elected commissioner

Public Citzen's Guide to Amending the PUC Sunset Bill - TexasVox: The Voice of Public Citizen in Texas


Input: [From] 1:00 AM [Thunderstorms] No [Snow] No [Fog] No [Frost] No [Rain]

Output: No

Omeo Detailed Forecast - Bureau of Meteorology


Input: [From] 4:00 AM [Thunderstorms] No [Snow] No [Fog] No [Frost] No [Rain]

Output: Yes

Omeo Detailed Forecast - Bureau of Meteorology


Input: [From] 7:00 AM [Thunderstorms] No [Snow] No [Fog] No [Frost] No [Rain]

Output: Yes

Omeo Detailed Forecast - Bureau of Meteorology


Input: [From] 10:00 AM [Thunderstorms] No [Snow] No [Fog] No [Frost] No [Rain]

Output: Yes

Omeo Detailed Forecast - Bureau of Meteorology


Input: [From] 1:00 PM [Thunderstorms] No [Snow] No [Fog] No [Frost] No [Rain]

Output: Yes

Omeo Detailed Forecast - Bureau of Meteorology


Input: [From] 4:00 PM [Thunderstorms] No [Snow] No [Fog] No [Frost] No [Rain]

Output: No

Omeo Detailed Forecast - Bureau of Meteorology


Input: [From] 7:00 PM [Thunderstorms] No [Snow] No [Fog] No [Frost] No [Rain]

Output: No

Omeo Detailed Forecast - Bureau of Meteorology


Input: [From] 10:00 PM [Thunderstorms] No [Snow] No [Fog] No [Frost] No [Rain]

Output: No

Omeo Detailed Forecast - Bureau of Meteorology


Input: [Genotype] ara-14 [Description]

Output: Blocks arabinose catabolism


Input: [Genotype] argF [Description]

Output: Ornithine carbamoyltransferase mutation blocks ability to use arginine


Input: [Genotype] dam/dcm [Description]

Output: Abolishes endogenous adenine methylation at GATC sequences (dam) or cytosine methylation at CCWGG sequences (dcm). Used to propagate DNA for cleavage with certain restriction enzymes (e.g. Ava II, Bcl I)


Input: [Genotype] DE3 [Description]

Output: Lysogen that encodes T7 RNA polymerase. Used to induce expression in T7-driven expression systems


Input: [Genotype] endA [Description]

Output: endA Mutation in the non-specific endonuclease Endonuclease I; eliminates non-specific endonuclease activity, resulting in improved plasmid preps


Input: [Genotype] F´ [Description]

Output: A self-transmissible, low-copy plasmid used for the generation of single-stranded DNA when infected with M13 phage; may contain a resistance marker to allow maintenance and will often carry the lacI and lacZ∆M15 genotypes


Input: [Genotype] galK [Description]

Output: Galactokinase mutation blocks catabolism of galactose—cells that are galK minus grow in the presence of galactose as the sole carbon source


Input: [Genotype] galU [Description]

Output: Glucose-1-phosphate uridylyltransferase mutation blocks ability to use galactose—cells that are galU minus can grow on media that contains galactose as the sole carbon source


Input: [Genotype] gyrA96 [Description]

Output: DNA gyrase mutant produces resistance to nalidixic acid


Input: [Genotype] hsd [Description]

Output: Mutations in the system of methylation and restriction that allow E. coli to recognize DNA as foreign. The hsd genotype allows efficient transformation of DNA generated from PCR reactions *hsdR–eliminates restriction of unmethylated EcoK I sites. (1) **hs


Input: [Genotype] lacI [Description]

Output: Encodes the lac repressor that controls expression from promoters that carry the lac operator; IPTG binds the lac repressor and derepresses the promoter; often used when performing blue/white screening or to control expression of recombinant genes


Input: [Genotype] lacY1 [Description]

Output: Blocks use of lactose via β-D-galactosidase mutant


Input: [Genotype] lacZ [Description]

Output: β-D-galactosidase gene; mutations yield colorless (vs. blue) colonies in the presence of X-gal


Input: [Genotype] lacZ∆M15 [Description]

Output: Element required for β-galactosidase complementation when plated on X-gal; used in blue/white screening of recombinants; usually carried on the lambdoid prophage φ80 or F´


Input: [Genotype] leuB [Description]

Output: Requires leucine for growth on minimal media via β-isopropyl malate dehydrogenase mutation


Input: [Genotype] lon [Description]

Output: lon Deficiency in the Lon ATPase-dependent protease; decreases the degradation of recombinant proteins; all B strains carry this mutation


Input: [Genotype] mcrA, mcrBC,or mrr [Description]

Output: Mutations that allow methylated DNA to not be recognized as foreign; this genotype is necessary when cloning genomic DNA or methylated cDNA


Input: [Genotype] nupG [Description]

Output: Mutation for the transport of nucleosides


Input: [Genotype] ompT [Description]

Output: Indicates that the E. coli lack an outer membrane protease—reduces degradation of heterologous the strains and recovery of intact recombinant proteins is improved in ompT minus strains


Input: [Genotype] P3 [Description]

Output: A 60-kb low-copy plasmid that carries the ampicillin and tetracycline resistance genes with amber mutations; used predominantly for selection of supF-containing plasmids; carries the kanamycin resistance gene for selection


Input: [Genotype] pLys [Description]

Output: pLys Plasmid that encodes T7 lysozyme; used to reduce basal expression in T7-driven expression systems by inhibiting basal levels of T7 RNA polymerase


Input: [Genotype] proAB [Description]

Output: proAB Requires proline for growth on minimal media


Input: [Genotype] recA [Description]

Output: Mutation in a gene responsible for general recombination of DNA; particularly desirable when cloning genes with direct repeats


Input: [Genotype] relA [Description]

Output: RNA is synthesized in absence of protein synthesis (relaxed phenotype) relA locus regulates the coupling between transcription and translation. In the wild type, limiting amino acid concentrations results in the shutdown of RNA synthesis (also known as th


Input: [Genotype] rpsL [Description]

Output: Confers resistance to streptomycin (this makes a mutant ribosomal protein, small subunit, the target of the drug)


Input: [Genotype] supE,F [Description]

Output: tRNA glutamine suppressor of amber (supE)(UAG) or tyrosine (supF)


Input: [Genotype] thi-1 [Description]

Output: Requires thiamine for growth on minimal media


Input: [Genotype] Tn10 [Description]

Output: Confers tetracycline resistance via a transposon


Input: [Genotype] tonA [Description]

Output: Confers resistance to the lytic bacteriophage T1, T5 and f80


Input: [Genotype] traD, D36 [Description]

Output: Prevents transfer of F' episome via transfer factor mutation


Input: [Genotype] tsx [Description]

Output: Confers resistance to phage T6 and colicin K


Input: [Genotype] xyl-5 [Description]

Output: Blocks catabolism of xylose


Input: Total Loss No total loss reported to CARFAX. [Owner 3] No Issues Reported [Owner 4] No Issues Reported [Owners 1-2]

Output: No Issues Reported

CARFAX Vehicle History Report for this 2002 VOLVO V70 AWD CROSS COUNTRY: YV1SZ58D621054669


Input: Structural Damage No structural damage reported to CARFAX. [Owner 3] No Issues Reported [Owner 4] No Issues Reported [Owners 1-2]

Output: No Issues Reported

CARFAX Vehicle History Report for this 2002 VOLVO V70 AWD CROSS COUNTRY: YV1SZ58D621054669


Input: Airbag Deployment No airbag deployment reported to CARFAX. [Owner 3] No Issues Reported [Owner 4] No Issues Reported [Owners 1-2]

Output: No Issues Reported

CARFAX Vehicle History Report for this 2002 VOLVO V70 AWD CROSS COUNTRY: YV1SZ58D621054669


Input: Odometer Check No indication of an odometer rollback. [Owner 3] No Issues Indicated [Owner 4] No Issues Indicated [Owners 1-2]

Output: No Issues Indicated

CARFAX Vehicle History Report for this 2002 VOLVO V70 AWD CROSS COUNTRY: YV1SZ58D621054669


Input: Accident / Damage No accidents or damage reported to CARFAX. [Owner 3] No Issues Reported [Owner 4] No Issues Reported [Owners 1-2]

Output: No Issues Reported

CARFAX Vehicle History Report for this 2002 VOLVO V70 AWD CROSS COUNTRY: YV1SZ58D621054669


Input: Manufacturer Recall Check with an authorized Volvo dealer for any open recalls. [Owner 3] No Recalls Reported [Owner 4] No Recalls Reported [Owners 1-2]

Output: No Recalls Reported

CARFAX Vehicle History Report for this 2002 VOLVO V70 AWD CROSS COUNTRY: YV1SZ58D621054669


Input: Basic Warranty Original warranty estimated to have expired. [Owner 3] Warranty Expired [Owner 4] Warranty Expired [Owners 1-2]

Output: Warranty Expired

CARFAX Vehicle History Report for this 2002 VOLVO V70 AWD CROSS COUNTRY: YV1SZ58D621054669


Input: [Column 18] farm laborer [Column 19] working out [Column 19_3] dry goods [Column 18_2]

Output: commercial traveler

Census Questionnaires and Instructions: 1790 to 2000 - Measuring America: The Decennial Censuses From 1790 to 2000 - Survey Census 1930 - Social Explorer


Input: [Column 18] farm laborer [Column 19] home farm [Column 19_3] department store [Column 18_2]

Output: salesman

Census Questionnaires and Instructions: 1790 to 2000 - Measuring America: The Decennial Censuses From 1790 to 2000 - Survey Census 1930 - Social Explorer


Input: [Column 18] laborer [Column 19] odd jobs [Column 19_3] department store [Column 18_2]

Output: bookkeeper

Census Questionnaires and Instructions: 1790 to 2000 - Measuring America: The Decennial Censuses From 1790 to 2000 - Survey Census 1930 - Social Explorer


Input: [Column 18] laborer [Column 19] street work [Column 19_3] department store [Column 18_2]

Output: cash girl

Census Questionnaires and Instructions: 1790 to 2000 - Measuring America: The Decennial Censuses From 1790 to 2000 - Survey Census 1930 - Social Explorer


Input: [Column 18] laborer [Column 19] garden [Column 19_3] department store [Column 18_2]

