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{{ result.added ? "check" : "" }}
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This order is pending and hasn't completed
This order was a success
This order was refunded
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{{ ::result.username | truncate:30 }}
Stop: {{ ::result.acctstoptime | humanTime }}
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Filter by client
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{{ ::(result.client_mac | uppercase)}}View client
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{{ result.username | truncate:30 }}
{{ ::result.username }}
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{{ ::(result.ap_mac | uppercase )}}
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{{::((result.download + result.upload)| humanData)}}
Inbound: {{ ::result.download | humanData }}. Outbound: {{ ::result.upload | humanData }}
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{{ result.first_name }} {{ result.last_name }}
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{{ result.updated_at | humanTimeShort }}
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{{ result.gender == 'male' ? 'M' : 'F' }}
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by Curtis Edmonds --<EMAIL_ADDRESS>An early Wednesday evening at home. Walk in the door, open a bag of chips, check e-mail. Nothing interesting, much. Change clothes, put on running shoes. Walk outside. Raining too hard. Walk back inside. Decide to wait and see if rain stops. Turn computer monitor back on, pull up game for a few minutes. Rain gets heavier, thunder gets louder. ZOT!!! Power goes off. Power stays off.
Hunger builds, dinnertime approaches. No microwave, no oven, no refrigerator, even. Dry cleaners close at seven. Walk to car in driving rain, start engine, get to dry cleaners five minutes before close. Still hungry. Stop by Chuy's, get chicken enchiladas in green chile sauce. Have to stop eating like this. Diet starts soon.
Rain stops on drive home. Check mailbox on way in. Get electric bill. Chuckle at irony. Get dry cleaning out of car. Rain stops. Walk in door, power still not on. Open window, read paper until too dark to read anymore. Power still not on.
True Crime starts in twenty minutes at dollar theater. Clint Eastwood stars and directs. Better than sitting around in dark room.
Drive to movie theater, arrive as previews start. Trailer for The Mummy looks cooler than expected.  Wonder who would ever want to go back to high school.
Movie starts. San Quentin Prison, exterior scene. Didn't know San Quentin was on the Pacific. Scene where warden talks to condemned criminal. Blah sort of scene.
Here is Clint, at a bar, with a young girl. Clint drinks a tall drink with a stalk of celery in it. Wonder how much celery a bar goes through in a week.  Girl feels uncomfortable, leaves bar, drives away.
Girl is driving drunk in the rain. Worse yet, girl decides to change radio stations. Girl comes up on Deadman's Curve, spins out, dies in horrible preventable car crash. Yet another innocent life sacrificed to make a corny plot point. Wonder when we will ever learn from these tragedies?
Clint is needed to replace girl on story about imminent execution of condemned criminal from first scene. James Woods and Denis Leary talk bad about Clint behind his back. Woods actually looks like he's doing a Denis Leary impression. Denis Leary glowers a lot, not wanting to upstage Woods while he's doing his Denis Leary impression.
Clint comes into newsroom and is shocked and horrified over girl's death for about two minutes. Clint starts to investigate story, asking questions about murder that the condemned man allegedly committed.  Wonder if anybody ever told Dirty Harry Callahan to stop smoking.
Clint also calls his wife, who is Diane Venora, who was pretty good in The Jackal, which was otherwise pretty bad. Clint's wife reminds him to take his daughter to the zoo. Clint intersperses investigation into innocence of condemned man with family life, doing neither well. Dirty Harry Callahan never would have stopped to take anyone to the zoo that he wasn't feeding to the tigers.
Scenes go in in prison in the meantime. Michael McKean plays a smarmy-looking prison chaplain who gives a bad name to chaplains everywhere. The warden and the prison guards are nice enough people, doing their jobs. The condemned man shares some awkward moments with his family. He decides to have steak for his last meal. Would choose some more of those chicken enchiladas myself.
Clint drives around Bay Area, confronting people. Eventually, he confronts the condemned man (Isaiah Washington), who explains why he is not guilty. Clint believes him, so he must not be guilty. Can Clint save him before time runs out? Remind self that Clint is the director and the producer and Clint can pretty much do what he wants.
Finish watching movie. Marvel at silliness of ending. Wonder if this is just a potboiler for Clint to make other, better movies. Hope that this is indeed the case. Respect the quality of Clint's acting, and the good work of the supporting cast, but wonder what the screenwriter was thinking. Ask self if this was really better than sitting alone in a dark room waiting for the power to come back on.
Leave theater disappointed. Drive home. The power is back on! Write review, reset clocks, go to sleep.
-- Curtis D. Edmonds<EMAIL_ADDRESS>"First, you show up. Then you see what happens." -- Napoleon Bonaparte
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


This is to see if the sources can be built. It is not an attempt to make them run on Mac.
See this about Jam on Mac.
“unzip main.zip” produces directories “__MACOSX” and “main”. I don’t know what that’s all about. There is little of interest in __MACOSX. The content of main is plausible.
I “cd main” and “jam”. The first problem is that this version of gcc does not know the “-mv8” option which directs the compiler to produce SPARC code for model v8 SPARCs. This is no surprise. I delete line “CCFLAGS = -mv8 ;” and subsequent text “-mv8” from Jamrules.
Source file src/kernel/sun4m/genassym.c wants header keyh.h . src/include/sparc/keyh.h is the right file, I think. I don't see the command line for gcc. I guess I must learn some Jam.
I remember thinking that the tree of .c files was poorly organized. This was a result of shifting concepts of modularity over several years. I might try a flat directory for each of


Estimates the longitudinal concordance correlation to access the longitudinal agreement profile. The estimation approach implemented is variance components approach based on polynomial mixed effects regression model, as proposed by Oliveira, Hinde and Zocchi (2018) <doi:10.1007/s13253-018-0321-1>. In addition, non-parametric confidence intervals were implemented using percentile method or normal-approximation based on Fisher Z-transformation.
| Version: | 1.0 |
| Depends: | R (≥ 3.2.3), nlme (≥ 3.1-124), ggplot2 (≥ 2.2.1), grid (≥ 3.2.3), gdata (≥ 2.18.0) |
| Suggests: | roxygen2 (≥ 3.0.0) |
| Published: | 2018-11-16 |
| Author: | Thiago de Paula Oliveira [aut, cre], Rafael de Andrade Moral [aut], John Hinde [aut], Silvio Sandoval Zocchi [aut, ctb], Clarice Garcia Borges Demetrio [aut, ctb] |
| Maintainer: | Thiago de Paula Oliveira <thiago.paula.oliveira at usp.br> |
| License: | GPL-2 | GPL-3 [expanded from: GPL (≥ 2)] |
| NeedsCompilation: | yes |
| CRAN checks: | lcc results |
| Reference manual: | lcc.pdf |
| Package source: | lcc_1.0.tar.gz |
| Windows binaries: | r-devel: lcc_1.0.zip, r-release: lcc_1.0.zip, r-oldrel: lcc_1.0.zip |
| OS X binaries: | r-release: lcc_1.0.tgz, r-oldrel: lcc_1.0.tgz |
Please use the canonical form https://CRAN.R-project.org/package=lcc to link to this page.


Livestock: Relocation planning should be considered to help ensure producers are as prepared as possible for a range of emergencies that may require the relocation of their livestock. Further information and support may be available through the Ministry of Agriculture.
 Further information and support may be available from your Local Authority or First Nation and through the Canadian Disaster Animal Response Team (CDART).


DA demands Mbalula apologises to Judge John Hlophe over 'Mickey Mouse' remark | IOL News
Cape Town - The Democratic Alliance has called on Transport Minister Fikile Mbalula to apologise to Western Cape Judge President John Hlophe for criticism of the court ruling against the Passenger Rail Agency of South Africa.
DA member of Parliament (MP) Chris Hunsinger called Mbalula's remarks, made on Thursday as he inspected the damage wreaked by an arson attack at Cape Town Central station, childish and vile.
Mbalula seemingly took issue with the high court ruling that Prasa must reinstate contracts with security companies it had terminated until it had finalised a new tender or put in place alternative security measures.
The minister, when asked about the matter, reportedly replied: “Does he [Judge Hlophe] know how to run trains? He must ask himself that particular question before he makes himself a Mickey Mouse and turns our courts into something that must not be respected”.
He went on to add: “I will never look away from a decision of the court - if the courts say we must implement the decision to bring the security companies back, the board must take that decision … we either implement or challenge those decisions”.


Description
Cross Tap is an interesting and challenging puzzle game. Puzzles can be solved simply by tapping on square grids. Each tap changes the color of the row and column, and your task is to make them all light blue.
Core Features:
• Time limited challenge mode
• Over 50 different regular levels
• Collect stars to unlock backgrounds
• Well-balanced difficulty


Contrary to popular belief, Lorem Ipsum is not simply random text. It has roots in a piece of classical Latin literature from 45 BC.
Popular belief Contrary to , Lorem Ipsum is not simply random text. It has roots in a piece of classical Latin literature from 45 BC.
Lorem Ipsum is not simply random text. Contrary to popular belief, It has roots in a piece of classical Latin literature from 45 BC.
TRIBECA LIVING
$500.00
ESSENTIAL
CLARISSA
LITTLE HOME


High value of Point in the given position.
Low value of Point in the given position.
Position of Point.
Datapoint with X and Y values.
Ordered tuple that contains values for:
Calculate standard deviation for a set of values.
Array of values.
Standard deviation value.
Datapoint with one X value and two Y values.


12 days to go!
Well...we kind of fail at updating this. Oops.
Time has just flown by these last couple months. We've been super busy planning our trip, packing up our apartment, and getting all of the last-minute things sorted out. Of course, it is us, so we had to throw a couple more small trips in there too - to the Shuswap and the Rockies for a week, to Rossland and Kamloops to visit our families, and to Whistler with some friends for Alan to compete in the Canadian Orienteering Championships.
We have two days of work left, and then we're moving everything from our apartment into a storage unit. After that, we're planning on camping for a couple of days on the way up to Kamloops. We'll spend a few days there, and then it's off to Summerland for my cousin's wedding. The next day we will be driving back to Vancouver and leaving on a plane that evening!
In two weeks we will be in Bangkok! Our plan as of now is to spend around 4 weeks in Thailand, 2 weeks in Cambodia, 4 weeks in Vietnam, a few days in Malaysia, 7 weeks in Australia, and 6 weeks in New Zealand. We fly back February 9th, so Alan will spend his birthday in New Zealand.


--- layout: post title: Manage your life tagline: " by means of Emacs' toolbox" permalink: /emacs/time-management.html categories: [Learning Technology, Emacs] tags: [agenda, time-management] ---


--- layout: article published: true title: Testimonials ---
I like the way you proofread because you not only correct my mistakes but also give me your comments and feedback on my writing. It is very helpful and useful to me.
I want to thank you for being willing to help my friends proofread their work and the clear explanation of how you work.
Thank you for the article, the suggestions and everything. I am interested in what you have to say regarding any aspect of my dissertation. Your opinion is welcomed and respected.
Thank you very much for your swift response and comments. They are all excellent.


