Vim documentation: hebrew
main help file*hebrew.txt* For Vim version 7.2. Last change: 2007 Jun 14 VIM REFERENCE MANUAL by Ron Aaron (and Avner Lottem) Hebrew Language support (options & mapping) for Vim *hebrew* The supporting 'rightleft' functionality was originally created by Avner Lottem. <alottem at gmail dot com> Ron Aaron <ron at ronware dot org> is currently helping support these features. {Vi does not have any of these commands} All this is only available when the |+rightleft| feature was enabled at compile time. Introduction Hebrew-specific options are 'hkmap', 'hkmapp' 'keymap'=hebrew and 'aleph'. Hebrew-useful options are 'delcombine', 'allowrevins', 'revins', 'rightleft' and 'rightleftcmd'. The 'rightleft' mode reverses the display order, so characters are displayed from right to left instead of the usual left to right. This is useful primarily when editing Hebrew or other Middle-Eastern languages. See |rileft.txt| for further details. Details + Options: + 'rightleft' ('rl') sets window orientation to right-to-left. This means that the logical text 'ABC' will be displayed as 'CBA', and will start drawing at the right edge of the window, not the left edge. + 'hkmap' ('hk') sets keyboard mapping to Hebrew, in insert/replace modes. + 'aleph' ('al'), numeric, holds the decimal code of Aleph, for keyboard mapping. + 'hkmapp' ('hkp') sets keyboard mapping to 'phonetic hebrew' NOTE: these three ('hkmap', 'hkmapp' and 'aleph') are obsolete. You should use ":set keymap=hebrewp" instead. + 'delcombine' ('deco'), boolean, if editing UTF-8 encoded Hebrew, allows one to remove the niqud or te`amim by pressing 'x' on a character (with associated niqud). + 'rightleftcmd' ('rlc') makes the command-prompt for searches show up on the right side. It only takes effect if the window is 'rightleft'. + Encoding: + Under Unix, ISO 8859-8 encoding (Hebrew letters codes: 224-250). + Under MS DOS, PC encoding (Hebrew letters codes: 128-154). These are defaults, that can be overridden using the 'aleph' option. + You should prefer using UTF8, as it supports the combining-characters ('deco' does nothing if UTF8 encoding is not active). + Vim arguments: + 'vim -H file' starts editing a Hebrew file, i.e. 'rightleft' and 'hkmap' are set. + Keyboard: + The 'allowrevins' option enables the CTRL-_ command in Insert mode and in Command-line mode. + CTRL-_ in insert/replace modes toggles 'revins' and 'hkmap' as follows: When in rightleft window, 'revins' and 'nohkmap' are toggled, since English will likely be inserted in this case. When in norightleft window, 'revins' 'hkmap' are toggled, since Hebrew will likely be inserted in this case. CTRL-_ moves the cursor to the end of the typed text. + CTRL-_ in command mode only toggles keyboard mapping (see Bugs below). This setting is independent of 'hkmap' option, which only applies to insert/replace mode.  / ז ס ב ה נ מ צ ת ץ . This is also the keymap when 'keymap=hebrew' is set. The advantage of 'keymap' is that it works properly when using UTF8, e.g. it inserts the correct characters; 'hkmap' does not. The 'keymap' keyboard can also insert niqud and te`amim. To see what those mappings are,look at the keymap file 'hebrew.vim' etc. Typing backwards If the 'revins' (reverse insert) option is set, inserting happens backwards. This can be used to type Hebrew. When inserting characters the cursor is not moved and the text moves rightwards. A <BS> deletes the character under the cursor. CTRL-W and CTRL-U also work in the opposite direction. <BS>, CTRL-W and CTRL-U do not stop at the start of insert or end of line, no matter how the 'backspace' option is set. There is no reverse replace mode (yet). If the 'showmode' option is set, "-- REVERSE INSERT --" will be shown in the status line when reverse Insert mode is active. When the 'allowrevins' option is set, reverse Insert mode can be also entered via CTRL-_, which has some extra functionality: First, keyboard mapping is changed according to the window orientation -- if in a left-to-right window, 'revins' is used to enter Hebrew text, so the keyboard changes to Hebrew ('hkmap' is set); if in a right-to-left window, 'revins' is used to enter English text, so the keyboard changes to English ('hkmap' is reset). Second, when exiting 'revins' via CTRL-_, the cursor moves to the end of the typed text (if possible). Pasting when in a rightleft window When cutting text with the mouse and pasting it in a rightleft window the text will be reversed, because the characters come from the cut buffer from the left to the right, while inserted in the file from the right to the left. In order to avoid it, toggle 'revins' (by typing CTRL-? or CTRL-_) before pasting. Hebrew characters and the 'isprint' variable Sometimes Hebrew character codes are in the non-printable range defined by the 'isprint' variable. For example in the Linux console, the Hebrew font encoding starts from 128, while the default 'isprint' variable is @,161-255. The result is that all Hebrew characters are displayed as ~x. To solve this problem, set isprint=@,128-255. top - main help file


Yongkil Kwon
CEO
Yongkil is the CEO of NEOPLY, Korea’s leading start-up accelerator, and a board member of NEOWIZ Holdings. He previously worked at Samsung Electronics and GameOn (Japan).
Yongkil is the CEO of NEOPLY, Korea’s leading start-up accelerator, and a board member of NEOWIZ Holdings. He previously worked at Samsung Electronics and GameOn (Japan).
Currently head of technology at NEOWIZ and have experience in web development, DBA and architecture.
CISO/CPO of NEOWIZ. He has worked at Korea Internet and Security Agency(KISA) focusing on network security breach and personal information leaks. He has also worked at NCA in setting up the national super highway information network
Head of NEOWIZ China and NEOPLY China. He has many years of experience working in China. He currently manages EOSeoul’s Chinese communication and his previous workplace include Daum China, KT and LG U+.
Currently Head of technology at NEOWIZ PLAYSTUDIO. He previously worked at Ssangyong Telecommunications, SK communications, NCsoft and NEOWIZ in designing and developing system platform architecture.
Sungmin is the system Engineer at NEOWIZ Games and he has experience of managing over 1,500 servers since 2005.
Engineer at NEOWIZ with focus on game servers and DB middleware.
Leading smart contract development and EOS code analysis at EOSeoul. Previous employers include Samsung electronics, NEOWIZ PLAYSTUDIO and MP Lab.
He has 18 years experience in the IT field and currently leads the LAB, Technology Strategy, and PMO as Neowiz Technical Planning Team Manager. Previously, he was an IT architect and consultant at IBM.
Software engineer at NEOWIZ. He has 18 years of experience in network engineering and developing products such as security appliances and backend systems.
He has more than 9 years of business development experience in the game industry and currently the product manager of EOSeoul.
Product Manager of EOSeoul. He is a member of the business development team at NEOWIZ PLAYSTUDIO and primarily focuses on blockchain research.
Business development mananger at NEOWIZ PLAYSTUDIO and is the main contact for English communication for EOSeoul.
Venture capitalist of NEOPLY’s China branch and in charge of Chinese communication for EOSeoul.
She is in charge of new technology research and planning at NEOWIZ Technology Development Department. She is a communications manager at EOSeoul.
Team Leader of the Investment team at Korea’s start-up accelerator NEOPLY. She searches for blockchain start-ups for investment and is responsible for media communication
He is in charge of technology department in NEOWIZ's Japanese subsidiary, GameOn. He is responsible for EOSeoul's Japanese channel communications.
He is in charge of the infrastructure in NEOWIZ's Japanese subsidiary, GameOn. He is responsible for EOSeoul's Japanese channel communications.


