| Line |
Column |
Severity |
Message |
| 167 |
1 |
error
|
Spaces must be used to indent lines; tabs are not allowed |
| 167 |
12 |
error
|
Visibility must be declared on method "initReceivePayment" |
| 167 |
41 |
error
|
Opening brace should be on a new line |
| 168 |
1 |
error
|
Spaces must be used to indent lines; tabs are not allowed |
| 169 |
1 |
error
|
Spaces must be used to indent lines; tabs are not allowed |
| 170 |
1 |
error
|
Spaces must be used to indent lines; tabs are not allowed |
| 171 |
1 |
error
|
Spaces must be used to indent lines; tabs are not allowed |
| 172 |
1 |
error
|
Spaces must be used to indent lines; tabs are not allowed |
| 173 |
1 |
error
|
Spaces must be used to indent lines; tabs are not allowed |
| 174 |
1 |
error
|
Spaces must be used to indent lines; tabs are not allowed |
| 174 |
9 |
error
|
Expected 1 space(s) after IF keyword; 0 found |
| 174 |
43 |
error
|
Expected 1 space(s) after closing parenthesis; found 0 |
| 175 |
1 |
error
|
Spaces must be used to indent lines; tabs are not allowed |
| 175 |
13 |
error
|
Expected 1 space(s) after TRY keyword; 0 found |
| 176 |
1 |
error
|
Spaces must be used to indent lines; tabs are not allowed |
| 177 |
1 |
error
|
Spaces must be used to indent lines; tabs are not allowed |
| 178 |
1 |
error
|
Spaces must be used to indent lines; tabs are not allowed |
| 179 |
1 |
error
|
Spaces must be used to indent lines; tabs are not allowed |
| 179 |
53 |
error
|
No space found after comma in argument list |
| 179 |
58 |
error
|
No space found after comma in argument list |
| 179 |
91 |
error
|
No space found after comma in argument list |
| 179 |
97 |
error
|
No space found after comma in argument list |
| 180 |
1 |
error
|
Spaces must be used to indent lines; tabs are not allowed |
| 180 |
108 |
error
|
No space found after comma in argument list |
| 180 |
110 |
error
|
No space found after comma in argument list |
| 180 |
114 |
error
|
No space found after comma in argument list |
| 181 |
1 |
error
|
Spaces must be used to indent lines; tabs are not allowed |
| 183 |
1 |
error
|
Spaces must be used to indent lines; tabs are not allowed |
| 184 |
1 |
error
|
Spaces must be used to indent lines; tabs are not allowed |
| 184 |
17 |
error
|
Expected 1 space(s) after IF keyword; 0 found |
| 184 |
77 |
error
|
No space found after comma in argument list |
| 184 |
83 |
error
|
Expected 1 space(s) after closing parenthesis; found 0 |
| 185 |
1 |
error
|
Spaces must be used to indent lines; tabs are not allowed |
| 186 |
1 |
error
|
Spaces must be used to indent lines; tabs are not allowed |
| 186 |
17 |
error
|
Expected 1 space after closing brace; 0 found |
| 186 |
18 |
error
|
Expected 1 space(s) after ELSE keyword; 0 found |
| 187 |
1 |
error
|
Spaces must be used to indent lines; tabs are not allowed |
| 188 |
1 |
error
|
Spaces must be used to indent lines; tabs are not allowed |
| 190 |
1 |
error
|
Spaces must be used to indent lines; tabs are not allowed |
| 190 |
62 |
error
|
No space found after comma in argument list |
| 190 |
64 |
error
|
No space found after comma in argument list |
| 190 |
68 |
error
|
No space found after comma in argument list |
| 191 |
1 |
error
|
Spaces must be used to indent lines; tabs are not allowed |
| 191 |
62 |
error
|
No space found after comma in argument list |
| 191 |
64 |
error
|
No space found after comma in argument list |
| 191 |
68 |
error
|
No space found after comma in argument list |
| 193 |
1 |
error
|
Spaces must be used to indent lines; tabs are not allowed |
| 194 |
1 |
error
|
Spaces must be used to indent lines; tabs are not allowed |
| 195 |
1 |
error
|
Spaces must be used to indent lines; tabs are not allowed |
| 196 |
1 |
error
|
Spaces must be used to indent lines; tabs are not allowed |
| 197 |
1 |
error
|
Spaces must be used to indent lines; tabs are not allowed |
| 198 |
1 |
error
|
Spaces must be used to indent lines; tabs are not allowed |
| 199 |
1 |
error
|
Spaces must be used to indent lines; tabs are not allowed |
| 199 |
70 |
error
|
No space found after comma in argument list |
| 199 |
72 |
error
|
No space found after comma in argument list |
| 200 |
1 |
error
|
Spaces must be used to indent lines; tabs are not allowed |
| 201 |
1 |
error
|
Spaces must be used to indent lines; tabs are not allowed |
| 202 |
1 |
error
|
Spaces must be used to indent lines; tabs are not allowed |
| 203 |
1 |
error
|
Spaces must be used to indent lines; tabs are not allowed |
| 204 |
1 |
error
|
Spaces must be used to indent lines; tabs are not allowed |
| 205 |
1 |
error
|
Spaces must be used to indent lines; tabs are not allowed |
| 206 |
1 |
error
|
Spaces must be used to indent lines; tabs are not allowed |
| 207 |
1 |
error
|
Spaces must be used to indent lines; tabs are not allowed |
| 209 |
1 |
error
|
Spaces must be used to indent lines; tabs are not allowed |
| 209 |
17 |
error
|
Expected 1 space(s) after IF keyword; 0 found |
| 209 |
73 |
error
|
Expected 1 space(s) after closing parenthesis; found 0 |
| 210 |
1 |
error
|
Spaces must be used to indent lines; tabs are not allowed |
| 212 |
1 |
error
|
Spaces must be used to indent lines; tabs are not allowed |
| 212 |
166 |
warning
|
Line exceeds 120 characters; contains 166 characters |
| 213 |
1 |
error
|
Spaces must be used to indent lines; tabs are not allowed |
| 213 |
56 |
error
|
No space found after comma in argument list |
| 213 |
62 |
error
|
No space found after comma in argument list |
| 214 |
1 |
error
|
Spaces must be used to indent lines; tabs are not allowed |
| 214 |
60 |
error
|
No space found after comma in argument list |
| 214 |
66 |
error
|
No space found after comma in argument list |
| 215 |
1 |
error
|
Spaces must be used to indent lines; tabs are not allowed |
| 215 |
52 |
error
|
No space found after comma in argument list |
| 216 |
1 |
error
|
Spaces must be used to indent lines; tabs are not allowed |
| 216 |
49 |
error
|
No space found after comma in argument list |
| 217 |
1 |
error
|
Spaces must be used to indent lines; tabs are not allowed |
| 217 |
77 |
error
|
No space found after comma in argument list |
| 217 |
79 |
error
|
No space found after comma in argument list |
| 218 |
1 |
error
|
Spaces must be used to indent lines; tabs are not allowed |
| 218 |
55 |
error
|
No space found after comma in argument list |
| 218 |
106 |
error
|
No space found after comma in argument list |
| 218 |
108 |
error
|
No space found after comma in argument list |
| 219 |
1 |
error
|
Spaces must be used to indent lines; tabs are not allowed |
| 219 |
55 |
error
|
No space found after comma in argument list |
| 219 |
118 |
error
|
No space found after comma in argument list |
| 219 |
120 |
error
|
No space found after comma in argument list |
| 219 |
124 |
error
|
No space found after comma in argument list |
| 219 |
129 |
warning
|
Line exceeds 120 characters; contains 129 characters |
| 220 |
1 |
error
|
Spaces must be used to indent lines; tabs are not allowed |
| 220 |
53 |
error
|
No space found after comma in argument list |
| 220 |
64 |
error
|
No space found after comma in argument list |
| 220 |
66 |
error
|
No space found after comma in argument list |
| 221 |
1 |
error
|
Spaces must be used to indent lines; tabs are not allowed |
| 221 |
57 |
error
|
No space found after comma in argument list |
| 222 |
1 |
error
|
Spaces must be used to indent lines; tabs are not allowed |
| 222 |
55 |
error
|
No space found after comma in argument list |
| 222 |
72 |
error
|
No space found after comma in argument list |
| 222 |
74 |
error
|
No space found after comma in argument list |
| 223 |
1 |
error
|
Spaces must be used to indent lines; tabs are not allowed |
| 223 |
58 |
error
|
No space found after comma in argument list |
| 224 |
1 |
error
|
Spaces must be used to indent lines; tabs are not allowed |
| 224 |
56 |
error
|
No space found after comma in argument list |
| 225 |
1 |
error
|
Spaces must be used to indent lines; tabs are not allowed |
| 225 |
53 |
error
|
No space found after comma in argument list |
| 226 |
1 |
error
|
Spaces must be used to indent lines; tabs are not allowed |
| 226 |
49 |
error
|
No space found after comma in argument list |
| 227 |
1 |
error
|
Spaces must be used to indent lines; tabs are not allowed |
| 227 |
144 |
warning
|
Line exceeds 120 characters; contains 144 characters |
| 228 |
1 |
error
|
Spaces must be used to indent lines; tabs are not allowed |
| 228 |
47 |
error
|
No space found after comma in argument list |
| 229 |
1 |
error
|
Spaces must be used to indent lines; tabs are not allowed |
| 229 |
56 |
error
|
No space found after comma in argument list |
| 230 |
1 |
error
|
Spaces must be used to indent lines; tabs are not allowed |
| 230 |
56 |
error
|
No space found after comma in argument list |
| 231 |
1 |
error
|
Spaces must be used to indent lines; tabs are not allowed |
| 231 |
17 |
error
|
Expected 1 space after closing brace; 0 found |
| 231 |
18 |
error
|
Expected 1 space(s) after ELSE keyword; 0 found |
| 232 |
1 |
error
|
Spaces must be used to indent lines; tabs are not allowed |
| 232 |
89 |
error
|
No space found after comma in argument list |
| 232 |
124 |
error
|
No space found after comma in argument list |
| 232 |
142 |
warning
|
Line exceeds 120 characters; contains 142 characters |
| 233 |
1 |
error
|
Spaces must be used to indent lines; tabs are not allowed |
| 234 |
1 |
error
|
Spaces must be used to indent lines; tabs are not allowed |
| 234 |
13 |
error
|
Expected 1 space after closing brace; 0 found |
| 234 |
14 |
error
|
Expected 1 space(s) after CATCH keyword; 0 found |
| 234 |
32 |
error
|
Expected 1 space(s) after closing parenthesis; found 0 |
| 235 |
1 |
error
|
Spaces must be used to indent lines; tabs are not allowed |
| 236 |
1 |
error
|
Spaces must be used to indent lines; tabs are not allowed |
| 236 |
67 |
error
|
No space found after comma in argument list |
| 236 |
84 |
error
|
No space found after comma in argument list |
| 237 |
1 |
error
|
Spaces must be used to indent lines; tabs are not allowed |
| 238 |
1 |
error
|
Spaces must be used to indent lines; tabs are not allowed |
| 239 |
1 |
error
|
Spaces must be used to indent lines; tabs are not allowed |
| 240 |
1 |
error
|
Spaces must be used to indent lines; tabs are not allowed |
| 241 |
1 |
error
|
Spaces must be used to indent lines; tabs are not allowed |