--- title: "Main Content Figures" type: media scss: _assets/stylesheets/_base.scss usage: "Default figure display for images or videos." ---


public class RecoveriesCollection
extends java.lang.Object
RecoveriesCollection.RecoveryRef
inner class verifies that recovery temporary files
and store will only be cleared once on going usage is finished.| 限定符和类型 | 类和说明 |
|---|---|
static class |
RecoveriesCollection.RecoveryRef
a reference to
RecoveryTarget , which implements AutoCloseable . closing the reference
causes AbstractRefCounted.decRef() to be called. |
| 构造器和说明 |
|---|
RecoveriesCollection(org.apache.logging.log4j.Logger logger,
ThreadPool threadPool,
java.util.function.LongConsumer ensureClusterStateVersionCallback) |
| 限定符和类型 | 方法和说明 |
|---|---|
boolean |
cancelRecoveriesForShard(ShardId shardId,
java.lang.String reason)
cancel all ongoing recoveries for the given shard
|
boolean |
cancelRecovery(long id,
java.lang.String reason)
cancel the recovery with the given id (if found) and remove it from the recovery collection
|
void |
failRecovery(long id,
RecoveryFailedException e,
boolean sendShardFailure)
fail the recovery with the given id (if found) and remove it from the recovery collection
|
RecoveriesCollection.RecoveryRef |
getRecovery(long id)
gets the
RecoveryTarget for a given id. |
RecoveriesCollection.RecoveryRef |
getRecoverySafe(long id,
ShardId shardId)
Similar to
getRecovery(long) but throws an exception if no recovery is found |
RecoveryTarget |
getRecoveryTarget(long id) |
void |
markRecoveryAsDone(long id)
mark the recovery with the given id as done (if found)
|
RecoveryTarget |
resetRecovery(long recoveryId,
TimeValue activityTimeout)
Resets the recovery and performs a recovery restart on the currently recovering index shard
|
int |
size()
the number of ongoing recoveries
|
long |
startRecovery(IndexShard indexShard,
DiscoveryNode sourceNode,
PeerRecoveryTargetService.RecoveryListener listener,
TimeValue activityTimeout)
Starts are new recovery for the given shard, source node and state
|
public RecoveriesCollection(org.apache.logging.log4j.Logger logger, ThreadPool threadPool, java.util.function.LongConsumer ensureClusterStateVersionCallback)
public long startRecovery(IndexShard indexShard, DiscoveryNode sourceNode, PeerRecoveryTargetService.RecoveryListener listener, TimeValue activityTimeout)
public RecoveryTarget resetRecovery(long recoveryId, TimeValue activityTimeout)
IndexShard.performRecoveryRestart()
public RecoveryTarget getRecoveryTarget(long id)
public RecoveriesCollection.RecoveryRef getRecovery(long id)
RecoveryTarget
for a given id. The RecoveryStatus returned has it's ref count already incremented
to make sure it's safe to use. However, you must call AbstractRefCounted.decRef()
when you are done with it, typically
by using this method in a try-with-resources clause.
Returns null if recovery is not found
public RecoveriesCollection.RecoveryRef getRecoverySafe(long id, ShardId shardId)
getRecovery(long)
but throws an exception if no recovery is foundpublic boolean cancelRecovery(long id, java.lang.String reason)
public void failRecovery(long id, RecoveryFailedException e, boolean sendShardFailure)
id
- id of the recovery to faile
- exception with reason for the failuresendShardFailure
- true a shard failed message should be sent to the masterpublic void markRecoveryAsDone(long id)
public int size()
public boolean cancelRecoveriesForShard(ShardId shardId, java.lang.String reason)
reason
- reason for cancellationshardId
- shardId for which to cancel recoveries


Laluna’s quiet beach is the ideal location for your Grenada destination wedding. Our boutique resort’s Caribbean setting is what you’ve always dreamed of for your beach ceremony: Tropical flowers and lush greenery wrap the white sand beach, and the crystal clear sea, brilliant with colors of blue and green, quietly laps the shore. Say your vows under a Caribbean wedding arch while your invited guests watch on and share your special day. Following the ceremony, stay on-resort, as the Laluna Sunset Lounge and Italian Restaurant can be transformed to an inviting reception venue. Laluna’s dedicated staff have been planning destination weddings for over 14 years. From arranging the photographer to ordering the cake to helping with the marriage license, our staff helps you with it all. Give as much or as little input as you like, and we will take care of the details. To take the guesswork out of Grenada destination wedding planning, we have special packages that include everything needed to create your perfect wedding in paradise. Laluna's Seven Night Wedding Program for Two Includes:
Accommodation for the bride and groom in a romantic Cottage Suite with private veranda with plunge pool An intimate and relaxing Balinese couples massage Daily yoga/meditation sessions A pampering manicure and pedicure for both the bride and groom Delicious meals in Laluna's Italian restaurant with daily a-la-carte American breakfast and dinner (excluding beverages) A bottle of Prosecco A beautiful wedding cake A locally crafted bridal bouquet and groom's boutonniere A professional wedding photographer, which includes digital files of all photos. Ceremony essentials including the minister's fee, marriage license and certificate, and venue staging A gift from Laluna to congratulate you on your big day US $ 7,088 December 20th, 2015 to January 8th, 2016 US $ 6,388 January 9th to April 7th, 2016 US $ 5,688 April 8th to June 24th, 2016 US $ 5,338 June 25th to October 14th, 2016 Package accommodations can be upgraded to a Cottage Deluxe for US $65.00 per night plus tax. All rates are quoted in US dollars and are subject to an additional 20% tax & service.


|
Jaded
(Aerosmith) |
|
Hey...


Reset »
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Credit
Mozilla Taiwan Community
×
Explorer Cyber Browserer Comic
Illustrated by ECBp,
licensed under CC:BY-NC-SA-3.0-TW
Music: Mozilla-Blues, composed by MGdesigner,
licensed under CC:BY-3.0-TW
Programed by WM, Derived from Dino Pair Game
by Matt Walker, Thank him for the original game.


Sir Lenny Henry and Stephen Fry set to star in Doctor Who
The TV stars will appear alongside Jodie Whittaker when the Tardis lands once more, but it is not yet known if they will be friend or foe to the Time Lord and her friends
by James Rodger, https://www.facebook.com/jamesrodgerjournalistSir Lenny Henry and Stephen Fry will star in "major roles" in the first episode of the new series of Doctor Who.
The TV stars will appear alongside Jodie Whittaker when the Tardis lands once more, but it is not yet known if they will be friend or foe to the Time Lord and her friends.
It will be a debut stint for both Sir Lenny and Fry in the sci-fi drama.
Fry said: "Short of being picked for a British space exploration programme and I readily concede that I'm past the age where I'd be considered (if I was ever the right age for such a posting) - then being in an episode of Doctor Who will certainly do as a very sweet second-place excitement."
Sir Lenny added: "It was absolutely brilliant to be welcomed into the fantastical world of Doctor Who.
"The nearest I have been to the Tardis was when I played the Caribbean Doctor in the Lenny Henry Show, so as a life-long (hiding behind the sofa type) Doctor Who fan this is a very special moment for me."
Doctor Who showrunner Chris Chibnall said that the series will return "with a bang - with two great British icons in major roles".
He added: "One of the great joys of Doctor Who is getting to work with actors from your wish list. Stephen and Lenny are two of my absolute favourite actors - and to be able to bring them into Doctor Who, in our one of our biggest ever stories to kick off the new series, is an absolute thrill."
Whittaker will return as the Thirteenth Doctor alongside co-stars Tosin Cole, Mandip Gill and Bradley Walsh in the new series, which will air next year.