here are your options...
Fields are automatically saved as it is filled.
Configuration
backend api server:
worksheet key:
Column Mappings
Add Column
Save All Changes


Probe ordered into police officer’s death
by Special CorrespondentThe government has ordered a probe into the cause of death of sub-inspector of Nettapakkam Police Station, Vibal Kumar, Chief Minister V. Narayanasamy said here on Saturday.
Shortly after meeting the family members of Kumar at the Legislative Assembly, the Chief Minister told reporters that the death of the sub-inspector was an unfortunate incident.
A team headed by a Senior Superintendent of Police was probing the allegations raised by family members of the deceased officer, he said. The family had held a superior officer in Nettapakkam Police Station responsible for the death of Mr. Kumar, he added.
Mr. Narayanasamy announced a compensation of ₹5 lakh to the family of the deceased police officer.
Earlier in the day, the family members met Director-General of Police Balaji Srivastava. He assured the family members of prompt action.
Following the assurance by the Chief Minister and the DGP, the family accept the body of the sub-inspector.


RAIDERS OF THE LOST ARK (1980)
A film review by Mike Watson Copyright 1997 Mike Watson
Rating: 5 out of 5
You know what most adventure films ultimately lack? A sense of wonder, that's what. But RAIDERS OF THE LOST ARK is an utterly delightful exception. Not to say that this is a deeply philosophical film.  But it does possess something that adventure films often strive for but rarely achieve: a real sense of the mystical.
Archaeologist Indiana Jones' quest to beat the Nazis in the search for the fabled Ark Of The Covenant is certainly a pretty intriguing premise. Still, in less inspired hands such a story could easily have fallen prey to limp writing and empty spectacle. Luckily for us, the team of writer George Lucas and director Steven Speilberg have created such cracking good action sequences and invested the film with such a sense of awe and mystery that RAIDERS is able to stand alongside the most thrilling Hollywood movies ever made.
Of course, the other vital components of a great action film are also in place: solid storytelling, colourful characters, spicy romance, and exotic mid-Eastern locales, topped off with some very convincing - and horrifying - special effects. Oh, and a terrific sense of humour. One short sequence about mid-way through when Jones is confronted by a showy sabre-wielding bad guy is a bonafide all-time classic sight gag. If by chance you haven't yet seen it, you're guaranteed a belly laugh.
Although RAIDERS is based on the old Saturday-afternoon matinees of the 30's & 40's, it doesn't date the film one iota. Indeed, Karen Allen's strong, gutsy female lead is very much an exception in action films.  Nor of sequels to come, I might add: witness Kate Capshaw's unbearable hysterics in the follow-up TEMPLE OF DOOM. As Indiana Jones, Harrison Ford is more the traditional action hero, but what a hero he makes.
A nod must also go to composer John Williamson for his near-perfect score, particularly that haunting minor-chord theme which appears right on cue at the most awe-inspiring moments. And the film is beautifully photographed by Douglas Slocombe, so if you're seeing it on video, the widescreen version is a must.
RAIDERS OF THE LOST ARK is absolutely terrific American filmmaking, worth seeing again and again as an example of Hollywood at its most inspired. A massive box office success, and richly deserved.
The review above was posted to the
rec.arts.movies.reviews newsgroup (de.rec.film.kritiken for German reviews).
The Internet Movie Database accepts no responsibility for the contents of the
review and has no editorial control. Unless stated otherwise, the copyright
belongs to the author.
Please direct comments/criticisms of the review to relevant newsgroups.
Broken URLs inthe reviews are the responsibility of the author.
The formatting of the review is likely to differ from the original due
to ASCII to HTML conversion.
Related links: index of all rec.arts.movies.reviews reviews


Welcome to the Web App
Click here to show all messages from database
Please enter your message to post into database
Please enter your message to search from database
Please enter your message to delete from database


Subscribe to our email newsletter. We will update you on new event updates.
{% import 'macros/subscribe.html' as subscribe with context %}
{{ subscribe.render('USCFPB_93') }}
{% import 'rss.html' as rss %}
{{ rss.render(vars.rss_path) }}
{%- import 'related-links.html' as related_links -%}
{{- related_links.render([
[
'/newsroom/',
'Newsroom'
],
[
'/the-bureau/',
'About us'
],
[
'/blog/',
'The blog'
]
]) -}}


security doesn't have to be complex
A quick start
Easily deploy apps to flexible cloud infrastructure.
Data encryption
Encryption by default so that you can be confident your data isn't open to the world. Everything controlled by you.
Cost effective
You don’t need expensive specialist teams to run your infrastructure. drie meet the needs of developers.
Segregation of your services
Your service is run in its own “cell”, segregated from other customers and attackers on the internet.


Before Change
_current_user = users.first(id=_current_user_id)
// Owner / Admin
if users.can_manage_infrastructure(user_id=_current_user_id):
node.environments.delete_associations(environment_id=_worker_id)
node.environments.delete(id=_worker_id)
else: // Env Owner
envs = [
int(env.id)
for env in node.environments.get_environments(user=_current_user_id)
]
if int(_worker_id) in envs:
node.environments.delete_associations(environment_id=_worker_id)
node.environments.delete(id=_worker_id)
else:
raise AuthorizationError(
"You"re not allowed to delete this environment information!"
)
return DeleteWorkerResponse(
address=msg.reply_to,
status_code=200,
content={"msg": "Worker was deleted succesfully!"},
After Change
created_by_current_user = int(worker_id) in envs
// Owner / Admin
if not is_admin and not created_by_current_user:
raise AuthorizationError("You"re not allowed to delete this worker!")
env = node.environments.first(id=worker_id)
_config = Config(provider=env.provider, app=Config(name="worker", id=worker_id))
success = Provider(_config).destroy()
if success:
node.environments.set(