{% extends "base.html" %} {% block title %}Home{% endblock %} {% block content %}
I've migrated the database to a new data source, which means - Evolutions, Kalos Starter and other missing cards should be included now.
It also added a lot of editions of cards - I'm thinking about redesigning the public set page, because there is so much editions for some sets it doesn't work anymore.
With the changes I've probably introduced a lot of bugs - so if you find anything, I'll be happy to hear about it at<EMAIL_ADDRESS>Thanks
This site is dedicated to catalog every english pokemon tcg card edition ever made, with corresponding card image or scan.
Along with providing the most detailed pokemon card edition database, it easily allows you to keep track of your card collection.
The site provides a searching field, where you can search by pokemon name, number or expansion set.
Say, you found a hidden Azumarill card from steam siege expansion set under your bed and you want to add it to your collection! Easy!
The website searches through the database to find the corresponding Pokemon based on your query.
You'll see something like this:
{% set single_card = find_card_with_code("xy11-77") %} {% include 'widgets/single_card.jinja2' %}On the top you see the card number, name and set it belongs to.
Under the card, you can see the list of editions this card came in.
(Psst... you can click the Pokeball under the card image to switch the card edition images!)
After you create a free user account, you can add this card to your collection!
You can also have multiple collections per account - this might come in handy, for example if you want to keep track of the cards you have for trade, or to catalog the cards per binder!
The site then keeps track of the cards you have, and provides simple charts showing your completionist progress, if you're into that.
Say we have the listed Azumarill in reverse holo edition, and some normal cards too. Here's how a steam siege progress chart might look like.
{% include 'widgets/single_chart.jinja2' %}You can see there are lines for Normal and Reverse holo editions, but also a line for Set cards.
The Set cards line shows the number of cards you have from the set, regardless of the edition.
You can also share a link to your account to post to your friends and show your collection to them!
There's also a detailed view of one expansion set with checkboxes on your public page.
I've come across my own collection of pokemon cards I've collected when I was young - and being a techie and such, I wanted to catalog my collection online. I've looked left and right, and I couldn't find any solid existing solution - either the app missed reverse holos, or it didn't track multiple copies, or it was just super difficult to use.
Adam Capriola
for creating and maintaining the great pkmncards
jab2004 (of Reddit)
for creating and maintaining the amazing checklist of all the english cards
Charlie Hurlocker and Samantha Gaskill
for making a collection and scans of the Fossil 1999-2000 cards
If you have any questions about the site, suggestions for what you really need, any kind of feedback or you just find one of the bugs, you can write to<EMAIL_ADDRESS>and I'll get back to you as soon as possible!
I believe the usage of the content on this website is to be considered a fair use.
The copyright is held by the respective owners of the media.
created and maintained with by gyfis


| Instructions | |||
|---|---|---|---|
| Wait for the applet and sounds to load, then click on the applet area and press the 'S' key or click the mouse on the applet area to start. Enemy ships are pursuing your cruiser. Shoot them down before they get close enough to fire. Your shields will protect you but they can only take so much damage. Once they're gone, so are you. | |||
|
|
|||
| Keyboard Controls | |||
| Key | Description | Mouse | Description |
| S | Start Game | Move | Aim Crosshairs |
| P | Pause Game | Button | Fire |
| M | Mute | ||
| Scoring | |||
| Point values for each type of enemy ship are based on the ship's speed and firepower. See the applet display for a description of each ship type. | |||
| Source and Download | |||
|
Source: TailGunner.java All files: TailGunner.zip (78KB) |


CHASING AMY A film review by Marty Mapes Copyright 1997 Marty Mapes
*** (out of 4) There is something about Kevin Smith's style that I just don't like. I enjoyed Chasing Amy while I was watching it, but afterwards I was glad it was over. In that sense it was like Pulp Fiction. Both are fun to watch, but I was relieved to come out of the theater and see that reality isn't like what was on screen.
To chase Amy is to regret having ruined your once-in-a-lifetime relationship, as Holden (Ben Affleck) learns the hard way.
Holden lives with Banky (Jason Lee), and the two of them collaborate on the comic book "Chronic and Bluntman." After a comic book convention, they join two friends, Hooper and Alyssa (Dwight Ewell and Joey Lauren Adams) for drinks.
While Banky and Hooper argue over the sexual orientation of the characters in Archie comics, Holden and Alyssa get to know each other.
Alyssa invites Holden to a night club the next day and they hit it off well. Holden is just starting to see the beginnings of a relationship when Alyssa runs into her girlfriend and starts making out with her. Naturally, Holden is disappointed and shocked. Later, while Alyssa and Banky compare cunnilingus-related injuries, Holden moves from disappointment to disgust and despair.
A few days later, Alyssa shows up to make amends with Holden. She doesn't want their friendship to end. They become very good friends, but Holden still wants more.
It turns out that Alyssa loves Holden enough to allow the relationship to grow beyond friendship and all is well until Holden learns of her sexual history with men.  There is much soul-searching by all of the characters before the movie reaches its logical conclusion.
The story is a refreshing twist on the standard romantic comedy, but something about Kevin Smith's style leaves me feeling a little dirty.
First of all, this movie (like Clerks, his debut) is very sex-centered. His characters talk a lot about sex, which makes for interesting, honest, and funny dialog, but the sum of the movie, then, feels -- well, dirty. It seems that these characters live in a mystical land far away from this reality -- another world where everybody has sex with ten different partners by high school graduation, then talks about it at length with strangers and acquaintances.
Also, this movie has a very heterosexual male point of view. One might say it borders on prejudice. Holden is okay with Alyssa's promiscuity as a lesbian, but he can't accept the idea of her promiscuity with men. Also, Alyssa's homosexuality is "cured" when she meets the right man. The movie does handle this issue sensitively and carefully -- it is within Alyssa's character to choose Holden -- but the whole idea seems heterosexist.  Imagine the gay friend falling hopelessly in love with the straight friend. The straight friend is not likely to be swayed, no matter how persistent the gay friend is. In fact, the awkwardness of the situation might ruin their friendship. But we accept the situation when a charming heterosexual man wins over a sexually confused lesbian.
Still, Chasing Amy has good characters, good dialog, and a good screenplay.
Alyssa is a well developed character. She is not merely the object of another character's desire, as is too often the case in romantic comedies. Hooper is a minor comic character but his wisdom adds a rational voice to the movie.  (This is another instance of Smith the screenwriter walking a fine line between creating interesting autonomous characters and furthering stereotypes.)
Banky and Holden share some good dialog. They disagree enough that their discussions are always interesting, exposing all sorts of different layers within different topics. When Holden and Alyssa talk, they reveal their hearts to each other with a bare honesty uncommon in most movies.
The story is simple enough, but Holden introduces an interesting twist near the end which itself would have made for a clever ending. Smith carries the story just a little further to explore the consequences of that twist.
As repellent as I sometimes find Kevin Smith, I must admit that he is a talented filmmaker. Chasing Amy appears to have been made on a shoestring (albeit a bigger one than Clerks). Smith realizes that he doesn't need special effects, slick lighting, or expensive sets to make a good move. A good script, a few friends, and a promise to thank all of his backers in the credits is all he needs.
Check out more current movie reviews at http://www.indra.com/~mmapes
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


