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https://people.ast.cam.ac.uk/~xmmssc/lplogs/20000625.int
https://people.ast.cam.ac.uk/~xmmssc/lplogs/20000625.int24 Nov 2001: COVER (%): (1st half) 0 (2nd half) 0 DUST (0-2): (1st half) 0 (2nd half) 0 SEEING (arcsec): (1st half) 0.8 (2nd half) 0.9 DOME OPENED (UT): 20:30 ... METEOROLOGICAL PARAMETERS UT AirT Hum% Wspd Gust Wdir Press LocT IntT Mirr LocRH IntRH SUNSET(UT) 20:21 -
CIRPASS TECHNICAL STUDY
https://people.ast.cam.ac.uk/~optics/cirpass/hdf.htm16 Jun 2015: The galaxy sample was broken down into three magnitude bins: J < 20, 20 < J < 22, and J > 22. ... The bright galaxy sample (J < 20) requires somewhat larger aperture sizes than the fainter sample does. -
WFS Status
https://people.ast.cam.ac.uk/~mike/casu/WFCsur/wfsj0801.html24 Nov 2000: Nominal grid centre: 08 01 42.00 40 19 00.0 j2000 RA step size : 30.00 arc mins Dec step size : 20.00 arc mins Filters: U B V R -
https://people.ast.cam.ac.uk/~rgm/vhs/v4/vdes-coi.log
https://people.ast.cam.ac.uk/~rgm/vhs/v4/vdes-coi.log5 Jun 2007: 20 v1.0o Standard LaTeX Graphics (DPC,SPQR) (/usr/local/teTeX/share/texmf.local/tex/latex/graphics/trig.sty Package: trig 1999/03/16 v1.09 sin cos tan (DPC) ) ... words of font info for 20 fonts, out of 2000000 for 2000 58 hyphenation exceptions out of -
WFS Status
https://people.ast.cam.ac.uk/~mike/casu/WFCsur/wfsjngc.html14 Nov 2000: B SN rep wfsngc011 10 20 00.00 00 00 00.0 j2000! ... B r' z SN rep wfsngc131 14 20 00.00 00 00 00.0 j2000! -
Observing and Proposal Material Blain/Gray Lensing Cluster proposal…
https://people.ast.cam.ac.uk/~optics/cirsi/ociw/DuPontIoaTimeProposals/16 Jun 2015: Last modified: Thu Apr 20 22:40:22 2000. -
https://people.ast.cam.ac.uk/~optics/cirsi/ociw/lcirs_standards.info
https://people.ast.cam.ac.uk/~optics/cirsi/ociw/lcirs_standards.info16 Jun 2015: Keep the peak counts below about 8K (you could put the telescope somewhat out of focus, eg 20 units, if necessary). ... The following standards are used: 9185 22 02 05.7 -01 06 02 J2000 NEAR SSA22 9104 01 03 15.8 -04 20 44 J2000 NEAR NOAO FIELD 9106 03 -
https://people.ast.cam.ac.uk/~optics/cirsi/ing/2000a/20000620.al
https://people.ast.cam.ac.uk/~optics/cirsi/ing/2000a/20000620.al16 Jun 2015: AM on 2000 Sep 24; standard zone = 0 hrs W For the night of: Tue, 2000 Jun 20 --- Wed, 2000 Jun 21 Local midnight = 2000 Jun 20, 23 hr UT, or -
Notes for APMCAT remote interrogation program.
