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https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_080207.txt
https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_080207.txt14 Feb 2008: 7th February 2008 Hoyle Committee Room 10:00-12:20 (with coffee break) Present: STH, PSB, MJI, EGS, MR, NAW, RGM Apologies: DWE, JRL, RWA Agenda ------ 1. ... STH fedback comments on Plone/HTML websites JRL replied to EVO questionnaire before 20 January -
https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_080806.txt
https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_080806.txt19 Aug 2008: LTO2's only store 5 nights of compressed data per tape (hence the large pile) so we will switch to LTO4's for 08B where we expect to get 20 nights ... In addition to the beautiful 2D images, and exquisite photometry in nebulous regions we also managed to -
https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_080103.txt
https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_080103.txt3 Jan 2008: and Phil Lucas regarding future of UKIRT/UKIDSS and circulate within group STH feedback comments on Plone/HTML websites New Actions ----------- JRL reply to EVO questionnaire by 20 January JRL implement -
https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_081127.txt
https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_081127.txt16 Dec 2008: are now: 5% variation in the nominal ZP represents photometric; 5-20% is thin cirrus, and 20% represents thick cirrus. -
https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_071211.txt
https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_071211.txt3 Jan 2008: quasars are excluded. The discrete CASU classification categories in the K-band are: -2 (probable star); 9 -1 (star-like); 1362 0 (noise); 10 1 (non-stellar); 269 Thus around 20% -
Microsoft PowerPoint - wyatt
https://people.ast.cam.ac.uk/~wyatt/wyatt_hst08.pdf7 Feb 2008: 1984). photosphere. dust. Debris disk history: … to present dayNow >300 debris disks known from thermal emission (more numerous and common than extrasolar planets), of which 20 have been imaged. -
https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_080623.txt
https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_080623.txt27 Jun 2008: Transfers of UKIDSS and CAL data to ESO proceed apace with about 20 nights of 08A to go. -
Change Record
https://people.ast.cam.ac.uk/~wfcam/docs/jul2007_linearity.doc20 Jan 2008: 18Figure 2‑20 Median flux (ADU) of monitor exposures versus time (fraction of day) for 2007-07-12 (Detectors 9-16). ... Figure 2‑20 Median flux (ADU) of monitor exposures versus time (fraction of day) for 2007-07-12 (Detectors 9-16). -
WFCAM Catalogues Document Number: VDF-SPE-IOA-00009-0001 Version 5…
https://people.ast.cam.ac.uk/~wfcam/docs/catalogues.pdf2 Sep 2008: 20 Aperture flux 1 These are a series of different radii soft-edged apertures designed toadequately sample the curve-of-growth of the majority of images and toprovide fixed-sized aperture ... aperture has a radius of rcore.26 Aperture flux 427 Error in -
arX iv:0 810. 5087 v1 [ astr o-ph ] ...
https://people.ast.cam.ac.uk/~wyatt/scwm08.pdf3 Nov 2008: The con-tours shown in the images are at 20%, 40%, 60% and 80% ofthe peak in each case (peak value in Qa 5.24mJy/pixel, in Si-5 ... Solid line contours are at the 20%, 40%, 60%, and 80% of the peak levels for all images.
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