Commit b4e05a81 authored by Danny Boxhoorn's avatar Danny Boxhoorn
Browse files

Version from 2006/11/30

parents
1164802414
Fri Apr 1 2005 Claus Goessl <cag@usm.uni-muenchen.de>
* cvs checkin as module and autoconf extension
<html><head><title>curvemaker</title></head>
<body bgcolor="#ffffff">
<hr>
<font size="7"><b>curvemaker</b></font>
<hr>
<!-- NAME -->
<h2>NAME</h2>
<p>curvemaker -- extract lightcurves via accurate psf-photometry </p><br>
<!-- USAGE -->
<h2>USAGE</h2>
<p>
<tt>curvemaker [flags] image(s)</tt><br><br>
<table width="30%" cellpadding="0" cellspacing="0" border="0">
<tbody>
<tr><td align="left"> verbose </td><td align="center"> v </td><td align="right"> 0 </td></tr>
</tbody>
</table>
</p><br>
<!-- PARAMETERS -->
<h2>PARAMETERS</h2>
<dl>
<dt> verbose = 0 </dt>
<dd> Verbose level. If <tt>verbose</tt> >= </dd>
</dl>
<dl>
<dt> image(s) </dt>
<dd> Input image(s). </dd>
</dl><br>
<!-- DESCRIPTION -->
<h2>DESCRIPTION</h2>
<p> The task curvemaker ... </p><br>
<!-- OUTPUT -->
<h2>OUTPUT</h2>
<dl>
<dt> curvemaker-... </dt>
<dd> </dd>
</dl><br>
<!-- EXAMPLES -->
<h2>EXAMPLE</h2>
<p> curvemaker <p>
<hr>
<center><a href="overview.html">Task index</a></center>
<center><i>
This task was implemented by J. Koppenhfer and A. Riffeser<br>
Dokumentation maintained by J. Koppenhfer<br>
This file was last time updated on 22 Mar 2005
</i></center>
<hr>
</body></html>
\ No newline at end of file
<html><head><title>diffima</title></head>
<body bgcolor="#ffffff">
<hr>
<font size="7"><b>diffima</b></font>
<hr>
<!-- NAME -->
<h2>NAME</h2>
<p>diffima -- compute difference images </p><br>
<!-- USAGE -->
<h2>USAGE</h2>
<p>
<tt>diffima [flags] reference_image image(s)</tt><br><br>
<table width="40%" cellpadding="0" cellspacing="0" border="0">
<tbody>
<tr><td align="left"> backord </td><td align="center"> b </td><td align="right"> 1 </td></tr>
<tr><td align="left"> cut_sat_radius </td><td align="center"> y </td><td align="right"> 0 </td></tr>
<tr><td align="left"> error </td><td align="center"> e </td><td align="right"> false </td></tr>
<tr><td align="left"> factor </td><td align="center"> o </td><td align="right"> 0.0 </td></tr>
<tr><td align="left"> field </td><td align="center"> f </td><td align="right"> 200 </td></tr>
<tr><td align="left"> kreis </td><td align="center"> j </td><td align="right"> false </td></tr>
<tr><td align="left"> ksize </td><td align="center"> k </td><td align="right"> 17, 17 </td></tr>
<tr><td align="left"> model </td><td align="center"> l </td><td align="right"> 4, 6,1.0, 4,3.0, 2,9.0, 0,0.1, 0,0.0, 0,0.0 </td></tr>
<tr><td align="left"> normerror </td><td align="center"> q </td><td align="right"> false </td></tr>
<tr><td align="left"> notnormref </td><td align="center"> n </td><td align="right"> false </td></tr>
<tr><td align="left"> npara </td><td align="center"> a </td><td align="right"> 1 </td></tr>
<tr><td align="left"> part </td><td align="center"> p </td><td align="right"> 0, 0, 0, 0 </td></tr>
<tr><td align="left"> refbas </td><td align="center"> r </td><td align="right"> false </td></tr>
<tr><td align="left"> table </td><td align="center"> t </td><td align="right"> diffima.tab </td></tr>
<tr><td align="left"> varmask </td><td align="center"> m </td><td align="right"> "" </td></tr>