Plots can be configured with several keyword arguments that control appearance:
These parameters can be passed to glyph functions such a circle or rect but it is often useful to pass them to a call to figure:
figure(
title="My Plot",
title_text_font_size="20pt",
plot_width=200,
plot_height=300,
outline_line_color="red",
x_axis_type="datetime"
)
Bokeh plots are centered around glyphs, which generally have some combination of line, fill, or text properties, depending on what is appropriate for a given glyph. For example, the Circle glyph has both line and fill properties, but the Bezier glyph only has line properties. These properties may be specified as keyword arguments when calling the glyph functions:
rect(x, y, radius, fill_color="green", fill_alpha=0.6, line_color=None)
Markers are a subset of Bokeh glyphs that have a prescribed interface. Markers all respond to:
Many of the styling options are grouped into three categories of properties: Line Properties, Fill Properties, and Text Properties.
Note
There is currently only support for filling text. An interface to stroke the outlines of text have not yet been exposed.
To control the ranges that Bokeh plots show, there are two keyword parameters x_range and y_range. These may be passed into the bokeh.plotting.figure function, or they may also be set as attributes on a plot object.
If None is passed in as the value of x_range or y_range, then the plot will be configured with a DataRange1d which computes the envelope of all the plot data to determine the range. This is the default behavior.
Note
For non-scatter glyphs with spatial extent, the DataRange1d may not compute the necessary bounds fully.
To set the range on a plot that has numerical range values, you can pass a sequence of numbers with length two:
figure(xrange=[0, 100])
This will prepare a new plot that has an x-axis range that spans the interval [0, 100]. You can also pass a bokeh.models.Range1D object explicitly:
figure(xrange=Range1d(start=2, end=8))
This will prepare a new plot that has an x-axis range that spans the interval [2, 8]. Alternatively, you can set the range as a property on a Plot object:
plot.y_range = Range1d(start=0, end=10)
For plots with categorical ranges, it is necessary to specify the range as a sequence of strings that give the categories in the desired order. For example:
figure(y_range=["foo", "bar", "baz"])
will prepare a plot whose y-axis range is categorical, with the categories “foo”, “bar”, and “baz”. Please see this categorical example from the gallery for a concrete example.
You can also pass in a FactorRange explicitly as well.
Axes in Bokeh also have line properties for the axis rule line, as well as for the major ticks. These standard line properties are prefixed with axis_ and major_tick_ respectively. Axes also have text properties, for the axis label and major tick labels. These are prefixed axis_label_ and major_tick_label_, respectively.
Some examples:
ax.axis_line_color = "red"
ax.bounds = (3, 7)
ax.major_label_orientation = pi/4
Axes for a plot may be conveniently obtained using the xaxis, yaxis, and axis properties. These return collections of axes that can be indexed to retrieve individual axes, or can that have attributes set directly on them to update all axes. Examples:
p.xaxis.axis_line_width = 2 # update all x-axes
p.yaxis[0].axis_line_color = "red" # only updates the first y-axis
p.axis.bounds = (2, 8) # set bounds for all axes
Typically after updating these attributes, a call to bokeh.plotting.show() will be required.
Note
The bounds attribute here controls only the extent of the axis! It does not set the range of the plot. For that, see Ranges. As an example, a plot window may extend from 0 to 10, but you may only want the axis to render between 4 and 8, in order to highlight a particular sub-area of the plot.
Grids for a plot may be conveniently obtained using the xgrid, ygrid, and grid properties. These return collections of axes that can be indexed to retrieve individual grids, or can that have attributes set directly on them to update all axes. Examples:
p.xgrid.axis_line_dash = "3 3" # update all x-grids
p.ygrid[0].axis_line_color = None # only updates the first y-grid
p.grid.bounds = (2, 8) # set bounds for all grids
Typically after updating these attributes, a call to bokeh.plotting.show() will be required.
Note
The bounds attribute here controls only the extent of the grid! It does not set the range of the plot. For that, see Ranges. As an example, a plot window may extend from 0 to 10, but you may only want the grid to render between 4 and 8, in order to highlight a particular sub-area of the plot.
Bokeh comes with a number of interactive tools. There are five categories of tool interactions:
For the first three categories, one tool can be active at any given time, and the active tool is indicated on the toolbar by a highlight next to to the tool. Actions are immediate or modal operations that are only activated when their button in the toolbar is pressed. Inspectors are passive tools that merely report information or annotate the plot in some way.
When using the Basic Plotting with Glyphs interface, tools are added to plots with the tools keyword argument, which has as its value a comma separated string listing the tools to add to the plot, for example:
tools = "pan,wheel_zoom,box_zoom,reset,resize"
These tools are employed by panning (on touch devices) or left-dragging (on mouse devices). Only one pan/drag tool may be active at a time.
The box selection tool allows the user to define a rectangular selection region by left-dragging a mouse, or dragging a finger across the plot area. The box select tool may be configured to select across only one dimension by setting the dimension property to width or height.
Note
To make a multiple selection, you have to press the SHIFT key and to clear the selection you have to press ESC key.
The box zoom tool allows the user to degine a rectangular region to zoom the plot bounds too, by left-dragging a mouse, or dragging a finger across the plot area.
The lasso selection tool allows the user to define an arbitrary region for selection by left-dragging a mouse, or dragging a finger across the plot area.
Note
To make a multiple selection, you have to press the SHIFT key and to clear the selection you have to press ESC key.
The pan tool allows the user to pan the plot by left-dragging a mouse or dragging a finger across the plot region.
It is also possible to constraint the pan tool to only act on either just the x-axis or just the y-axis by setting the dimension property to width or height. Additionally, there are tool aliases 'xpan' and 'ypan', respectively.
The resize tool allows the user to left-drag a mouse or drag a finger to resize the entire plot.
These tools are employed by tapping (on touch devices) or left-clicking (on mouse devices). Only one click/tap tool may be active at a time.
The polygon selection tool allows the user to define an arbitrary polygonal regions for selection by left-clicking a mouse, or tapping a finger at different locations.
Note
To complete the selection, you have to make a double left-click or tapping Also, to make a multiple selection, you have to press the SHIFT key and to clear the selection you have to press ESC key.
The tap selection tool allows the user to select at single points by clicking a left mouse button, or tapping with a finger.
Note
To make a multiple selection, you have to press the SHIFT key and to clear the selection you have to press ESC key.
These tools are employed by pinching (on touch devices) or scrolling (on mouse devices). Only one scroll/pinch tool may be active at a time.
The wheel zoom tool will zoom the plot in and out, centered on the curren t mouse location.
It is also possible to constraint the wheel zoom tool to only act on either just the x-axis or just the y-axis by setting the dimension property to width or height. Additionally, there are tool aliases 'xwheel_zoom' and 'ywheel_zoom', respectively.
Actions are operations that are activated only when their button in the toolbar is tapped or clicked. They are typically modal or immediate-acting.
The reset tool will restore the plot ranges to their original values.
The save tool pops up a modal dialog that allows the user to save a PNG image of the plot.
Inpectors are passive tools that annotate or otherwise report information about the plot, based on the current cursor position. Any number of inspectors may be active at any given time. The inspectors menu in the toolbar allows users to toggle the active state of any inspector.
Th crosshair tool draws a crosshair annotation over the plot, centered on the current mouse position. The crosshair tool may be configured to draw accross only one dimension by setting the dimension property to width or height.
The hover tool pops up a tooltip div whenever the cursor is over a glyph. The information comes from the glyphs data source and is configurable through a simple tooltips dictionary that maps displayed names to columns in the data source, or to special known variables. Here is an example of how to configure the hover tool:
# We want to add some fields for the hover tool to interrogate, but first we
# have to get ahold of the tool. We can use the 'select' method for that.
hover = plot.select(dict(type=HoverTool))
# Add tooltip (name, value) pairs to tooltips. Variables from the data source
# are available with a "@" prefix, e.g., "@foo" will display the value for
# the 'foo' column value under the cursor. There are also some special known
# values that start with "$" symbol:
# - $index index of selected point in the data source
# - $x, $y "data" coordinates under cursor
# - $sx, $sy canvas coordinates under cursor
# - $color color data from data source, syntax: $color[options]:field_name
# available options for $color are: hex, swatch
# NOTE: we use an OrderedDict here to preserve the order in the displayed tooltip
hover.tooltips = OrderedDict([
("index", "$index"),
("(x,y)", "($x, $y)"),
("radius", "@radius"),
("fill color", "$color[hex, swatch]:fill_color"),
("foo", "@foo"),
("bar", "@bar"),
])
Note
Point hit testing is not currently available on all glyphs. Hover tool currently does not work with line or image type glyphs.


The Pipelines
Overview
The Pipelines is the part of the code interacting with the transport protocol, defined in Net, to download and parse:
- the Manifest
- media Segments
Each of those task is performed by a discrete component of the Pipeline:
-
The Manifest Pipeline is used to download and parse the manifest file.
-
The SegmentPipelinesManager is used to download and parse media segments.


{% extends 'profile_base.html' %} {% block title %} Your information | {{ block.super }} {% endblock %} {% block profile_content %} {% if not profile.description %}
You have not written anything in your "description".
If you intend to join one or more teams you can use the profile to help the team responsible understand who you are and what you have to offer. Please also include availability if you are not joining us for the entire week.
|
Name Not visible to the public. |
{{ profile.name|default:"N/A" }} |
|
Description Not visible to the public. |
{{ profile.description|default:"N/A" }} |
|
Public Credit Name Visible to the public, leave empty if you want no credits on this website. |
{{ profile.public_credit_name|default:"N/A" }} {% if profile.public_credit_name %}({% if profile.public_credit_name_approved %}approved{% else %}pending approval{% endif %}){% endif %} |
|
NickServ username Visible to the public on IRC, used to handle team channel ACLs. |
{{ profile.nickserv_username|default:"N/A" }} |


{% extends 'base.html' %} {% block content %} {# Show welcome message if user is authenticated#} {% if request.user.is_authenticated %}
Created at {{ game.created_date }}
Join {{ game.player1.username }} now!
Do you want to join {{ game.player1.username }} to play Connect 4?


Montana, as the saying goes, is one big small town with really long streets.
The state’s communities, from Libby to Helena to Ekalaka, have plenty in common when it comes to the issues facing their future. Even so, Montana’s wide geography sometimes makes it hard for us to learn from our neighbors. Journalism is one of the best tools we have for bridging that distance.
The Long Streets Project focuses on issues and trends facing Montana’s economy: examining where Montanans can and can’t find decent jobs, investigating how public policy decisions have panned out and exploring how economic constraints shape our communities.
Made possible by a $10,000 grant from the Greater Montana Foundation, we are publishing a series of narrative and multimedia stories in partnership with the Montana Free Press starting in November 2018 and continuing into 2019. Each piece is available for free republication by newspapers and other news outlets across the state.
With the help of readers like you, we’re hoping to spur productive conversations about what Montanans can do to build a healthy economy and stronger communities. You can follow along by subscribing to our weekly-ish newsletter or chiming in on Facebook or Twitter. We’re all ears if you want to drop us a line and suggest our next story idea, too.
A journalist, cartographer and web developer, Eric's work combines data analysis and visualization with old-fashioned reporting. He was trained as a civil engineer at Montana State University and has covered Montana as a staff reporter and freelance writer, working for the Great Falls Tribune, Bozeman Daily Chronicle and Solutions Journalism Network Montana Gap Project.
Over the past five years, Derek's incisive reporting has spanned issues ranging from K-12 education to bitcoin-powered economic development, with his specialty in-depth pieces able to remind readers of their neighbors' humanity. He graduated from Montana State University and has worked for the Helena Independent Record, Billings Gazette and Missoula Independent.


Interet can be accessed by using any of the following methods :
Dial-up :
Dial-up connections are one type of internet connection available from ISPs, they are the slowest and (usually) the most inexpensive.
A dial-up connection allows you to connect to the internet via a local server using a standard 56k modem. Your PC literally dials (hence the name) a phone number (provided by your ISP) and connects to the server and therefore the internet.
DSL :
Digital Subscribers Line connections are becoming more and more widely available and can provide an excellent internet connection.
The connections work by splitting your phone line into two separate channels, one for data (internet) and one for voice (phone calls), which means you can talk on the phone and be connected to the internet at the same time.
Broadband wireless access :
Wireless Broadband is a fairly new technology that provides high-speed wireless internet and data network access over a wide area. According to the 802.16-2004 standard, broadband means having instantaneous bandwidth greater than around 1 MHz and supporting data rates greater than about 1.5 Mbit/s.
Cable Internet:
Cable connections are considered one of the best types of internet connection available to the home user, they offer very fast and reliable connections with a fixed monthly fee.
Cable companies usually offer different packages to suit different internet subscribers, your choice of package will depend on how you intend to use the internet.
The different packages will offer different speed specifications and bandwidth limits.
Because a cable connection uses a totally separate medium to transfer data, it doesn't affect your ability to make/receive phone calls.
FTTH (Fiber To The Home)
FTTH or Fiber To The Home, refers to fiber optic cable that replaces the standard copper wire. FTTH is desirable because it can carry high-speed broadband services integrating voice, data and video and runs directly to the junction box at the home or building. For this reason, it is sometimes called Fiber To The Building or FTTB. Fiber optic cables are made of glass fiber that can carry data at speeds exceeding 2.5 gigabits per second (gbps).
ISDN
Integrated Services Digital Network, an international communications standard for sending voice, video and data over digital telephone lines or normal telephone wires. ISDN supports data transfer rates of 64 Kbps (64,000 bits per second).
There are two types of ISDN:
Basic Rate Interface (BRI) -- consists of two 64-Kbps B-channels and one D-channel for transmitting control information.
Primary Rate Interface (PRI) -- consists of 23 B-channels and one D-channel (U.S.) or 30 B-channels and one D-channel (Europe).
Wireless(Wi-Fi)
Wireless Internet uses radio waves as a means of transmission. The most convenient thing about wireless is that more than one person can log onto the connection. Wireless Internet provides you Internet access in your home, on the road or at the office. Many cell phone providers bundle phone and Internet service that save you money. Wireless Internet is free in many public areas. You can use it as long as you have a wireless connection on your laptop.