CrimPapers
Articles published on 24 August 2020
On 24 August 2020, 7 new articles were published in 5 journals.
A Police Partnership Targeting Truancy: Study Protocol For A Cluster Randomised Controlled Trial
The Nuanced Relationship Between Adverse Childhood Experiences and Recidivism Risk Scores Among Women Leaving Jail: A Preliminary Exploration by Vanessa Schick,
isabel Roth,
andrea Link,
alycia Welch
Prevalence of Intimate Partner Violence and Association With Wealth in Myanmar
The Changing Perceptions of St. Lucian Policing: How St. Lucian Police Officers View Contemporary Policing by Perry Stanislas
Attitudinal Differences Between Female and Male Police Cadets/officers in Taiwan: the Nexus Between Gender, Immigration, and Crime by Kyler R. Nielson, Jurg Gerber, Wen-Chih Huang
Guest Editors’ Introduction: Violence Against Women—reflecting on 25 Years of the Violence Against Women Act and Directions For the Future by Angela Moore, Angela Gover
A Review of the Effects of the Violence Against Women Act on Law Enforcement by Wesley G. Jennings, Ráchael A. Powers, Nicholas M. Perez


on
eink calendar: Part 1
UPDATE 2020, Oct 16 I stopped trying to modify my kobo ereader a long while back. When I started the project, I was enjoy a ready access to nearby libraries and the joys of physical books. I’ve come to find that there is room for the Kobo in my library, especially for the heavier books like Les Miserable and The Count of Monte Cristo that are just too big to carry around. I imagine I’ll return to this project one-day when I get a new ereader, but that probably won’t be for a long, long time. I’m more likely to substitute the ereader for a dedicated eink display.
When I first started using org-mode on Emacs, the agenda option seemed like too much hassle. There was too much programming involved, too many shortcuts to remember (like anything Emacs), and it just wasn’t pretty. But mid-2019, most other methods to become organized just didn’t click, and org-agenda seemed ever-more appealing. With a little bit of effort (or in my case, copy-paste) in the configuration, I’ve managed to get something that works. What I need now is someway to get a device to give me daily notifications when something is coming up. That’s when I realized that my eink Kobo reader could be it!
I love my Kobo e-reader, but its not as useful as the newer versions with a direct link to the library. I’ve gone back to regular old paper and pen. Besides, my need to get organized takes priority.
Here’s the rough plan: with a bit of effort, the Kobo can be reprogrammed to display my org-agenda, along with little snippets of extra information (weather for instance) using Python. My Emacs will generate an iCal file. This file will be uploaded to my Kobo reader through the internet for the Python program to process and generate an eink display of my calendar.
However, here’s the main challenge to getting this project working; I can’t seem to hack into the Kobo e-reader. I’ve come across resources, and can detect my Kobo on Linux. But something is preventing that final step…Once I hack into the reader, it’s another thing to understand the operating system to get a python script working. I suspect I’ll have to get a raspberry pi involved at some step, or drop the Kobo for a dedicated eink display hooked directly to my raspberry pi.
The iCal files can be read using python package iCalendar. The details can then be easily extracted, requiring only formatting to get working. Setting up the python program to generate a display should not be difficult. There is still a good deal of information to read to ensure I understand what is necessary to influence the display of an eink display, and what is possible.
To get my Emacs to generate a new iCal file whenever modifications are made, I’m referring to this site. I’m hesitant to post details on my current approach just yet as I suspect it will change. Using a file sharing service (ssh, sync-thing, etc.), the iCal file will be shared to the Kobo. However, if the Kobo OS is too foreign, the Raspberry Pi will be used to process the iCal file, and dictate to the Kobo how to display the calendar. The best case scenario is that the Kobo is able to run python and have access to a file sharing service.


Before Change
original_shape = x_data.shape
if x.volumetric:
x_data = skimage.transform.resize(x_data, (original_shape[0], 256, 256), order=0, mode="edge")
distance = scipy.ndimage.distance_transform_edt(x_data)
distance = mahotas.stretch(distance)
After Change
factor = self.downsample.value
if factor > 1:
if x.volumetric:
factors = (1, factor, factor)
else:
factors = (factor, factor)
x_data = skimage.transform.downscale_local_mean(
x_data,
factors
)
threshold = skimage.filters.threshold_otsu(x_data)
x_data = x_data > threshold


Flowering is an important life history trait of flowering plants. It has been mainly analyzed with respect to flowering onset and duration of flowering. This tools provide some functions to compute the temporal distribution of an flowering individual related to other population members. fCV() measures the temporal variation in flowering. RIind() measures the rank order of flowering for individual plants within a population. SI(), SI2(), SI3(), and SI4() calculate flowering synchrony with different methods.
| Version: | 1.0 |
| Published: | 2015-01-28 |
| Author: | Xie WANG |
| Maintainer: | Xie WANG <wangxiechangde at hotmail.com> |
| License: | GPL-2 | GPL-3 [expanded from: GPL (≥ 1.0)] |
| NeedsCompilation: | no |
| CRAN checks: | flower results |
| Reference manual: | flower.pdf |
| Package source: | flower_1.0.tar.gz |
| Windows binaries: | r-devel: flower_1.0.zip, r-release: flower_1.0.zip, r-oldrel: flower_1.0.zip |
| OS X binaries: | r-release: flower_1.0.tgz, r-oldrel: flower_1.0.tgz |
Please use the canonical form https://CRAN.R-project.org/package=flower to link to this page.


