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VHS nominal exposure time and flux limits Waveband Exposure ...
https://people.ast.cam.ac.uk/~rgm/vhs/vhs-summary.html6 Mar 2009: Last modified: Fri Mar 6 09:52:24 GMT 2009. -
CASU WFCAM/VISTA Documentation (Sorted)
https://people.ast.cam.ac.uk/~wfcam/documentation_sorted.html13 May 2009: Pipeline science requirements. 23-10-2002. 24-01-2003 [ps]. ... Pipeline document (old version submitted to CDR). 23-10-2002. 24-01-2003 [ps]. -
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https://people.ast.cam.ac.uk/~cdm/cdm_CV_130509.htm14 May 2009: 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 -
https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_090715.txt
https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_090715.txt20 Jul 2009: 7. VISTA update Raw data has been received via Garching for up to and including June 24. -
https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_091119.txt
https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_091119.txt30 Nov 2009: within 24 hours of the final bit of data being taken. -
https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_090518.txt
https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_090518.txt7 Jun 2009: takes 24 hours from observing finishing for the data to be transferred, verified and ingested here). -
https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_090619.txt
https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_090619.txt26 Jun 2009: 6. WFCAM update. MR has further automated the WFCAM raw data ingestion and verification, which, as noted before, is ready and assembled to go roughly 24 hours after the night's -
Debris disk dynamical theory Mark Wyatt Institute of Astronomy, ...
https://people.ast.cam.ac.uk/~wyatt/MarkWyatt_Spitzer2008Conference.pdf12 Jan 2009: Spitzer imaging of Vega disk. 850µm (Holland et al.). 24 and 70µm (Su et al. ... Diameter, D. σ(D), AU2. Dmin. Dmax. Evolution of size distribution. Steady-state evolution explains 24 and 70µm stats. -
Craig Mackay
https://people.ast.cam.ac.uk/~cdm/cdm_pub_list_130509.htm14 May 2009: 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. -
Planets and Debris Disks: Results from a Spitzer/MIPS Search ...
https://people.ast.cam.ac.uk/~wyatt/bbcr09.pdf15 Sep 2009: 24 µm, indicative of warm dust in the inner system analogous to that produced. ... 16 –. wavelength (13 at 70 µm, plus HD 69830 at only 24 µm).
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