Schedule a Ride
Upcoming Rides
Ride History
My Profile
Account
Preferences
Payment
Logout
Kelly Patterson
Driver Miles:
3,300
Passenger Miles:
850
Reviews
Update User Information
Phone Number
Home Address
Work Address
Ratings
Star Ratings and Reviews
Close


Blosxom Plug-in: storytitle
Allows you to include the story title in the page header for individually viewed blosxom stories.
Put storytitle in your plug-ins directory.
Alter the formatting if desired, see "OPTIONS".
Finally place $storytitle::page_title in your <title> tag in head.flavour where you want to display the story title, something like this:
<title>$blog_title $storytitle::page_title</title>
If required change the $sep variable. This controls the separator that goes at the start of the story title, and between path entries for categories and archives. E.g. if $sep is ' : ' and the story title is 'A blosxom entry' then $storytitle::page_title will return ' : A blosxom entry'. If the category path is Categories/Blosxom then the plugin will return ' : Categories : Blosxom'.
Now all individually displayed stories can have their title in the pages title tag, or anywhere else in the page header you want. Just place $storytitle::page_title anywhere in the flavours where you want to display the story title.
If you have a need for a left aligned title (e.g. you want to have 'story title : blog title') there are two ways to achieve it:
You can also individually configure the left and right sided separators with the $left_sep and $right_sep configuration options. $storytitle::page_title_left will have $left_sep appended on the right, and $storytitle::page_title_right will have $right_set prepended to the left. If they are not set, they both default to $sep.
0.7
0.7 - Provide title for Category pages as well as Stories and Archive pages. - Also included rus.berrett's patch to remove formatting, from http://rus.berrett.org/blog/contrib/blosxom/storytitle_plugin.html
0.6 - Now uses the users file extension setting rather than always .txt
0.5 - deals with filenames with like foo.bar.txt and foo-bar.txt (thanks to Antti VÃ¤hÃ¤-SipilÃ¤ for pointing this out) catches titles containing only white space.
0.4 - bugfix to stop title values hanging around under static generation
0.3 - fixed left_title to actually be a left title
0.2 - introduced left and right options
Struan Donald<EMAIL_ADDRESS>http://exo.org.uk/code/
Lim Chee Aun http://phoenity.com/ for the left/right sided titles idea.
Anthony DeLorenzo<EMAIL_ADDRESS>for fix to make it use the users file extension setting.
Rus Berrett http://rus.berrett.org/blog/ for patch to remove formatting.
Nick Leverton<EMAIL_ADDRESS>http://www.leverton.org/blosxom for Category page titles.
Blosxom Home/Docs/Licensing: http://blosxom.sourceforge.net/
Blosxom Plugin Docs: http://blosxom.sourceforge.net/documentation/users/plugins.html
Copyright (C) 2003-2005 Struan Donald.
This program is free software; you can redistribute it and/or modify it under the same terms as Perl itself.


Sales Force Form
First Name
Last Name
Email
Garage usage (check all that apply):
Standard - Vehicles regularly parked in garage
Mechanical Workshop (oil changes)
Woodworking Workshop
Other (please explain below)
Check all that describe your garage:
Dry
Humid
Constant Water Flow
Snow
Muddy
Other ( please explain below)
Comments and Questions:
Would you like us to send you a sample?:


Lorem Ipsum is simply dummy text of the printing and typesetting industry. Lorem Ipsum has been the industry's standard dummy text ever since the 1500s Lorem Ipsum is simply dummy text of the printing and typesetting industry. Lorem Ipsum has been the industry's standard dummy text ever since the 1500s
Lorem Ipsum is simply dummy text of the printing and typesetting industry. Lorem Ipsum has been the industry's standard dummy text ever since the 1500s
Lorem Ipsum is simply dummy text of the printing and typesetting industry. Lorem Ipsum has been the industry's standard dummy text ever since the 1500s
WEBSITE DESIGN89%
WEBSITE DEVELOPMENT97%
PLUGINS85%
FRONT END95%


sphinx¶
Library for processing the sphinxQ tags and generating the ReST style documents.
Tags¶
Following are the tags currently supported by this library
tags
--------
table
desc
header
row
function
param
return
package
alias
error
code
see
name
todo
version
tags
schema
desc
toggle
bullet
eval
table
Todo
in case of schema add an extra index of schema
parseFile¶
Steps how a file will be proceesed
- Read the comments containing the tokens
- Extract only the comment part
- Assign desc tag explicitly to the lines which are not multiline comment and does not have any tag
- add an extra space at the end of each comment and then raze the whole list to a simple string.
- Tokenise the string by tags
- Get meta information that will be used in creating the labels and indexing
- Start processing each tag


Preparation time
30 mins to 1 hour
Cooking time
10 to 30 mins
Serves
Serves 4
Embrace the flavours of autumn with game dumplings in a soothing squash broth.
For the dumplings, mix all the ingredients, except the pastry and cornflour, together. Roll the mixture into balls weighing approximately 35g/1¼oz each.
Lay one sheet of wonton pastry on a board and brush with the cornflour mixture. Place a pheasant ball on top and lay another pastry sheet over the top. Press down to seal and stick. Cut around the pheasant mixture using a pastry cutter to neaten the dumpling. Continue this process until you have used all the pheasant balls. Rest the dumplings in the fridge for at least an hour.
For the broth, heat half the butter in a large saucepan. Very gently fry the squash, shallots and garlic until softened, but not coloured (this will take around 20-30 minutes).
Add the cayenne pepper, stock or water, remaining butter and a little salt and cook for around 10 minutes over a medium heat until tender. Add the orange zest and juice. Pour into a blender, blitz and pass through a fine sieve. Season with salt and pepper.
Steam the dumplings in a steamer or in a colander over a pan of boiling water for around 7–8 minutes, or until the filling is cooked through and reads 65C on a cooking thermometer.
Meanwhile, toast the pumpkin seeds in a dry pan until fragrant.
Divide the dumplings between deep, wide bowls and spoon over the squash broth. Garnish with the toasted seeds and pumpkin seed oil. Grate some fresh orange zest over and serve immediately.