hstpolpoints -- Reduce linear polarization data for HST instruments for a set of aperturesUSAGE hstpolpoints imalis errlis instpoltab pointab iterej sigsky outtab
- imalis = "" [list of file names]
- The list of input sky-subtracted images to be reduced. Upto 64 images can be input. They must all be of the same dimensions and are assumed to be aligned.
- errlis = "" [list of file names]
- The list of input error files corresponding to the sky-subtracted images. They must be of the same dimensions and the same as the input sky-subtracted images.
- instpoltab = "" [table file name]
- Name of STSDAS table file giving the parameters for polarization determination for the instrument corresponding to the input images. The table lists the polarizer filter name, the polarizer angle, the transmission for the components parallel and perpendicular to the polarizer axis, the transmission of the s and p rays (parallel and perpendicular to the pick-off mirror surface for the WFPC2 case) and the retardation of the s ray relative to the p ray, the instrumental polarization and its instrumental position angle.
- pointab = "" [table file name]
- Name of the STSDAS table detailing the input apertures for summing flux and sky. The table lists the aperture name, X and Y pixel centre, radius of object aperture, gap radius between object circle and sky annulus and width of sky annulus.
- iterej = "" [integer]
- Number of iterations for sigma clipping of mean sky.
- sigsky = "" [real]
- Factor times rms on mean for rejecting points from inclusion in the mean for the sky aperture.
- outtab = "" [name]
- Name of the STSDAS table for the output results. A 13 column table is produced listing the aperture names, X and Y positions (from the input pointab table) together with the normalised Stokes I, Q and U parameters and errors, the linear polarization and position angle and errors.
This task is a tool for performing aperture polarimetry for data from those HST instruments with imaging polarizer facilities (currently FOC, WFPC2 and NICMOS and in future ACS). A non-HST instrument can also be handled - called 'SPECIAL'. The error frames are required to produce output error files and should contain all sources of error (photon noise, systematics (e.g. flat fielding errors) and read-out noise).All instrument specific parameters are picked up from the header and the telescope rotation angle is read from the PA_V3 or ORIENTAT descriptor (see below for details and also examples). The polarizer and or colour filter name in the header is matched with values found in the instpoltab table file and these are used to set the instrument specific polarization parameters required to compute the Stokes parameter and linear polarization data. The correction for polarizer transmission and pick-off mirror induced polarization follows closely the treatment for WFPC2 by Biretta and McMaster (WFPC2 ISR 97-11). The instrumental polarization is included for effects that are not collected by these physically based parameters. If the values of the polarizer efficiences for calculating each Stokes parameter are equal for all input images (such as by specifying the same polarizer orientation and instrument position angle), then no calculation of polarization is possible. The task exits with an error in this case.
All errors are computed by Gaussian error propagation. To correct for the bias in linear polarization values which occurs when the Stokes parameter errors are large and the determination of linear polarization is no longer Gaussian error dominated, the method advocated by Wardle & Kronberg (ApJ, 194, 249, 1974) is employed, using the solution of the Rice distribution (see also Simmons & Stewart, A&A, 142, 10, 1985 for a discussion). Tests with synthetic data show that this correction does an adequate job to pol/sigma(pol) of about 2. Below that value it is best to use Monte Carlo methods which are not directly dealt with here. The method of computing the errors on the polarization position angle depends on the polarization signal-to-noise (i.e. pol/sigma(pol)). If pol/sigma(pol) is greater than 8 then the simple method (sigma(theta) = 28.65*sigma(pol)/pol) is employed (Serkowski, Adv. in Astron. & Astrophys. 1, 289, 1962); if pol/sigma(pol) is less than 8 then the distribution function of the position angle errors is integrated to derive the 1 sigma error (see Naghizadeh-Khouei & Clarke, A&A, 274, 968, 1993). Of course if the input error frames are all zero, no correction for bias is performed and all output errors are set to zero.
The parameters of the apertures for performing polarimetry are read from an input STSDAS table. Circular apertures are specified by an X and Y centre (currently only pixel coordinates are supported), the radius of the circle over which to sum counts for the object, the distance between the outer radius of the object circle and the inner radius of the sky annulus and the width of the sky annulus. A name for identification purposes can be given for each aperture.
The mean value of the sky/background per pixel is calculated and subtracted from the object signal. The mean sky can be determined by sigma clip iterations where values differing by greater than SIGSKY*rms on the mean are excluded at each iteration.
The following header keywords are required in order that the instrumental polarization parameters can be matched against the instrument table files:
for FOC - INSTRUME, FILTNAM1, FILTNAM2, ORIENTAT for NICMOS - INSTRUME, FILTER, ORIENTAT for WFPC2 - INSTRUME, FILTNAM1, FILTNAM2, DETECTOR, PA_V3 for ACS - INSTRUME, FILTNAM1, FILTNAM2, ORIENTAT for SPECIAL - INSTRUME, FILTER, POLANG, ORIENTAT
1. To reduce a set of FOC aperture polarimetry data:cl> hstpolpoints<EMAIL_ADDRESS><EMAIL_ADDRESS>instpoltab="foc-pol-filt-001.tab" pointab="focap1.tab" nrej=3 sigsky=2.5 outtab="focapol1"
FOC polarization data usually consist of a set of three images taken at the three rotation angles of the polarizer of 0, 60 and 120 degrees at approximately the same ORIENTAT. See the HST Data Handbook, Section 8-7).
2. To reduce a set of NICMOS polarimetry images in a set of apertures:
cl> hstpolpoints<EMAIL_ADDRESS><EMAIL_ADDRESS>instpoltab="nicmos-pol-filt-001.tab" pointab="nicap1.tab" nrej=7 sigsky=3.0 outtab="nicpolap.tab"
NICMOS polarization data usually consist of a set of three images taken at the three rotation angles of the polarizer which are close to 0, 120 and 240 degrees (depending on the polarizer used short (S) or long wavelength (L)) at a similar ORIENTAT. See the HST Data Handbook Section 18-12 and Hines, D. C., 1998, NICMOS and the VLT Workshop proceedings, eds. Freduling, W. & Hook, R., p. 63.
3. To reduce the aperture polarization for a set of WFPC2 polarimetry images:
cl> hstpolpoints<EMAIL_ADDRESS><EMAIL_ADDRESS>instpoltab="wfpc2-pol-filt-001.tab" pointab="wfpcap2" nrej=1 sigsky=2.7 outtab="wfpc_1.tab"
WFPC2 polarization data can consist of three or four images taken with three or four rotation angles of the polarizer quad filter at a given PA_V3, or three or more images taken on the same chip at differing values of PA_V3 and covering a range of rotation of at least 90 degrees. See the HST Data Handbook Section 28-16 and Biretta, J. & McMaster, M., WFPC2 Instrument Science Report 97-11. The header parameters FILTNAM1 and FILTNAM2 are translated to provide the polarizer position angle in conjunction with the chip number (for POLQ only).
4. To reduce the aperture polarization for a set of ACS polarimetry images:
cl> hstpolpoints<EMAIL_ADDRESS><EMAIL_ADDRESS>instpoltab="acs-pol-hrc-v-filt-001.dat" pointab="specaper.tab" nrej=1 sigsky=3.0 outtab="acs_aper.tab"
ACS polarization data usually consist of a set of three images taken at the three rotation angles of the polarizer, which are 0, 60 and 120 degrees, for a given camera (WFC or HRC), polarizing filter (POLV or POLUV) and colour filter. See the ACS Instrument Handbook, Chapter 5 for details.
5. To reduce a set of polarimetry images originating from a non-HST instrument and determine the polarization for a set of sources:
cl> hstpolpoints<EMAIL_ADDRESS><EMAIL_ADDRESS>instpoltab="special-pol-001" pointab="specaper.tab" nrej=0 sigsky=0.0 outtab="specpol_2"
If the parameter INSTRUME is set to SPECIAL then non-HST imaging polarimetry data can be reduced. The filter name given by the header parameter FILTER must match the name in the instrument table file. The polarizer angle is indicated by the header parameter POLANG. The instrument rotation is indicated by the ORIENTAT parameter which may need to be translated into the instrumental system.
The STSDAS table file is a nine column file with the following columns: Name of colour/polarizing filter Position angle of polarizer filter Normalised transmission parallel to polarizer axis Normalised transmission perpendicular to polarizer axis Reflectance of mirror E-vector parallel to surface (s wave) Reflectance of mirror E-vector normal to surface (p wave) Retardance (deg.) of s wave relative to p wave Instrumental polarization (%) Position angle (deg.) of instrumental polarization (in instrument frame)with the following column names and format: FILTER CH*16 POLANG R F6.2 TRANSPAR R E10.4 TRANSPER R E10.4 REFLECTRS R F6.4 REFLECTRP R F6.4 RETARDPHI R F8.4 INSTPOL R F6.2 INSTPA R F6.2
Thus table files for different instruments can be produced for use with this routine.
The STSDAS table file defining the apertures for which the polarization is to be determined has the following columns: Identification name for aperture X centre of aperture (pixels) Y centre of aperture (pixels) Radius of aperture over which to sum object counts (pixels) Width of the gap between the object circle and the annulus for determining background counts (pixels) Width of the annulus for measuring the mean background (pixels)with the following column names and format (the latter mandatory only for OBJECT_NAME): OBJECT_NAME CH*16 POS_X R F7.2 POS_Y R F7.2 RADIUS R F7.2 GAP R F7.2 ANNULUS R F7.2
The output STSDAS table file listing the derived Stokes parameters, linear polarization and position angle and all propagated errors has the following columns: Identification name for aperture X centre of aperture (pixels) Y centre of aperture (pixels) Stokes I (ADU) Stokes I error (ADU) Normalised Stokes Q Error on normalised Stokes Q Normalised Stokes U Error on normalised Stokes U Linear polarization (%) Error on linear polarization (%) Polarization position angle (degrees) Error on polarization position angle (degrees).The first three columns are simply copied from the input aperture definition table.
 R F8.4 Lin._Poln.Error R F8.4 Poln._PA R F8.4 Poln._PA_Error R F8.4
Some care should be taken if ORIENTAT is much different between the input images and there is substantial instrumental polarization, since the position angle of instrumental polarization is (probably) fixed in the reference frame of the instrument. This situation is not correctly handled.
hstpolima, hstpolsim, polimodel