https://people.ast.cam.ac.uk/~mike/apmcat/apmcat_notes.html24 Nov 2003: Current status: Full northern POSS1 to approximately 20 degrees from Galactic plane is available. -
https://people.ast.cam.ac.uk/~optics/cirpass/datared/list_xml.txt
https://people.ast.cam.ac.uk/~optics/cirpass/datared/list_xml.txt16 Jun 2015: GY-11 16:23:20.8 -24:17:21 2349.8-2601 16:23:49.8 -24:26:01 CRBR-14 16:23:17.3 -24:19:25 GY-10 ... 23:20.8 -24:17:08 2MASSW-J2049197-194432 20:49:19.74 -19:44:32.5 2MASSW-J2147446-264406 21:47:44.62 -26:44:06.6 2MASSW-J2206228-204705 -
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 -
https://people.ast.cam.ac.uk/~rgm/wfcsur/int_ao.txt
https://people.ast.cam.ac.uk/~rgm/wfcsur/int_ao.txt1 Mar 1998: For details on QE see Spectrum No. 15 Sep 1997 page 20] Limiting magnitude estimates for a 10-15 min exposure are given in the following table, assuming a dark sky -
SIGNAL_CIRSI WWW Interface (24-Sept-1998)
https://people.ast.cam.ac.uk/~rgm/forms/cirsi/signal_cirsi_form.html25 Mar 2002: Sanity checks. ESO SOFI on NTT(3.5m): 1 minute sensitivities J: 20.7; H: 19.7; K: 18.7 (assumed DARK ZENITH sky: 16.7, 15.0, 13.0). -
CASU WFCAM/VISTA Documentation (Sorted)
https://people.ast.cam.ac.uk/~wfcam/documentation_sorted.html13 May 2009: CASU Analysis of RAL VIRCAM data. 20-6-2006. 20-6-2006 [pdf]. ... Example WFCAM FITS header (based on INT CIRSI data). 30-06-2003. 20-06-2003 [fits]. -
https://people.ast.cam.ac.uk/~optics/cirsi/ing/2000a/20000517.al
https://people.ast.cam.ac.uk/~optics/cirsi/ing/2000a/20000517.al16 Jun 2015: evening twilight: 11 59 Morning twilight: 5 49 GDT; LMST at morning twilight: 19 22 12-degr twilight: 21 54 GDT -- 6 22 GDT; night center: 2 08 GDT Moonrise: 20 -
https://people.ast.cam.ac.uk/~optics/cirsi/ing/2000a/20000612.al
https://people.ast.cam.ac.uk/~optics/cirsi/ing/2000a/20000612.al16 Jun 2015: evening twilight: 13 59 Morning twilight: 5 39 GDT; LMST at morning twilight: 20 54 12-degr twilight: 22 10 GDT -- 6 13 GDT; night center: 2 11 GDT Moonset : 5 -
https://people.ast.cam.ac.uk/~optics/cirsi/ing/2000a/20000616.al
https://people.ast.cam.ac.uk/~optics/cirsi/ing/2000a/20000616.al16 Jun 2015: evening twilight: 14 16 Morning twilight: 5 39 GDT; LMST at morning twilight: 21 10 12-degr twilight: 22 11 GDT -- 6 14 GDT; night center: 2 12 GDT Moonrise: 20 -
https://people.ast.cam.ac.uk/~optics/cirsi/ing/2000a/20000617.al
https://people.ast.cam.ac.uk/~optics/cirsi/ing/2000a/20000617.al16 Jun 2015: JD 2451713.458 Local Mean Sidereal Time at midnight = 15 34 29.1 Sunset ( 2326 m horizon): 21 20 GDT; Sunrise: 7 05 GDT Evening twilight: 22 46 GDT; LMST at -
https://people.ast.cam.ac.uk/~optics/cirsi/ing/2000a/20000618.al
https://people.ast.cam.ac.uk/~optics/cirsi/ing/2000a/20000618.al16 Jun 2015: JD 2451714.458 Local Mean Sidereal Time at midnight = 15 38 25.6 Sunset ( 2326 m horizon): 21 20 GDT; Sunrise: 7 06 GDT Evening twilight: 22 47 GDT; LMST at -
https://people.ast.cam.ac.uk/~optics/cirsi/software/SOFTS/README
https://people.ast.cam.ac.uk/~optics/cirsi/software/SOFTS/README16 Jun 2015: cubemean.c Assume new controler in place, loop1 not skipped Version 0.94 (November 2001) - Carine Babusiaux Add 2mass catalogue option in astrometry.pl (using 2mass.pl) Version 0.93 (20 -
https://people.ast.cam.ac.uk/~optics/cirsi/ing/2000a/20000613.al
https://people.ast.cam.ac.uk/~optics/cirsi/ing/2000a/20000613.al16 Jun 2015: evening twilight: 14 03 Morning twilight: 5 39 GDT; LMST at morning twilight: 20 58 12-degr twilight: 22 10 GDT -- 6 13 GDT; night center: 2 12 GDT Moonrise: 18 -
SDSS DR4 page on Richard G. McMahon Last ...
