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https://people.ast.cam.ac.uk/~optics/cirsi/ociw/g133_dupont.tcs
https://people.ast.cam.ac.uk/~optics/cirsi/ociw/g133_dupont.tcs16 Jun 2015: position! G133_NW_D 01 03 42.43 -06 34 24.2 J2000.0 G133_NW_A 01 03 29.57 -06 34 24.2 J2000.0 G133_NW_C 01 ... G133_NE_D 01 04 30.43 -06 34 24.2 J2000.0 G133_NE_A 01 04 17.57 -06 34 24.2 J2000.0 G133_NE_C 01 04 -
https://people.ast.cam.ac.uk/~optics/cirsi/ociw/xmm-sds-1_dupont.tcs
https://people.ast.cam.ac.uk/~optics/cirsi/ociw/xmm-sds-1_dupont.tcs16 Jun 2015: position! XMM-SDS-1-C_D | 02:18:06.41 | -04:58:24.2 | 2000 | 0 | XMM-SDS-1-C_A | 02:17:53.59 | -04:58:24.2 | 2000 | 0 | ... SDS-1-C_X | 02:18:00.00 | -05:00:00.0 | 2000 | 0 | XMM-SDS-1-NW_D | 02:17:42.41 | -04:52:24.2 | 2000 | 0 | -
https://people.ast.cam.ac.uk/~optics/cirsi/ociw/xmm-lbqs2215_dupont.tc…
https://people.ast.cam.ac.uk/~optics/cirsi/ociw/xmm-lbqs2215_dupont.tcs16 Jun 2015: position XMM-LBQS2215-C_D | 22:15:38.71 | -17:42:24.2 | 2000 | 0 | XMM-LBQS2215-C_A | 22:15:25.29 | -17:42:24.2 | 2000 | 0 | ... 15:32.00 | -17:44:00.0 | 2000 | 0 | XMM-LBQS2215-NW_D | 22:15:13.70 | -17:36:24.2 | 2000 | 0 | XMM-LBQS2215-NW_A | -
Observing guide for CIRSI (WFIRC) at LCO du Pont ...
https://people.ast.cam.ac.uk/~optics/cirsi/cirsi-guide-lco-0.6.html16 Jun 2015: s recorded, eg: 19991118,19,20,21,22,23,24 c) In the afternoon, make a backup copy to stay on the mountain. ... of 750 kHz for Nov 21,22,23 (LCIRS) observations, and 666.7 kHz for Nov 24,25,26,27 (IoA) observations, and previously at 428 kHz. -
CIRPASS TECHNICAL STUDY
https://people.ast.cam.ac.uk/~optics/cirpass/hdf.htm16 Jun 2015: Even more puzzling is the fact that the galaxy used in the VIRMOS simulation has I = 21, while the galaxies used for the AUSTRALIS study have 24 < I < 25. -
New Page 1
https://people.ast.cam.ac.uk/~optics/people/cdm_CV_130509.htm16 Jun 2015: Taught the Introductory Astrophysics Lecture course, 24 lectures, 1998-2001 inclusive, and Topics in Contemporary Astrophysics, 2002-6 and 2008-present. ... Ph.D Awarded: 24.4.87. 8. Student: C A Haniff, Admission Date: 1.10.84, Title: High resolution -
design study report
https://people.ast.cam.ac.uk/~optics/cirpass/design-study-a.htm16 Jun 2015: Elston and Barden (NOAO newsletter #19, 1 Sept 1989) reached a magnitude of R=22.3 (approximately B=24) by using a beam-switching technique. ... A spreadsheet showing the estimated system throughput is attached. The peak efficiency is 24%. -
Craig Mackay
https://people.ast.cam.ac.uk/~optics/people/cdm_pub_list_130509.htm16 Jun 2015: ApJ, 270, 342 (1983). 24. Mackay, C.D. and Astill, D.M., CCD Development at Cambridge, England'. ... 31. Mackay, C.D., CCDs in Astronomy'. Ann. Rev. Ast. And Astrophys., 24, 255, 1986. -
arX iv:1 501. 0131 9v1 [as tro- ph.E P] ...
https://people.ast.cam.ac.uk/~wyatt/wbkr15.pdf8 Jan 2015: K2.5V 0.072 1.30 n (T08)9826 υ And 01:36:47.84 41:24:19.6 3.5 F9V 0.136 2.36 n (A13) n ... 55.84 -09:27:29.7 3.2 K2V 0.172 7.39 n (A13) y (B09)22484 LHS 1569 03:36:52.38 00:24:06.0 14.0 F8V -
This is the text of the SAM microcode that ...
https://people.ast.cam.ac.uk/~optics/cirsi/SAM/cirsi_sam_microcode_code_27may98.html16 Jun 2015: else = normal but reset after each line also pick up y-size from adds_24 9/6/97 4.09: Modified Black level read to enable proper set-up ... 18 % RAMA5 / LINE % F6 @ 19 % HOLD / LSYNC % F7 @ 20 % RESI / PIXEL % F8 @ 22 % OUT / OPEN1 % F9 @ 23 % RESET /
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