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https://people.ast.cam.ac.uk/~rgm/vhs/vhs-baseline-v3.txt
https://people.ast.cam.ac.uk/~rgm/vhs/vhs-baseline-v3.txt17 Mar 2006: -
Astrometric and Photometric Distortion for WFCAM and VISTA
https://people.ast.cam.ac.uk/~wfcam/docs/reports/astrom/index.html28 Sep 2006: World Coordinate Systems and FITS Headers. After a mere 20 years the FITS community finally agreed upon a standard way of defining a World Coordinate System (WCS) for telescopes with focal -
Persistence
https://people.ast.cam.ac.uk/~wfcam/docs/reports/persistence/index.html26 May 2006: The variation measured from faint to bright perturbing star was about 20 counts in the level of the persistent image. ... This indicates that the simple model would only be accurate at the 10-20 counts level. -
Richard McMahon, Institute of Astronomy, Cambridge University:…
https://people.ast.cam.ac.uk/~rgm/presentations/26 Jul 2006: Last modified: Wed Jul 26 20:32:26 2006. -
Contents
https://people.ast.cam.ac.uk/~wfcam/docs/reports/psf3/index.html17 Jan 2006: A reasonable estimate to account for this is that the 2x2 plots need to be adjusted by 20% (ie. ... However, one of the frames exhibited a large magnitude term in y amounting to 0.05 pixel (20 mas) over the observed magnitude range. -
CASU analysis of SV data for WFCAM
https://people.ast.cam.ac.uk/~wfcam/docs/reports/sv/index.html26 Jan 2006: The images mimic fuzzy looking galaxies and in this image peak at typically 5-20 counts above sky. ... measured using a conventional method) is therefore also 1.20 (Parseval's Theorem and power spectrum <-- FT --> autocorrelation). -
CASU analysis of WFCAM commissioning data - I
https://people.ast.cam.ac.uk/~wfcam/docs/reports/commissioning/index.html2 Nov 2006: The above plots are all in the WFCAM instrumental system and the 5-sigma limiting magnitudes for stellar objects in this data in this system are approximately Y = 20.9, J = ... 20.6, H = 19.8, K = 19.1 ,all in a Vega system. -
CASU WFCAM/VISTA Explanation of documentation numbering system>
https://people.ast.cam.ac.uk/~wfcam/docs_exp.html26 May 2006: scheme.. Dafydd Wyn Evans (dwe @ ast.cam.ac.uk). Last modified: Wed Apr 28 16:20:53 2004. -
https://people.ast.cam.ac.uk/~vasily/sdss/456/readme456.txt
https://people.ast.cam.ac.uk/~vasily/sdss/456/readme456.txt27 Jun 2006: The resulting distance moduli are: dmag = [18.2, 20.9, 16.8] In principle, from the CMD matching, you can't really shift the ridgeline by more than 0.05 mag -
Contents
https://people.ast.cam.ac.uk/~wfcam/docs/reports/psf3/17 Jan 2006: A reasonable estimate to account for this is that the 2x2 plots need to be adjusted by 20% (ie. ... However, one of the frames exhibited a large magnitude term in y amounting to 0.05 pixel (20 mas) over the observed magnitude range.
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