Output: cashier

Census Questionnaires and Instructions: 1790 to 2000 - Measuring America: The Decennial Censuses From 1790 to 2000 - Survey Census 1930 - Social Explorer


Input: [Column 18] laborer [Column 19] nursery [Column 19_3] bank [Column 18_2]

Output: cashier

Census Questionnaires and Instructions: 1790 to 2000 - Measuring America: The Decennial Censuses From 1790 to 2000 - Survey Census 1930 - Social Explorer


Input: [Column 18] laborer [Column 19] railroad [Column 19_3] steam railroad [Column 18_2]

Output: conductor

Census Questionnaires and Instructions: 1790 to 2000 - Measuring America: The Decennial Censuses From 1790 to 2000 - Survey Census 1930 - Social Explorer


Input: [Column 18] brakeman [Column 19] railroad [Column 19_3] street car [Column 18_2]

Output: conductor

Census Questionnaires and Instructions: 1790 to 2000 - Measuring America: The Decennial Censuses From 1790 to 2000 - Survey Census 1930 - Social Explorer


Input: [Column 18] weaver [Column 19] cotton mill [Column 19_3] general farm [Column 18_2]

Output: farmer

Census Questionnaires and Instructions: 1790 to 2000 - Measuring America: The Decennial Censuses From 1790 to 2000 - Survey Census 1930 - Social Explorer


Input: [Column 18] laborer [Column 19] cotton mill [Column 19_3] truck farm [Column 18_2]

Output: farmer

Census Questionnaires and Instructions: 1790 to 2000 - Measuring America: The Decennial Censuses From 1790 to 2000 - Survey Census 1930 - Social Explorer


Input: [Column 18] doffer [Column 19] cotton mill [Column 19_3] private estates [Column 18_2]

Output: gardener

Census Questionnaires and Instructions: 1790 to 2000 - Measuring America: The Decennial Censuses From 1790 to 2000 - Survey Census 1930 - Social Explorer


Input: [Column 18] engineer [Column 19] locomotive [Column 19_3] general practice [Column 18_2]

Output: lawyer

Census Questionnaires and Instructions: 1790 to 2000 - Measuring America: The Decennial Censuses From 1790 to 2000 - Survey Census 1930 - Social Explorer


Input: [Column 18] engineer [Column 19] lumber mill [Column 19_3] general farm [Column 18_2]

Output: manager

Census Questionnaires and Instructions: 1790 to 2000 - Measuring America: The Decennial Censuses From 1790 to 2000 - Survey Census 1930 - Social Explorer


Input: [Column 18] fireman [Column 19] lumber mill [Column 19_3] truck farm [Column 18_2]

Output: overseer

Census Questionnaires and Instructions: 1790 to 2000 - Measuring America: The Decennial Censuses From 1790 to 2000 - Survey Census 1930 - Social Explorer


Input: [Column 18] fireman [Column 19] fire department [Column 19_3] life insurance co. [Column 18_2]

Output: president

Census Questionnaires and Instructions: 1790 to 2000 - Measuring America: The Decennial Censuses From 1790 to 2000 - Survey Census 1930 - Social Explorer


Input: [Column 18] civil engineer [Column 19] general practice [Column 19_3] bank [Column 18_2]

Output: president

Census Questionnaires and Instructions: 1790 to 2000 - Measuring America: The Decennial Censuses From 1790 to 2000 - Survey Census 1930 - Social Explorer


Input: [Column 18] electrical engineer [Column 19] street railway [Column 19_3] cotton mill [Column 18_2]

Output: superintendent steel works

Census Questionnaires and Instructions: 1790 to 2000 - Measuring America: The Decennial Censuses From 1790 to 2000 - Survey Census 1930 - Social Explorer


Input: [Column 18] carpenter [Column 19] car factory [Column 19_3] street [Column 18_2]

Output: foreman

Census Questionnaires and Instructions: 1790 to 2000 - Measuring America: The Decennial Censuses From 1790 to 2000 - Survey Census 1930 - Social Explorer


Input: [Column 18] carpenter [Column 19] ship yard [Column 19_3] store [Column 18_2]

Output: newsboy

Census Questionnaires and Instructions: 1790 to 2000 - Measuring America: The Decennial Censuses From 1790 to 2000 - Survey Census 1930 - Social Explorer


Input: [Column 18] carpenter [Column 19] house [Column 19_3] groceries [Column 18_2]

Output: newsdealer

Census Questionnaires and Instructions: 1790 to 2000 - Measuring America: The Decennial Censuses From 1790 to 2000 - Survey Census 1930 - Social Explorer


Input: [Column 18] blacksmith [Column 19] carriage factory [Column 19_3] express [Column 18_2]

Output: wagon driver

Census Questionnaires and Instructions: 1790 to 2000 - Measuring America: The Decennial Censuses From 1790 to 2000 - Survey Census 1930 - Social Explorer


Input: [Column 18] blacksmith [Column 19] own shop [Column 19_3] express wagon [Column 18_2]

Output: wagon driver

Census Questionnaires and Instructions: 1790 to 2000 - Measuring America: The Decennial Censuses From 1790 to 2000 - Survey Census 1930 - Social Explorer


Input: [Column 18] agent [Column 19] real estate [Column 19_3] private family [Column 18_2]

Output: chauffeur

Census Questionnaires and Instructions: 1790 to 2000 - Measuring America: The Decennial Censuses From 1790 to 2000 - Survey Census 1930 - Social Explorer


Input: [Column 18] agent [Column 19] insurance [Column 19_3] coal miner [Column 18_2]

Output: chauffeur

Census Questionnaires and Instructions: 1790 to 2000 - Measuring America: The Decennial Censuses From 1790 to 2000 - Survey Census 1930 - Social Explorer


Input: [Column 18] cook [Column 19] hotel [Column 19_3] coal mine [Column 18_2]

Output: miner

Census Questionnaires and Instructions: 1790 to 2000 - Measuring America: The Decennial Censuses From 1790 to 2000 - Survey Census 1930 - Social Explorer


Input: [Column 18] servant [Column 19] private family [Column 19_3] marble [Column 18_2]

Output: laborer

Census Questionnaires and Instructions: 1790 to 2000 - Measuring America: The Decennial Censuses From 1790 to 2000 - Survey Census 1930 - Social Explorer


Input: [Column 18] retail merchant [Column 19] groceries [Column 19_3] house [Column 18_2]

Output: quarryman

Census Questionnaires and Instructions: 1790 to 2000 - Measuring America: The Decennial Censuses From 1790 to 2000 - Survey Census 1930 - Social Explorer


Input: [Column 18] wholesale merchant [Column 19] leather [Column 18_2]

Output: janitor

Census Questionnaires and Instructions: 1790 to 2000 - Measuring America: The Decennial Censuses From 1790 to 2000 - Survey Census 1930 - Social Explorer


Input: [Feature] OS X* Standalone SKU [Benefit]

Output: Applications that use read-write locks can take additional advantage of Intel® Transactional Syncronization Extenstions (Intel® TSX) via tbb::speculative_spin_rw_mutex


Input: [Feature] Pre-Optimized for Performance, Throughput, & Power Efficiency [Benefit]

Output: Functions are highly optimized using SSE and Intel® AVX instruction sets enabling your compute heavy algorithms to achieve maximum performance, beyond what an optimized compiler could produce alone. See above for detailed performance data.


Input: [Feature] Future Proofed Optimizations [Benefit]

Output: Enables you to code once now and then in the future – simply rebuild with the latest version of Intel IPP to realize future processor and instruction set performance gains. This future proofing saves you both time and money on application development.


Input: [Feature] Royalty-free Redistribution [Benefit]

Output: Allows you to redistribute unlimited copies of its runtime libraries with your application, saving you money long term.


Input: [Feature] Thousands of Pre-defined Functions [Benefit]

Output: Speeds your application development letting you focus on differentiating your application, not algorithmic optimization.


Input: [Feature] Samples Jumpstart your Application [Benefit]

Output: Take advantage of source code samples.


Input: [Detail] Job ID [Description]

Output: Displays the number of the job currently being processed.


Input: [Detail] Job Type [Description]

Output: Displays a description of the job being processed.


Input: [Detail] Description [Description]

Output: Displays more information about the job in the queue.


Input: [Detail] Status [Description]

Output: Displays the current state of the Job Processor.


Input: [Detail] Status Bar [Description]

Output: Displays the server name and the user account.


Input: [Detail] Processing Start Time [Description]

Output: Time at which the Job Processor began working on a job.


Input: [parameter] T [permitted values] class name [default value] none [description]

Output: target class

Serialization - Class Serialization Traits


Input: [parameter] Level [permitted values] not_serializable primitive_type object_serializable object_class_info [default value] none [description]

Output: implementation level

Serialization - Class Serialization Traits


Input: [parameter] Tracking [permitted values] track_never track_selectivly track_always [default value] none [description]

Output: tracking level

Serialization - Class Serialization Traits


Input: [parameter] Version [permitted values] unsigned integer [default value] 0 [description]

Output: class version

Serialization - Class Serialization Traits


Input: [parameter] ETTI [permitted values] extended_type_info_typeid extended_type_info_no_rtti [default value] default type_info implementation [description]

Output: type_info implementation

Serialization - Class Serialization Traits


Input: [parameter] IsWrapper [permitted values] mpl::false_ mpl::true_ [default value] mpl::false_ [description]

Output: is the type a wrapper?

Serialization - Class Serialization Traits


Input: [Date Answered] May 11, 2010 [Questioner (age, location)] Dorna (Scotland) [Answer] According to Einstein's General Relativity Theory, light is also affected by gravity. Black holes are very massive objects with extremely intense gravitational field. There is something call "event horizon" around black holes. It is the point where the gravitational attraction becomes so strong that the velocity at which an object would have to move to escape the gravitational field equals the speed of light. Since the speed of light is, according to the relativity theory, the maximum possible speed, nothing, not even light, could escape the black hole once it is inside the event horizon. [Question]

Output: how does blackhole act with the light?

Quickie Questions - Astronomy - Black Holes


Input: [Date Answered] May 3, 2010 [Questioner (age, location)] Albie (Indian) [Answer] Black holes are formed as the result of the collapse of a very massive star at its death. They can´t "appear" from nowhere. But let´s assume that they do, then the huge gravitational field of the black hole would surely atract the Earth towards the black hole. [Question]

Output: suppose a Blackhole appeared just 1cm from Earth,will Earth be safe or will Earth be sucked into the Blackhole?