https://people.ast.cam.ac.uk/~rgm/ukidss/sciver/classification.html10 Dec 2005: Last modified: Sat Dec 10 18:55:20 2005. -
https://people.ast.cam.ac.uk/~xmmssc/lplogs/20000624.int
https://people.ast.cam.ac.uk/~xmmssc/lplogs/20000624.int24 Nov 2001: CLOUD COVER (%): (1st half) 0 (2nd half) 0 DUST (0-2): (1st half) 0 (2nd half) 0 SEEING (arcsec): (1st half) 1.2 (2nd half) 1 DOME OPENED (UT): 20:30 ... METEOROLOGICAL PARAMETERS UT AirT Hum% Wspd Gust Wdir Press LocT IntT Mirr LocRH IntRH SUNSET(UT) -
https://people.ast.cam.ac.uk/~vasily/data/sims/mw_props/mw_props_4498.…
https://people.ast.cam.ac.uk/~vasily/data/sims/mw_props/mw_props_4498.txt15 Apr 2020: 2608 195876293938.0 9.30660379627 5.25241 20 0.2696 230191459912.0 11.3220087604 4.70566 21 0.2784 273195864601.0 10.2495479714 5.67929 22 0.2872 335640645373.0 ... 14.8638113635 6.54747 30 0.3576 696465404984.0 20.2183562818 5.00706 31 0.3664 -
Night Sky Brightness at Cerro Pachon
https://people.ast.cam.ac.uk/~rgm/vista/site/pachon_sky/12 Jul 1999: 11-50 nL. Backround stars (V>20 interstellar scattering):. 13 nL. Galaxies:. 0.1 nL. ... U = 22.0 mag/arcsec2. B = 22.7. V = 21.8. R = 20.9. -
The picture shows the evolution of a thin representative ...
https://people.ast.cam.ac.uk/~haehnelt/rtnigmwebbackup/reion/figcaption1.html24 Jan 2018: The picture shows the evolution of a thin representative slice of the universe (4 Mpc/h x 4 Mpc/h comoving) as a function of time (represented as a scale factor a). The evolution starts at z20 (a0.05) and stops at z=4 (a=0.2). The respective panels -
Detection of HeII reionization, due to its effect on ...
https://people.ast.cam.ac.uk/~haehnelt/rtnigmwebbackup/reion/figcaption5.html24 Jan 2018: The hashed region for the simulation delineates the 20 and 80 per centile of bootstrap re-sampled mock samples. -
Sky Brightness Primer
https://people.ast.cam.ac.uk/~rgm/vista/site/pachon_sky/page2.html9 Jul 1999: 11-50 nL. Backround stars (V>20 interstellar scattering):. 13 nL. Galaxies:. 0.1 nL. -
WFC - Photometric Calibration
https://people.ast.cam.ac.uk/~mike/casu/WFCsur/photom_old.html13 Dec 1999: RGO z'. 22.08. Oct 98. -. -. -. -0.52 R-I. -. 22.20. Dec 98. -. -. -. -0.39 R-I. -. 22.24. Feb 99. -. -. -. -
https://people.ast.cam.ac.uk/~vasily/data/sims/mw_props/mw_props_4778.…
https://people.ast.cam.ac.uk/~vasily/data/sims/mw_props/mw_props_4778.txt15 Apr 2020: 2608 214874808742.0 6.94480811379 7.2585 20 0.2696 229307809744.0 9.51461666855 5.59283 21 0.2784 247864511529.0 16.5022734363 3.4147 22 0.2872 261266575270.0 ... 6.98233 47 0.5072 677908679069.0 20.2461692471 6.83744 48 0.516 680412366610.0 -
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 -
Version 1.0 FITS header document