<tr><td align="left"> varpsforder </td><td align="center"> w </td><td align="right"> 0 </td></tr>
<tr><td align="left"> verbose </td><td align="center"> v </td><td align="right"> 1 </td></tr>
</tbody>
</table>
</p><br>
<!-- PARAMETERS -->
<h2>PARAMETERS</h2>
<dl>
<dt> backord = 1 </dt>
<dd> </dd>
</dl>
<dl>
<dt> cut_sat_radius = 0 </dt>
<dd> </dd>
</dl>
<dl>
<dt> error = false </dt>
<dd> If true, </dd>
</dl>
<dl>
<dt> factor = 0.0 </dt>
<dd> </dd>
</dl>
<dl>
<dt> field = 200 </dt>
<dd> Before kernel compilation, the image is divided into quadratic sub-images of this size. The difference image analysis is done individually on
each of the sub-images. At the end the images are re-merged. </dd>
</dl>
<dl>
<dt> kreis = false </dt>
<dd> </dd>
</dl>
<dl>
<dt> ksize = 17, 17 </dt>
<dd> Kernel size in pixel. </dd>
</dl>
<dl>
<dt> model = 4, 6,1.0, 4,3.0, 2,9.0, 0,0.1, 0,0.0, 0,0.0 </dt>
<dd> </dd>
</dl>
<dl>
<dt> normerror = false </dt>
<dd> </dd>
</dl>
<dl>
<dt> notnormref = false </dt>
<dd> </dd>
</dl>
<dl>
<dt> npara = 1 </dt>
<dd> </dd>
</dl>
<dl>
<dt> part = 0, 0, 0, 0 </dt>
<dd> Subimage coordinates x1, x2, y1, y2. If not "0, 0, 0, 0", the difference image analysis is only done in this subimage. </dd>
</dl>
<dl>
<dt> refbas = false </dt>
<dd> If true, the kernel base functions are calculated from the <tt>reference_image</tt> and written to the files "cc???.fits". If false, the kernel
base functions are read from the files "cc???.fits". </dd>
</dl>
<dl>
<dt> table = diffima.tab </dt>
<dd> </dd>
</dl>
<dl>
<dt> varmask = "" </dt>
<dd> Input image used to mask variable stars. Pixel having value "0" in the mask are not taken into accout for the determination of the kernel. </dd>
</dl>
<dl>
<dt> varpsforder = 0 </dt>
<dd> Order of PSF-cariation. </dd>
</dl>
<dl>
<dt> verbose = 0 </dt>
<dd> Verbose level. If <tt>verbose</tt> >= </dd>
</dl>
<dl>
<dt> reference_image </dt>
<dd> Input reference image. </dd>
</dl>
<dl>
<dt> image(s) </dt>
<dd> Input image(s). </dd>
</dl><br>
<!-- DESCRIPTION -->
<h2>DESCRIPTION</h2>
<p> The task diffima ... </p><br>
<!-- OUTPUT -->
<h2>OUTPUT</h2>
<dl>
<dt> d... </dt>
<dd> </dd>
</dl><br>
<dl>
<dt> k... </dt>
<dd> </dd>
</dl><br>
<dl>
<dt> diffima.tab </dt>
<dd> </dd>
</dl><br>
<dl>
<dt> bildr.fits </dt>
<dd> </dd>
</dl><br>
<dl>
<dt> e2bildr.fits </dt>
<dd> </dd>
</dl><br>
<dl>
<dt> rmask.fits </dt>
<dd> </dd>
</dl><br>
<dl>
<dt> If <tt>error</tt> >= true:</dt>
</dl>
<dl>
<dt> e.d... </dt>
<dd> </dd>
</dl><br>
<dl>
<dt> e.k... </dt>
<dd> </dd>
</dl><br>
<dl>
<dt> If <tt>refbas</tt> >= false:</dt>
</dl>
<dl>
<dt> cc???.fits </dt>
<dd> </dd>
</dl><br>
<dl>
<dt> If <tt>verbose</tt> >= 1:</dt>
</dl>
<dl>
<dt> </dt>
<dd> </dd>
</dl><br>
<dl>
<dt> If <tt>verbose</tt> >= 2:</dt>
</dl>
<dl>
<dt> bildi.fits </dt>
<dd> </dd>
</dl><br>
<dl>
<dt> ebildi.fits </dt>
<dd> </dd>
</dl><br>
<dl>
<dt> bg-... </dt>
<dd> </dd>
</dl>
<dl>
<dt> abs-... </dt>
<dd> </dd>
</dl>
<dl>
<dt> kern-... </dt>
<dd> </dd>
</dl>
<dl>
<dt> kernpara-... </dt>
<dd> </dd>
</dl><br>
<!-- EXAMPLES -->
<h2>EXAMPLE</h2>
<p> diffima -e -m mask.fits -v 2 -a 1 -o 1. -b -1. -k 17 -f 250 -p 1,1000,1,1000 reference.fits stars_*.fits <p>
<hr>
<center><a href="overview.html">Task index</a></center>