{% extends "base.html" %} {% block page_content %}
| Admission Test : |
Will be announced |
| Admission Form Collection & Submission (Up to) : | Will be announced |
| Class Start : | MAY 17, 2020 (SUNDAY) |
1. For EEE/ IPE/ Architecture/ B.Science (CSE):
2. For Bachelor of Business Administration (BBA):
3. For Arts & Social Science (BA in English or MMC/ BSS in Economics/ LLB ):
Required Documents for Form Submission:
***Selected applicants in FF quota are requested to bring all these original papers during their admission.
Written Exam Waiver Conditions (will be called for viva interview):
1. Requirements For Regular MBA /MDS/ MsCS / M.TEL/ MEEE:
4 Years Graduation degrees is required in CS, CSE, CIS,SE, CSSE, EEE, COE, ECE, MIS, Electronics, Mathematics, Physics, or in any other science or Technical disciplines (To be decided by Prog. Director)
4 Years Graduation degrees is required in EEE, COE, ECE, ETE, CS, CSE, CIS, SE, CSSE, App. Physics & Electronics, ICT, ICE, APEE, APECE or in any other science or Technical disciplines (decided by Prog.Director)
2. Requirements For EMBA:
3. Requirements For MDS:
4. Requirements For MPH:
Required Documents for Form Submission:
***Selected applicants in FF quota are requested to bring all these original papers during their admission.
Written Exam Waiver Conditions (will be called for viva interview):
During office hours, Admission Forms are available at the Admission/ Information office, 408/1, Kuratoli, Khilkhet, Dhaka 1229, Bangladesh. +880 18 4411 5000,+88 02 989 4229, +88 02 989 7387, +88 02 588 15387 (Ext. 100,199)
Admission Forms are also available during evening hours (2 PM – 8 PM) at the MBA Program Office, 408/1, Kuratoli, Khilkhet, Dhaka 1229, Bangladesh. +880 18 4411 5010, +88 02 841 4046-9, (Ext. 201)
|
|