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Hurricane Streets * * * (out of * * * * )
Directed by Morgan J. Freeman. Cast: Brendan Sexton III, Isidra Vega, Shawn Elliott, David Roland Frank, L.M. "Kit" Carson, Edie Falco, Jose Zuniga, Lynn Cohen, Heather Matarazzo. 1998 - 89 minutes. Rated R (for violence and profanity). Reviewed November 29, 1998.
"Hurricane Streets," which won an unprecedented three 1997 Sundance Film Festival awards, for Best Director, Best Cinematography, and the Audience Award, is one of the most accurate films about teenagers I've seen in a while.
Marcus (Brendan Sexton III), who lives in the East Village in NYC with his grandmother, is about to turn fifteen, and spends his day stealing petty things from stores with his friends. His mother is in prison, and he hopes that for his birthday, his father will send him a plane ticket so he can visit him in New Mexico. While selling some CD's that he has stolen to a bunch of young kids, he meets a 14-year-old girl, Melena (Isidra Vega), and they quickly become friends, much to the disapproval of her abusive father. To his surprise, Marcus finally does get the ticket to go to New Mexico, but his hopes begin to diminish when he discovers some secrets that his mother has been hiding from him.
Although the story is occasionally a little bleak, at its center is the sweet, gentle love story between Marcus and Melena, played marvelously by Brendan Sexton III (1996's brilliant, "Welcome to the Dollhouse) and newcomer Isidra Vega. To prove that the screenplay is so well-written and unpredictable, director Morgan J. Freeman (not to be confused with the actor) does not include exploitation and sex to their relationship, which is what a typical film would have done, but relies more on the realism of being 15 and in love.
One of the pleasures of, "Hurricane Streets," is watching all of the characters interact with each other, which is basically what the film is about. There is no particular storyline, because it would have put a damper on the effectiveness of the relationships. Watching it, I was surprised by how completely uncliched the film was. Since Marcus is a teenage thief, the banal thing to do would to simply make him act tough and uncaring. Instead, Marcus is a kid with a pretty good head on his shoulders. He does not do drugs, is not promiscuous, but does have the insecurities that teens his age have, and has a very good relationship with his grandmother, who owns a bar.
"Hurricane Streets," did not, or rarely, step wrong until the very ending, which abruptly ends while in midstream, as if the final ten minutes had never been shot. A great many twists and revelations comes during the climax, but they are not solved, and I cared so much for the two main characters of Marcus and Melena that I desperately wanted to see what would happen next. Maybe this is just a sign of an exceptional film, since I got so involved in it, but the conclusion could have been better.
What came before the end, however, was masterfully written and memorably performed. An added bonus was briefly seeing Heather Matarazzo (also of, "Welcome to the Dollhouse), one of the best young actresses working today, as Vega's friend, Ashley. "Hurricane Streets," is a gritty, highly impressive directing debut by Morgan J. Freeman, and I greatly look forward to seeing his next film called, "Desert Blue," which is due out in 1999, and stars Sexton III, Christina Ricci, Casey Affleck, Sara Gilbert, among others. To get so many talents in only your second picture is a sign of a talented director.
- Copyright 1999 by Dustin Putman Http://hometown.aol.com/FilmFan16/index.html
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Jun 28, 2013 Funnyman Stephen Colbert has had a special relationship with Pipeline safety: Canada lags U S. on making data public. video; Major Jul 26, 2013 How can you not watch Stephen Colbert's take on Weiner-gate? Answer: By living in Canada Comedy Network blocks it's videos here not
Feb 12, 2013 Stephen Colberts Thoughts on a Canadian Pope. Alert icon. You need Adobe Flash Player. to watch this video Download it from Adobe Feb 17, 2010 Comedy Central's Stephen Colbert arrived to a 'polite mob' to tape two shows in. Raw Video: Colbert Meets 'Polite. Mob' in Canada.
Watch the latest full episodes of The Colbert Report in Canada for free at CTV ca Join host Stephen Colbert for the most patriotically. American show on television 158 videos; 194,126 views. The Colbert Report: Recap - Week of 10/21/13. Canadian Mounties stop a terror plot, Eric Schmidt looks to the digital future,
Jul 11, 2013. Stats have been disabled for this video Report Published on. Jul 11, 2013. Canada has a campaign to make Stephen. Colbert their King - But It stars political humorist Stephen Colbert, a former correspondent for The Daily. in front of a green screen and asked fans to complete the video, Colbert He has criticized the bird for migrating to Canada, and has attempted to lure him
Sep 19, 2013. Popular U S political satirist Stephen Colbert quoted one of my postings last night on his comedy show It's quite the honour (as we spell it in Canada). Colbert. Here's the VIDEO clip of. part of the Colbert segment It's pretty
A documentary about wounded veterans that Roger championed gets a screening at the Rehabilitation Institute of Chicago and screenings in New York and Los Angeles…
Feb 4, 2010 A former CIA operative admits to lying about the effectiveness of waterboarding, and The Beaver changes its name to Canada's History Related. Videos Stephen opposes gays in the military. and learns about his white
Aug 7, 2013. Electro stars Daft. Punk infuriated U. S. TV host Stephen Colbert by axing a. Colbert: Cardinal Ouellet too Canadian to be. pope · Stephen Colbert pokes fun at. at the MTV Video Music Awards in New York City on August 25
Oct 22, 2013 On last night's Colbert Report, Stephen welcomed Win and Will Butler of the Reflektors -- AKA the Steely Dan of Canada -- who admit that that other popular. The 5 Best Videos Of The Week · Read Lou Reed's Obituary,
May 1, 2013 Stephen Colbert discusses one. of his favorite topics LOOP HOLE http://www. colbertnation com/the-colbert-report-videos/81003/. For example, in January, 2007 Colbert was disrespected by a Canadian Jr League Hockey
Aug 23, 2013. I remember the handoffs between Jon Stewart. and Stephen Colbert, which got. Because Comedy Central isn't available. in Canada, there's nothing to is available through cable companies' video on demand systems.


Highest-energy light from a gamma-ray burst ever
Previously unseen component of extreme stellar explosions
| Source: | George Washington University |
| Summary: | Researchers have observed a gamma-ray burst with an afterglow that featured the highest energy photons — a trillion times more energetic than visible light — ever detected in a burst. |
Gamma-ray bursts are the most powerful explosions in the cosmos. These explosive events last a fraction of a second to several minutes and emit the same amount of gamma rays as all the stars in the universe combined. Such extreme amounts of energy can only be released during catastrophic events like the death of a very massive star, or the merging of two compact stars, and are accompanied by an afterglow of light over a broad range of energies that fades with time.
It has been decades since the discovery of the first gamma-ray burst, yet some of their fundamental traits remain unclear. An international team of researchers, including two astrophysicists from the George Washington University, Chryssa Kouveliotou and Alexander van der Horst, now has taken the next step in understanding the physical processes at work during these events with a recent discovery published today in the journal Nature.
The researchers observed a gamma-ray burst with an afterglow that featured the highest energy photons — a trillion times more energetic than visible light — ever detected in a burst.
"This very high energy emission had been previously predicted in theoretical studies but never before directly observed," Dr. van der Horst, an assistant professor of physics at GW, said.
"After over 45 years of observing GRBs, we just confirmed the existence of yet another unknown component in their afterglows, which increases the gamma-ray burst overall energy budget dramatically," Dr. Kouveliotou, a professor of physics at GW, added.
On Jan. 14, 2019, researchers detected a burst labeled GRB 190114C. The discovery triggered an extensive campaign of observations across the electromagnetic spectrum using more than 20 observatories and instruments around the world. This collaborative effort allowed an international team to gather an unprecedented level of information about GRB 190114C, capturing the evolution of the gamma-ray burst afterglow emission across 17 orders of magnitude in energy.
As part of the joint efforts, Dr. van der Horst and Dr. Kouveliotou were part of a subteam responsible for tracking the emission of radio waves in the afterglow of GRB 190114C. The team used the new MeerKAT radio telescope in South Africa to record the emission, which is at the opposite end of the spectrum compared to very high energy gamma rays.
"MeerKAT is a new radio observatory with very good sensitivity," Dr. van der Horst said. "It is a great facility to observe this kind of event. Our team is carrying out a multi-year program to observe many more gamma-ray bursts and other cosmic explosions in the coming years."
GRB 190114C is unique in that researchers were able to observe photons with teraelectronvolt (TeV) energies for the first time in its afterglow emission. Using the MAGIC Collaboration telescopes in La Palma, Spain, researchers noticed this emission of TeV photons was 100 times more intense than the brightest known steady source at TeV energies, the Crab Nebula. As expected though, this very high energy emission quickly faded in about half an hour after the event onset, while the afterglow emission in other parts of the spectrum persisted for much longer.
The researchers noted that the shape of the observed spectrum of afterglow light was indicative of an emission process called inverse Compton emission. This event supports the possibility that inverse Compton emission is commonly produced in gamma-ray bursts.
"MAGIC, the TeV photon detector in La Palma, Spain, opened up a new window for research on gamma-ray bursts," Dr. Kouveliotou said. "We are looking forward to understanding their physics and true energy release in gamma-ray bursts with more detections in the future."
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Journal Reference:
- V. A. Acciari et al. Observation of inverse Compton emission from a long γ-ray burst. Nature, 2019 DOI: 10.1038/s41586-019-1754-6
Cite This Page:
| MLA | George Washington University. "Highest-energy light from a gamma-ray burst ever: Previously unseen component of extreme stellar explosions." ScienceDaily. ScienceDaily, 20 November 2019. <www.sciencedaily.com/releases/2019/11/191120131300.htm>. |
| APA | George Washington University. (2019, November 20). Highest-energy light from a gamma-ray burst ever: Previously unseen component of extreme stellar explosions. ScienceDaily. Retrieved November 21, 2019 from www.sciencedaily.com/releases/2019/11/191120131300.htm |
| Chicago | George Washington University. "Highest-energy light from a gamma-ray burst ever: Previously unseen component of extreme stellar explosions." ScienceDaily. www.sciencedaily.com/releases/2019/11/191120131300.htm (accessed November 21, 2019). |


{% extends "archiver/base.html" %} {% block title %}Questions & Answers{% endblock %} {% block content %} {% load humanize %}
...we're working on opening up the community features. Track our progress on GitHub