Quickie Questions - Astronomy - Black Holes


Input: [Date Answered] May 3, 2010 [Questioner (age, location)] Narayanan (India) [Answer] Black Holes may form as the result of the collapse of a very massive star at its death. All the matter of the star's core is crushed to an infinitely small point, a singularity. Now, although it is true that mass can't be destroyed, it can be transform into energy (that's the meaning of the famous equation E = mc2). Black holes may be an important source of gravitational waves, and may also be important for helping other stars to form. For example the gravity of black holes (like other large stellar objects) may promote nebulae to form stars. [Question]

Output: Black hole absorbs everything into it.Mass cannot be destroyed.So where do it go?Why don't we think of a star evolving from a black hole?

Quickie Questions - Astronomy - Black Holes


Input: [Date Answered] March 10, 2010 [Questioner (age, location)] chervon (malaysia) [Answer] Nowhere. All of the mass of the star from which the black hole was formed is still there, maybe even mass from more than one star! [Question]

Output: where does a black hole leads to?

Quickie Questions - Astronomy - Black Holes


Input: [Date Answered] February 5, 2010 [Questioner (age, location)] Van (California) [Answer] In 2002 it was discovered that the stellar-mass black hole called GRO J1655-40, is moving across space at a rate of 250,000 miles per hour, four times faster than the average velocity of the stars in that galactic neighborhood! More information here. [Question]

Output: How fast is a black hole?

Quickie Questions - Astronomy - Black Holes


Input: [Date Answered] February 3, 2010 [Questioner (age, location)] Narayanan (India) [Answer] I don't think there is anything considered "absolute" regarding black holes. One of the hypothesized fate of a black hole depends on the temperature of its surroundings. If the universe is cold enough it will evaporate incredibly slowly. If the background is warmer it will grow slowly until the temperature drops low enough for the hole to start to evaporate. [Question]

Output: What is the absolute fate of a Black Hole ?

Quickie Questions - Astronomy - Black Holes


Input: [Date Answered] January 7, 2010 [Questioner (age, location)] L.Prashanth (Karnataka/India) [Answer] Black holes can be observed through its interaction with other matter, for example, by tracking the movement of a group of stars that orbit a region in space. This animation is a simulation of gravitational lensing caused by a black hole. [Question]

Output: If not even light can escape a black hole,it means that they are invisible. Then how do we know that there are black holes ??

Quickie Questions - Astronomy - Black Holes


Input: [Date Answered] January 7, 2010 [Questioner (age, location)] L.Prashanth (India) [Answer] According to the theory, at the center of a black hole lies the singularity, where matter is crushed to infinite density. More information in our web pag Black Holes. [Question]

Output: Does the SINGULARITY of a black hole have any mass and is the universe infinitely vast ??

Quickie Questions - Astronomy - Black Holes


Input: [Date Answered] January 5, 2010 [Questioner (age, location)] Hassan (USA) [Answer] Albert Einstein's theory of General Relativity states that as you approach a black hole your time slows down. The closer you get to the black hole the more you appear to be in slow motion as seen by Earth. If you were to change your mind right before crossing the event horizon and return to Earth you would find it in the very distant future.More information on our web page Black Holes. [Question]

Output: if a black hole speeds up time in a way that if i went near it and didn't get sucked in ( impossible feat by the way) time would speed up but to me it would feel as though little time passed what would happen to atomic clock ( since it supposedly adjusts to different time speeds because of the speed atoms move differs in space and clock adjusts to it) would it move very fast near a black hole or would it move at regular speed ?

Quickie Questions - Astronomy - Black Holes


Input: [Date Answered] October 27, 2009 [Questioner (age, location)] Narayanan (India) [Answer] Yes, you are right, it was recently published in the article a href="http://news.bbc.co.uk/2/hi/science/nature/7924414.stm">Dancing black hole twins spotted. From this article I quote, "As matter falls into black holes, it emits light of a characteristic colour that in turn gives information about the direction in which the black hole is moving. In a binary system, two beams should be emitted, each a slightly different colour. The black holes emit two beams, each a slightly different colour Todd Boroson and Tod Lauer of the US National Optical Astronomy Observatory analysed some 17,500 spectra from the Sloan Digital Sky Survey, and have now found just such a pair of emissions coming from a distant quasar." [Question]

Output: Sir , from this site itself I heard the news of two black Holes orbiting themselves . How does Scientists got information about this ?

Quickie Questions - Astronomy - Black Holes


Input: [Date Answered] October 19, 2009 [Questioner (age, location)] Alec (Arizona) [Answer] Black Holes are theoretical objects. A black hole is an object which has such high gravitational pull that not even light can escape. Hence it is black. Which makes it pretty hard to observe directly. Black Holes may form as the result of the collapse of a very massive star at its death. Just as neutron stars form during a supernova explosion of a very massive star so do black holes. But in the black hole case the initial star was so massive that nothing could stop its gravitational collapse. All the matter of the star's core is crushed to an infinitely small point, a singularity. More information can be found at our web page Black Holes. [Question]

Output: How do black holes work?

Quickie Questions - Astronomy - Black Holes


Input: [Date Answered] October 13, 2009 [Questioner (age, location)] Phil (ct,usa) [Answer] An explicit relationship between the size of a black hole and the energy it has absorbed has been recently published. See this article for a discussion on this topic. [Question]

Output: Scientists say that matter in a black hole gets crushed out of existence. If that is true then how can a black hole grow? Matter must remain in existence to have an affect in our universe, and thereby adding to the mass of the black hole causing it to grow.

Quickie Questions - Astronomy - Black Holes


Input: [Date Answered] October 8, 2009 [Questioner (age, location)] Narayanan (India) [Answer] Extracted from our web page Black Holes: Black Holes are theoretical objects. A black hole is an object which has such high gravitational pull that not even light can escape. Hence it is black. Which makes it pretty hard to observe directly. Black Holes may form as the result of the collapse of a very massive star at its death. Just as neutron stars form during a supernova explosion of a very massive star so do black holes. But in the black hole case the initial star was so massive that nothing could stop its gravitational collapse. All the matter of the star's core is crushed to an infinitely small point, a singularity. [Question]

Output: Will all neutron stars become black holes?

Quickie Questions - Astronomy - Black Holes


Input: [Date Answered] September 30, 2009 [Questioner (age, location)] Narayanan (India) [Answer] Black Holes may form as the result of the collapse of a very massive star at its death, so massive that nothing could stop its gravitational collapse. All the matter of the star's core is crushed to an infinitely small point, a singularity. [Question]

Output: Sir, is there any possibility for a black hole to become a star again?Or is black hole the last stage of the evolutional process of star?Sir please give me an answer.I am really waiting for this reply.

Quickie Questions - Astronomy - Black Holes


Input: [Date Answered] August 21, 2009 [Questioner (age, location)] APARAJITH (India) [Answer] Theoretically, once you have passed the event horizon, it is not possible to escape the black hole. Under this premise, your question doesn't have an answer. [Question]

Output: gravity slows down time,so IF we reach the event horizon,the time will stop,then if we pass near a black hole and return to the earth then the time which passes on earth will be more than the time which passes on the spaceship.then if we keep passing the blackhole for a year,can we return to earth and find that 20 or so years have passed?

Quickie Questions - Astronomy - Black Holes


Input: [Date Answered] July 23, 2009 [Answer] From our web page Black Holes: What would it be like to enter a black hole? Not pleasant. First, as you approach the black hole the difference in the gravitaional pull on your head compared to your feet (known as tidal forces) would rip you apart. [Question]

Output: what the odds of are planet getting caught in a black hole and us surviving.

Quickie Questions - Astronomy - Black Holes


Input: [Date Answered] July 20, 2009 [Questioner (age, location)] Liam (Georgia, North America) [Answer] Yes, they could orbit a twin, as it as recently published in the article Dancing black hole twins spotted. [Question]

Output: Do supermassive black holes orbit anything? If not, how do they travel?

Quickie Questions - Astronomy - Black Holes


Input: [Date Answered] July 20, 2009 [Questioner (age, location)] Owen (alberta) [Answer] I am not sure if there is an answer to your question. Black Holes are theoretical objects with such high gravitational pull that not even light can escape. They are supposed to exist in the center of galaxies. Our web site Black Holes provides more information. [Question]

Output: Can a black hole be destroyed

Quickie Questions - Astronomy - Black Holes


Input: [Date Answered] July 17, 2009 [Questioner (age, location)] Owen (Canada) [Answer] I am not sure if there is an nswer to your question. Black Holes are theoretical objects with such high gravitational pull that not even light can escape. They are supposed to exist in the center of galaxies. Our web site Black Holes provides more information. [Question]

Output: Can a black hole be destroyed

Quickie Questions - Astronomy - Black Holes


Input: [Date Answered] June 2, 2009 [Questioner (age, location)] Aparajith (India) [Answer] Nothing. Black holes are so massive that they will swallow the planet without changing their own state. [Question]

Output: There is a planet near a blackhole.what will happen to the position of the black hole?

Quickie Questions - Astronomy - Black Holes


Input: [Date Answered] March 25, 2009 [Questioner (age, location)] anthony (ma) [Answer] Pull is a force, and in this case is due to gravity. The huge gravitational field around a black hole exerts an immense attractional force over all masses, including light. Visit our web page Black Holes for more information. [Question]

Output: pondering on this for a while. is pull a speed? if so than black holes would be pulling faster then the speed of light which would mean black holes are the fastest? is this true? i feel like it could be. id rather you let me know on your thought. thanks in return. i get this idea from the knowledge that light cant escape black holes. light is sucked in black holes. thanks.

Quickie Questions - Astronomy - Black Holes


Input: [Date Answered] March 11, 2009 [Questioner (age, location)] Bilal (Canada) [Answer] From our web page Black Holes: What would it be like to enter a black hole? Not pleasant. First, as you approach the black hole the difference in the gravitaional pull on your head compared to your feet (known as tidal forces) would rip you apart. But suppose you survived that. Once you cross the event horizon there is no turning back. Then the only thing to do is avoid the black hole itself at all costs. If you run into that singularity it will crush your body right out of existence. If people from Earth were watching your journey into a black hole they would never see you cross the event horizon. Albert Einstein's theory of General Relativity says that as you approach a black hole your time slows down. The closer you get to the black hole the more you appear to be in slow motion as seen by Earth. Eventually you appear to be frozen in time as you cross the event horizon. You would notice nothing different whatsoever. If you were to change your mind right before crossing the event horizon and return to Earth you would find it in the very distant future. You've become a time traveler! [Question]

Output: what would happen "if" a human were to go inside a black hole?? what would he see??