Manual¶
This manual explains how astrolyze can be used to ease reduction, analysis and modification of (radio-)astronomical data and images.
astrolyze¶
I started to develop astrolyze to be able to inter-operate the Programs PyFits, MIRIAD and GILDAS. One reason was that the Gildas task are very cumbersome to script and once scripted, the scripts are not very flexible. Also there are some tasks in GILDAS that are (in my opinion) easier to use than in miriad and vice-versa, due to different sets of features.
However, the real power of astrolyze comes from it’s internal tracking of changes to the most important parameters of the maps (or spectral-files), which are stored directly in the file-names. This principle is based on a naming-convention. An additional databases can be setup so that more informations can be loaded depending on the file-name-keywords.
Naming Convention¶
A Name that follows the ‘Naming Convention’ is for example:
M33_30m-HERA_CO21_Ta*_12_cube_regrid.fits
All items MUST be separated by an underscore (_) and HAVE to include at the following properties in this very order:
- source
- telescope
- species (wavelength OR frequency OR line-name)
- flux unit
- resolution
When opening a map with astrolyze these items are transferred to python variables of the Map class (see below). All additional items separated by underscores are treated as comments. Comments are not transferred to individual internal variables of the map objects but are passed on as a list to the single variable comments.
The last item is followed by the files extension:
- .fits -> FITS
- .gdf, .mean, .velo, .width, .lmv -> GILDAS
- nothing -> MIRIAD (Miriads file format uses directories to store the data.)
Maps that are not following this name convention are not supported. This is to assure that all parts of the program work, since they strongly depend on the parameters passed on by the file-name.
Using the example file-name above, opening this file with astrolyze as follows:
from astrolyze import *
map_ = FitsMap('M33_30m_12CO10_Tmb_12_cube_regrid.fits')
would generate the following variables:
map_.source = 'M33'
map_.telescope = '30m'
map_.species = '12CO10'
map_.fluxUnit = 'Tmb'
map_.resolution = '12'
map_.comments = ['cube', 'regrid']
map_.dataFormat = 'fits'
Using the parameter database with line-names, objects and telescope parameters, that can be edited by the user (see Installation of astrolyze), astrolyze pulls more information about the object, telescope and line emission of the map. When the information is present it generates automatically the following variables:
map_.frequency [Hz]
map_.wavelength [m]
map_.calibrationError
map_.type [Hubble Type]
map_.distance [pc]
map_.vlsr [km/s]
map_.centralPosition [RA, DEC] J2000
map_.pa [degrees]
map_.inclination [degrees]
map_.R25 [kpc]
If not present in the database these variables are set to ‘NaN’ (Not a Number).
Although, all of this information is somewhat redundant to the header information in the files, it has been decided to go that way since unfortunately not all headers are kept up to date and manipulating the file name is easier to do.
Nevertheless, the maps module tries to keep track if a variable that should go into the header of a fits file is changed and up-dates the header subsequently (This is however hard to maintain and not true in all cases, though.).
Last but not least using this name convention has another benefit since it makes the life of your fellow astronomers easier when they have to work with your data since they readily know their most important basic properties.
Modules¶
astrolyze is divided in different modules and classes which can inter-operate with each other and which are:
- maps
- spectra
- sed
- functions
- lte
In the following I will introduce the individual modules of astrolyze and their functionality.
Not all functions of the individual astrolyze modules will be covered in this manual-page. All functions are documented and can be found HERE TODO. The next sections attempts to show the basis principles, structure and work-flow of astrolyze.
maps¶
The maps
module is the heart of the astrolyze package. It provides the
framework to work with astronomical images (and spectra). It is able to modify
and to track the most important properties of the maps such that they are always
fast at hand if needed. Further it contains genuine functions written in python
(and pyGildas), alongside wrapper functions to functions and tasks of GILDAS
and MIRIAD.
The maps
module contains the following modules/Classes itself:
- main.Main
- fits.FitsMap
- gildas.GilsdasMap
- miriad.MiriadMap
- stack.Stack
- tools
main¶
This module contains the class: Main
, which
is the parent class for all actions not depending on the actual data-type. In
principle it is the implementation of the Naming Convention and is
not directly used to open a map. All other classes in maps inherit from the
Main
class, such that it is used any time
the other modules of maps are used. Also the Using the sed module uses Main.
Variables created by Main¶
When opening a map with Main
variables are
created that contain information about the maps and can be used to work with
the data. The variables are class attributes. They can be accessed by attaching
them to the object with a dot between object and attribute:
object.attribute
In astrolyze the maps that are opened are objects. The information for the variables come from different places:
From naming convention¶
map_name
prefix
source
telescope
species
fluxUnit
resolution
comments
dataFormat
Calculated Values¶
Assuming a Gaussian beam size the following variables are calculates from the
resolution
keyword.
beamSizeM2 Beam-Size in m^2
beamSizeSterad Beam-Size in sterad
Known Format endings of the different file types¶
These variables contain a list that contain all strings that are recognized by the system as a valid file name ending (TODO: find the correct name for file ending).
fits_formats
miriad_formats
gildas_formats
class_formats
Warning
These are hard-coded, should be initialized via the cfg/ folder of the package when installing.
Variables loaded from Database¶
As explained in TODO. Astrolyze uses a database to store additional informations about maps. The database is set-up during installation as explained in Installation of astrolyze.
From Galaxy Database¶
Using the source
keyword.:
centralPosition : [RA, DEC]
distance : [kpc]
R25 : [kpc TODO]
inclination : [degrees]
vlsr : [km/s]
pa : [degrees]
type : The Hubble type of the galaxy.
fits¶
The fits module contains the class FitsMap
. This class inherits all functions from
Main
but adds functionality and methods
needed to work with fits data. This class makes use of the python-pyfits
package. Please check the pyfits web-page (follow the previous link) for the
pyfits documentation.
To open a fits-map do, e.g.
from astrolyze import *
map = FitsMap('M33_30m_12CO10_Tmb_12.fits')
Variables created by FitsMap¶
Opening a Fits map creates, besides the variables discussed in
Main the following additional variables specific to the
FitsMap
:
Variables loaded with pyfits¶
header : a dictionary with the fits-header cards
data : numpy.ndarray containing the data
hdulist : Some fits-files have more than one plane. HDUlist contains all
planes.
Calculated values¶
Because the fits-header is read via python-pyfits the pixel dimensions are known and thus the pixel-sizes can be caluclated:
pixelSizeM2 : [m^2]
pixelSizeSterad [sterad] .
Known header keywords¶
headerKeywords : A dictionary containing different fits-header keywords that
are used for the same quantity.
Known names of units¶
The FitsMap
class contains the
method change_unit
which is able to
check the conversion that is needed to change to the desired unit. However for
this another Unit Naming Convention
is needed. The following variables
contain lists of valid names for certain variables:
tmb_names
jansky_beam_names
MJy_per_sterad_names
erg_sec_pixel_names
erg_sec_beam_names
jansky_pixel_names
erg_sec_sterad_names
known_units .
Warning
This should also be setup during installation of astrolyze to be able to customize unit-names easily.
Working with Fits Maps¶
Changing Formats¶
Note
Changing formats works the same way in all maps
modules.
The loaded fits map can be transformed to the Gildas and Miriad Formats via the methods:
toGildas()
toMiriad()
and from either of the other two Formats to Fits via:
toFits()
This creates a copy of the image in the Gildas, Miriad (or Fits) Format on the disk in the same folder as the actual map. To keep working with the map in the new format one can use:
map = map.toGildas()
to change the out-put folder there are two ways:
1. Set the ``map.prefix`` variable to the new path prior to
changing the map format as shown above.
2. Give the new path to the function, e.g. map.toGildas(folder='new_path')
Thus e.g.:
map.prefix = 'new_path'
map = map.toGildas()
or:
map = map.toGildas(folder='new_path')
Making use of Pyfits¶
As listed in Variables created by FitsMap a data
and a header
variable is created. These are a numpy.ndarray of the image data and a
dictionary containing the header keywords with their arguments. Thus changing
the properties of the fits map and the header variables is straight-forward.
For example you may want to change the units of a map
M33_30m_12CO10_Tmb_12.fits
that is in main beam temperature to Jansky/beam
by multiplying all pixels with the corresponding conversion factor. This can be
done via:
from astrolyze import *
map = FitsMap('M33_30m_12CO10_Tmb_12.fits')
conversion_factor = map.flux_conversion()
map.data = map.data * conversion_factor
The conversion factor between the two units is calculated here via
flux_conversion
please refer to
the function fro more details.
Having changed the unit it may be a good idea to change the header variables that stores the actual unit as well as the unit-keyword from the naming convention., this can be done as follows:
from astrolyze import *
map = FitsMap('M33_30m_12CO10_Tmb_12.fits')
print map.header['BUNIT']
map.unit = 'JyB'
map.header['BUNIT'] = 'Jy/beam'
Note
The individual functions in of the FitsMap
-class change the header of
the Fits file automatically if map properties are changed. At the same time
they have access to all fits-header variables if needed.
Finally you may want to save the modified image as a new fits file which can be done with:
map.updateFile()
This creates a file called M33_30m_12CO10_JyB_12.fits
Change Map Units¶
Since it is easy to modify all pixel via python-pyfits the function
change_unit
that converts
units into another is implemented in the FitsMap
-class. See the
documentation of change_unit
for the conversions that are implemented.
Using the information from the “Naming Convention” and the additional information from the database, the code has all information to calculate the conversion factors. And also to decide which conversion is to be applied. Changes are possible between any of the units that are implemented.
Warning
This is not thoroughly tested yet!!
For example the same change of units as in the previous section can be done as follows:
from astrolyze import *
map = FitsMap('M33_30m_12CO10_Tmb_12.fits')
map = map.change_unit('JyB')
Using gildas¶
When Opening a Gildas map with:
from astrolyze import *
map = GildasMap('M33_30m_12CO10_Tmb_12.gdf') ,
astrolyze uses pyGildas to read some of the header variables and stores them as python variables. The following values are read.
Variables¶
Gildas Specific¶
dimensions
naxis_1 : number of pixels in x-axis.
naxis_2 : number of pixels in y-axis.
crpix_1 : The reference pixel (x-axis).
crval_1 : The coordinate value at crpix_1 [radians].
cdelt_1 : The pixel increment.
crpix_2 : Same as crpix_1 for y-axis.
crval_2 : Same as crval_1 for y-axis.
cdelt_2 : Same as crdelt_1 for y-axis.
ra_coordinate : RA coordinate.
dec_coordinate : DEC coordinate
ra_coordinate : TODO
dec_coordinate : TODO
central_coordinate_degrees : TODO
central_coordinate_equatorial : TODO
Note
If needed more variables can be loaded when opening a Gildas map without problems , so far only those that were needed are implemented.
How is Gildas used by astrolyze¶
Gildas is used in two different ways in Atrolyze:
1. A Gildas script, with a final exit at the end is created and executed via
the os python package, sending commands to the bash.
2. The pyGildas package is used directly by astrolyze to tun command in SIC.
The first method is mainly used to wrap GREG (and maybe later CLASS) tasks
since these are cumbersome to script so far in Gildas. To do so the GildasMap
method create an init
file and a temporary Greg script that is (normally)
deleted after execution. The standard script looks as follows:
exit
Wrapping Gildas Tasks¶
Direc use of pyGildas¶
Using miriad¶
A miriad map is opened with:
from astrolyze import *
map = GildasMap('M33_30m_12CO10_Tmb_12.gdf') ,
In this mode only the variables created by main
are created.
Only the "smooth"
function from miriad is implemented in astrolyze see
smooth()
. When all header
variables are set correctly this function is aware of the map units and beam
sizes and can calculate the correct scaling that has to be applied after
convolution. The way astrolyze is set up the smooth function expects the map
to be in units of Jy/beam
.
Warning
Miriad could be excluded from astrolyze in the future if the GILDAS smooth wrapper is programmed such that it is aware of different input variables.
Using the stack module¶
The Stack
class builds on top of the
classes:
Main
FitsMap
GildasMap
MiriadMap
It provides the possibility to load a “stack” of maps inside a folder at once and perform changes on all maps. It’s intention is mainly to provide means to unify maps for further processing. Tasks such as for example pixel-to-pixel comparisons or the creation of temperature-maps from SED-fits needs individual maps to be on the same resolution and/or the same pixel grid.
Using the sed module¶
The module SED makes extensive use of the stack functionality of the maps module...
Using Functions¶
The module functions
contains all functions that are not directly related
to manipulation of maps or spectra and counter intuitive also all constants used
in astrolyze as long as they are not available by the standard python
installation (this may not be true however.).
Using LTE¶
References¶
| [GILDAS] | http://www.iram.fr/IRAMFR/GILDAS |
| [MIRIAD] | http://www.atnf.csiro.au/computing/software/miriad/taskindex.html |
| [python-pyfits] | http://www.stsci.edu/institute/software_hardware/pyfits |