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Equal opportunities Policy(EEO)
This equal employment opportunity policy is the pillar of a healthy and productive working environment.
Everyone should feel supported and valued to work productively so we are invested in treating everyone with respect and consideration.
Our equal opportunity employer policy applies to all employees, job candidates, freelancers, contractors, stakeholders, partners and visitors.
Equal opportunity is for everyone,
but it mainly concerns members of underrepresented groups – they’re the ones who are traditionally disadvantaged in the work selection.
We don’t guarantee employment or promotions for people in those groups,
but we will treat them fairly and avoid discriminating against them either via conscious or unconscious biases.
Being an equal opportunity company means that we provide the same opportunities for hiring,
advancement and benefits to everyone without discriminating due to protected characteristics like:


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#7. Interaction & Engagement
#7.1 Designing Effective Navigation
- Planning Screens & Their Relationships
- Planning for Multiple Touchscreen Sizes
- Providing Descendant & Lateral Navigation
- Providing Ancestral & Temporal Navigation
- Wireframing the Example App
#7.1.1 Planning Screens & Their Relationships
Information Model: What 'types' of things does your user interact with?
#<IP_ADDRESS> Create a Screen List
- When does user interact with data (contexts)
- How does he interact (read, create, update, delete)
- What is the exhaustive set of screens?
- Category List, Story List, Photos List
- Story Detail, Photo Detail
- (Saved) Story List, (Saved) Photo List
- Home (lobby), Profile, Settings,..
#7.1.3 Screen Map for News App
Enough for 'Simplistic' UI Design
Buttons for navigating, lists for information, layouts for detail
#7.1.4 Plan for Multiple Screen Sizes
Determine the screen size at which you want to flip from single pane to multi-pane layouts
Screen implemented as Activity. Content always implemented as Fragment.
#7.1.5 Design for Table 'Orientation'
(Clockwise, from top-left) Stretch-to-fit (some panes may be fixed), Collapse-left (e.g., list shrunk, details expanded), Show-Hide (e.g., list hidden, needs affordances), Stack (for multi-pane content)
#7.1.6 Screen Map for News App
Revisit your exhaustive screen maps list. Identify 'groups' that can be shown in multi-pane layouts
#7.1.7 Descendant and Lateral Navigation
Understand navigation hierarchy.
Descendant navigation is for child content, Lateral navigation is for sibling content
#7.1.8 Sibling Screens (2 Types)
Collection = Items in collecton represented by 'parent'
Section = Different aspects of information about 'parent'
User Interface Design Patterns for both
#7.1.9 Buttons & Targets
'Dashboard' Pattern (touchable, kb-focusable targets.
Ideal for Section Siblings. Rethink for large devices.
#7.1.10 Lists, Grids, Carousels, Stacks
Note: 'Drill Down' list navigation can get cumbersome.
Ideal for Collection Siblings.
#7.1.11 Tabs (Section Siblings)
Lateral navigation. Think Tabs vs. Dashboard.
Ideal for parent with 4-or-less section siblings
#7.1.12 Swipes (Collection Siblings)
Lateral navigation. AKA Horizontal Paging.
Ideal for collection siblings.
Needs complementary 'context' hints
#7.1.13 Temporal Navigation ("Back")
Recall Task BackStack. System typically handles 'Back'
Override within context (e.g., browser) with path to default.
#7.1.14 Ancestral Navigation ("Up")
"Home" (pre 3.0) vs. "Up" (post 3.0 ActionBar)
Safe 'exit' to familiar place (typically parent screen)
Can be contextual (e.g., differs based on device orientation)
TIP: Proactively clear backstack of 'descendant' screens
#7.2 Wireframing the Example App
- Choose Patterns
- Sketch and Wireframe
- Create Digital Wireframes
#<IP_ADDRESS> App Screen Map
Choose patterns to maximize navigation speed
minimize touches, create consistent UI
Choose targeted screen sizes (tablet/phone?)
#<IP_ADDRESS> Step 1: Choose Patterns
- Identify Section Siblings (lateral nav.)
- Identify Collection Siblings (descendant nav.)
- Define Content 'Fragment' (smallest items)
- Define 'Activity' screen for device (phone vs. tablet)
- Think 'alternative layouts' (e.g., for orientation)
#<IP_ADDRESS> Step 1: Tablet (Alt.)
#<IP_ADDRESS> Creating Wireframes
- Physical sketch (paper/board)
- Refine thinking (details, flow, adaptation)
- Peer reviews (errors, omissions)
- Digital mapping (interactive)
- User reviews (effort + clarity)
- Android build (graphical XML)
1: Setup
- Create 'cv-project-name' repo in your GitHub
- Pick a unique 'name' for you (let me know)
- Create a branch (1-data-model)
- Create a filename (README.1.datamodel.md) in branch
2: Populate
- In README.1.datamodel.md, describe your information model
- Add document showing entity relationships
- Add document showing screen maps
- Add document showing v1 of screen wireframe
- Update README.1.datamodel.md with reasons for decisions
First Version: ready to review Fri (Mar 7)
Final version: submit (PDF) on Tue (Mar 11)
#7.2 Implementing Effective Navigation
- Creating Swipe Views with Tabs
- Creating a Navigation Drawer
- Providing Up Navigation
- Providing Proper Back Navigation
- Implementing Descendant Navigation
#7.3 Notifying the User
- Buildng a Notification
- Preserving Navigation when Starting an Activity
- Updating Notifications
- Using Big View Styles
- Display Progress in a Notification
#7.4 Adding Search Functionality
- Setting up the Search Interface
- Storing and Searching for Data
- Remaining Backward Compatible
#7.5 Making Your App Content Searchable By Google
- Enabling Deep Links for App Content
- Specifying App Content for Indexing


What you should know about Latin today is that it is a language in the indo-european family. It was once spoken by the Romans, and is now extinct. Note that Latin learning is hard: the nouns changes; the adjectives changes; the verbes changes. To give you a feeling, a typical verb can change into 140 different forms under different circunstances. So... have fun! And don't give up. Colonel Vibius Vibidius Zosimus is on your side.
Getting a Latin name will be your very first step toward Latin learning. You can pick, amongst millions of combinations, from Wikipedia pages, or you can download the random-Latin-name generator written in python 3 by me.
| my name | Vibius | Vibidius | Zosimus |
| name of the part | praenōmen | nōmen | cōgnōmen |
| list of | (wiktionary page) | (wikipedia page) | (as well) |
Fortunately, the verbs in Latin are relatively easy (at least for present active indicative : ). The rule, simplest amongst all, is also easy to remember.
| verb conjugation rules | tense: present voice: active mood: indicative |
(person) | sing. | pl. |
|---|---|---|
| 1st | m / ō | mus |
| 2nd | s | tis |
| 3rd | t | nt |
For example, given a verb "to love," namely amō, amāre, the conjugation is:
| amō | I love |
| amās | you love |
| amāt | he loves |
| amāre | we love |
| amātis | y'all love |
| amānt | they love |
The way to remember is: MŌST MUST ISNT; you can temporarily ignore the 'M' in "MŌST" for now.
These are just so little about Latin on day 1. The important thing is, Latin learning starts really easily, then it gradually gets harder, then it gets SUUUUUPER HARD, then it'll be better. Then it will be hard some more.
Things to remember: your Latin name, "MŌST MUST ISNT" for general verb conjugations, and to visit day 2 tomorrow.
... back next day→


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March 23 - 24, 2019
Juniper Aspiration Dome
1081 Innovation Way, Sunnyvale, CA


You have to log in via Eve Single-Sign-On in order to protect your own waitlist and to protect your entry on other waitlists. Without the authentication, everybody could delete everybody from waitlists. Or Alice could x-up as Bob. Or a spambot could just kill the entire tool without any way to block him.
None at all. The only thing I learn is that this is in fact you. The page you enter your login credentials is managed by CCP, I never see your credentials. You can check this by inspecting the URL in your browser, it should look something like the folling example:


Driving
The village of Welschneudorf is about 1 hour’s drive from both Frankfurt airport and Cologne/Bonn airport.
By train
From Frankfurt airport train station (Frankfurt Flughafen), there is a direct train service to the nearest town of Montabaur (ICE-Bahnhof Montabaur), which takes approximately 30 minutes. From Cologne/Bonn airport train station (Köln/Bonn Flughafen), there is also a train service to Montabaur, which takes approximately 1 hour and includes one change. Please visit bahn.de for train times and bookings.
Montabaur train station is about 10 minutes’ drive from the wedding venue. We can assist with booking taxis from the train station nearer the time if required.
We are anticipating that most guests will arrive on Friday afternoon or evening.
Food will be provided on the farm in the Gutshaus restaurant in the evening. As guests will be arriving at different times, there won’t be a set time for food. We will be around and everyone can arrive in their own time and join us to eat whenever it suits.
The wedding venue is in a rustic location. There is a smart dress code for the church service, but guests may also wish to bring more comfortable/flat shoes for the rest of the weekend. There will be time to stroll around the grounds, play games and watch the children feeding the animals or horse riding...


--- layout: post title: Radiators date: '2010-12-08T12:53:31-05:00' tags: [] tumblr_url: http://poetry.liabogoev.com/post/122628728520/radiators ---
Above, I hear the sounds
of workmens’ boots and clanking
of radiator pipes as they are
knocked, and pounded into place.
The sounds resonate, through the
yellow walls, with the sponging
the ones painted by the architect
the ones with the white trim
and lavender panel.
They shake the poster of Salvador Dali’s
Swans reflecting elephants
and I hear the buzzing of the paper
They shake me from sleep
and I fight it, enveloped in
warm clouds, the blue and green
comfort, green side up,
and I press my nose between
your back and the sheets
and pull the covers up.
Another day has greeted me,
each more rudely as the next
as I sit, passing time, unwisely,
Day after day after day


Two Killed As Robbers Attack Bank In Ekiti
The robbers overpowered the police officer attached to the bank to gain access to the facility before killing him.
by SaharaReporters, New York
Two people have been killed after armed robbers attacked a bank in Oye, Ekiti State, on Thursday.
The robbers overpowered the police officer attached to the bank to gain access to the facility before killing him.
A school girl was also hit by a stray bullet and died on the spot.
It was gathered that the robbers went away with millions of naira, which was stolen from the vault of the bank.
Customers of the bank, who were inside during the incident were also robbed of valuables.