https://people.ast.cam.ac.uk/~wfcam/docs/headers_1p0.html22 Oct 2003: AMEND = 1.769 / Airmass at end of observation. TELRA = 20.0123456 / [h] Current telescope right ascension. ... TELDEC = 29.9876543 / [deg] Current telescope declination. GSRA = 20.0103456 / [h] Right ascension of guide star. -
https://people.ast.cam.ac.uk/~optics/cirpass/datared/BINTABLE.txt
https://people.ast.cam.ac.uk/~optics/cirpass/datared/BINTABLE.txt16 Jun 2015: 17. 18. 33. 1. 18. 19. 34. 0. 19. 20. 35. ... 1. 20. 21. 34. -2. 21. 22. 33. -1. 22. 23. -
NAME: STRINGAD PURPOSE: Converts a string of sexigesimal coordinates…
https://people.ast.cam.ac.uk/~xmmssc/xidops/docs/idl/stringad.html15 Feb 2001: CALLED: Getopt Ten HISTORY: 09-AUG-90 Version 1 written by Kerry McQuade 20-AUG-90 Put code to account for '-0' back in after it was removed by someone. -
https://people.ast.cam.ac.uk/~vasily/data/sims/mw_props/mw_props_69684…
https://people.ast.cam.ac.uk/~vasily/data/sims/mw_props/mw_props_69684.txt15 Apr 2020: 2608 181885130085.0 8.4224187872 5.66212 20 0.2696 213402058462.0 15.6506970643 3.31974 21 0.2784 231369660135.0 19.7733712413 2.7852 22 0.2872 236524298180.0 ... 4544 102 0.9912 888365285231.0 20.1904081202 12.4813 103 1.0 891605311717.0 20.8571424189 12 -
Reset-subtraction test 21 Dec 1999 Test to determine if ...
https://people.ast.cam.ac.uk/~optics/cirsi/documents/reset/reset.html16 Jun 2015: cl> imstat irx.9135-9137.c3.00?fits IMAGE MIDPT MODE STDDEV irx.9135-9137.c3.001.fits -19.20 -23.52 66.7 irx.9135-9137.c3.002.fits ... irx.9138-9137.c3.00?fits IMAGE MIDPT MODE STDDEV irx.9138-9137.c3.001.fits -16.15 -20.62 66.58 -
Observing Plan
https://people.ast.cam.ac.uk/~optics/cirsi/ociw/DuPontObservingPlans/20010410/16 Jun 2015: RA:15:03:52 Dec:-12:40.4. set:. rise : 19:48. [8:20. 18:11? :? :? 19:49. ... RA:15:57:18 Dec:-16:45.3. set:. rise : 20:27. [8:22. 18:16? :? :? 19:48. -
https://people.ast.cam.ac.uk/~xmmssc/xidops/xidobs/ukirt0210/almanac.t…
https://people.ast.cam.ac.uk/~xmmssc/xidops/xidobs/ukirt0210/almanac.txt25 Sep 2002: Dates: 19,20 Oct Almanac for Mauna Kea, Hawaii: long. 10 21 53 (h.m.s) W, lat. ... For the night of: Sat, 2002 Oct 19 --- Sun, 2002 Oct 20 Local midnight = 2002 Oct 20, 10 hr UT, or JD 2452567.917 Local Mean Sidereal Time at midnight = 1 -
https://people.ast.cam.ac.uk/~optics/dazle/f.clarke/cirpass-lines.txt
https://people.ast.cam.ac.uk/~optics/dazle/f.clarke/cirpass-lines.txt16 Jun 2015: 39 12726.1 20 12744.6 24 12749.3 45 12760.9 76 12776.0 32 12779.1 149 12798.0 57 12803.5 107 12824.8 25 12831.1 58 ... 2 8.25 15183.0 20 15236.8 90 15283.6 45 15328.2 177 15391.1 54 15427.9 163 15457.9 4 15496.6 17 15505.5 44 -
https://people.ast.cam.ac.uk/~vasily/data/sims/mw_props/mw_props_70074…