JEE-Adv Previous Year Solutions
HOME
VIDEO SOLUTIONS
PDF SOLUTIONS
ABOUT ME
CONTACT
Contact us
Ask me a doubt and I will get back to you within the next 24 hours.
Name
Email
Message
Submit


{include file="public/header" /}
{include file="public/top" /}
文章修改
标题
内容
操作
{include file="public/footer" /}


function Something() { goog.events.EventHandler.call(this); ... set up object ... // Add event listeners this.listen(this.starEl, 'click', this.handleStar); this.listen(this.headerEl, 'click', this.expand); this.listen(this.collapseEl, 'click', this.collapse); this.listen(this.infoEl, 'mouseover', this.showHover); this.listen(this.infoEl, 'mouseout', this.hideHover); } goog.inherits(Something, goog.events.EventHandler); Something.prototype.disposeInternal = function() { Something.superClass_.disposeInternal.call(this); goog.dom.removeNode(this.container); }; // Then elsewhere: var activeSomething = null; function openSomething() { activeSomething = new Something(); } function closeSomething() { if (activeSomething) { activeSomething.dispose(); // Remove event listeners activeSomething = null; } }
|
Initial count for the keyPool_
|
Code » | |
|
Max count for the keyPool_
|
Code » | |
|
SimplePool to cache the key object. This was implemented to make IE6
performance better and removed an object allocation in the listen method
when in steady state.
|
Code » | |
|
Keys for event that is being listened to if only one event is being listened
to. This is a performance optimization to avoid creating an extra object
if not necessary.
|
Code » | |
|
Keys for events that are being listened to. This is used once there are more
than one event to listen to. If there is only one event to listen to, key_
is used.
|
Code » |


Billing Address
Name:
Address:
City:
State:
CA
MA
NY
MD
OR
OH
IL
DC
Zip:
Country:
Email:
Test Button


| Package | Description |
|---|---|
| org.smooks |
Smooks Content Transformation/Analysis - *** STARTING POINT ***.
|
| org.smooks.api | |
| org.smooks.api.bean.repository | |
| org.smooks.api.delivery |
Content Delivery.
|
| org.smooks.api.delivery.event | |
| org.smooks.api.resource.config | |
| org.smooks.engine | |
| org.smooks.engine.bean.repository | |
| org.smooks.engine.converter | |
| org.smooks.engine.delivery | |
| org.smooks.engine.delivery.dom |
DOM based Content Delivery.
|
| org.smooks.engine.delivery.event | |
| org.smooks.engine.delivery.sax.ng | |
| org.smooks.engine.injector | |
| org.smooks.engine.lookup | |
| org.smooks.engine.resource.config | |
| org.smooks.engine.resource.extension |
Smooks Configuration Extension Classes.
|
| org.smooks.engine.resource.visitor.smooks |
| Class and Description |
|---|
| ReaderConfigurator
Reader configurator.
|
| ResourceConfig
A configuration for a Smooks resource.
|
| Class and Description |
|---|
| ResourceConfig
A configuration for a Smooks resource.
|
| ResourceConfigSeq
An ordered list of
ResourceConfig . |
| Class and Description |
|---|
| ResourceConfig
A configuration for a Smooks resource.
|
| Class and Description |
|---|
| ResourceConfig
A configuration for a Smooks resource.
|
| Class and Description |
|---|
| ResourceConfig
A configuration for a Smooks resource.
|
| Class and Description |
|---|
| ConfigSearch
Configuration lookup metadata.
|
| Parameter
ResourceConfig Parameter.
|
| ParameterDecodeException
Unable to decode smooks-resource parameter value.
|
| ProfileTargetingExpression
Represents a single parsed profile targeting expression.
|
| ResourceConfig
A configuration for a Smooks resource.
|
ResourceConfigChangeListener
ResourceConfig change listener. |
| ResourceConfigSeq
An ordered list of
ResourceConfig . |
| Class and Description |
|---|
| ResourceConfig
A configuration for a Smooks resource.
|
| ResourceConfigSeq
An ordered list of
ResourceConfig . |
| Class and Description |
|---|
| ResourceConfig
A configuration for a Smooks resource.
|
| Class and Description |
|---|
| Configurable
Configurable component.
|
| Class and Description |
|---|
| ResourceConfig
A configuration for a Smooks resource.
|
| Class and Description |
|---|
| ResourceConfig
A configuration for a Smooks resource.
|
| Class and Description |
|---|
| ResourceConfig
A configuration for a Smooks resource.
|
| Class and Description |
|---|
| ResourceConfig
A configuration for a Smooks resource.
|
| Class and Description |
|---|
| ResourceConfig
A configuration for a Smooks resource.
|
| Class and Description |
|---|
| ConfigSearch
Configuration lookup metadata.
|
| ResourceConfig
A configuration for a Smooks resource.
|
| ResourceConfigSeq
An ordered list of
ResourceConfig . |
| Class and Description |
|---|
| ConfigSearch
Configuration lookup metadata.
|
| Parameter
ResourceConfig Parameter.
|
| ParameterDecodeException
Unable to decode smooks-resource parameter value.
|
| ProfileTargetingExpression
Represents a single parsed profile targeting expression.
|
| ReaderConfigurator
Reader configurator.
|
| ResourceConfig
A configuration for a Smooks resource.
|
ResourceConfigChangeListener
ResourceConfig change listener. |
| ResourceConfigFactory
Constructs a
ResourceConfig from its corresponding Element . |
| ResourceConfigListFactory
ResourceConfig Factory.
|
| ResourceConfigSeq
An ordered list of
ResourceConfig . |
| ResourceConfigSortComparator
Sort Comparator for
ResourceConfig Objects based on their "specificity". |
| Class and Description |
|---|
| ConfigSearch
Configuration lookup metadata.
|
| ResourceConfig
A configuration for a Smooks resource.
|
| ResourceConfigSeq
An ordered list of
ResourceConfig . |
| Class and Description |
|---|
| ResourceConfig
A configuration for a Smooks resource.
|
| ResourceConfigSeq
An ordered list of
ResourceConfig . |
Copyright © 2023. All rights reserved.