Jordanian cuisine
Jordanian cuisine is a traditional style of food preparation originating from, or commonly used in Jordan
that has developed through centuries of social and political change.
There are a wide variety of techniques used in Jordanian cuisine ranging from baking, sautéeing and grilling
to stuffing of vegetables (carrots, leafy greens, aubergine, etc.),
meat, and poultry. Also common in Jordanian cuisine is roasting or preparing foods with special sauces.
As one of the largest producers of olives in the world,olive oil is the main cooking oil in Jordan. Herbs,
garlic, onion, tomato sauce and lemon are typical flavours found in Jordan. Yogurt is commonly served
alongside food and is a common ingredient itself; in particular, jameed, a form of dried yogurt is unique to
Jordanian cuisine and a main ingredient
in mansaf the national dish of Jordan, and a symbol in Jordanian culture for generosity.
Mansaf
What is Mansaf?
There’s a certain Jordanian pride and significance that goes along with mansaf – and once you taste it, and experience a communal meal of it, you’ll know why. Mansaf is a food that runs deep in the culture of Jordan, and when you take your first bite, you’ll actually taste Jordan. There are only a few main components of any platter of mansaf; rice, lamb, jameed (more about this below), and lastly nuts and shrak (a type of bread) are also commonly present.
Makmoura
What is Makmoura?
This is an old Jordanian-oriented dish, eaten mostly by people in North Jordan.  Makmoura, meaning buried, is exactly what it sounds like. Boiled chicken and onions are buried under a thick blanket of dough and cooked in the oven until well-done. It is later served in triangle pieces, exactly like cake.
Rashouf
What is Rashouf?
Rashouf is another deeply oriented food tightly linked to the Jordanian culture, and is also served as a winter dish. Adding the same yogurt essence used in cooking mansaf to a blend of lentils, groats, and wheat, is it cooked over medium heat and served with sour pickles and vegetable. Careful though, as beneficial as this dish is, it is also very high in protein and fibers, so don’t eat it and take a nap.
Shorabet Adas
What is Shorabet Adas?
om The famous lentil soup is the official sponsor of every winter in Jordan.Whenever it is cold and rainy outside, Jordanian mothers would immediately start preparing lentil soup—it even goes down as the most ordered dish on restaurant menus during the winter season. This cozy cup of warmth will immediately heat you up, enhance your energy, and strengthen your immune system. Try it hot with toasted bread, a squeeze of lemon juice, and green onions.
Mujadara
What is Mujadara?
Mujadara is a healthy protein-filled dish which is easy to prepare. Raw rice and lentils are cooked together and seasoned with lots of cumin and spices. Some like to add partially burned onions atop their plates, but it is best eaten with yogurt, salad, or both.
Maqluba
What is Maqluba?
Translating to the “turned over” dish, this particular food is more interesting to watch being cooked than eaten. The ingredients are nothing out of the ordinary: rice, potatoes, chicken, and aubergine or cauliflower, all stirred in a big pot. When the cooking is done comes the magical moment; children would gather to watch the Jordanian mother flip the huge pot over a flat plate and then remove it, revealing what looks like a neat cake of rice and chicken.
Mulukhiyah
What is Mulukhiyah?
Jordanians and Palestinians have been living together for decades, sharing blood, traditions and, of course, delicious recipes. Mulukhiyah originated in Egypt from the time of the Pharaohs. Back then it was called mulukiyah, the food of the kings, and was only to be later adapted by Palestinians. Mulukhiyah is a rather odd looking dish that doesn’t quite please the eye on first sight, but will instantly have you head over heels from the first bite.


In Mirror Cache you have two nodes, Active and Passive. The default node will act as an Active node, where all clients are connected. You can make a passive node active any time. To make a node active, right click on the passive node and select 'Make Active Node' option from the context menu. If the Mirror Cache is stopped then status of the nodes is immediately changed. The passive node becomes active and the active node becomes passive. But if Mirror Cache is running then the status of the nodes is changed only after the cache is restarted.
Start NCache Service on a Node | Stop NCache Service on a Node | Balance data load | Select Network Interface Card


THE MYTH OF FINGERPRINTS (Sony Pictures Classics - 1997) Starring Arija Bareikis, Blythe Danner, Hope Davis, Laurel Holloman, Brian Kerwin, James LeGros, Julianne Moore, Roy Scheider, Michael Vartan, Noah Wyle Screenplay by Bart Freundlich Produced by Mary Jane Skalski, Tim Perell, Bart Freundlich Directed by Bart Freundlich Running time: 93 minutes
*** (out of four stars) Alternate Rating: B
Note: Some may consider portions of the following text to be spoilers. Be forewarned.
-------------------------------------------------------------
Bart Freundlich's feature film debut, THE MYTH OF FINGRPRINTS, is exciting -- not for the film itself, but for the promise it heralds for its helmer and screenwriter. He demonstrates a real gift for sharp, clever dialogue and has created a series of rich, interesting, and well-developed credible characters, while his direction of the film is astonishingly assured for a first-timer, with good comic pacing and adept camera work. Although THE MYTH OF FINGERPRINTS features a large ensemble cast and a myriad of concurrent subplots, Mr. Freundlich skillfully juggles his many characters in an evenly focused fashion where no single storyline inadvertently takes dominance in the film.
The shame is that THE MYTH OF FINGERPRINTS doesn't have a terribly interesting plot: Mr. Freundlich's film is an all-too-familiar tale of a dysfunctional family reuniting for Thanksgiving weekend, where closeted skeletons eventually are revealed after much wistful retrospective discussion by family members over the course of the holiday. THE MYTH OF FINGERPRINTS handles this routine storyline in a solid fashion -- it *is* an entertaining film -- but it's somewhat frustrating that such witty dialogue and such great characters as those Mr. Freundlich have fashioned are used in service of a plot which is not their equal in terms of calibre or ambition.
Set in chilly New England, the film opens with Lena (Blythe Danner) and Hal (Roy Scheider) in preparation for the return of their four adult children after an absence of three years. In quick succession, siblings Leigh (Laurel Holloman), Jake (Michael Vartan), Mia (Julianne Moore), and Warren (Noah Wyle) pass through the front doors of the family home, with Jake bringing along forthright free-spirited girlfriend Margaret (Hope Davis), and Mia towing sadsack boyfriend Elliot (Brian Kerwin). While appearing on the surface to be a typical happy American family, eccentricities and quirks are unveiled and buried secrets are unsurfaced which reveal the deep-rooted dysfunctionality which has splintered apart the family.
While the pensive moments in THE MYTH OF FINGERPRINTS register nicely, the film's greatest strength is in the interaction between the characters, which come off as easy, amusing and boisterous. Each of the siblings have grown up coping with the dour family environment in different fashions. Leigh is mischievous and brash, while Mia is consumed by bitterness and has not a kind word to snap at anyone. Jake and younger brother Warren appear on the exterior to be wholesome, clean-cut, well-adjusted young men, but they are fighting their own interior demons: Jake is nagged by self-doubt, while Warren is haunted by the loss of his relationship with high school sweetheart Daphne (Arija Bareikis) and is masking a sense of overwhelming sadness. None of them are able to relate on a personal level to their father Hal, who is decidedly eccentric and unable to communicate with his children on any level, even skulking off to the treehouse to avoid discussion. The family's patient matriarch Lena is the single common element in these two disparate sets.
Mr. Freundlich benefits from a fine ensemble cast, all of whom turn in good performances and have good chemistry with one another. Ms. Holloman, a rising new star, is particularly good as Leigh, the playful imp of the family, while Ms. Davis turns in a very funny performance as Margaret, whose sprightly demeanour and propensity to speak what's foremost on her mind brings about many embarrassing and amusing moments. Ms. Moore's performance is the most interesting in the group; she successfully depicts Mia's unmitigated rage masking a well of sorrow, and when she encounters old grade schoolmate Leonard/Cezanne (James LeGros) during a trip into town, one can feel her desperation as she listens to his wistful story -- she *wants* to believe him, and that comes through in Ms. Moore's performance.
THE MYTH OF FINGERPRINTS marks the first major feature film for Mr. Wyle since his emergence as a public figure with the success of the television drama ER. I first noticed him in Michael Bortman's CROOKED HEARTS (and subsequently spent several years wondering whatever happened to this promising young actor), which is extremely similar on a thematic basis to THE MYTH OF FINGERPRINTS; the number of parallels between the two films is striking. As Mr. Wyle was very keen on THE MYTH OF FINGERPRINTS, being the first in the cast to sign on to the project and even obtaining a credit as an associate producer, there is ample cause to assume that he has some sort of predisposed affinity for material of this nature.
THE MYTH OF FINGERPRINTS doesn't break any new ground with its routine storyline -- it follows the familiar path tread by all films of this sort -- but it generates some big laughs and is a solid and successfully amusing diversion. The film is a wholly respectable first feature, and Mr. Freundlich demonstrates a great deal of promise as a screenwriter and, to a slightly lesser extent, as a director -- keep an eye out for him: if his next project is built around a more interesting and ambitious story, it could be very good indeed.
- Alex Fung email<EMAIL_ADDRESS>web : http://www.ncf.carleton.ca/~aw220/
-- Alex Fung<EMAIL_ADDRESS>| http://www.ncf.carleton.ca/~aw220/ "Man, that was a big spider. It was so big I thought I saw a small dog caught in its web. We are talking big.  - Hope Davis, THE MYTH OF FINGERPRINTS
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


Phone & SMS with Twilio
In this week's episode, we'll be taking a look at Twilio, a cloud-based service for adding telephony features to applications through a RESTful web service API. Using Twilio, developers can send and receive phone calls and SMS text messages, enabling the creation of interfaces that pass beyond the reach of smart phones.
Learn how to send and receive phone calls and text messages in your mobile applications in this week's episode of Forging Titanium.
Episode Resources:


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Pan-IIT Odia Community
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Hide pictures inside others!
Gammux merges two pictures, a full-sized picture in a smaller thumbnail picture. When websites resize the merged picture, the thumbnail is visible, but when view full the larger one is seen.
After selection the Thumbnail and Full Image above, the result will appear here.
(You can right-click and save the image.)
An explanation of how this work can be found on my blog. The source code available on GitHub.
Made by Carl Mastrangelo.


Welcome to The Literate Listener -- bringing together your favorite
books and your love of podcasts.
To get started finding related podcasts, simply enter the book's title or author above.
To get started finding related podcasts, simply enter the book's title or author above.