<center><i>
This task was implemented by A. Riffeser<br>
Dokumentation maintained by J. Koppenhfer<br>
This file was last time updated on 21 Mar 2005
</i></center>
<hr>
</body></html>
\ No newline at end of file
<html><head><title>getsky</title></head>
<body bgcolor="#ffffff">
<hr>
<font size="7"><b>getsky</b></font>
<hr>
<!-- NAME -->
<h2>NAME</h2>
<p> getsky -- skysubtract image </p><br>
<!-- USAGE -->
<h2>USAGE</h2>
<p>
<tt>getsky [flags] image</tt><br><br>
<table width="17%" cellpadding="0" cellspacing="0" border="0">
<tbody>
<tr><td align="left"> kappa </td><td align="center"> k </td><td align="right"> 4.0 </td></tr>
<tr><td align="left"> nan </td><td align="center"> n </td><td align="right"> 0.0 </td></tr>
<tr><td align="left"> order </td><td align="center"> o </td><td align="right"> 2 </td></tr>
<tr><td align="left"> radius </td><td align="center"> r </td><td align="right"> 0 </td></tr>
</tbody>
</table>
</p><br>
<!-- PARAMETERS -->
<h2>PARAMETERS</h2>
<dl>
<dt> kappa = 4.0 </dt>
<dd> </dd>
</dl>
<dl>
<dt> nan = 0.0 </dt>
<dd> </dd>
</dl>
<dl>
<dt> order = 2 </dt>
<dd> </dd>
</dl>
<dl>
<dt> radius = 0 </dt>
<dd> </dd>
</dl>
<dl>
<dt> image </dt>
<dd> </dd>
</dl><br>
<!-- DESCRIPTION -->
<h2>DESCRIPTION</h2>
<p>
The task getsky
</p><br>
<!-- OUTPUT -->
<h2>OUTPUT</h2>
<dl>
<dt> sub_... </dt>
<dd> </dd>
</dl><br>
<dl>
<dt> sky_... </dt>
<dd> </dd>
</dl><br>
<dl>
<dt> cut_... </dt>
<dd> </dd>
</dl><br>
<!-- EXAMPLES -->
<h2>EXAMPLE</h2>
<p> getsky -k 12 -r 0 reference.fits <p>
<hr>
<center><a href="overview.html">Task index</a></center>
<center><i>
This task was implemented by J. Koppenhfer & A. Riffeser<br>
Dokumentation maintained by J. Koppenhfer<br>
This file was last time updated on 31 Mar 2005
</i></center>
<hr>
</body></html>
\ No newline at end of file
<html><head><title>mupipe - Task Index</title></head>
<body bgcolor="#ffffff">
<center><font size="7"><b>
mupipe - Task Index
</b></font></center>
<hr>
<ul>
<li><a href="curvemaker.html">
<b>curvemaker</b></a> -- create lightcurves using PSF-photometry on difference images
</li>
<li><a href="diffima.html">
<b>diffima</b></a> -- compute difference images
</li>
<li><a href="getsky.html">
<b>getsky</b></a> -- skysubtract image
</li>
<li><a href="skycalc.html">
<b>skycalc</b></a> -- photometrically align images
</li>
<li><a href="starphot.html">
<b>starphot</b></a> -- photometry tool
</li>
<li><a href="subby.html">
<b>subby</b></a> -- replace masked regions and optionally do weighted stacking of images
</li>
<li><a href="weight.html">
<b>weight</b></a> -- compute optimal stacking weights from background and seeing
</li>
</ul>
<hr>
<center><i>
Dokumentation maintained by J. Koppenhfer<br>
This file was last time updated on 28 Nov 2006
</i></center>
</body></html>
\ No newline at end of file
<html><head><title>mupipe - Task Index</title></head>
<body bgcolor="#ffffff">
<center><font size="7"><b>
mupipe - Task Index
</b></font></center>
<hr>
<ul>
<li><a href="adder.html">
<b>adder</b></a> -- weighted stacking of images
</li>
<li><a href="biasredux.html">
<b>biasredux</b></a> -- compute initial standard CCD-reduction and creates an error-frame
</li>
<li><a href="boxfitting.html">