Quickie Questions - Astronomy - Black Holes


Input: [Date Answered] November 4, 2008 [Questioner (age, location)] Emily (texas) [Answer] Extracted from our web page Black Holes: Black Holes are theoretical objects. A black hole is an object which has such high gravitational pull that not even light can escape. Hence it is black. Which makes it pretty hard to observe directly. Black Holes may form as the result of the collapse of a very massive star at its death. What would it be like to enter a black hole? Not pleasant. First, as you approach the black hole the difference in the gravitaional pull on your head compared to your feet (known as tidal forces) would rip you apart. But suppose you survived that. Once you cross the event horizon there is no turning back. Then the only thing to do is avoid the black hole itself at all costs. If you run into that singularity it will crush your body right out of existence. [Question]

Output: What happens after wew get into a black hole, how do we know there is a black hole in side of every sprial and elpitical galaxy if we cant go near one because we would get sucked in?

Quickie Questions - Astronomy - Black Holes


Input: [Date Answered] September 18, 2008 [Questioner (age, location)] fara (malaysia) [Answer] I am not sure what your father meant by that. Black holes are an enormous amount of mass confined in a very small volume, so they have a well define limit all around. [Question]

Output: is it true black hole doesn't have an ending?my father said black hole doesn't have an ending,howcome?everything do have an ending.

Quickie Questions - Astronomy - Black Holes


Input: [Date Answered] September 16, 2008 [Questioner (age, location)] priyanka (india) [Answer] This limit is known as event horizon. This is the boundary within which the black hole's escape velocity (minimum velocity to escape a gravitational field) is greater than the speed of light. In other words, within this radius a radiation will have to moves faster than light to escape, but because the speed of light in a vacuum is the speed limit, nothing can escape from inside the event horizon of a black hole!. [Question]

Output: why can't light escape blackhole only within a particular radius?

Quickie Questions - Astronomy - Black Holes


Input: [Date Answered] September 3, 2008 [Questioner (age, location)] John (United States) [Answer] Extracted from our web page Black Holes: Black Holes are theoretical objects. A black hole is an object which has such high gravitational pull that not even light can escape. Hence it is black. Which makes it pretty hard to observe directly. Black Holes may form as the result of the collapse of a very massive star at its death. Just as neutron stars form during a supernova explosion of a very massive star so do black holes. But in the black hole case the initial star was so massive that nothing could stop its gravitational collapse. All the matter of the star's core is crushed to an infinitely small point, a singularity. [Question]

Output: What is a dark hole, what causes it, and how many years from now until there is another one?

Quickie Questions - Astronomy - Black Holes


Input: [Date Answered] August 19, 2008 [Questioner (age, location)] Tom (Kansas USA) [Answer] Anything about black holes is purely theoretical. Keeping this in mind, this link will answer your question. [Question]

Output: Does time exist in a super massive black hole or is it completely stopped?

Quickie Questions - Astronomy - Black Holes


Input: [Date Answered] August 15, 2008 [Questioner (age, location)] roli (india) [Answer] Black holes are supposed to exist in the center of galaxies, but be aware that they are theoretical objects! See more in our web page Black Holes. [Question]

Output: how do you locate a black hole

Quickie Questions - Astronomy - Black Holes


Input: [Date Answered] August 15, 2008 [Questioner (age, location)] Mary (Tanzania) [Answer] Black Holes are theoretical objects. A black hole is an object which has such high gravitational pull that not even light can escape. Hence it is black. Which makes it pretty hard to observe directly. Black Holes may form as the result of the collapse of a very massive star at its death. More information can be found in our web page Black Holes. [Question]

Output: what are black holes and what are they made out of???

Quickie Questions - Astronomy - Black Holes


Input: [Date Answered] April 7, 2008 [Questioner (age, location)] joshua (north carolina) [Answer] A black hole is a very massive object with such an enormous gravity that almost nothing can escape from its atraction (except what is known as Hawkings radiation). There are other theories that mention new dimensions, but are not related to black holes. [Question]

Output: scientists theory about the black hole is that if you go in it, is there a 5th demention? if there is, how does a 5th demention go like? i need your answers. peace!"

Quickie Questions - Astronomy - Black Holes


Input: [Date Answered] February 4, 2008 [Questioner (age, location)] Nicco (Indiana, U.S.A) [Answer] They will merge in an extremely big and dense object, releasing in the process huge amount of energy. [Question]

Output: What happens if 2 black holes get extremely close to eachother and/or collide.

Quickie Questions - Astronomy - Black Holes


Input: [Date Answered] December 17, 2007 [Questioner (age, location)] Conrad (Australia) [Answer] No, once you are in the vicinity of the black holes, strong forces will act over you, and several interesting things will happen. This site offers detailed answers to the comon questions about black holes. [Question]

Output: Is this true that when you go into a black hole and cannot escape with the speed of light, when your inside it do appear in a diffrent universe or time or is this what wormholes do?

Quickie Questions - Astronomy - Black Holes


Input: [Date Answered] December 10, 2007 [Questioner (age, location)] shania (TX) [Answer] I don't think there is a unique theoretical answer to this question, but what seems to be generally accepted by physicists is that if an event occurs close enough to a black hole where antimatter is thrown in but the matter escapes from the black hole (this is known as Hawking Radiation), and this happens enough, the black hole will begin to "evaporate". [Question]

Output: on average about how long do black holes last????

Quickie Questions - Astronomy - Black Holes


Input: [Date Answered] August 21, 2007 [Questioner (age, location)] Mark (New Zealand Christchurch) [Answer] The gravitational force is a function of the product of the interacing masses and the inverse of he square of the distance between them. Black holes masses are enormous, for example, the giant elliptical galaxy M87 is believed to contain a supermassive black hole of several billion solar masses at its center. The observations indicate that approximately 3 billion solar masses are concentrated in a region at the galactic core that is only about the size of the Solar System. [Question]

Output: What causes black holes to have such a gravitational pull?

Quickie Questions - Astronomy - Black Holes


Input: [Date Answered] July 25, 2007 [Questioner (age, location)] veena (india) [Answer] The short answer is yes, but we can't get out of there! [Question]

Output: can we go in black hole?

Quickie Questions - Astronomy - Black Holes


Input: [Date Answered] July 25, 2007 [Questioner (age, location)] Veena (india) [Answer] We have a very massive black hole at the center of our own galaxy, the Milky Way. [Question]

Output: where did a nearest black hole was?

Quickie Questions - Astronomy - Black Holes


Input: [Date Answered] July 23, 2007 [Questioner (age, location)] vik (america) [Answer] Black Holes are theoretical objects. A black hole is an object which has such high gravitational pull that not even light can escape. Hence it is black (which makes it pretty hard to observe directly). Black Holes may form as the result of the collapse of a very massive star at its death. More detailed information at our web page Black Hole. [Question]

Output: what is black hole .

Quickie Questions - Astronomy - Black Holes


Input: [Date Answered] July 21, 2007 [Questioner (age, location)] piyu (india) [Answer] Black Holes are theoretical objects. A black hole is an object which has such high gravitational pull that not even light can escape. Hence it is black. Which makes it pretty hard to observe directly. Black Holes may form as the result of the collapse of a very massive star at its death. More information in our web page Black Holes. [Question]

Output: what is black hole?

Quickie Questions - Astronomy - Black Holes


Input: [Date Answered] July 21, 2007 [Questioner (age, location)] Elric (Iowa) [Answer] Although there is no observational evidence of the collision of two black holes, the theory predicts what will happen to them. This article from the National Science Foundation discusses the latest finding. This impressive video shows how it is predicted that the black holes will behave. [Question]

Output: Can black holes escape echoter, or rip echothers mass apart?

Quickie Questions - Astronomy - Black Holes


Input: [Date Answered] July 18, 2007 [Questioner (age, location)] Elric (Iowa) [Answer] The mass of a supermassive black hole is of the order of a billion solar masses at their center. [Question]

Output: How big is a supermassive black hole?

Quickie Questions - Astronomy - Black Holes


Input: [Date Answered] July 11, 2007 [Questioner (age, location)] Kim Hale (Minnesota) [Answer] Because due to their incredible gravitational field, almost nothing, including light, can escape from them, and so no radiation can be detected friom them. [Question]

Output: Why are black holes said to be black?

Quickie Questions - Astronomy - Black Holes


Input: [Date Answered] July 9, 2007 [Questioner (age, location)] DEEPSHIKA (INDIA) [Answer] Black holes are the evolutionary endpoints of stars at least 10 to 15 times as massive as the Sun. And all that mass will end concentrated in a very small (for cosmic standards) region. [Question]

Output: why do black holes have so much of gravitational force?

Quickie Questions - Astronomy - Black Holes


Input: [Date Answered] May 30, 2007 [Questioner (age, location)] Aheli ( India) [Answer] Black holes are theoretical objects. A black hole is an object which has such high gravitational pull that not even light can escape. Hence it is black (which makes it pretty hard to observe directly). Black holes may form as the result of the collapse of a very massive star at its death. More detailed information at our web page Black Holes. [Question]

Output: What is a black holl? Do they really exists? please try to explaim me in full details.

Quickie Questions - Astronomy - Black Holes


Input: [Date Answered] March 2, 2007 [Questioner (age, location)] Veena (india) [Answer] Black Holes are theoretical objects. A black hole is an object which has such high gravitational pull that not even light can escape. Hence it is black (which makes it pretty hard to observe directly). Black Holes may form as the result of the collapse of a very massive star at its death. More detailed information at our web page Black Hole. [Question]

Output: What is a black hole?

Quickie Questions - Astronomy - Black Holes


Input: [Date Answered] March 1, 2007 [Questioner (age, location)] karthick (india) [Answer] Black Holes are theoretical objects. A black hole is an object which has such high gravitational pull that not even light can escape. Hence it is black (which makes it pretty hard to observe directly). Black Holes may form as the result of the collapse of a very massive star at its death. More detailed information at our web page Black Holes. [Question]

Output: what is black hole?what is the range of its gravity?what is the age of the star which can turn into a black hole?

