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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. -
https://people.ast.cam.ac.uk/~vasily/sdss/orphan/orphan_south_fields.t…
https://people.ast.cam.ac.uk/~vasily/sdss/orphan/orphan_south_fields.txt29 Jan 2009: 19 167.94027 -11.87500 20 166.64250 -11.87500 21 165.34473 -11.87500 22 168.65123 -13.42500 23 167.34556 -13.42500 24 166.03988 -13.42500 25 ... 21.17500 38 171.17104 -21.17500 39 169.80908 -21.17500 40 173.37749 -22.72500 41 172.00060 -22.72500 42 -
lecture7_debrisdiskmod
https://people.ast.cam.ac.uk/~wyatt/lecture7_debrisdiskmod.pdf12 Feb 2009: The largest fragment in a collision, flr = Mlr/M is given by Q < QD flr = 1 – 0.5 (Q/QD) Q > QD flr = 0.5(QD/Q)1.24. -
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). -
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]. -
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. -
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. -
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. -
SOMs 4 OGLE
https://people.ast.cam.ac.uk/~vasily/ogle_som/map.html29 Jan 2009: Cataclysmic/Eruptive/Microlensing. Node x=8, y=25. Node x=9, y=26. Node x=9, y=24. Node x=8, y=23. -
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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