PyMultiNest tutorial
Casual parameter estimation and model selection
Johannes Buchner
Max Planck Institute for Extraterrestrial Physics
November 2013
About me
- implemented MCMC sampler for Bachelor thesis
- since then, 5 years of experience with Monte Carlo methods for Bayesian inference
- Numerical Likelihood functions (0.1-5s), low-dimensional (<20)
- Research on accreting supermassive black hole in X-ray (Poisson spectra)
- Recent interest: smooth field reconstruction with numerical likelihoods (20-500 dimensions)
https://www.mpe.mpg.de/~jbuchner/ -- Johannes Buchner
Go-to Methods
(for numerical likelihoods)
Parameter estimation
- Optimize to maximum (ML/MAP)
- explore around it with MCMC
- High-dimensional, misbehaved: MCMC (?), HMC (?)
-
Model selection
- High-dimensional:
- Low-dimensional:
- Nested models:
Tools so far
(for numerical likelihoods)
Parameter estimation
- Optimize to maximum (ML/MAP)
- explore around it with MCMC
- High-dimensional, misbehaved: MCMC (?), HMC (?)
- Low-dimensional, multi-modal: MultiNest
Model selection
- High-dimensional: give up
- Low-dimensional (<20), multi-modal: MultiNest
- Nested models: AIC + DE
also for Low-dimensional, multi-modal: MultiNest
What will we do today?
Goal: solving integrals
- Write likelihood functions
- Write prior functions
- run nested sampling code
- look at marginal plots and compare evidence
Software: PyMultiNest
- based on MultiNest: written by Farhan Feroz and Mike Hobson (2007)
- Finds clusters -> sampling from ellipses
- Python instead of writing Fortran or C functions
- parses output, and does a bit of plotting
- Also produces "Markov Chain" for uncertainty propagation
Prior functions: A math trick
Based on transforming unit cube:
where is the cumulative distribution of :
- transformation through inverse of CDF
- compresses unimportant regions
- "native units":
- can also do this in MCMC!
Prior functions: A math trick
- Transform from unit cube to parameter space
- Using inverse CDF of prior
def prior(cube, ndim, nparams):
cube[0] = cube[0] * (3 - 1) + 1
cube[1] = 10**(cube[1] * (1 + 0.5) - 1)
Shortest Code Example
import pymultinest
def prior(cube, ndim, nparams):
cube[0] = cube[0] * 2
def loglikelihood(cube, ndim, nparams):
return -0.5 * ((cube[0] - 0.2) / 0.1)**2
pymultinest.run(loglikelihood, prior, n_params=1)
Tutorial
http://johannesbuchner.github.io/pymultinest-tutorial/
$ ssh -Y<EMAIL_ADDRESS>$ bash
$ source /afs/desy.de/group/school/mc-school/setup_pymultinest.sh
$ git clone https://github.com/JohannesBuchner/pymultinest-tutorial
- Example 1: 1d multi-modal problem
- Example 2: Spectral line analysis -- 1 line or 2 lines?
- Example 3: Hierarchical Bayes, Your own, Lighthouse problem, further reading
Final points
- Correlation of parameters from posterior samples SysCorr
- Throw multiple algorithms against problem (jbopt)
- Fully automated model selection, but is model a good one? Systematic errors? Confidence on model choice?
- PyMultiNest reference: Buchner et al (in prep), MultiNest: arXiv:0704.3704, arXiv:0809.3437 & arXiv:1306.2144


A SIMPLE WISH (Universal) Starring: Martin Short, Kathleen Turner, Mara Wilson, Robert Pastorelli. Screenplay: Jeff Rothberg. Producers: Sid, Bill and Jon Sheinberg. Director: Michael Ritchie. MPAA Rating: PG (mild profanity) Running Time: 90 minutes. Reviewed by Scott Renshaw.
I have a theory that, in an earlier stage of development, the premise for A SIMPLE WISH went something like this: Murray (Martin Short), who aspires to being the first male fairy godmother, turns out to be completely inept at the job, but an affirmative action mandate forces the godmothers to admit him. This would be before the real-world affirmative action debate heated up, forcing controversy-shy Universal executives to drop that angle entirely.
The theory, I'll admit, is based on no evidence in the version of A SIMPLE WISH which actually made it to the screen. The alternative, unfortunately, is that the story never made a shred of sense at _any_ point in its development. It's the kind of exasperating kiddie fantasy where stuff just happens, without any character, story or internal logic to guide it.
Of course, the stuff which does happen may be plenty to satisfy young viewers. In the course of his repeatedly bungled attempts to help young Anabel Greening (Mara Wilson) turn her father (Robert Pastorelli) into a Broadway star, Murray gets caught in an iron gate, causes a wind storm to sweep a teacher down a school hallway, turns a redneck into a 50 foot tall rabbi, turns a horse into a mouse and has the father's chief rival begin vomiting up frogs at an inopportune moment during his audition. Meanwhile, evil excommunicated godmother Claudia (Kathleen Turner), who has an axe to grind and magic wands to steal, has fun with computer graphics, rendering folks either two-dimensional or extremely pliable depending on the whim which seizes her.
The special effects are, admittedly, temporarily distracting. When they stop, however, A SIMPLE WISH borders on the unbearable. Martin Short, who should be taken only in small doses even on his best days, turns Murray into a flinching, snorting and generally annoying creation without a glimmer of charm. Mara Wilson, who was so appealing in last year's delightful MATILDA, barely registers here at all, while Francis Capra registers far too often as Wilson's big brother. There is not a single likeable character in the film, turning every scene into a long wait for some kind of goofy visual effect to snap you out of your stupor.
All of these problems make the gaping hole at the center of the film all the more evident. A SIMPLE WISH is based around a high-concept premise -- a male fairy godmother, and an incompetent one at that -- yet not once is there any attempt to explain why he wanted to be a fairy godmother, how he managed to become one, or why no one is keeping an eye on him. In fact, A SIMPLE WISH is comprised of nothing but missed opportunities and half-developed ideas. What goes on at the fairy godmothers' convention which takes place during the film? Does it matter that Murray is using a broken wand for much of the film? Why not make more use of the complicated rules of fairy godmother-hood, which apparently are so abstruse that Murray has to carry around a cheat sheet? And why does Claudia's assistant Boots (Amanda Plummer), who is supposed to be a dog turned into a human, look instead like a refugee from "Cats"?
Time and again, A SIMPLE WISH wanders from scene to scene as though blissfully unconcerned about arriving at anything resembling a point. Then again, maybe someone got cold feet and stripped it of its point. It's more charitable, I think, to imagine the darkly satirical film A SIMPLE WISH might have been than to dwell on the muddled mess it turned out to be.
On the Renshaw scale of 0 to 10 wanded men: 2.
Visit Scott Renshaw's MoviePage http://www-leland.stanford.edu/~srenshaw Subscribe to receive reviews directly via email
"'Elitist' [is] a word _meaningless_ in a profession that tries to seek out and spotlight the best. 'Elite' is from the Old French root eslire, to choose, and choosing is what a critic does for a living. Calling a critic 'elitist' is like calling an accountant 'mathist.'" --Richard Von Busack
The review above was posted to the
rec.arts.movies.reviews newsgroup (de.rec.film.kritiken for German reviews).
The Internet Movie Database accepts no responsibility for the contents of the
review and has no editorial control. Unless stated otherwise, the copyright
belongs to the author.
Please direct comments/criticisms of the review to relevant newsgroups.
Broken URLs inthe reviews are the responsibility of the author.
The formatting of the review is likely to differ from the original due
to ASCII to HTML conversion.
Related links: index of all rec.arts.movies.reviews reviews