| Top |
Functions
Properties
| gboolean | compute-inv-comoving | Read / Write / Construct |
| NcRecomb * | recomb | Read / Write / Construct |
| double | zf | Read / Write / Construct |
Description
This object implements several distances used in cosmology, here we have the following definitions.
$ \newcommand{\RH}{{R_H}} \newcommand{\RHc}{{R^\mathrm{c}_H}} $
The Hubble radius (or scale) is defined as the inverse of the Hubble
function $H(z)$ [nc_hicosmo_H()
],
\begin{equation}\label{eq:def:RHc}
\RH = \frac{c}{H(z)}, \qquad \RH_0 = \frac{c}{H_0},
\end{equation}
where $c$ is the speed of light [ncm_c_c()
], $z$ is the redshift and
$H_0 \equiv H(0)$ is the Hubble parameter [nc_hicosmo_H0()
]. Similarly,
we also define the comoving Hubble radius as
\begin{equation}\label{eq:def:DH}
\RHc(z) = \frac{c}{aH(z)} = \frac{c(1+z)}{a_0H(z)}, \qquad \RHc_0 = \frac{c}{a_0H_0}
\end{equation}
where ${}_0$ subscript means that the function is calculated at the
present time and the redshift $z$ is defined by the expression
$$1 + z = \frac{a_0}{a}.$$
The comoving distance $D_c$ is defined as
\begin{equation}\label{eq:def:dc}
d_c(z) = \RHc_0\int_0^z \frac{dz^\prime}{E (z^\prime)},
\end{equation}
where $E(z)$ is the normalized Hubble function [nc_hicosmo_E()
], i.e.,
\begin{equation}\label{eq:def:Ez}
E(z) \equiv \frac{H(z)}{H_0}.
\end{equation}
In this object we will compute the dimensionless version of the distances, for the comoving distance we define \begin{equation}\label{eq:def:Dc} D_c(z) \equiv \frac{d_c(z)}{\RHc_0}. \end{equation} note, however, that $D_c(z)$ coincides with the proper distance today $r(z) \equiv a_0 d_c(z)$ in unit of the Hubble radius, i.e., $D_c(z) = r(z) / \RH_0$. Therefore, both the comoving distance and the proper distance today can be obtained by multiplying $D_c(z)$ by $\RHc_0$ and $\RH_0$ respectively.
The transverse comoving distance $D_t$ and its derivative with respect to
$z$ are given by
\begin{equation}\label{eq:def:Dt}
D_t(z) = \frac{\sinh\left[\sqrt{\Omega_{k0}}D_c(z)\right]}{\sqrt{\Omega_{k0}}},
\qquad \frac{dD_t}{dz}(z) = \frac{\cosh\left[\sqrt{\Omega_{k0}}D_c(z)\right]}{E(z)},
\end{equation}
where $\Omega_{k0}$ is the value of the curvature today [nc_hicosmo_Omega_k0()
].
Using the definition above we have that the luminosity and angular diameter distances
are respectively:
\begin{equation}\label{eq:def:Dl}
D_l = (1 + z)D_t(z), \qquad D_A = D_t (z) / (1 + z),
\end{equation}
and the distance modulus is given by
\begin{equation}\label{eq:def:dmu}
\delta\mu(z) = 5\log_{10}(D_l(z)) + 25.
\end{equation}
Note that the distance modulus is defined as
$$\mu(z) = 5\log_{10}[\RH_0D_l(z)/(1\,\text{Mpc})] + 25.$$
Thus, this differs from our definition by a factor of
$5\log_{10}[\RH_0/(1\,\text{Mpc})]$, i.e.,
$$\mu(z) = \delta\mu(z) + 5\log_{10}[\RH_0/(1\,\text{Mpc})],$$
where $\text{Mpc}$ is megaparsec [ncm_c_Mpc()
].
We also implement the following distances between $z_1$ and $z_2$: \begin{align}\label{eq:def:Dt12} D_t(z_1, z_2) &= \frac{\sinh\left\{\sqrt{\Omega_{k0}}\left[D_c(z_2)-D_c(z_1)\right]\right\}}{\sqrt{\Omega_{k0}}}, \\ \label{eq:def:DA12} D_A(z_1, z_2) &= D_t (z_1, z_2) / (1 + z_2). \end{align}
Functions
nc_distance_new ()
NcDistance *
nc_distance_new (gdouble zf
);
Creates a new NcDistance object optimized to perform distance calculations
to redshift up to zf
.
nc_distance_ref ()
NcDistance *
nc_distance_ref (NcDistance *dist
);
Increases the reference count of dist
atomically.
nc_distance_require_zf ()
void nc_distance_require_zf (NcDistance *dist
,const gdouble zf
);
Requires the final redshift of at least zf
.
nc_distance_set_recomb ()
void nc_distance_set_recomb (NcDistance *dist
,NcRecomb *recomb
);
This function sets recomb
into dist
.
nc_distance_compute_inv_comoving ()
void nc_distance_compute_inv_comoving (NcDistance *dist
,gboolean cpu_inv_xi
);
Enable/Disable the computation of $z(\xi)$
nc_distance_prepare ()
void nc_distance_prepare (NcDistance *dist
,NcHICosmo *cosmo
);
This function prepares the object dist
using cosmo
,
such that all the available distances functions can be evaluated,
e.g. nc_distance_comoving()
.
nc_distance_prepare_if_needed ()
void nc_distance_prepare_if_needed (NcDistance *dist
,NcHICosmo *cosmo
);
This function prepares the object dist
using cosmo
if it was changed since last preparation.
nc_distance_free ()
void
nc_distance_free (NcDistance *dist
);
Atomically decrements the reference count of dist
by one.
If the reference count drops to 0, all memory allocated by dist
is released.
nc_distance_clear ()
void
nc_distance_clear (NcDistance **dist
);
Atomically decrements the reference count of dist
by one.
If the reference count drops to 0, all memory allocated by dist
is released.
Set pointer to NULL.
nc_distance_hubble ()
gdouble nc_distance_hubble (NcDistance *dist
,NcHICosmo *cosmo
);
Calculate the curvature scale today as defined in Eq $\eqref{eq:def:DH}$ in
units of megaparsec (Mpc) [ncm_c_Mpc()
].
nc_distance_decoupling_redshift ()
gdouble nc_distance_decoupling_redshift (NcDistance *dist
,NcHICosmo *cosmo
);
The decoupling redshift $z_\star$ corresponds to the epoch of the last scattering surface of the cosmic microwave background photons.
This function computes $z_\star$ using [nc_hicosmo_z_lss()
], if cosmo
implements
it, or using Hu & Sugiyama fitting formula Hu (1996)[arXiv],
$$ z_\star = 1048 \left(1 + 1.24 \times 10^{-3} (\Omega_{b0} h^2)^{-0.738}\right) \left(1 + g_1 (\Omega_{m0} h^2)^{g_2}\right),$$
where $\Omega_{b0} h^2$ [nc_hicosmo_Omega_b0h2()
] and $\Omega_{m0} h^2$ [nc_hicosmo_Omega_m0h2()
]
are, respectively, the baryonic and matter density parameters times the square
of the dimensionless Hubble parameter $h$, $H_0 = 100 \, h \, \text{km/s} \, \text{Mpc}^{-1}$.
The parameters $g_1$ and $g_2$ are given by
$$g_1 = \frac{0.0783 (\Omega_{b0} h^2)^{-0.238}}{(1 + 39.5 (\Omega_{b0} h^2)^{0.763})}
\; \text{and} \; g_2 = \frac{0.56}{\left(1 + 21.1 (\Omega_{b0} h^2)^{1.81}\right)}.$$
nc_distance_drag_redshift ()
gdouble nc_distance_drag_redshift (NcDistance *dist
,NcHICosmo *cosmo
);
Drag redshift is the epoch at which baryons were released from photons.
If the dist
object constains a NcRecomb object, it calculates the drag
redshift through the recombination history. Otherwise, it computes $z_d$
using the fitting formula given in Eisenstein & Hu (1998) [arXiv],
$$z_d = \frac{1291 (\Omega_{m0} h^2)^{0.251}}{(1 + 0.659 (\Omega_{m0} h^2)^{0.828})}
\left(1 + b_1 (\Omega_{b0} h^2)^{b_2}\right),$$
where $\Omega_{b0} h^2$ [nc_hicosmo_Omega_b0h2()
] and $\Omega_{m0} h^2$ [nc_hicosmo_Omega_m0h2()
]
are, respectively, the baryonic and matter density parameters times the square
of the dimensionless Hubble parameter $h$, $H_0 = 100 \, h \, \text{km/s} \, \text{Mpc}^{-1}$.
The parameters $b_1$ and $b_2$ are given by
$$b_1 = 0.313 (\Omega_{m0} h^2)^{-0.419} \left(1 + 0.607 (\Omega_{m0} h^2)^{0.674}\right) \;
\text{and} \; b_2 = 0.238 (\Omega_{m0} h^2)^{0.223}.$$
nc_distance_shift_parameter_lss ()
gdouble nc_distance_shift_parameter_lss (NcDistance *dist
,NcHICosmo *cosmo
);
Compute the shift parameter $R(z)$ [nc_distance_shift_parameter()
] at the
decoupling redshift $z_\star$ [nc_distance_decoupling_redshift()
].
nc_distance_comoving_lss ()
gdouble nc_distance_comoving_lss (NcDistance *dist
,NcHICosmo *cosmo
);
Compute the comoving distance $D_c(z)$ [Eq. \eqref{eq:def:Dc}] at the
decoupling redshift $z_\star$ [nc_distance_decoupling_redshift()
].
nc_distance_acoustic_scale ()
gdouble nc_distance_acoustic_scale (NcDistance *dist
,NcHICosmo *cosmo
);
Compute the acoustic scale $l_A (z_\star)$ at $z_\star$ [nc_distance_decoupling_redshift()
],
\begin{equation*}
l_A(z_\star) = \pi \frac{D_t (z_\star)}{r_s (z_\star)},
\end{equation*}
where $D_t(z_\star)$ is the comoving transverse distance [nc_distance_transverse()
]
and $r_s(z_\star)$ is the sound horizon [nc_distance_sound_horizon()
] both computed at $z_\star$.
nc_distance_theta100CMB ()
gdouble nc_distance_theta100CMB (NcDistance *dist
,NcHICosmo *cosmo
);
Compute the $100\theta_\mathrm{CMB}$ angle at $z_\star$ [nc_distance_decoupling_redshift()
],
\begin{equation*}
100\theta_\mathrm{CMB} = 100 \times \frac{r_s (z_\star)}{D_t (z_\star)},
\end{equation*}
where $D_t(z_\star)$ is the comoving transverse distance [nc_distance_transverse()
]
and $r_s(z_\star)$ is the sound horizon [nc_distance_sound_horizon()
] both
both computed at $z_\star$.
nc_distance_angular_diameter_curvature_scale ()
gdouble nc_distance_angular_diameter_curvature_scale (NcDistance *dist
,NcHICosmo *cosmo
);
We define the angular diameter curvature scale $D_a(z_\star)$ as
$$D_a(z_\star) = \frac{E(z_\star)}{1 + z_\star} D_t(z_\star),$$
where $z_\star$ is the decoupling redshift, given by [nc_distance_decoupling_redshift()
],
$E(z_\star)$ is the normalized Hubble function [Eq. $\eqref{eq:def:Ez}$] and
$D_t(z_\star)$ is the transverse comoving distance [Eq. $\eqref{eq:def:Dt}$] both computed at $z_\star$.
nc_distance_r_zd ()
gdouble nc_distance_r_zd (NcDistance *dist
,NcHICosmo *cosmo
);
This function computes the sound horizon [nc_distance_sound_horizon()
]
at the drag redshift [nc_distance_drag_redshift()
].
nc_distance_r_zd_Mpc ()
gdouble nc_distance_r_zd_Mpc (NcDistance *dist
,NcHICosmo *cosmo
);
Similar as nc_distance_r_zd()
, but now in units of $\mathrm{Mpc}$, i.e., $ R_H \times r(z_d)$.
nc_distance_comoving ()
gdouble nc_distance_comoving (NcDistance *dist
,NcHICosmo *cosmo
,const gdouble z
);
Calculate the comoving distance $D_c (z)$ as defined in Eq. $\eqref{eq:def:Dc}$.
nc_distance_transverse ()
gdouble nc_distance_transverse (NcDistance *dist
,NcHICosmo *cosmo
,const gdouble z
);
Compute the transverse comoving distance $D_t (z)$ defined in Eq. $\eqref{eq:def:Dt}$.
nc_distance_dtransverse_dz ()
gdouble nc_distance_dtransverse_dz (NcDistance *dist
,NcHICosmo *cosmo
,const gdouble z
);
Compute the derivative of $D_t(z)$ with respect to $z$ defined in Eq. $\eqref{eq:def:Dt}$.
nc_distance_luminosity ()
gdouble nc_distance_luminosity (NcDistance *dist
,NcHICosmo *cosmo
,const gdouble z
);
Compute the luminosity distance $D_l(z)$ defined in Eq. $\eqref{eq:def:Dl}$.
nc_distance_angular_diameter ()
gdouble nc_distance_angular_diameter (NcDistance *dist
,NcHICosmo *cosmo
,const gdouble z
);
Compute the angular diameter $D_A(z)$, defined in Eq. $\eqref{eq:def:Dl}$.
nc_distance_dmodulus ()
gdouble nc_distance_dmodulus (NcDistance *dist
,NcHICosmo *cosmo
,const gdouble z
);
Compute the distance modulus $\delta\mu(z)$ defined in Eq. $\eqref{eq:def:dmu}$.
nc_distance_luminosity_hef ()
gdouble nc_distance_luminosity_hef (NcDistance *dist
,NcHICosmo *cosmo
,const gdouble z_he
,const gdouble z_cmb
);
Calculate the luminosity distance $D_l$ corrected to our local frame.
nc_distance_dmodulus_hef ()
gdouble nc_distance_dmodulus_hef (NcDistance *dist
,NcHICosmo *cosmo
,const gdouble z_he
,const gdouble z_cmb
);
Calculate the distance modulus [Eq. $\eqref{eq:def:dmu}$] using the frame corrected luminosity
distance [nc_distance_luminosity_hef()
].
nc_distance_shift_parameter ()
gdouble nc_distance_shift_parameter (NcDistance *dist
,NcHICosmo *cosmo
,const gdouble z
);
The shift parameter $R(z)$ is defined as
\begin{equation*}
R(z) = \frac{\sqrt{\Omega_{m0} H_0^2}}{c} (1 + z) D_A(z) = \sqrt{\Omega_{m0}} D_t(z),
\end{equation*}
where $\Omega_{m0}$ is the matter density paremeter [nc_hicosmo_Omega_m0()
],
$D_A(z) = D_{H_0} D_t(z) / (1 + z)$ is the angular diameter distance and
$D_t(z)$ is the tranverse comoving distance [Eq. $\eqref{eq:def:Dt}$].
nc_distance_dilation_scale ()
gdouble nc_distance_dilation_scale (NcDistance *dist
,NcHICosmo *cosmo
,const gdouble z
);
The dilation scale is the spherically averaged distance for perturbations along and
orthogonal to the line of sight,
$$D_V(z) = \left[D_{H_0}^2 D_t(z)^2 \frac{cz}{H(z)} \right]^{1/3},$$
where $D_t(z)$ is the transverse comoving distance [Eq. $\eqref{eq:def:Dt}$], $c$ is the speed of light
[ncm_c_c()
] and $H(z)$ is the Hubble function [nc_hicosmo_H()
].
See Eisenstein et al. (2005) [arXiv].
This function computes the dimensionless dilation scale:
$$D_V^\star(z) = \left[D_t(z)^2 \frac{z}{E(z)} \right]^{1/3} = \frac{D_V(z)}{D_{H_0}},$$
where $E(z)$ is the normalized Hubble function [nc_hicosmo_E2()
].
nc_distance_bao_A_scale ()
gdouble nc_distance_bao_A_scale (NcDistance *dist
,NcHICosmo *cosmo
,const gdouble z
);
This function returns the BAO $A$ parameter.
It is defined as
$$ A \equiv D_V (z) \frac{\sqrt{\Omega_{m0} H_0^2}}{z c},$$
where $\Omega_{m0}$ is the matter density parameter [nc_hicosmo_Omega_m0()
], $c$ is the speed of light [ncm_c_c()
],
$H_0$ is the Hubble parameter [nc_hicosmo_H0()
] and $D_V(z)$ is the dilation scale [nc_distance_dilation_scale()
].
See Section 4.5 from Eisenstein et al. (2005) [arXiv].
nc_distance_sound_horizon ()
gdouble nc_distance_sound_horizon (NcDistance *dist
,NcHICosmo *cosmo
,const gdouble z
);
Compute the sound horizon $r_s$,
\begin{equation}
\theta_s (z) = \int_{z}^\infty \frac{c_s(z^\prime)}{E(z^\prime)} dz^\prime, \quad r_s (z) = \frac{\mathrm{sinn}\left(\sqrt{\Omega_{k0}}\theta_s\right)}{\sqrt{\Omega_{k0}}},
\end{equation}
where $c_s = \sqrt{c^{b\gamma 2}_s(z)}$ is the baryon-photon plasma speed of sound
(see nc_hicosmo_bgp_cs2()
for more details)
and $E(z)$ is the normalized Hubble function [nc_hicosmo_E()
].
nc_distance_dsound_horizon_dz ()
gdouble nc_distance_dsound_horizon_dz (NcDistance *dist
,NcHICosmo *cosmo
,const gdouble z
);
Calculate the sound horizon [nc_distance_sound_horizon()
] derivative with respect to $z$,
$$\frac{d r_s(z)}{dz} = - \frac{c_s(z)}{E(z)}\, ,$$
where $c_s = \sqrt{c^{b\gamma 2}_s(z)}$ is the baryon-photon plasma speed of sound
(see nc_hicosmo_bgp_cs2()
for more details)
and $E(z)$ is the normalized Hubble function [nc_hicosmo_E()
].
nc_distance_bao_r_Dv ()
gdouble nc_distance_bao_r_Dv (NcDistance *dist
,NcHICosmo *cosmo
,const gdouble z
);
This function computes $r(z_d) / D_V(z)$,
where $r(z_d)$ is given by nc_distance_r_zd()
and $D_V(z)$ by nc_distance_dilation_scale()
.
For more information see Percival et al. (2007) [arXiv].
nc_distance_DH_r ()
gdouble nc_distance_DH_r (NcDistance *dist
,NcHICosmo *cosmo
,const gdouble z
);
Computes the ratio between the Hubble (distance) radius and the sound horizon at the drag epoch, $$\frac{R_H}{r_s(z_d)} = \frac{c}{H(z) r_d}.$$
nc_distance_DA_r ()
gdouble nc_distance_DA_r (NcDistance *dist
,NcHICosmo *cosmo
,const gdouble z
);
Computes the ratio between the angular-diameter distance and the sound horizon at the drag epoch, $$\frac{D_A(z)}{c \, r_s(z_d)}.$$
nc_distance_Dt_r ()
gdouble nc_distance_Dt_r (NcDistance *dist
,NcHICosmo *cosmo
,const gdouble z
);
Computes the ratio between the transverse distance and the sound horizon at the drag epoch, $$\frac{D_t(z)}{c \, r_s(z_d)}.$$
nc_distance_comoving_z_to_infinity ()
gdouble nc_distance_comoving_z_to_infinity (NcDistance *dist
,NcHICosmo *cosmo
,const gdouble z
);
Computes the comoving distance from z
to infinity.
nc_distance_transverse_z_to_infinity ()
gdouble nc_distance_transverse_z_to_infinity (NcDistance *dist
,NcHICosmo *cosmo
,const gdouble z
);
Compute the transverse comoving distance $D_t (z)$ (defined in Eq. $\eqref{eq:def:Dt}$)
but from z
to infinity.
nc_distance_transverse_z1_z2 ()
gdouble nc_distance_transverse_z1_z2 (NcDistance *dist
,NcHICosmo *cosmo
,const gdouble z1
,const gdouble z2
);
Compute the transverse comoving distance between $z_1$ and $z_2$, $D_t (z1, z2)$ defined in Eq. $\eqref{eq:def:Dt12}$.
nc_distance_angular_diameter_z1_z2 ()
gdouble nc_distance_angular_diameter_z1_z2 (NcDistance *dist
,NcHICosmo *cosmo
,const gdouble z1
,const gdouble z2
);
Compute the angular diameter $D_A(z_1, z_2)$, defined in Eq. $\eqref{eq:def:DA12}$.
nc_distance_inv_comoving ()
gdouble nc_distance_inv_comoving (NcDistance *dist
,NcHICosmo *cosmo
,gdouble xi
);
Computes the inverse of $\xi(z)$.
nc_distance_cosmic_time ()
gdouble nc_distance_cosmic_time (NcDistance *dist
,NcHICosmo *cosmo
,const gdouble z
);
This function computes the cosmological time, $t(z)$, defined as \begin{equation*} t(z) = \int_z^{\infty} \frac{dx}{(1+x)E(x)}. \end{equation*}
nc_distance_lookback_time ()
gdouble nc_distance_lookback_time (NcDistance *dist
,NcHICosmo *cosmo
,const gdouble z
);
This functions computes the look-back time, $t_{lb}(z)$, defined as
\begin{equation*} t_{lb}(z) = \int_0^{z} \frac{dx}{(1+x)E(x)}. \end{equation*}
nc_distance_conformal_time ()
gdouble nc_distance_conformal_time (NcDistance *dist
,NcHICosmo *cosmo
,const gdouble z
);
This function computes the cosmological conformal time $\eta(z)$ defined as $$ \eta(z) = \int_z^\infty \frac{dz}{E(z)} \, . $$
nc_distance_conformal_lookback_time ()
gdouble nc_distance_conformal_lookback_time (NcDistance *dist
,NcHICosmo *cosmo
,const gdouble z
);
This function computes the conformal look-back time $\eta_{lb}(z)$.
Within the chosen units it becomes the same as the comoving distance [nc_distance_comoving()
],
given in Eq. $\eqref{eq:def:dc}$.
Types and Values
enum NcDistanceComovingMethod
Enumeration to define which method to be applied in order to compute the cosmological distances.
Members
|
performs a numerical evaluation. |
||
|
uses the method defined by the implementation of NcHICosmo. |
Property Details
The “compute-inv-comoving”
property
“compute-inv-comoving” gboolean
Whether to compute the inverse comoving function.
Owner: NcDistance
Flags: Read / Write / Construct
Default value: FALSE
The “recomb”
property
“recomb” NcRecomb *
The recombination object, NcRecomb, used by NcDistance.
Owner: NcDistance
Flags: Read / Write / Construct


