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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. -
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: of 20,000 degree decreases by around 10% for the J/K part. ... 90secs in J/K. UKIDSS LAS Survey ---------------- Median limits(5sigma in 2arcsec aperture) Vega Ks 18.2 H 18.8 J 19.6 Y 20.2. -
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 -
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/~rgm/wfcsur/meetings/announcement_2.txt
https://people.ast.cam.ac.uk/~rgm/wfcsur/meetings/announcement_2.txt5 Dec 2006: products and archive 14:00 Photometric Calibration (Jones/Hodgkin) 14:20 Astrometric Calibration (Bunclark/Lewis/Irwin) 14:40 Pipeline processing I(including demo) (Lewis/Irwin) 15:20 Tea 15:40 Pipeline -
Persistence
https://people.ast.cam.ac.uk/~wfcam/docs/reports/persistence/26 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. -
Astrometric and Photometric Distortion for WFCAM and VISTA
https://people.ast.cam.ac.uk/~wfcam/docs/reports/astrom/28 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 -
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. -
CASU analysis of SV data for WFCAM
https://people.ast.cam.ac.uk/~wfcam/docs/reports/sv/26 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). -
WFAU Tapes === Store 6 x dual PCs 3GHz ...
https://people.ast.cam.ac.uk/~wfcam/talks/ukirt_may2006.ppt31 Jul 2006: 2 Tbyte ingest buffer. 10 Tbytes of raw. 20 Tbytes of processed. -
Flat Exposure Properties of VIRCAM Detectors
https://people.ast.cam.ac.uk/~wfcam/docs/reports/vircam_flatreport/vircam_flatreport.html8 Dec 2006: 10. VIRCAM_IMG_FLAT255_0049. 15. VIRCAM_IMG_FLAT255_0050. 10. VIRCAM_IMG_FLAT255_0051. 20. VIRCAM_IMG_FLAT255_0052. 10. VIRCAM_IMG_FLAT255_0053. 25. -
Estimate of the Number of CPU Nodes to Execute ...
https://people.ast.cam.ac.uk/~wfcam/ukreview/vircam_cpu_estimate.pdf29 Sep 2006: increase the data processing time by approximately 10 to 20%. ... The detailed processing time of this test is:. recipe time = 320 seconds ( 20% for missing functionalities). -
CASU analysis of WFCAM commissioning data - I
https://people.ast.cam.ac.uk/~wfcam/docs/reports/commissioning/2 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. -
L93 The Astrophysical Journal, 570:L93–L96, 2002 May 10 �� ...
https://people.ast.cam.ac.uk/~wyatt/jhkg02.pdf19 Apr 2006: Thirty-two frames with 20 s integration times each were ob-tained for 55 Cnc. ... We azimuthally smoothed this PSF byrotating the image in 20 increments and median-combiningthe resulting frames. -
Basic Debris Disk Model
https://people.ast.cam.ac.uk/~wyatt/wyatt_tpf_jul04.ppt19 Apr 2006: They used this result to explain the inner hole in the Pictoris disk by a planet at 20 AU:. ... 850 m : 320 m – 20 cm. Since the size cut-off for resonance is 300 m – 2 mm, I predict:. -
mnr9848.tex
https://people.ast.cam.ac.uk/~wyatt/gfw05.pdf19 Apr 2006: than 20 per cent for stars with twice the metal content of theSun (Fischer & Valenti 2005; Santos et al. ... HD 13445 (K1V) 0.20 HD 10700 (G8V) 0.36HD 143761 (G0V) 0.14 HD 196378 (F7V) 0.32HD 192263 (K2V) 0.07 HD 20794 (G8V) 0.23HD 117176 (G5V) -
LOCAL HEATING IN THE GALACTIC CENTER WESTERN ARC N. ...
https://people.ast.cam.ac.uk/~wyatt/mtpf03.pdf19 Apr 2006: Large-scale mapping of the central 5 pc of the Galaxy at10, 20, and 30 lm at 400 angular resolution by Telesco et al.(1996) found a temperature gradient consistent with ... We estimate a uni-form ISM across our 11.7 and 18.2 lm passbands of 2.86and 2.20, -
, EUROPEAN SOUTHERN OBSERVATORY Organisation Européenne pour des…
https://people.ast.cam.ac.uk/~rgm/vhs/eso-p79b-vhs.pdf5 Oct 2006: whole southern celestial hemisphere (20,000deg2) to a depth 4 magnitudes fainterthan 2MASS/DENIS in at least two wavebands J and K. -
L187 The Astrophysical Journal, 619:L187–L190, 2005 February 1� 2005. …
https://people.ast.cam.ac.uk/~wyatt/ghwd05.pdf19 Apr 2006: Dominik,5 and H. J. Walker6. Received 2004 September 17; accepted 2004 December 20; published 2005 January 10. ... The total dust flux within a diameter circle is′1 37.0mJy at 850mm and mJy at 450mm, in good2.5 250 20.
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