<b>boxfitting</b></a> -- either search for box-shaped transit signatures within a lightvurve or fold a lightcurve
</li>
<li><a href="compare.html">
<b>compare</b></a> -- align the surface of images using a polynomial fit
</li>
<li><a href="curvemaker.html">
<b>curvemaker</b></a> -- create lightcurves using PSF-photometry on difference images
</li>
<li><a href="diffima.html">
<b>diffima</b></a> -- compute difference images
</li>
<li><a href="divvy.html">
<b>divvy</b></a> -- shift images
</li>
<li><a href="getsky.html">
<b>getsky</b></a> -- skysubtract image
</li>
<li><a href="masterbias.html">
<b>masterbias</b></a> -- getsky -- create a masterbias image
</li>
<li><a href="masterflat.html">
<b>masterflat</b></a> -- create a masterflatfield image
</li>
<li><a href="psfphot.html">
<b>psfphot</b></a> -- create lightcurves using PSF-photometry on difference images
</li>
<li><a href="simulator.html">
<b>simulator</b></a> -- create a series of simulated images of stars, variables and transiting planet host stars
</li>
<li><a href="skycalc.html">
<b>skycalc</b></a> -- photometrically align images
</li>
<li><a href="starfind.html">
<b>starfind</b></a> -- locate stars and measure their parameters
</li>
<li><a href="starphot.html">
<b>starphot</b></a> -- photometry tool
</li>
<li><a href="subby.html">
<b>subby</b></a> -- replace masked regions and optionally do weighted stacking of images
</li>
<li><a href="weight.html">
<b>weight</b></a> -- compute optimal stacking weights from background and seeing
</li>
</ul>
<hr>
<center><i>
Dokumentation maintained by J. Koppenhfer<br>
This file was last time updated on 5 Apr 2005
</i></center>
</body></html>
\ No newline at end of file
<html><head><title>skycalc</title></head>
<body bgcolor="#ffffff">
<hr>
<font size="7"><b>skycalc</b></font>
<hr>
<!-- NAME -->
<h2>NAME</h2>
<p>skycalc -- photometrically align images </p><br>
<!-- USAGE -->
<h2>USAGE</h2>
<p>
<tt>skycalc [flags] reference_image image(s)</tt><br><br>
<table width="30%" cellpadding="0" cellspacing="0" border="0">
<tbody>
<tr><td align="left"> diffima </td><td align="center"> d </td><td align="right"> false </td></tr>
<tr><td align="left"> error </td><td align="center"> e </td><td align="right"> false </td></tr>
<tr><td align="left"> inputtab </td><td align="center"> t </td><td align="right"> "" </td></tr>
<tr><td align="left"> ordabs </td><td align="center"> </td><td align="right"> -1 </td></tr>
<tr><td align="left"> ordsky </td><td align="center"> </td><td align="right"> -1 </td></tr>
<tr><td align="left"> prefix </td><td align="center"> p </td><td align="right"> b </td></tr>
<tr><td align="left"> ref </td><td align="center"> </td><td align="right"> false </td></tr>
<tr><td align="left"> verbose </td><td align="center"> v </td><td align="right"> 0 </td></tr>
</tbody>
</table>
</p><br>
<!-- PARAMETERS -->
<h2>PARAMETERS</h2>
<dl>
<dt> diffima = true </dt>
<dd> difference imaging around stars (circular area with radius 50) to extract absorption and sky</dd>
</dl>
<dl>
<dt> error = false </dt>
<dd> Use error images too. If false, the error images are created simply by using the sqrt of the images. Only if true error files are created</dd>
</dl>
<dl>
<dt> inputab = "" </dt>
<dd> Table with stars used for difference imaging.</dd>
</dl>
<dl>