model.js |
|
|---|---|
|
This file contains two model mixins, Duckbone.AssociableModel, and Duckbone.ModelHelpers. Typically both will be mixed into an application’s base model class. Adding them directly to Backbone.Model will also work, but is perhaps less tidy. Duckbone.AssociableModelBackbone deliberately provides the flexibility for the developer to manage associated models and collections in any way that makes sense for the application. This flexibility is the cause of much confusion among beginning developers, and so Duckbone provides this straightforward framework for managing Rails-like associations. The simple philosphy behind AssociableModel is that nested objects within JSON data
(or model attributes) are transformed into fully fledged Backbone Models or Collections.
These exists as properties on the original model, in an analagous way to
In addition, further changes to those nested attributes result in changes to the associations. But this relationship is a one way street. Once the attribute data is used to create associated models, it is removed from the attributes. So changes to associated models are never reflected in the attributes of the original model. There is a clear logic behind this approach:
UsageAssociableModel can be mixed into all models and collections that require it, or extend Backbone.Model and Backbone.Collection themselves if desired. The In almost all cases, these functions will be called from the model’s initialize method. SyntaxSeveral associations can be created in each call to hasOne or hasMany. A single object is passed. Each key in the object defines the association name. In a call to If a reciprocal link is desired on the association, then the For example:
In use:
Has One BehaviorWhen a hasOne association is initially created, the following occurs:
When the attribute used to create the association is set again, then the association setter is called instead. When the setter function is called, the following occurs:
If a belongsTo relationship is specified:
Has Many BehaviorWhen a hasMany association is initially created:
When the original attribute is set again (ie from a call to
If a belongsTo relationship is specified:
Special CasesIf the desired association should have a different name from that naturally occuring in the JSON,
then the model’s In the event that the developer absolutely must package associations back together as JSON to save
to the server, then the model’s |
(function(){
Duckbone.AssociableModel = { |
Mixin |
|
property isAssociableModelIndicates a class with AssociableModel included |
isAssociableModel: true, |
function includedCreates a new set function that manages the movement of attributes to associated models. |
included: function() {
if (!this.setWithoutAssociations) {
this.setWithoutAssociations = this.set
this.set = setWithAssociations;
}
}, |
Association Methods |
|
function hasOne
Creates a number of given hasOne associations on the model. Each association will be a new Backbone.Model. |
hasOne: function(assocs) {
_.each(assocs, function(assoc, key) {
this._associations = this._associations || {};
this._associations[key] = "hasOne";
createHasOneAssociation(this, key, assoc['model'], assoc['belongsTo']);
}, this);
}, |
function hasMany
Creates a number of given hasMany associations on the model. Each association will be a new Backbone.Collection. |
hasMany: function(assocs) {
_.each(assocs, function(assoc, key) {
this._associations = this._associations || {};
this._associations[key] = "hasMany";
createHasManyAssociation(this, key, assoc['collection'], assoc['belongsTo']);
}, this);
}
}; |
Duckbone.ModelHelpersThis set of helpers provides conveniences for many common situations not already covered by Backbone.Model. |
Duckbone.ModelHelpers = { |
function simpleSave
Posts only the given data to the server, leaving existing model attributes unchanged. |
simpleSave: function(attrs) {
var data = {}
if (this.id) attrs.id = this.id;
if(this.paramRoot) {
data[this.paramRoot] = attrs;
} else {
data = attrs;
}
var json = JSON.stringify(data);
return this.save({}, {
contentType: 'application/json',
data: json
});
}, |
function urlOverrides Backbone’s default url method with a new version that respects a function-style |
url : function() {
var urlRoot = (typeof this.urlRoot == 'function') ? this.urlRoot() : this.urlRoot;
var base = getUrl(this.collection) || urlRoot || urlError();
if (this.isNew()) return base;
return base + (base.charAt(base.length - 1) == '/' ? '' : '/') + encodeURIComponent(this.id);
}, |
function setOne
Sets a single attribute on the model. |
setOne: function(attr, val, options) {
var attrs = {};
attrs[attr] = val;
return this.set(attrs, options);
}, |
function createGetters
Creates simple getter functions for all desired attributes.
Getters are renamed in js syntax, so for example: |
createGetters: function() {
var model = this;
var getterList = arguments;
var getterFunctions = {};
_.each(getterList, function(getter) {
getterFuncName = underToCamel(getter);
getterFuncName = 'get' + upCaseFirstChar(getterFuncName);
if (!model[getterFuncName]) {
getterFunctions[getterFuncName] = function() { return this.get(getter); }
}
});
_.extend(this, getterFunctions);
}, |
function isValidAttributeDetermines if an attribute is valid to set, avoiding setting attributes to NaN or undefined. In almost all cases, better compatibility with Rails will be achieved by setting attributes to null instead. |
isValidAttribute: function(val) {
return (!_.isNaN(val) && !_.isUndefined(val))
}
}; |
Internal functions |
|
|
Do the work of creating a hasOne association |
function createHasOneAssociation(model, key, modelClass, belongsTo) {
var setterName = underToCamel('set_'+key);
var relName = underToCamel(key);
var setter = function(assocModel, settingUp) { // create the setter
if (assocModel instanceof Backbone.Model) { // Model case
if (assocModel === model[relName]) return assocModel; // return if same
if (model[relName]) {
model.trigger('remove:'+relName); // trigger if something is removed
if (belongsTo) model[relName][belongsTo] = null; // delete reciprocal
}
model[relName] = assocModel; // set new associated model
if (belongsTo) callReciprocalSetter(model, model[relName], belongsTo, settingUp);
model.trigger('add:'+relName);
} else if (assocModel) { // Attributes Object case
if (model[relName]) { // Existing model case
var bubbleChange = function() {
model.trigger('change:'+relName); // trigger change only if it changes
};
model[relName].bind('change', bubbleChange);
model[relName].set(assocModel); // set new attributes on the association
model[relName].unbind('change', bubbleChange);
} else { // New model case
model[relName] = new modelClass(assocModel); // create the model with the new attributes
if (belongsTo) callReciprocalSetter(model, model[relName], belongsTo, settingUp);
model.trigger('add:'+relName);
}
} else { // Null case, remove association
if (model[relName]) { // existing model case
model.trigger('remove:'+relName);
if (belongsTo) model[relName][belongsTo] = null; // destroy reciprocal association
}
model[relName] = null; // destroy association
}
return assocModel;
} // end setter
try {
setter.call(model, model.get(key), true); // call the setter to initialize
} catch(e) {
throw('Error creating association for ' + key + ':\n' + e);
}
delete model.attributes[key]; // remove associations data from attributes
model[setterName] = _.bind(setter, model); // bind setter to model
} |
|
Do the work of creating a hasMany association |
function createHasManyAssociation (model, key, assoc, belongsTo) {
try {
var relName = underToCamel(key);
var relData = model.get(key);
var collection = model[relName] = new assoc(relData); // create the collection
delete model.attributes[key]; // delete the association data from attributes
if (belongsTo) {
collection[belongsTo] = model; // create reciprocal link
collection.each(function(m) { // create reciprocal link on all models
callReciprocalSetter(model, m, belongsTo);
});
collection.bind('add', function (m) { // on add(), also give new models reciprocal links
callReciprocalSetter(model, m, belongsTo);
});
collection.bind('remove', function (m) { // on remove(), remove reciprocal links
m[belongsTo] = null;
});
collection.bind('reset', function(c) { // on reset(), give all new models reciprocal links
c.each(function(m) {
callReciprocalSetter(model, m, belongsTo);
});
});
}
} catch (e) {
throw('Error creating association for ' + key + ':\n' + e);
}
} |
|
Call the setter on a reciprocal association to establish the belongsTo |
function callReciprocalSetter(model, assocModel, belongsTo, settingUp) {
var setterName = 'set' + belongsTo.slice(0, 1).toUpperCase() + belongsTo.slice(1);
if (typeof assocModel[setterName] == "function") {
assocModel[setterName].call(assocModel, model, settingUp);
} else if (settingUp) {
assocModel[belongsTo] = model;
} else { // Complain if a hasOne association has not been defined for the reciprocal link
_.log("Model:");
_.log(assocModel);
throw('To use belongsTo, model must define hasOne for ' + belongsTo);
}
} |
|
Replacement function for |
function setWithAssociations(attrs, options) {
var nonAssocAttrs = {};
if (attrs instanceof Backbone.Model || !this._associations) {
nonAssocAttrs = attrs;
} else {
_(attrs).each(function(v, k) {
var assocType = this._associations[k];
if (assocType == "hasOne") {
var setterName = underToCamel('set_' + k);
this[setterName](v);
} else if (assocType == "hasMany") {
var relName = underToCamel(k);
if (typeof this[relName].freshen == "function") {
this[relName].freshen(v);
} else {
this[relName].reset(v);
}
} else {
nonAssocAttrs[k] = v;
}
}, this);
}
return this.setWithoutAssociations.call(this, nonAssocAttrs, options);
} |
|
Convert |
function underToCamel(word) {
return word.replace(/(\_[a-z])/g, function($1) {
return $1.toUpperCase().replace('_','');
});
} |
|
Capitalize the first character |
function upCaseFirstChar(word) {
return word.replace(/^\w/, function($0) {
return $0.toUpperCase();
});
} |
|
Get a URL from a Model or Collection as a property or as a function. |
var getUrl = function(object) {
if (!(object && object.url)) return null;
return _.isFunction(object.url) ? object.url() : object.url;
};
}).call(this); |