Quickie Questions - Astronomy - Black Holes


Input: [Date Answered] May 19, 1999 [Questioner (age, location)] Linda and Ellen (Alaska, USA) [Answer] Magnetic field lines are generated by movement of electric field lines. An electric field forms when electric charge falls into a black hole. In this case, the "swallowing" of photons produces an electric charge within the hole, creating an electric field around it. When the black hole rotates, this electric field rotates as well. This creates a magnetic field. [Question]

Output: According to Quantum Electrodynamics, the electromagnetic force is transmitted by photons, yet black holes are said to have the characteristic of a magnetic field. How can this be when photons are transmitting the field and they travel slower than the escape velocity of a black hole?

Quickie Questions - Astronomy - Black Holes


Input: [Date Answered] May 13, 1999 [Questioner (age, location)] Carly(British Columbian, Canada) [Answer] There really couldn't be a black hole at the edge of the solar system because a black hole would devour the solar system! [Question]

Output: Why do scientists suspect a black hole just on the outer edges of the Solar System and what are the chances of it really being there?

Quickie Questions - Astronomy - Black Holes


Input: [Date Answered] September 2, 1998 [Questioner (age, location)] Lalita (Maharashtra, India) [Answer] Black holes can gain mass that falls into them from their surroundings and grow. They also can evaporate if there is nothing entering them. However, for star-sized black holes, this evaporation can take more than 10^100 years. [Question]

Output: Can a black hole be destroyed , is it true that a black hole gets larger and larger ????

Quickie Questions - Astronomy - Black Holes


Input: [Date Answered] August 5, 1998 [Questioner (age, location)] Steve (England) [Answer] A white hole is the purely theoretical counterpart to a black hole from which light and matter are expelled. Such an object has never been detected, and our current understanding of the physics involved argues that even if they had existed at one tim e, they would necessarily have been destroyed by now. [Question]

Output: If there are black holes, are there such a thing as white holes?

Quickie Questions - Astronomy - Black Holes


Input: [Date Answered] May 27, 1998 [Questioner (age, location)] Kaelyn (Oklahoma, USA) [Answer] The most massive star known is R136a1, a star 155 times as massive as our Sun. It is one of many extremely massive stars in a very young "super cluster", R136, in the 30 Doradus region of the Large Magellanic C loud. Black holes don't have names like the bright stars in our sky, such as Betelgeuse. We cannot detect black holes directly, but we can sometimes detect x-ray emission from the material surrounding them. This related x-ray source may be named. Cygnus X-1, for example, is the 1st x-ray source detected in Cygnus, and is probably a disk of gas and dust spiraling into a black hole. [Question]

Output: What is the name of the largest known star? Do black holes have names?

Quickie Questions - Astronomy - Black Holes


Input: [Date Answered] April 30, 1998 [Questioner (age, location)] Travis ( Minnesota, U.S.A.) [Answer] Yes. Only elementary particles ever could come out of a black hole. Even things as small as molecules are destroyed. [Question]

Output: Is it true that the gravity of a black hole is so strong that it can even pull molecules apart?

Quickie Questions - Astronomy - Black Holes


Input: [Date Answered] April 30, 1998 [Questioner (age, location)] Rahul (New Jersey, U.S.A.) [Answer] This question is a very difficult one... the answer is that no one knows the answer. For a (complicated) discussion on this topic, you might try this page. The thing about white holes is that based on our current knowledge of the universe, they are not possible. (They violate the second law of thermodynamics.) However, as the article says, there is no guarantee that the rest of the universe is like what we know now. Thus, we can't totally rule out the possibility of the universe having come from a white hole. [Question]

Output: Could the universe have formed by a white Hole? Suppose another physical universe such as our own underwent a big crunch. Could not have all the matter in the big crunch create a black hole powerful enough to entirely devour all the matter in that uni verse and eject it into a new universe in the form of a white hole. Thus this theory partly accepts the big bang theory, that states that the universe started from a single point from which space and time started, except this big bang was created by an enormous and powerful black hole. Can this be possible?

Quickie Questions - Astronomy - Black Holes


Input: [Date Answered] April 14, 1998 [Questioner (age, location)] Howard (Australia) [Answer] The extraordinary effects of gravity for a small black hole are only felt up to a few hundred miles away. Farther than this, the gravity felt is that corresponding to the original mass of the star. However, as the light which enters that radius is u nable to escape and becomes part of the black hole, the black hole grows and its gravity is felt at a greater distance. [Question]

Output: If black holes have the same attractive force as the star from which it formed, why then is it black. I.e. why can't light escape as it could from the preceding star?

Quickie Questions - Astronomy - Black Holes


Input: [Date Answered] April 8, 1998 [Questioner (age, location)] Howard (Australia) [Answer] They actually do have exactly the same gravitational force. Gravity is proportional to mass, so if the mass is exactly the same, they will have the same gravitational attraction. For example, if our Sun were to suddenly become a black hole, the plan ets would experience no change in orbit, because the gravitational pull of the Sun would remain constant. [Question]

Output: Why is the attraction of a black hole so much greater than the star from which it formed, shouldn't they have the same gravitational attraction?

Quickie Questions - Astronomy - Black Holes


Input: [Date Answered] April 7, 1998 [Questioner (age, location)] Maggie (Norway) [Answer] So far, the existance of dark matter is only a theory. We would have to prove its existence before making any use of it! [Question]

Output: Is it possible for us humans to make any use of black matter?

Quickie Questions - Astronomy - Black Holes


Input: [Date Answered] April 3, 1998 [Questioner (age, location)] Michael (Denmark) [Answer] The reason it is a theory is that it hasn't been proved yet. Since we are unable to see dark matter, we can only see its effects on other objects, such as gravitational pull. Based on calculations involving things like gravity, it seems very likely that dark matter does exist. [Question]

Output: How come the theory about dark matter is that common, when nobody has ever proved the excistance of it?

Quickie Questions - Astronomy - Black Holes


Input: [Date Answered] March 19, 1998 [Questioner (age, location)] Giulio (Milan, Italy) [Answer] Current data indicates that there is a very dense 'point mass' at the center of our galaxy, containing mass up to 1 million times the mass of our sun. This indicates that there is probably a black hole located there. [Question]

Output: What makes people think that in the center of our galaxy thers'a black hole?

Quickie Questions - Astronomy - Black Holes


Input: [Date Answered] March 17, 1998 [Questioner (age, location)] Camille and Ken (Massachusetts, USA) [Answer] A black hole would certainly disrupt the asteroids and comets, but you underestimate the strength of a black hole. Such a thing would destroy the solar system, not just divert the orbits of asteroids. [Question]

Output: We were just wondering, if there were a black hole in our solar system, that went in and out of the solar system (we'll call it Thesus) every 26 million years, wouldn't it disrupt the cycles of the asteroids, comets and planets, causing many of those asteroids to crash on the planets? That could be why the dinosaurs became extinct, right? Do you think that is a debatable theory?

Quickie Questions - Astronomy - Black Holes


Input: [Date Answered] March 13, 1998 [Questioner (age, location)] Thomaz ( Brazil) [Answer] As their name implies, black holes are black! Not even light can escape from the strong gravity of a black hole. Does that mean astronomers have no hope of ever detecting one? Fortunately, while direct detection of light from a black hole is not possible, astronomers can indirectly detect them via their gravitational effect on other objects. For example, some black holes are sucking in the material around them, formin g what is known as an accretion disk. As the material in the disk is packed together, spiraling in towards the black hole, it gets heated up and emits high energy photons such as x-rays, which can be detected by astronomers. Black holes in bina ry systems can be "weighed" by measuring the orbital parameters of the system. Evidence of supermassive black holes in the centers of galaxies has been provided by the Hubble Space Telescope. HST observed stars very near to the centers of galaxies. By measuring the velocities of these stars, it was possible to tell how much mass w as contained in the center of the galaxy. These measurements showed that as much as 100 million times the mass of the Sun may be contained in an area only a few parsecs across. Matter of this density almost certainly implies the existence of a supermass ive black hole. [Question]

Output: Is that proved the black holes exists?How can they (astronomers)prove that?

Quickie Questions - Astronomy - Black Holes


Input: [Attribute] AffectViewingBox [Default Value] TRUE [Purpose]

Output: influence of objects on the ViewingBox of a scene

Numerical approximation of an integral - MATLAB


Input: [Attribute] AntiAliased [Default Value] TRUE [Purpose]

Output: antialiased lines and points?

Numerical approximation of an integral - MATLAB


Input: [Attribute] Color [Default Value] RGB::PaleBlue [Purpose]

Output: the main color

Numerical approximation of an integral - MATLAB


Input: [Attribute] Filled [Default Value] TRUE [Purpose]

Output: filled or transparent areas and surfaces

Numerical approximation of an integral - MATLAB


Input: [Attribute] FillColor [Default Value] RGB::PaleBlue [Purpose]

Output: color of areas and surfaces

Numerical approximation of an integral - MATLAB


Input: [Attribute] FillPattern [Default Value] Solid [Purpose]

Output: type of area filling

Numerical approximation of an integral - MATLAB


Input: [Attribute] Frames [Default Value] 50 [Purpose]

Output: the number of frames in an animation

Numerical approximation of an integral - MATLAB


Input: [Attribute] Function1 [Purpose]

Output: first function/curve delimiting hatch

Numerical approximation of an integral - MATLAB


Input: [Attribute] HorizontalAlignment [Default Value] Left [Purpose]

Output: horizontal alignment of text objects w.r.t. their coordinates

Numerical approximation of an integral - MATLAB


Input: [Attribute] IntMethod [Default Value] Exact [Purpose]

Output: method for integral approximation

Numerical approximation of an integral - MATLAB


Input: [Attribute] Legend [Purpose]

Output: makes a legend entry

Numerical approximation of an integral - MATLAB


Input: [Attribute] LegendText [Purpose]

Output: short explanatory text for legend

Numerical approximation of an integral - MATLAB


Input: [Attribute] LegendEntry [Default Value] FALSE [Purpose]

Output: add this object to the legend?

Numerical approximation of an integral - MATLAB


Input: [Attribute] LineColor [Default Value] RGB::Black [Purpose]

Output: color of lines

Numerical approximation of an integral - MATLAB


Input: [Attribute] LineWidth [Default Value] 0.35 [Purpose]

Output: width of lines

Numerical approximation of an integral - MATLAB


Input: [Attribute] LineColor2 [Default Value] RGB::Grey [Purpose]

Output: color of lines

Numerical approximation of an integral - MATLAB


Input: [Attribute] LineStyle [Default Value] Solid [Purpose]

Output: solid, dashed or dotted lines?