Created by Troy Dey And Stephen Erstad
It's....
Disclaimer
What features do we need?
What are our performance requirements
We know this is occurring but why?
Or maybe we don't and our sites run like Windows Vista?
Processes Watchers
Changes while processing trigger more Digest() calls
To avoid infinite loops, an arbitrary limit of 10 cycles is set
//let's assume that scope was dependency injected as the $rootScope
var scope = $rootScope;
scope.name = 'misko';
scope.counter = 0;
expect(scope.counter).toEqual(0);
scope.$watch('name', function(newValue, oldValue) {
scope.counter = scope.counter + 1;
});
expect(scope.counter).toEqual(0);
scope.$digest();
//the listener is always called during the first $digest loop
//after it was registered
expect(scope.counter).toEqual(1);
scope.$digest();
//but now it will not be called unless the value changes
expect(scope.counter).toEqual(1);
scope.name = 'adam';
scope.$digest();
expect(scope.counter).toEqual(2);
Doing recursion that triggers a recursive process...
Too many watches and things get crazy
Testing is often happening outside a cycle
How do these actually work???
Black magic voodoo and magnets???
Believing that Google has your best interests at heart???
makeTemplate(String || DOM)
Transformation happen here
This is not often used
//`tElement` The element where the directive has been declared.
//`tAttrs` Normalized list of attributes declared on this element
// shared between all directive compile functions.
//`transclude` [*DEPRECATED*!]
// A transclude linking function: `function(scope, cloneLinkingFn)`
compile: function compile(tElement, tAttrs, transcludeFn) {
return {
pre: function preLink(scope, iElement, iAttrs, controller) {
... },
post: function postLink(scope, iElement, iAttrs, controller) {
... }
}
// or
// return function postLink( ... ) { ... }
}
What is it?
Is it a made up word?
Isn't this what Thoreau and Emerson where into?
Copying a collection of DOM elements
Putting them into a different part of the DOM
(potentially multiple times)
The copies maintain their link to the parent scope
Digest cycles maybe triggered for this...
//Directive definition
...
tranclude: true,
...
//OR
...
transclude: 'element',
...
Allowing a user to pass in a template to be used in your directive...
Open/Closed Principle
I will be used as the tranclusion template.
I will have access to the parent scope.
This is the template of the directive
... link: function (scope, element, attrs, ctrl, transclude) {
transclude(scope, function (clone) {
clone.after(element);
});
transclude(scope, function (clone) {
clone.after(element);
});
}
ngTransclude and the digest cycle...
Remember you are in the deepest bowels of Ng
Wire up the template to data... Registrar of watches
Happens after cloning
Keeper of the directive logic
Comes in 'pre' and 'post' flavors
DOM transforms only in 'post'
//Defined by the compile function
// OR off of the directive definition object like the compile
link: {
pre: function preLink(scope,
iElement,
iAttrs,
controller,
transcludeFn) {
... },
post: function postLink(...) {
... }
}
//or
//link: function postLink( ... ) { ... }
But this is Ng, so it isn't quite that simple...
To create a tree directive
Example from ng-tree
My Node Template
(function () {
'use strict';
angular.module('rlTree.directives').directive('rlTree', rlTree);
rlTree.$inject = ['$compile', 'treeService', 'treeTemplateFactory'];
function rlTree($compile, treeService, treeTemplateFactory) {
var directive = {
restrict: 'E',
scope: {
tree: '='
},
link: link
};
return directive;
//Post link function, let angular compile and link the directive
//once this is done we can safely modify the contents of our directive
//and start a new compile process
function link(scope, element, attrs, controllers) {
//get the user's html template
var customDisplayTemplate = element.html();
//get our containing template
treeTemplateFactory.setDisplayTemplate(customDisplayTemplate);
//clear the user's template
element.empty();
//Add the actual tree directive to the DOM
element.html(' ');
//patch in the tree data
scope.tree = treeService.createTree(scope.tree);
//Compile the directive we added
$compile(element.contents())(scope);
}
}
})();
(function () {
'use strict';
treeView.$inject = ['$parse', '$compile', 'treeTemplateFactory'];
angular.module('rlTree.directives').directive('treeView', treeView);
function treeView($parse, $compile, treeTemplateFactory) {
return {
restrict: 'E',
require: ['?^treeChildView', 'treeView'],
scope: true,
compile: function($element, attr) {
var tree = $parse(attr.tree);
var treeClick = $parse(attr.treeClick);
return {
//Use the pre link function because we need to create child
//elements as we compile the directive(s)
pre: function(scope, element, attrs) {
//set the html of this directive to our template
element.html(treeTemplateFactory.tree());
//start a new compile cycle on this directive
$compile(element.contents())(scope);
},
//Now all our children have html and have been wired up
//so we can wire ourself up.
post: function (scope, element, attrs, controllers) {
var treeChildViewController = controllers[0];
var treeViewController = controllers[1];
treeViewController.setTree(tree(scope));
treeViewController.setParentController(treeChildViewController);
treeViewController.setTreeClick(treeClick);
scope.tree = treeViewController.getRawTree();
}
};
},
controller: 'treeViewController',
controllerAs: 'treeViewController'
};
}
})();
(function () {
'use strict';
treeChildView.$inject = ['$compile', 'treeTemplateFactory'];
angular.module('rlTree.directives').directive('treeChildView', treeChildView);
function treeChildView($compile, treeTemplateFactory) {
return {
restrict: 'E',
require: ['^treeView', 'treeChildView'],
scope: {
tree: '='
},
compile: function (element) {
return {
//Once again we need to use the prelink becuase we are generating our children
//as we go; which is how we avoid the digest cycle limitations
pre: function(scope, element) {
//set the directive's html to our template
element.html(treeTemplateFactory.treeChild());
//Start a new compile cycle
$compile(element.contents())(scope);
},
//wire up
post: function (scope, element, attrs, controllers) {
var treeViewController = controllers[0];
var treeChildViewController = controllers[1];
treeChildViewController.setParentController(treeViewController);
}
};
},
controller: 'treeChildViewController',
controllerAs: 'treeChildViewController'
}
}
})();
Performance Indicators
Avoiding the Digest Cycle
Streamlining the DOM
ng-repeat track by
Time to initial render
Time to perform operations
Total memory consumption
Avoid excessive reflows
Avoid excessive gc
Digest cycle is expensive
Causes lots of DOM Manipulation
When using recursive includes it runs every time it encounters another include
Limit to ten levels deep
Convert tree structure to flat list