$().SPServices.SPLookupAddNew
The SPLookupAddNew function allows you to provide a link in forms for Lookup columns so that the user can add new values to the Lookup list easily. It is based on a blog post by Waldek Mastykarz.
The function works like this:
$().SPServices.SPLookupAddNew({
lookupColumn: "",
promptText: "Add new {0}",
newWindow: false,
ContentTypeID: "",
completefunc: null,
debug: true
});
The DisplayName of the Lookup column in the form.
The text to display as a link to add a new value to the lookup list. If you include the {0} placeholder, it will be replaced with the value of looukupColumn. The default value is "Add new {0}".
If true, the link will open in a new window without passing the Source. The default value is false.
If ContentTypeID is specified, it will be passed on the Query String to the NewForm for the Lookup column's list. e.g., "/SiteName/NewForm.aspx?ContentTypeID=0x0100FD8C376B70E78A46974ECF1B10F8D7AD"
completefunc If specified, the completefunc will be called upon successful completion of the call to SPLookupAddNew. Potential uses for the completefunc: consistent default formatting overrides, additional lookup customizations, image manipulations, etc. You can pass your completefunc in either of these two ways:
completefunc: function() {
...do something...
},
or
completefunc: doSomething, // Where doSomething is the name of your function
Setting debug: true indicates that you would like to receive messages if anything obvious is wrong with the function call, like using a column name which doesn't exist. I call this DebugMode.
$(document).ready(function() {
$().SPServices.SPLookupAddNew({
lookupColumn: "Region Name",
promptText: "Add new {0} "
});
});
The prompt in this example will be 'Add new Region Name'. Other prompt examples:


|
RelianceCore
1.4.0
Reliance Thermal Printer API
|
Required header for integration into your project. More...
Data Structures | |
| class | RelianceHID |
| Primary interface for interacting with Reliance Thermal Printer. More... | |
| struct | RelianceHID::Revision |
| Describes a firmware revision levels using semver syntax. More... | |
| struct | RelianceHID::Result |
| Describes response from all RelianceHID printer commands. More... | |
| struct | RelianceHID::RelianceStatus |
| Status response from Reliance printer. More... | |
Typedefs | |
| using | RelianceHID::ArgList = std::vector< std::string > |
| List of string arguments. More... | |
Enumerations |
Functions | |
| bool | RelianceHID::RelianceStatus::hasSensorFlag (SensorStatus flag) |
| Helper function to check if specified flag is set. More... | |
| bool | RelianceHID::RelianceStatus::hasErrorFlag (ErrorStatus flag) |
| Helper function to check if specified flag is set. More... | |
| bool | RelianceHID::RelianceStatus::hasSensorFlag (SensorStatus flag) const |
| Const function method to check if specified flag is set. More... | |
| bool | RelianceHID::RelianceStatus::hasErrorFlag (ErrorStatus flag) const |
| Const function method to check if specified flag is set. More... | |
| bool | RelianceHID::RelianceStatus::isPaperLow () |
| Helper function returns true if status report indicates paper low. More... | |
| bool | RelianceHID::RelianceStatus::isPaperOut () |
| Helper function returns true if status report indicates paper is out. More... | |
| static float | RelianceHID::RelianceStatus::adc2Voltage (uint16_t adc) |
| Returns the voltage given a raw ADC reading. This assumes a 12-bit ADC. More... | |
| RELIANCECORE_EXPORT Result | RelianceHID::initialize () |
| Attempt to connect to device. More... | |
| RELIANCECORE_EXPORT Result | RelianceHID::getRevision (Revision *rev) |
| Read firmware revision from target. More... | |
| RELIANCECORE_EXPORT Result | RelianceHID::ping () |
| Side effect free command to test for presence of printer. More... | |
| RELIANCECORE_EXPORT Result | RelianceHID::reboot () |
| Immediately perform a hard reboot of the printer. More... | |
| RELIANCECORE_EXPORT Result | RelianceHID::getStatus (RelianceStatus *status) |
| Get the current status of Reliance printer. More... | |
| RELIANCECORE_EXPORT Result | RelianceHID::getVirtualCommsEnabled () |
| Gets the state of the USB virtual comm port feature. More... | |
| RELIANCECORE_EXPORT Result | RelianceHID::setVirtualCommsEnabled (bool enabled) |
| Enable or disable the USB virtual comm port feature. More... | |
| RELIANCECORE_EXPORT Result | RelianceHID::getStartupTicketEnabled () |
| Gets the state of the startup ticket feature. More... | |
| RELIANCECORE_EXPORT Result | RelianceHID::setStartupTicketEnabled (bool enabled) |
| Sets the state of the startup ticket feature. More... | |
| RELIANCECORE_EXPORT Result | RelianceHID::getUnknownCommands (std::vector< int > &dst) |
| Returns a list of ESC/POS commands the Reliance does not understand. More... | |
| RELIANCECORE_EXPORT Result | RelianceHID::getPaperWidth () |
| Returns the current configured paper roll width. More... | |
| RELIANCECORE_EXPORT Result | RelianceHID::setPaperWidth (int width) |
| Change the paper roll width configuration. More... | |
| RELIANCECORE_EXPORT Result | RelianceHID::getMotorGen () |
| Returns the current motor configuration. More... | |
| RELIANCECORE_EXPORT Result | RelianceHID::setMotorGen (int gen) |
| Change the motor configuration to another gen. More... | |
| RELIANCECORE_EXPORT Result | RelianceHID::getMotorCurrent () |
| Returns the current motor current in milliamps. More... | |
| RELIANCECORE_EXPORT Result | RelianceHID::setMotorCurrent (int current) |
| Change the motor current. More... | |
Required header for integration into your project.
| using RelianceHID::ArgList = std::vector<std::string> |
List of string arguments.
|
strong |
Bit enumberation describes each error state that can be reported by Reliance.
|
strong |
|
strong |
Bit enumeration describes the state of each sensor.
|
strong |
|
static |
Returns the voltage given a raw ADC reading. This assumes a 12-bit ADC.
| RELIANCECORE_EXPORT Result RelianceHID::getMotorCurrent | ( | ) |
Returns the current motor current in milliamps.
This is the current that is applied to printer motor.
| RELIANCECORE_EXPORT Result RelianceHID::getMotorGen | ( | ) |
Returns the current motor configuration.
There are currently two motors, gen1 and gen2. The returned result will populate the value field with 0, 1, etc. which represent these motor gens.
| RELIANCECORE_EXPORT Result RelianceHID::getPaperWidth | ( | ) |
Returns the current configured paper roll width.
Reliance supports paper rolls width from 58mm though 80mm. This setting enables proper print margins for your chosen roll width.
| RELIANCECORE_EXPORT Result RelianceHID::getRevision | ( | Revision * | rev | ) |
Read firmware revision from target.
| rev | out parameter |
| RELIANCECORE_EXPORT Result RelianceHID::getStartupTicketEnabled | ( | ) |
Gets the state of the startup ticket feature.
When enabled, Reliance will print its configuration to a ticket on every power up. When disabled, this behavior is disabled.
| RELIANCECORE_EXPORT Result RelianceHID::getStatus | ( | RelianceStatus * | status | ) |
Get the current status of Reliance printer.
| status | will be written with current status |
| RELIANCECORE_EXPORT Result RelianceHID::getUnknownCommands | ( | std::vector< int > & | dst | ) |
Returns a list of ESC/POS commands the Reliance does not understand.
The list will be written to dst in the order cmd:arg where cmd is a known ESC/POS prefix such as ESC, FS, or GS (1B, 1C, 1D) and the arg is the first given parmeter. This is useful for legacy applications that send uncommon or customer ESC/POS commands to their printers.
| dst | vector to write log to |
| RELIANCECORE_EXPORT Result RelianceHID::getVirtualCommsEnabled | ( | ) |
Gets the state of the USB virtual comm port feature.
When enabled, Reliance will enumerate an additional USB interface as a CDC comm port. Check device manager or /dev/tty* to find the OS assigned port name.
| bool RelianceHID::RelianceStatus::hasErrorFlag | ( | ErrorStatus | flag | ) |
Helper function to check if specified flag is set.
| flag | to check |
| bool RelianceHID::RelianceStatus::hasErrorFlag | ( | ErrorStatus | flag | ) | const |
Const function method to check if specified flag is set.
| flag | to check |
| bool RelianceHID::RelianceStatus::hasSensorFlag | ( | SensorStatus | flag | ) |
Helper function to check if specified flag is set.
| flag | to check |
| bool RelianceHID::RelianceStatus::hasSensorFlag | ( | SensorStatus | flag | ) | const |
Const function method to check if specified flag is set.
| flag | to check |
| RELIANCECORE_EXPORT Result RelianceHID::initialize | ( | ) |
Attempt to connect to device.
| bool RelianceHID::RelianceStatus::isPaperLow | ( | ) |
Helper function returns true if status report indicates paper low.
| bool RelianceHID::RelianceStatus::isPaperOut | ( | ) |
Helper function returns true if status report indicates paper is out.
| RELIANCECORE_EXPORT Result RelianceHID::ping | ( | ) |
Side effect free command to test for presence of printer.
| RELIANCECORE_EXPORT Result RelianceHID::reboot | ( | ) |
Immediately perform a hard reboot of the printer.
| RELIANCECORE_EXPORT Result RelianceHID::setMotorCurrent | ( | int | current | ) |
Change the motor current.
| current | milliamps to apply to printer motor (min: 50, max: 1500) |
| RELIANCECORE_EXPORT Result RelianceHID::setMotorGen | ( | int | gen | ) |
Change the motor configuration to another gen.
| gen | 0 for gen1, 1 for gen 2 |
| RELIANCECORE_EXPORT Result RelianceHID::setPaperWidth | ( | int | width | ) |
Change the paper roll width configuration.
| width | value between 58 and 80, inclusive |
| RELIANCECORE_EXPORT Result RelianceHID::setStartupTicketEnabled | ( | bool | enabled | ) |
Sets the state of the startup ticket feature.
| enabled | true or false |
| RELIANCECORE_EXPORT Result RelianceHID::setVirtualCommsEnabled | ( | bool | enabled | ) |
Enable or disable the USB virtual comm port feature.
When enabled, Reliance will enumerate an additional USB interface as a CDC comm port. Check device manager or /dev/tty* to find the OS assigned port name.
| enabled | true or false |


6+
$25 / Per Pair
{{!--
Here's what you'll get!
The more socks you add the better the discount. See Tier Pricing.
Add 6 or more of the same sock to your cart the Grooms Bundle Wrapping will be free
Choose from any eligible socks. Eligable Socks
From color-coordinated matching sets to customizable for each guy’s personal style, we’ve got the best fitting socks your guys will love. We’ll even let you customize the packaging with your wedding hashtag or name, so each groomsmen will have his own. Our socks are designed and tailored just for you to put the final touch on your line of dapper men, and something they’ll always have to remember that special day with each wear.
Lorem ipsum dolor sit amet, consectetur adipisicing elit.