dsp56k - DSP56001 interface device
#include <asm/dsp56k.h>
ssize_t read(int fd, void *data, size_t length);
ssize_t write(int fd, void *data, size_t length);
int ioctl(int fd, DSP56K_UPLOAD, struct dsp56k_upload *program);
int ioctl(int fd, DSP56K_SET_TX_WSIZE, int wsize);
int ioctl(int fd, DSP56K_SET_RX_WSIZE, int wsize);
int ioctl(int fd, DSP56K_HOST_FLAGS, struct dsp56k_host_flags *flags);
int ioctl(int fd, DSP56K_HOST_CMD, int cmd);
The dsp56k device is a character device with major number 55 and minor number 0.
The Motorola DSP56001 is a fully programmable 24-bit digital signal processor
found in Atari Falcon030-compatible computers. The dsp56k special file
is used to control the DSP56001, and to send and receive data using the
bidirectional handshaked host port.
To send a data stream to the signal processor, use write(2)
to the device, and read(2) to receive processed data. The data can be
sent or received in 8, 16, 24, or 32-bit quantities on the host side, but
will always be seen as 24-bit quantities in the DSP56001.
The following ioctl(2) calls are used to control the
dsp56k device:
- DSP56K_UPLOAD
- resets the DSP56001 and uploads a program. The third ioctl(2)
argument must be a pointer to a struct dsp56k_binary with members
bin pointing to a DSP56001 binary program, and len set to
the length of the program, counted in 24-bit words.
- DSP56K_SET_TX_WSIZE
- sets the transmit word size. Allowed values are in the range 1 to 4, and
is the number of bytes that will be sent at a time to the DSP56001. These
data quantities will either be padded with zero bytes, or truncated to fit
the native 24-bit data format of the DSP56001.
- DSP56K_SET_RX_WSIZE
- sets the receive word size. Allowed values are in the range 1 to 4, and is
the number of bytes that will be received at a time from the DSP56001.
These data quantities will either truncated, or padded with a null byte
('\0') to fit the native 24-bit data format of the DSP56001.
- DSP56K_HOST_FLAGS
- read and write the host flags. The host flags are four general-purpose
bits that can be read by both the hosting computer and the DSP56001. Bits
0 and 1 can be written by the host, and bits 2 and 3 can be written by the
DSP56001.
- To access the host flags, the third ioctl(2) argument must be a
pointer to a struct dsp56k_host_flags. If bit 0 or 1 is set in the
dir member, the corresponding bit in out will be written to
the host flags. The state of all host flags will be returned in the lower
four bits of the status member.
- DSP56K_HOST_CMD
- sends a host command. Allowed values are in the range 0 to 31, and is a
user-defined command handled by the program running in the DSP56001.
linux/include/asm-m68k/dsp56k.h, linux/drivers/char/dsp56k.c,
http://dsp56k.nocrew.org/,
DSP56000/DSP56001 Digital Signal Processor User's Manual
This page is part of release 5.05 of the Linux man-pages project. A
description of the project, information about reporting bugs, and the latest
version of this page, can be found at https://www.kernel.org/doc/man-pages/.


Enter movie name to get recommendations!
Recommend
Top Rated Movies
Search for Top Rated Movies!
All
Action
Animation
Fantasy
Science Fiction
Crime
Drama
Thriller
Animation
Family
Western
Comedy
Romance
Horror
Mystery
History
War
Music
Documentary
Foreign
TV Movie
Recommend
Homepage


Analyzing works gives you points. More popular works awards more points.
| 90-100% | 5.00 points |
| 80-89% | 2.00 points |
| 70-79% | 1.00 point |
| 50-69% | 0.5 points |
| 25-49% | 0.1 points |
| < 25% | nothing |
So, for instance, {{#with work}}{{title}} {{/with}} has a score of {{score}}% for {{#with ideology}}{{name}}{{/with}}. Analyzing it will give you {{points}} points.
And, by gathering enough points you get badges.
5 points
15 points
50 points


Your gold:
{{ your_gold }}
Farm
(earns 10-20 golds)
Cave
(earns 5-10 golds)
House
(earns 2-5 golds)
Casino
(earns 0-50 golds)
Activities
{{ val['activity'] }}


Select sentences from a Wikipedia page that act as evidence to SUPPORT or REFUTE a claim (a simple factoid sentence). Each selected piece of evidence should be sufficient by itself: if a single sentence does not suffice, it can be joined with other sentences selected from the right hand column.


Appointment Picker
A lightweight, accessible and customizable javascript timepicker.
Appointment-Picker source on Github
Default (no options, jQuery)
$.fn.appointmentPicker = function(options) { this.appointmentPicker = new AppointmentPicker(this[0], options); return this; }; var $picker = $('#time-1').appointmentPicker();
Leading zero (large, jQuery)
var $picker2 = $('#time-2').appointmentPicker({ title: 'Select an appointment', interval: 15, startTime: 8, endTime: 14, leadingZero: true, large: true });
Disabled array and min/maxTime (am/pm, vanillajs)
var picker = new AppointmentPicker(document.getElementById('time-3'), { interval: 30, mode: '12h', minTime: 10, maxTime: 21, startTime: 09, endTime: 23, disabled: ['1:30 pm', '2:00 pm', '7:30 pm'] });
Custom time format (large, am/pm, vanillajs)
new AppointmentPicker(document.getElementById('time-4'), { interval: 15, mode: '12h', startTime: 11, endTime: 16, minTime: 11, maxTime: 16, disabled: ['3:00 pm', '3:30 pm'], allowReset: false, large: true, timeFormat12: 'H.M AP.M.' });
More Examples
- React Integration Example
- Calling exposed functions
- Form embed Example
- Rendering custom (markup) template
Tests
Report bugs or feature requests on Github Issues
Copyright Jan Suwart, MIT license