<node>Node template here</node>

<node>Node template here</node>

Another node....</>

<node>Node template here</node>

<node>Node template here</node>

<node>Node template here</node>

Use an actual tree data structure to perform tree operations
Use topological sort to create the display list
Simple approach of regenerating the display list on most changes
Top sort is heavily used and therefore needs to be optimised significantly
How does the consumer communicate with the tree?
How do you avoid broadcasts everywhere?
How do you maintain an isolate scope for you directive?
Provide endpoints for the consumer to pass a callback function that returns a promise.
The consumer performs the operations it needs and resolves the promise with the result structured as specified by the tree.
The tree registers a callback with the promise to perform the operations it needs when it is resolved/rejected.
This allows for very specific and controlled interaction points with the directive.
Disadvantage is that it adds more complexity to the setup of the directive.
It turns out trees are complicated
Pass this function into the tree's on-edit attribute
function editTag (node) {
var editResultDeferred = $q.defer();
if (!node) {
editResultDeferred.reject('node argument is required');
}
else {
var modalInstance = $modal.open({
templateUrl: 'views/templates/tag-modification-modal.tpl.html',
controller: 'TagModificationModalController as modTagVm',
resolve: {
tag: function () {
var tagToModify = node.data;
tagToModify._id = node.id;
tagToModify.parentId = node.parentId;
return tagToModify;
},
configuration: function () {
return tagModificationModalConfigurations.editing;
}
}
});
modalInstance.result.then(function (modifiedTagData) {
alertService.addAlert('success', messageText.savedChangesAlert);
editResultDeferred.resolve(modifiedTagData);
}, function() {
editResultDeferred.reject();
});
}
return editResultDeferred.promise;
}
Execute the on-edit function and register a callback to the returned promise
function edit(node) {
var onEditPromise = treeVm.onEdit({node: node});
onEditPromise.then(function (editEvent) {
var nodeToEdit = treeVm.masterTree.find(editEvent.editedNode.path);
nodeToEdit.remove();
parent.append(treeService.createSubTree(editEvent.editedNode, defaultNode));
treeVm.displayList = treeService.topologicalSort(treeVm.masterTree);
refreshSelectedState(editEvent.editedNode.id);
});
}
Unit testing is hard
Unit testing javasciprt is really hard
Unit testing AngularJS is really really hard
Unit testing Directives impossible....?


Create a new proxy list that will execute the mapped statement when any of the list's method are accessed for the first time.
TLazyLoadList
__construct
(
TMappedStatement $mappedStatement,
mixed $param,
object result $target,
string $propertyName)
-
TMappedStatement
$mappedStatement: statement to be executed to load the data.
-
mixed
$param: parameter value for the statement.
-
object result
$target: object that contains the lazy collection.
-
string
$propertyName: property of the result object to set the loaded collection.
Load the data by executing the mapped statement.
void
fetchListData
()
Try to fetch the data when any of the proxy collection method is called.
boolean
hasMethod
(string $method)
-
string
$method: method name.
Relay the method call to the underlying collection.
void
intercept
(string $method, array $arguments)
-
string
$method: method name.
-
array
$arguments: method parameters.
Create a new instance of a lazy collection.
-
TMappedStatement
$mappedStatement: statement to be executed to load the data.
-
mixed
$param: parameter value for the statement.
-
object result
$target: object that contains the lazy collection.
-
string
$propertyName: property of the result object to set the loaded collection.


R/hazards_influence_curve.R
getHazardInfluenceCurve.Rd
This function computes the hazard-based efficient influence curve at the final estimate of the fluctuated cause-specific hazard functions and evaluates it on the observed data. The influence function is computed on the long-format data but is subsequently summed over all timepoints for each observation and the function returns a new short-form data set with columns added corresponding to the sum over all timepoints of the estimated efficient influence function evaluated at that observation.
getHazardInfluenceCurve( dataList, dat, allJ, ofInterestJ, nJ, uniqtrt, t0, verbose, ... )
| dataList | A list of |
|---|---|
| dat | A |
| allJ | Numeric vector indicating the labels of all causes of failure. |
| ofInterestJ | Numeric vector indicating |
| nJ | The number of unique failure types. |
| uniqtrt | The values of |
| t0 | The timepoint at which |
| verbose | A |
| ... | Other arguments. Not currently used. |
An object of class data.frame
with columns D.jX.zZ
added for each value of X in ofInterestJ
and each value of Z in
uniqtrt
. These are the sum over all timepoints of the estimated
efficient influence function evaluated at that observation.


Pushes a new context message into this stack.
An IDisposable that can be used to clean up the context stack.
Pushes a new context onto this stack. An IDisposable is returned that can be used to clean up this stack. This can be easily combined with the using
keyword to scope the context.
Simple example of using the Push
method with the using
keyword.
[C#]
using(log4net.ThreadContext.Stacks["NDC"].Push("Stack_Message"))
{
log.Warn("This should have an ThreadContext Stack message");
}
ThreadContextStack Class | log4net.Util Namespace


{% set page = { nav: { section: 'Change password', subsection: 'Current', hidePrimary: true }, layout: prototype.current.layoutPath + 'layout.html', secondary: false } %} {% extends page.layout %} {% block primary %}
Your password must have at least 8 characters and contain at least 2 numbers.
{% endblock %}


Know More About Me
Born in the heart of Pakistan, Belonging to the clan of Raajput, the inner warrior
is always hungry for a competition, always up for a challenge. My favorite ones include
food, chess, coding, running
and sleeping as much as I can. Huge Fan of the Google tech and tools.
My maxim being a hardcore Lahori is:
We're Lahories, We're Loud and We're Proud.
My Accomplishments
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et, condimentum quis nulla. Nulla rutrum velit mauris, laoreet fermentum sem convallis sit amet.
Etiam luctus ut ante eu interdum. Praesent ullamcorper ut ligula eu blandit. Morbi luctus tristique
nulla a ornare. Sed malesuada, turpis dignissim commodo sodales, felis urna pellentesque enim,
fermentum congue mauris nulla quis mauris.
⚔
Weapons Of Mass Creation
When I'm Free Floating
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et, condimentum quis nulla. Nulla rutrum velit mauris, laoreet fermentum sem convallis sit amet.
Etiam luctus ut ante eu interdum.
Contact Me
Don't hesitate to ask me, if you have any queries. I will try my best to respond ASAP!