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CASU/ORACDR Pipeline Algorithm Comparative Tests
https://people.ast.cam.ac.uk/~wfcam/docs/reports/pipeline_tests/16 Feb 2004: CASU/ORACDR Pipeline Algorithm Comparative Tests. (Document number VDF-TRE-IOA-00007-0001). Jim Lewis. Draft 20040119. ... Whether this is the case generally is beyond the scope of this little test. -
VIRCAM Pipeline: Unit Test Recipes
https://people.ast.cam.ac.uk/~wfcam/docs/vista/vircam_manual/group__testrecipelist.html10 Apr 2013: Detailed Description. This is the group of recipes that are written to test the Data Reduction Modules. ... Test recipe to drive the vircam_platesol library function. Generated on Wed Apr 10 04:01:57 2013 for VIRCAM Pipeline by . -
Reset-subtraction test 21 Dec 1999 Test to determine if ...
https://people.ast.cam.ac.uk/~optics/cirsi/documents/reset/reset.html16 Jun 2015: Reset-subtraction test 21 Dec 1999 Test to determine if online processing done by PixCel (reset correction, rotate, and assembly) is working correctly. ... This is our standard observing mode. RRR mode assemble ON rotate ON subtract ON Test: Assemble and -
Ian Parry's Home Page
https://people.ast.cam.ac.uk/~irp/22 Oct 2021: Build and test a flight-ready unfolding CubeSat compatible space telescope. Launch and operate a CubeSat in-orbit technology demonstrator. -
1 Introduction
https://people.ast.cam.ac.uk/~wfcam/docs/reports/interleaving/index.html29 Oct 2004: Interleaving tests. Document number: VDF-TRE-IOA-00016-0001 Version 1.1. Dafydd Wyn Evans, IoA. ... 3 Simulations. The simulations carried out to test the effects of interleaving on the astrometric and photometric accuracies were done using the IRAF. -
Contents
https://people.ast.cam.ac.uk/~wfcam/docs/reports/psf3/index.html17 Jan 2006: Tests on real WFCAM data (the UDS test data, see Section 6) showed that a more detailed model was required. ... 7 Crowded field tests. Tests have been carried out using data covering M17 in order to test the performance in more crowded fields. -
Data Processing Philoshpy
https://people.ast.cam.ac.uk/~wfcam/docs/philosophy01.txt23 Jan 2003: can do for much of pipeline anyway test data: need to aquire test data from WFCAM to assess persistence, reset anomalies, dark stability, flat stability, bad pixel problems etc. ... asap what other UKIRT?WFCAM test data do we need? - more flats (dome cf. -
Difference imaging
https://people.ast.cam.ac.uk/~wfcam/docs/reports/subtract/3 Sep 2007: For the initial tests, images from the INT wide field camera (WFC) were used. ... These were included on the plots. For the tests, only one CCD of the WFC is shown. -
round($x),"y"=>round($y)); } if(empty($long))$long =…
https://people.ast.cam.ac.uk/~vasily/sdss/stellar_halo/test.phpround($x),"y"=>round($y)); } if(empty($long))$long = 202.015; if(empty($lat)) $lat = 33.556; $im = imagecreatefrompng("fos_dr6.png"); $red = imagecolorallocate ($im, 255,0,0); $scale_x = imagesx($im); $scale_y = imagesy($im); $pt = getlocationcoords( -
Availability of CIRPASS
https://people.ast.cam.ac.uk/~optics/cirpass/availability.bak216 Jun 2015: On July 9th 2001 we officially passed the Gemini acceptance test when we showed that the total measured noise in the system (sky, dark current, flat-field noise, thermal background and
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