https://people.ast.cam.ac.uk/~vasily/data/sims/mw_props/mw_props_70074.txt15 Apr 2020: 2608 74668632223.9 10.1769616815 3.48234 20 0.2696 100279822327.0 25.9002630561 1.55953 21 0.2784 144845357997.0 37.5056873134 1.25616 22 0.2872 183505155393.0 ... 33 0.384 405891038822.0 25.3287299986 3.57104 34 0.3928 425625916701.0 21.5027620074 -
MGB thesis Chapter 6
https://people.ast.cam.ac.uk/~optics/tech/mgb_phd/chapter6.htm16 Jun 2015: The telescope has recently produced its first map, an image of the binary star Aur (Cappella) with a resolution of 20 milli-arcsecond. -
https://people.ast.cam.ac.uk/~vasily/data/sims/mw_props/mw_props_16650…
https://people.ast.cam.ac.uk/~vasily/data/sims/mw_props/mw_props_166507.txt15 Apr 2020: 2608 64889543823.3 9.68147973167 3.4933 20 0.2696 68070694079.5 11.7452688489 3.02241 21 0.2784 69248894303.4 9.46970055555 3.8902 22 0.2872 134918994568.0 ... 0 20.8602879391 4.84299 37 0.4192 487334334398.0 19.1010729778 5.46265 38 0.428 496170836077.0 -
Index of…
https://people.ast.cam.ac.uk/~xmmssc/internal/lockman-hole/gh/html/20 Sep 2004: Objects with i-mag < 20 only: differential [or cumulative [S&S vs Rutledge et al. -
https://people.ast.cam.ac.uk/~xmmssc/xidops/xidobs/props/badseeing.lis…
https://people.ast.cam.ac.uk/~xmmssc/xidops/xidobs/props/badseeing.list11 Sep 2003: 15.28, 7.05, 50.11, g, 2.06, rtser , 17.67, -11.88, 9.93, g, 2.17, wr110 , 18.14, -19.37, 0.37, g, 1.81, Mkn509 , ... 11, z, 3.20, ridge_1 , 18.44, -12.19, -0.02, z, 2.31, pks2126 , 21.49, -15.64, -41.87, z, 1.85,. -
https://people.ast.cam.ac.uk/~optics/fits/year2000_agreement.txt
https://people.ast.cam.ac.uk/~optics/fits/year2000_agreement.txt16 Jun 2015: 19 to 20 shortly. -
CIRPASS at the AAT picture gallery index
https://people.ast.cam.ac.uk/~optics/cirpass/World-tour/AAT/Pictures/16 Jun 2015: Last modified: Fri Feb 20 2004. -
https://people.ast.cam.ac.uk/~rgm/vhs/v4/PS-VHS-v4p2.log
https://people.ast.cam.ac.uk/~rgm/vhs/v4/PS-VHS-v4p2.log5 Jun 2007: 20 v1.0o Standard LaTeX Graphics (DPC,SPQR) (/usr/local/teTex/share/texmf.local/tex/latex/graphics/trig.sty Package: trig 1999/03/16 v1.09 sin cos tan (DPC) ) ... DECam.png. /focalplane.png] [19] [20] AED: last page setting LastPage [21] -
CIRSI Astronomical Images
https://people.ast.cam.ac.uk/~rgm/cirsi/astronomical_images/20 Feb 2000: Last modified: Sun Feb 20 23:34:32 2000. -
Other IFUs
https://people.ast.cam.ac.uk/~optics/cirpass/docs/other_ifu.html16 Jun 2015: number of lenses. 2 IFU each with 20 fibres, or one with 300 fibres (ARGUS mode). -
Index of…
https://people.ast.cam.ac.uk/~xmmssc/internal/lockman-hole/fits/html/20 Sep 2004: ps gif]. Objects with i-mag < 20 only: differential [ps gif] or cumulative [ps gif] (S&S vs Rutledge et al.
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