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The STARS Web Pages
https://people.ast.cam.ac.uk/~stars/archive/IO.html31 May 2004: 1.187E07. 1.705E09. 6.304E-24. 131. 199. 0. 182. 136. 122. 0. 0. ... log-10 of the opacity (24). timestep in years (25). surface abundance of hydrogen (26). -
CASU analysis of SV data for WFCAM
https://people.ast.cam.ac.uk/~wfcam/docs/reports/sv/index.html26 Jan 2006: 24.2 [using an average gain of 5.1 = 4.3 after correcting for intrapixel capacitance] UFTI (e-/s) ---- ---- 24.5 24.7 24.2. ... 9.0 4.2 5.80 24.4 #4 49.1 4.4 5.17 22.7. -
WFCAM simulations
https://people.ast.cam.ac.uk/~wfcam/docs/reports/simul/3 Sep 2007: Passband. H. Magnitude zero-point. 24.8. Magnitudes. Sky brightness. 13.6. Mags/arcsec2. Magnitude limits. ... imcore_conf. only (Figure 23) and median magnitude difference (Figure 24) were made. -
CASU analysis of SV data for WFCAM
https://people.ast.cam.ac.uk/~wfcam/docs/reports/sv/26 Jan 2006: 24.2 [using an average gain of 5.1 = 4.3 after correcting for intrapixel capacitance] UFTI (e-/s) ---- ---- 24.5 24.7 24.2. ... 9.0 4.2 5.80 24.4 #4 49.1 4.4 5.17 22.7. -
Index of /~vasily/images/sdss_dwarfs
https://people.ast.cam.ac.uk/~vasily/images/sdss_dwarfs/2006-08-24 11:02. 70K. ... 2006-08-24 11:04. 9.3K. -
CIRSI Temperature Sensors
https://people.ast.cam.ac.uk/~rgm/cirsi/cirsi_temperature_sensors.html24 Nov 1999: Last modified: Wed Nov 24 10:36:39 1999. -
CASU analysis of WFCAM commissioning data - I
https://people.ast.cam.ac.uk/~wfcam/docs/reports/commissioning/2 Nov 2006: Z Y J H K Overall zero-point (count/s) 22.8 22.7 23.0 23.4 22.6 WFCAM (e-/s) 24.4 24.3 24.6 25.0 ... 24.2 [assumes above gain measures ok] UFTI (e-/s) ---- ---- 24.5 24.7 24.2. -
NAME: diffmag_wfc PURPOSE: this program makes differential magnitude…
https://people.ast.cam.ac.uk/~xmmssc/xidops/docs/idl/diffmag_wfc.html15 Feb 2001: Last modified: Thu Feb 15 12:24:40 2001. -
{\bf WFCAM Catalogues}
https://people.ast.cam.ac.uk/~wfcam/docs/catalogues.html4 Feb 2006: 24 Aperture flux 3 Recommended if a single number is required to represent the flux for ALL. ... 24 arcsec diameter. 45 Error in flux The aperture fluxes can be combined with later-derived aperture. -
Index of /~vasily/sdss/subaru
https://people.ast.cam.ac.uk/~vasily/sdss/subaru/2006-05-23 14:24. 10K.
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