Numerical approximation of an integral - MATLAB


Input: [Attribute] LinesVisible [Default Value] TRUE [Purpose]

Output: visibility of lines

Numerical approximation of an integral - MATLAB


Input: [Attribute] LineColorType [Default Value] Flat [Purpose]

Output: line coloring types

Numerical approximation of an integral - MATLAB


Input: [Attribute] LineColorFunction [Purpose]

Output: functional line coloring

Numerical approximation of an integral - MATLAB


Input: [Attribute] Name [Purpose]

Output: the name of a plot object (for browser and legend)

Numerical approximation of an integral - MATLAB


Input: [Attribute] Nodes [Default Value] [10] [Purpose]

Output: number of subintervals or list of x-values for subintervals

Numerical approximation of an integral - MATLAB


Input: [Attribute] ParameterEnd [Purpose]

Output: end value of the animation parameter

Numerical approximation of an integral - MATLAB


Input: [Attribute] ParameterName [Purpose]

Output: name of the animation parameter

Numerical approximation of an integral - MATLAB


Input: [Attribute] ParameterBegin [Purpose]

Output: initial value of the animation parameter

Numerical approximation of an integral - MATLAB


Input: [Attribute] ParameterRange [Purpose]

Output: range of the animation parameter

Numerical approximation of an integral - MATLAB


Input: [Attribute] PointSize [Default Value] 1.5 [Purpose]

Output: the size of points

Numerical approximation of an integral - MATLAB


Input: [Attribute] PointStyle [Default Value] FilledCircles [Purpose]

Output: the presentation style of points

Numerical approximation of an integral - MATLAB


Input: [Attribute] PointsVisible [Default Value] FALSE [Purpose]

Output: visibility of mesh points

Numerical approximation of an integral - MATLAB


Input: [Attribute] ShowInfo [Default Value] [2, IntMethod, Integral] [Purpose]

Output: Information about integral approximation

Numerical approximation of an integral - MATLAB


Input: [Attribute] TextFont [Default Value] [" sans-serif ", 11] [Purpose]

Output: font of text objects

Numerical approximation of an integral - MATLAB


Input: [Attribute] TextRotation [Default Value] 0 [Purpose]

Output: rotation of a 2D text

Numerical approximation of an integral - MATLAB


Input: [Attribute] TimeEnd [Default Value] 10.0 [Purpose]

Output: end time of the animation

Numerical approximation of an integral - MATLAB


Input: [Attribute] TimeBegin [Default Value] 0.0 [Purpose]

Output: start time of the animation

Numerical approximation of an integral - MATLAB


Input: [Attribute] TimeRange [Default Value] 0.0 .. 10.0 [Purpose]

Output: the real time span of an animation

Numerical approximation of an integral - MATLAB


Input: [Attribute] Title [Purpose]

Output: object title

Numerical approximation of an integral - MATLAB


Input: [Attribute] TitleFont [Default Value] [" sans-serif ", 11] [Purpose]

Output: font of object titles

Numerical approximation of an integral - MATLAB


Input: [Attribute] TitlePosition [Purpose]

Output: position of object titles

Numerical approximation of an integral - MATLAB


Input: [Attribute] TitleAlignment [Default Value] Center [Purpose]

Output: horizontal alignment of titles w.r.t. their coordinates

Numerical approximation of an integral - MATLAB


Input: [Attribute] TitlePositionX [Purpose]

Output: position of object titles, x component

Numerical approximation of an integral - MATLAB


Input: [Attribute] TitlePositionY [Purpose]

Output: position of object titles, y component

Numerical approximation of an integral - MATLAB


Input: [Attribute] VerticalAlignment [Default Value] Bottom [Purpose]

Output: vertical alignment of text objects w.r.t. their coordinates

Numerical approximation of an integral - MATLAB


Input: [Attribute] Visible [Default Value] TRUE [Purpose]

Output: visibility

Numerical approximation of an integral - MATLAB


Input: [Attribute] VisibleAfter [Purpose]

Output: object visible after this time value

Numerical approximation of an integral - MATLAB


Input: [Attribute] VisibleBefore [Purpose]

Output: object visible until this time value

Numerical approximation of an integral - MATLAB


Input: [Attribute] VisibleFromTo [Purpose]

Output: object visible during this time range

Numerical approximation of an integral - MATLAB


Input: [Attribute] VisibleAfterEnd [Default Value] TRUE [Purpose]

Output: object visible after its animation time ended?

Numerical approximation of an integral - MATLAB


Input: [Attribute] VisibleBeforeBegin [Default Value] TRUE [Purpose]

Output: object visible before its animation time starts?

Numerical approximation of an integral - MATLAB


Input: [Finding] All available types of evidence support the case for the candidate cause. [Score] + + + [Interpretation]

Output: This finding convincingly supports the case for the candidate cause.

Consistency of evidence | CADDIS: Stressor Identification | US EPA


Input: [Finding] All available types of evidence weaken the case for the candidate cause. [Score] - - - [Interpretation]

Output: This finding convincingly weakens the candidate cause.

Consistency of evidence | CADDIS: Stressor Identification | US EPA


Input: [Finding] All available types of evidence support the case for the candidate cause, but few types are available. [Score] + [Interpretation]

Output: This finding somewhat supports the case for the candidate cause, but is not strongly supportive because coincidence and errors may be responsible.

Consistency of evidence | CADDIS: Stressor Identification | US EPA


Input: [Finding] All available types of evidence weaken the case for the candidate cause, but few types are available. [Score] - [Interpretation]

Output: This finding somewhat weakens the case for the candidate cause, but is not strongly weakening because coincidence and errors may be responsible.

Consistency of evidence | CADDIS: Stressor Identification | US EPA


Input: [Finding] The evidence is ambiguous or inadequate. [Score] 0 [Interpretation]

Output: This finding neither supports nor weakens the case for the candidate cause.

Consistency of evidence | CADDIS: Stressor Identification | US EPA


Input: [Finding] Some available types of evidence support and some weaken the case for the candidate cause. [Score] - [Interpretation]

Output: This finding somewhat weakens the case for the candidate cause, but is not convincing because a few inconsistencies may be explained.

Consistency of evidence | CADDIS: Stressor Identification | US EPA


Input: [1] Name [2] Type [3] Description [0]

Output: Required


Input: [1] event [2] string [3] The event that you wish to segment on. [0]

Output: required


Input: [1] from_date [2] string [3] The date in yyyy-mm-dd format from which to begin querying for the event from. This date is inclusive. [0]

Output: required


Input: [1] to_date [2] string [3] The date in yyyy-mm-dd format from which to stop querying for the event from. This date is inclusive. The date range may not be more than 30 days. [0]

Output: required


Input: [1] on [2] string [3] The expression to average per unit time. The result of the expression should be a numeric value. If the expression is not numeric, a value of 0.0 is assumed. See the expressions section below. [0]

Output: required


Input: [1] unit [2] string [3] This can be "hour" or "day". This determines the buckets into which the property values that you segment on are placed. The default value is "day". [0]

Output: optional


Input: [1] where [2] string [3] An expression to filter events by. See the expressions section below. [0]

Output: optional


Input: [0] API [1] hostnamed [2] localed [3] timedated [4] initrd interface [5] Container interface [6] Boot Loader interface [7] Service bus API [8] logind [9] sd-login.h API [10] sd-daemon.h API [11] sd-id128.h API [12] sd-journal.h API [13] $XDG_RUNTIME_DIR [14] $LISTEN_FDS/$LISTEN_PID FD Passing [15] $NOTIFY_SOCKET Daemon Notifications [16] argv[0][0]='@' Logic [17] Unit file format [18] Journal File Format [19] Journal Export Format [20] Cooperation in cgroup tree [21] Password Agents [22] udev multi-seat properties [23] udev session switch ACL properties [24] CLI of systemctl,... [25] /etc/tmpfiles.d [26] /etc/machine-id [27] /etc/binfmt.d [28] /etc/hostname [29] /etc/locale.conf [30] /etc/machine-info [31] /etc/modules-load.d [32] /etc/os-release [33] /etc/sysctl.d [34] /etc/timezone [35] /etc/vconsole.conf [36] /run [37] Generators [38] System Updates [39] Presets [40]

Output: Udev rules


Input: [0] Type [1] D-Bus [2] D-Bus [3] D-Bus [4] Environment, flag files [5] Environment, Mounts [6] EFI variables [7] D-Bus [8] D-Bus [9] C Library [10] C Library or Drop-in [11] C Library [12] C Library [13] Environment [14] Environment [15] Environment [16] /proc marking [17] File format [18] File format [19] File format [20] Treaty [21] Socket+Files [22] udev Property [23] udev Property [24] CLI [25] File format [26] File format [27] File format [28] File format [29] File format [30] File format [31] File format [32] File format [33] File format [34] File format [35] File format [36] File hierarchy change [37] Subprocess [38] System Mode [39] File format [40]

Output: File format


Input: [0] Covered by Interface Stability Promise [1] yes [2] yes [3] yes [4] yes [5] yes [6] yes [7] yes [8] yes [9] yes [10] yes [11] yes [12] yes [13] yes [14] yes [15] yes [16] yes [17] yes [18] yes [19] yes [20] yes [21] yes [22] yes [23] no [24] yes [25] yes [26] yes [27] yes [28] yes [29] yes [30] yes [31] yes [32] yes [33] yes [34] yes [35] yes [36] yes [37] yes [38] yes [39] yes [40]

Output: yes


Input: [0] Fully documented [1] yes [2] yes [3] yes [4] yes [5] yes [6] yes [7] yes [8] yes [9] yes [10] yes [11] yes [12] yes [13] yes [14] yes [15] yes [16] yes [17] yes [18] yes [19] yes [20] yes [21] yes [22] yes [23] no [24] yes [25] yes [26] yes [27] yes [28] yes [29] yes [30] yes [31] yes [32] yes [33] yes [34] yes [35] yes [36] yes [37] yes [38] yes [39] yes [40]