[1]
around 16 euro 's a cocktail but you could be in a lovely cocktail bar anywhere .
[2]
nice although as you would expect it 's pretty busy with kids the majority of time .


|
Panda3D
|
This class is a wrapper around a NodePath that, unlike the actual NodePath class, doesn't hold a reference count to the node. More...
Public Member Functions | |
| __init__ (const NodePath node_path) | |
| __init__ (const WeakNodePath copy) | |
| clear () | |
| Sets this NodePath to the empty NodePath. More... | |
| int | compareTo (const NodePath other) |
| Returns a number less than zero if this NodePath sorts before the other one, greater than zero if it sorts after, or zero if they are equivalent. More... | |
| int | compareTo (const WeakNodePath other) |
| Returns a number less than zero if this WeakNodePath sorts before the other one, greater than zero if it sorts after, or zero if they are equivalent. More... | |
| int | getKey () |
| Returns the same values as NodePath::get_key(). More... | |
| NodePath | getNodePath () |
| Returns the NodePath held within this object, or an empty NodePath with the error flag set if the object was deleted. More... | |
| bool | isEmpty () |
| Returns true if the NodePath contains no nodes, or if it has been deleted. More... | |
| PandaNode | node () |
| Returns the PandaNode held within this object, or nullptr if the object was deleted. More... | |
| bool | operator!= (const NodePath other) |
| bool | operator!= (const WeakNodePath other) |
| bool | operator< (const NodePath other) |
| bool | operator< (const WeakNodePath other) |
| WeakNodePath | operator= (const NodePath node_path) |
| WeakNodePath | operator= (const WeakNodePath copy) |
| bool | operator== (const NodePath other) |
| bool | operator== (const WeakNodePath other) |
| output (Ostream out) | |
| bool | wasDeleted () |
| Returns true if the NodePath we were referencing has been quietly deleted outside of the WeakNodePath. More... | |
This class is a wrapper around a NodePath that, unlike the actual NodePath class, doesn't hold a reference count to the node.
Thus the node may be detached from the scene graph and destructed at any time.
You can call is_valid() or was_deleted() at any time to determine whether the node is still around; if it is, get_node_path() will return the associated NodePath.
| __init__ | ( | const NodePath | node_path | ) |
| __init__ | ( | const WeakNodePath | copy | ) |
| int compareTo | ( | const NodePath | other | ) |
Returns a number less than zero if this NodePath sorts before the other one, greater than zero if it sorts after, or zero if they are equivalent.
Two NodePaths are considered equivalent if they consist of exactly the same list of nodes in the same order. Otherwise, they are different; different NodePaths will be ranked in a consistent but undefined ordering; the ordering is useful only for placing the NodePaths in a sorted container like an STL set.
| int compareTo | ( | const WeakNodePath | other | ) |
Returns a number less than zero if this WeakNodePath sorts before the other one, greater than zero if it sorts after, or zero if they are equivalent.
Two WeakNodePaths are considered equivalent if they consist of exactly the same list of nodes in the same order. Otherwise, they are different; different WeakNodePaths will be ranked in a consistent but undefined ordering; the ordering is useful only for placing the WeakNodePaths in a sorted container like an STL set.
| int getKey | ( | ) |
Returns the same values as NodePath::get_key().
| NodePath getNodePath | ( | ) |
| bool isEmpty | ( | ) |
Returns true if the NodePath contains no nodes, or if it has been deleted.
| PandaNode node | ( | ) |
Returns the PandaNode held within this object, or nullptr if the object was deleted.
| bool operator!= | ( | const NodePath | other | ) |
| bool operator!= | ( | const WeakNodePath | other | ) |
| bool operator< | ( | const NodePath | other | ) |
| bool operator< | ( | const WeakNodePath | other | ) |
| WeakNodePath operator= | ( | const NodePath | node_path | ) |
| WeakNodePath operator= | ( | const WeakNodePath | copy | ) |
| bool operator== | ( | const NodePath | other | ) |
| bool operator== | ( | const WeakNodePath | other | ) |
| output | ( | Ostream | out | ) |
| bool wasDeleted | ( | ) |
Returns true if the NodePath we were referencing has been quietly deleted outside of the WeakNodePath.


J.Y. Park unveils the featuring artists of his new single 'Fever'
by beansssJ.Y. Park has unveiled the featuring artists of his new upcoming single, "Fever"!
Previously J.Y. Park hinted at the two featuring artists of his single with their initials 'S' and 'B', also adding a clue that both musicians made headlines in the past for their appearance on music competition programs. According to his 3rd moving teaser image just revealed, J.Y. Park's "Fever" will feature Superbee and Bibi!
Superbee is a rapper well-known for his appearance on 'Show Me The Money', while Bibi appeared on SBS's 'The Fan' alongside ITZY's Yeji. J.Y. Park was so impressed by rookie female musician Bibi's performance on 'The Fan' at the time, that he asked her to feature as a rapper in his new single, despite the fact that Bibi is not a rapper but a vocalist.
Stay tuned for the release of J.Y. Park's "Fever" feat. Superbee and Bibi, set for release on December 1 at 6 PM KST! The MV for the single will be out a day earlier, on November 30 at 6 PM KST.


BACK TO THE FUTURE, PART II A film review by Jeff Meyer Copyright 1989 Jeff Meyer
[Don't worry, kids, no real spoilers lurk within]
Actually, about the only spoiler that I will reveal about BACK TO THE FUTURE PART II is the fact that the story is left with a cliff-hanger of an ending, and is continued in BACK TO THE FUTURE PART III, coming to a Sequel Auditorium near you next summer. I remember people walking out of the LORD OF THE RINGS in an extremely peeved mood due to the annoying surprise that the film only covered half of Tolkien's trilogy; I wouldn't have that on my snow-white conscience, so, Happy Holidays. Now you can go prepared. (I must admit that I didn't hear too much grumbling on leaving BACK TO THE FUTURE PART II; I assume the knowledge of it being continued is either fairly common knowledge, or the film is more satisfying that LORD OF THE RINGS, installment or no. (A rather back-handed compliment...))
So, how is it? And, of course, the really *original* question: how does is stand up to its predecessor? Well, first of all, the high points of BACK TO THE FUTURE were a) a clever use of time-travel machinations (many already familiar to me through the wonders of science fiction and comix), b) Christopher Lloyd's Doc Brown, c) some cute humor, and d) Alan Silvestri's charged-up theme music. And I liked the car. However, the characters were mostly pastiches, keeping it at the level of an above-average exercise in comic plotting with an under-used plot device -- time-travel. A satisfying movie, but not something I was anxious to see over and over.
Thus, I have to say that BACK TO THE FUTURE II pretty well meets up to my expectations, because they weren't abnormally high in the first place. The cleverness and time-related in-jokes are pretty good, and the time-travel theme holds together if you don't think about it *too* closely. (See assorted heaps of rec.arts.movies articles for examples of intense chrono-temporal reflection.) No real plot shocks or surprises There's a sense of rushed urgency in this film that was absent in the first BACK TO THE FUTURE film, and this gives the film an edge (or at least becomes reminiscent enough of IT'S A WONDERFUL LIFE to simulate one); however, what it adds in suspense, in takes away from the one enjoyable friendship in the first film, the one between Doc Brown and Marty. Doc seems to be in the picture merely to hustle Marty from time-period to time-period, and (except for one pleasant sequence where Brown bumps into himself), gets to show very little personality; his main contributions to the film are the better historical jokes. (From the previews of Part III at the end of the film, this may be remedied in the concluding film.) Michael J. Fox seems to be trying to beat Cary Grant's record of double-takes in ARSENIC AND OLD LACE, and while he's adequate, he's no Archie Leech. (The idea of Cary Grant as the protagonist in a slightly-altered version of these films really appeals to me...) Everyone else is a cookie-cutout character (Biff especially); they also toil who only serve the plot, etc.
So, is it worth seeing? Depends how well you liked the original BACK TO THE FUTURE PART II is more of the same; the good news, in these sequel-riddled days, is it's not worse than the same.
Moriarty, aka Jeff Meyer INTERNET<EMAIL_ADDRESS>Manual UUCP: {uw-beaver, sun, microsoft, hplsla, uiucuxc}!fluke!moriarty
.
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