Output: yes


Input: [0] Known External Consumers [1] GNOME [2] GNOME [3] GNOME [4] dracut, ?ArchLinux [5] libvirt/LXC [6] gummiboot [7] system-config-services [8] GNOME [9] GNOME, PolicyKit, ... [10] numerous [11] - [12] - [13] glib, GNOME [14] numerous (via sd-daemon.h) [15] a few, including udev [16] mdadm [17] numerous [18] - [19] - [20] libvirt [21] - [22] X11, gdm [23] - [24] numerous [25] numerous [26] D-Bus [27] numerous [28] numerous (it's a Debian thing) [29] - [30] - [31] numerous [32] some [33] some (it's a Debian thing) [34] numerous (it's a Debian thing) [35] - [36] numerous [37] - [38] - [39] - [40]

Output: numerous


Input: [0] Reimplementable Independently [1] yes [2] yes [3] yes [4] yes [5] yes [6] yes [7] no [8] no [9] no [10] yes [11] yes [12] maybe [13] yes [14] yes [15] yes [16] yes [17] no [18] maybe [19] yes [20] yes [21] yes [22] no [23] no [24] no [25] yes [26] yes [27] yes [28] yes [29] yes [30] yes [31] yes [32] yes [33] yes [34] yes [35] yes [36] yes [37] no [38] no [39] no [40]

Output: no


Input: [0] Known Other Implementations [1] Ubuntu, Gentoo, BSD [2] Ubuntu, Gentoo, BSD [3] Gentoo, BSD [4] ?ArchLinux [5] - [6] - [7] - [8] - [9] - [10] - [11] - [12] - [13] - [14] - [15] - [16] - [17] - [18] - [19] - [20] libvirt [21] - [22] - [23] - [24] - [25] ?ArchLinux [26] - [27] - [28] Debian, ?ArchLinux [29] ?ArchLinux [30] - [31] - [32] Fedora, OpenSUSE, ?ArchLinux, Angstrom, Frugalware, others... [33] procps/Debian, ?ArchLinux [34] Debian [35] ?ArchLinux [36] OpenSUSE, Debian, ?ArchLinux [37] - [38] - [39] - [40]

Output: no


Input: [0] **systemd Implementation portable to other OSes or non-systemd distributions [1] partially [2] partially [3] partially [4] no [5] no [6] no [7] no [8] no [9] no [10] yes [11] no [12] no [13] no [14] no [15] no [16] no [17] no [18] no [19] no [20] no [21] no [22] no [23] no [24] no [25] partially [26] no [27] partially [28] no [29] partially [30] partially [31] partially [32] no [33] partially [34] partially [35] partially [36] no [37] no [38] no [39] no [40]

Output: partially


Input: [Topic] Website issues, feedback, or suggestions [Contact]

Output: Website Support

Contact the PDGA | Professional Disc Golf Association


Input: [Topic] Membership questions and information [Contact]

Output: Memberships Manager

Contact the PDGA | Professional Disc Golf Association


Input: [Topic] Event schedule and tournament information [Contact]

Output: Tour Manager

Contact the PDGA | Professional Disc Golf Association


Input: [Topic] Update your contact info [Contact]

Output: Change of Address

Contact the PDGA | Professional Disc Golf Association


Input: [Topic] Rules questions and situations [Contact]

Output: Rules Committee

Contact the PDGA | Professional Disc Golf Association


Input: [Topic] Player ratings: how they work, what they mean [Contact]

Output: Ratings Committee

Contact the PDGA | Professional Disc Golf Association


Input: [Topic] Course Directory: Course information, comments, updates [Contact]

Output: Course Directory

Contact the PDGA | Professional Disc Golf Association


Input: [Topic] Course Evaluation: Questions, comments, update [Contact]

Output: Course Evaluation

Contact the PDGA | Professional Disc Golf Association


Input: [Topic] Mobile Application support: iPhone & Android issues, feedback, suggestions [Contact]

Output: Mobile Applications

Contact the PDGA | Professional Disc Golf Association


Input: Total Loss No total loss reported to CARFAX. [Owner 3] No Issues Reported [Owner 4] No Issues Reported [Owners 1-2]

Output: No Issues Reported

CARFAX Vehicle History Report for this 2009 MERCEDES-BENZ E3504M AWD: WDBUF87XX9B426442


Input: Structural Damage No structural damage reported to CARFAX. [Owner 3] No Issues Reported [Owner 4] No Issues Reported [Owners 1-2]

Output: No Issues Reported

CARFAX Vehicle History Report for this 2009 MERCEDES-BENZ E3504M AWD: WDBUF87XX9B426442


Input: Airbag Deployment No airbag deployment reported to CARFAX. [Owner 3] No Issues Reported [Owner 4] No Issues Reported [Owners 1-2]

Output: No Issues Reported

CARFAX Vehicle History Report for this 2009 MERCEDES-BENZ E3504M AWD: WDBUF87XX9B426442


Input: Odometer Check No indication of an odometer rollback. [Owner 3] No Issues Indicated [Owner 4] No Issues Indicated [Owners 1-2]

Output: No Issues Indicated

CARFAX Vehicle History Report for this 2009 MERCEDES-BENZ E3504M AWD: WDBUF87XX9B426442


Input: Accident / Damage No accidents or damage reported to CARFAX. [Owner 3] No Issues Reported [Owner 4] No Issues Reported [Owners 1-2]

Output: No Issues Reported

CARFAX Vehicle History Report for this 2009 MERCEDES-BENZ E3504M AWD: WDBUF87XX9B426442


Input: Manufacturer Recall Check with an authorized Mercedes-Benz dealer for any open recalls. [Owner 3] No Recalls Reported [Owner 4] No Recalls Reported [Owners 1-2]

Output: No Recalls Reported

CARFAX Vehicle History Report for this 2009 MERCEDES-BENZ E3504M AWD: WDBUF87XX9B426442


Input: Basic Warranty Original warranty estimated to have expired. [Owner 3] Warranty Expired [Owner 4] Warranty Expired [Owners 1-2]

Output: Warranty Expired

CARFAX Vehicle History Report for this 2009 MERCEDES-BENZ E3504M AWD: WDBUF87XX9B426442


Input: [spatial terms in standard] region, area, environment, local, spatial heterogeneity [The student is able to:]

Output: Evaluate the ways in which technology has expanded human capability to modify the physical environment

Spatial concepts in U.S. science teaching standards | TeachSpatial

Theme V-Environment and Society


Input: [spatial terms in standard] area, landscape, environment, global, dispersion [The student is able to:]

Output: Explain the global impacts of human changes in the physical environment

Spatial concepts in U.S. science teaching standards | TeachSpatial

Theme V-Environment and Society


Input: [spatial terms in standard] landscape, environment, global, expand, adjacency [The student is able to:]

Output: Develop possible solutions to scenarios of environmental change induced by human modification of the physical environment

Spatial concepts in U.S. science teaching standards | TeachSpatial

Theme V-Environment and Society


Input: [spatial terms in standard] region, environment [The student is able to:]

Output: Analyze examples of changes in the physical environment that have reduced the capacity of the environment to support human activity

Spatial concepts in U.S. science teaching standards | TeachSpatial

Theme V-Environment and Society


Input: [spatial terms in standard] area, location, environment, grow, expand [The student is able to:]

Output: Apply the concept of "limits to growth" to suggest ways to adapt to or overcome limits imposed on human systems by physical systems

Spatial concepts in U.S. science teaching standards | TeachSpatial

Theme V-Environment and Society


Input: [spatial terms in standard] region, environment, local, pattern [The student is able to:]

Output: Explain the ways in which individuals and societies hold varying perceptions of natural hazards in different environments and have different ways of reacting to them

Spatial concepts in U.S. science teaching standards | TeachSpatial

Theme V-Environment and Society


Input: [spatial terms in standard] region, location, distribution, spatial organization, pattern [The student is able to:]

Output: Analyze the relationships between spatial distribution of settlement and resources

Spatial concepts in U.S. science teaching standards | TeachSpatial

Theme V-Environment and Society


Input: [spatial terms in standard] region, explore, route, access [The student is able to:]

Output: Explain the relationship between resources and exploration, colonization, and settlement of different regions of the world

Spatial concepts in U.S. science teaching standards | TeachSpatial

Theme V-Environment and Society


Input: [The student is able to:]

Output: Evaluate policy decisions regarding the use of resources in different regions of the world

Spatial concepts in U.S. science teaching standards | TeachSpatial

Theme V-Environment and Society


Input: [spatial terms in standard] global, local, access [The student is able to:]

Output: Identify the ways in which resources can be reused and recycled

Spatial concepts in U.S. science teaching standards | TeachSpatial

Theme V-Environment and Society


Input: [Credits Applied] Up to 15 [UMUC Degree] Master of Science in Management with a specialization in Financial Management [iCollege Certificate Program]

Output: Chief Financial Officer

Credit for Military Education and Training | UMUC


Input: [Credits Applied] Up to 15 [UMUC Degree] Master of Science in Information Technology with a specialization in Informatics [iCollege Certificate Program]

Output: Chief Information Officer

Credit for Military Education and Training | UMUC


Input: [Credits Applied] Up to 18 [UMUC Degree] Master of Science in Cybersecurity Policy [iCollege Certificate Program]

Output: Cyber-Leadership

Credit for Military Education and Training | UMUC


Input: [Credits Applied] Up to 9 [UMUC Degree] Master of Science in Information Technology with a specialization in Information Assurance [iCollege Certificate Program]

Output: Cyber-Security

Credit for Military Education and Training | UMUC


Input: [Credits Applied] Up to 15 [UMUC Degree] Master of Science in Management with a specialization in Information Systems and Services [iCollege Certificate Program]

Output: Government Strategic Leader

Credit for Military Education and Training | UMUC


Input: [Credits Applied] Up to 12 [UMUC Degree] Master of Science in Information Technology with a specialization in Project Management [iCollege Certificate Program]

Output: Information Technology Project Management

Credit for Military Education and Training | UMUC


Input: [EWS Setting] Copies [Purpose] The Copies value will be overridden by the value in the application.

Output: Range 1-999


Input: [EWS Setting] Blank Pages [Purpose] Helps control the printing of excess blank pages in application-specific scenarios.

Output: Do Not Print or Print


Input: [EWS Setting] Collation [Purpose] Determines whether multipage jobs exit the printer sequentially when removed from the exit tray, e.g. as numbered pages 123, 123, 123 or as pages 111, 222, 333 etc.

Output: On or Off


Input: [EWS Setting] Separator Sheets [Purpose] As jobs build up on the exit tray, this feature places a blank page between multiple individual job types.

Output: None Between Copies Between Jobs Between Pages


Input: [EWS Setting] Separator Source [Purpose] This setting allows you to specify the source tray of your separator sheets and is dependent on the number of installed and recognized input trays or drawers.

Output: Variable value plus MP Feeder.


Input: [EWS Setting] Multipage Print [Purpose] Also called N-Up under the software driver's Paper tab, this setting will typically be overridden by the driver setting. However, turning this on at the printer may benefit other job types, such as multipage faxes or copy jobs.

Output: Off 2,3,4,6,9,12,16 Up


Input: [EWS Setting] Multipage Order [Purpose] Determines the viewable layout configuration of individual pages of a multipage print job.

Output: Horizontal Vertical Reverse Horizontal Reverse Vertical


Input: [EWS Setting] Multipage View [Purpose] Determines whether a landscape or portrait layout of multipage print jobs is used.

Output: Auto Long Edge Short Edge


Input: [EWS Setting] Multipage Border [Purpose] Emulates the border of a piece of paper by printing a line around the perimeter of individual pages in a multipage print job.

Output: None or Solid


Input: [remedy] This distribution doesn't create a directory and extracts its content into this directory. Instead, it creates more than one directories (some of which are probably system-specific hidden files/directories), or it spews its content into the current directory, making it really hard/annoying to remove the unpacked package. Pack the distribution with a proper command such as "make dist" and "./Build dist", or use a distribution builder such as Dist::Zilla, Dist::Milla, Minilla. [metric]

Output: extracts nicely


Input: [remedy] The distribution hasn't got a Changelog (named something like m/^chang(es?|log)|history$/i. A Changelog helps people decide if they want to upgrade to a new version. Add a Changelog (best named 'Changes') to the distribution. It should list at least major changes implemented in newer versions. [metric]

Output: has changelog


Input: [remedy] The version number isn't a number. It probably contains letter besides a leading 'v', which it shouldn't Remove all letters from the version number. If you want to mark a release as a developer release, use the scheme 'Module-1.00_01' [metric]

Output: has proper version


Input: [remedy] The distribution name (eg. 'Foo-Bar' of Foo-Bar-1.42.tar.gz) does not match the 'name' field in META files. Use a proper tool to make a distribution. You might also need to fix META files if you keep them in the repository. [metric]

Output: distname matches name in meta


Input: [remedy] The documentation for this distribution contains syntactic errors in its POD. Note that this metric tests all .pl, .pm and .pod files, even if they are in t/. See 'pod_message' in the dist error view for more info. Remove the POD errors. You can check for POD errors automatically by including Test::Pod to your test suite. [metric]

Output: no pod errors


Input: [remedy] This distribution uses a module or a dist that's not listed as a prerequisite. List all used modules in META.yml requires [metric]

Output: prereq matches use


Input: [remedy] None of the package versions in this distribution matches the distribution version. Fix the version(s). [metric]

Output: package version matches dist version


Input: [LOCAL TIME] 09:30 [EVENT] 20 Kilometres Race Walk [ROUND] Final [4] Startlist [5] Result [SEX]

9th IAAF World Championships in Athletics IAAF World Championships | iaaf.org


Input: [LOCAL TIME] 09:45 [EVENT] Discus Throw [ROUND] Qualification Group A [4] Startlist [5] Result [6] Summary [SEX]

9th IAAF World Championships in Athletics IAAF World Championships | iaaf.org


Input: [LOCAL TIME] 10:00 [EVENT] 400 Metres Hurdles [ROUND] Heats [4] Startlist [5] Result [6] Summary [SEX]

9th IAAF World Championships in Athletics IAAF World Championships | iaaf.org


Input: [LOCAL TIME] 10:30 [EVENT] Long Jump [ROUND] Heptathlon [4] Startlist [5] Result [6] Summary [7] Points [SEX]

9th IAAF World Championships in Athletics IAAF World Championships | iaaf.org


Input: [LOCAL TIME] 11:20 [EVENT] 400 Metres [ROUND] Heats [4] Startlist [5] Result [6] Summary [SEX]

9th IAAF World Championships in Athletics IAAF World Championships | iaaf.org


Input: [LOCAL TIME] 11:35 [EVENT] Discus Throw [ROUND] Qualification Group B [4] Startlist [5] Result [6] Summary [SEX]

9th IAAF World Championships in Athletics IAAF World Championships | iaaf.org


Input: [How to learn] Deku Link learns the Song of Time on top of the Clock tower on the final day after midnight when he pegs the skull kid with a snot bubble and recalls a memory of Princess Zelda teaching him a song. [Where to play] The only use for this song is to turn back time to the dawn of the first day. Do this when you are finished with your current three day cycle and wish to save and begin on the first day. [How to play]

Output: Song of Time

The Legend of Zelda : Majora's Mask -- Songs


Input: [How to learn] You don't actually have to learn this song like you do most songs. Once you play the Song of Time and use it to return to the dawn of the first day, you can play this song, too. Though, if you want to be formal about it, you can go to one of the two scarecrows in Clock Town (one is in the Items shop in West Clock Town and the other one is in the observatory.) Talk to them and they will ask you if you want to learn the song. [Where to play] You can use this song whenever you wish. It slows down time for you by half so it would be wise to use it everytime you start back on the dawn of the first day. Though, if you are doing a quest and would like time to move at its normal pace, play it again to speed things up. [How to play]

Output: Inverted Song of Time

The Legend of Zelda : Majora's Mask -- Songs


Input: [How to learn] Like the Inverted Song of Time, this song can also be played without formally learning it, but if you want to be old school (for some reason, I've decided to make that old school...probably because I rarely get to say old school anymore...) you can talk to the scarecrows in either West Clock Town's Item shop or the observatory. [Where to play] Again, like its partner in crime, the Inverted Song of Time, you can play this guy anytime of the day. It will make time go ahead to the next interval of time. For example, if you play this song on the night of the first day, it will take you to the dawn of the second day. As you can see, you have one restriction. You can't play this song on the night of the final day. If you could then Link would wake up to a moon-smushed town. o_O;; Some Hero of Time he would be! [How to play]

Output: Song of Double Time

The Legend of Zelda : Majora's Mask -- Songs


Input: [How to learn] Once you have learned the Song of Time and you have returned to the dawn of the first day, go talk to the mask salesman in the clock tower. He'll keep his end of the bargain and teach you the song, though you didn't live up to your end.... [Where to play] There are many things you can do with this song. If you play it for a Gossip Stone, the stone will surrender a fairy you can bottle. Also, by playing it when you first learn it, you will transform back into human Link and create the Deku mask. You can also play it for Darmani the goron, Mikau the zora, Kamaro the dancing ghost and the father in Ikana Canyon to give you the Goron mask, the Zora mask, Kamaro's mask and the Gibdo mask, respectively. Finally, by playing it to the ledgekeeper in Ikana Canyon in his house, he will lower the price of his minigame! ^_^ [How to play]

Output: Song of Healing

The Legend of Zelda : Majora's Mask -- Songs


Input: [How to learn] To learn this song, Link has to finish Romani's archery game in under two minutes before the night of the first day at Romani Ranch. You'd think that Link would remember this song from his days back in Hyrule.... Seems to be a very important tune, if you ask me. [Where to play] Play this song anywhere in Termina Field, Romani Ranch, Milk Road or the entrances to the swamp, bay and canyon. Anywhere else, Epona cannot reach you. Another possibility for a use of this song is to play it for Gossip Stone since it will release a bottle-able fairy upon hearing it. [How to play]

Output: Epona's Song

The Legend of Zelda : Majora's Mask -- Songs


Input: [How to learn] Beside the waterfall entrance to Woodfall temple sits Kaepora Gaebora, the all-knowing, all-annoying owl from Hyrule. He sits on a tablet that has a song inscribed on it. Check it out and you will learn the Song of Soaring. [Where to play] One of the more useful songs in the game, the Song of Soaring will teleport you to any owl statue you have thwarted with your sword. This saves some time by eliminating the journey you'd normally have to take (though Link may need the exercise...) You must have hit an owl statue with your sword or else the statue will remain inactive, leaving you unable to warp. This is very similar to the warping songs from Ocarina of Time. [How to play]

Output: Song of Soaring

The Legend of Zelda : Majora's Mask -- Songs


Input: [How to learn] On the night of the first day, enter the Ikana graveyard, talk to one of the stalchildren circling a grave while wearing the Captain's Hat and tell them to open the grave. Jump on it and walk through the imaginary wall to get to a room with an iron knuckle in it. Defeat it and you will meet Flat and see what is behind the curtain. It's the Song of Storms! [Where to play] As you enter the mysterious cave by the musicbox house in Ikana Canyon, you will have to play the Song of Storms to save Flat's tormented brother, Sharp's soul. This makes the river flow and turns the waterwheel on the musicbox house, letting the good music ring out once more. If you get hit by a blue bubble, playing this song will lift the curse it casts on you after contact. [How to play]

Output: Song of Storms

The Legend of Zelda : Majora's Mask -- Songs


Input: [How to learn] Termina monkeys are much more intelligent than their crap-flinging Earthling counterparts! They can talk and teach you songs. Like what Mr. Monkey is going to do for you. All you have to do is find the jail the monkey is in (Termina even has criminal monkeys) talk to him as human Link, attempt to cut his ropes, transform into deku Link and pull out your ocarina which apparently were really pipes all along. O_o [Where to play] In Woodfall, right outside the temple is a little shrine thing with an owl statue, a pink deku flower and a wooden disk with a deku painted on it. Hop on the disk and play your little heart out as deku Link. As though controlled by magic or possibly vampires, the temple will be lifted from its watery bed, open to the public! Also, in the swamp's Gold Skulltula House, there is a deku in the room to the right of where you come in who is asleep. Play the song to get his lazy butt out of bed... or flower, rather. The Stalchildren's captain in Ikana graveyard also needs to be roused, so wake him up and chase him around! One last thing with this song. There are four holes in the ground in Termina field that have three normal sized Gossip Stones and one mammoth one. By playing this song as deku Link to the giant Gossip stone, it will spin around and turn green. Play it to all four giant stones and you'll receive a piece of heart. [How to play]

Output: Sonata of Awakening

The Legend of Zelda : Majora's Mask -- Songs