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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 -
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]. -
https://people.ast.cam.ac.uk/~vasily/sdss/sgr/bellazzini_clusters.txt
https://people.ast.cam.ac.uk/~vasily/sdss/sgr/bellazzini_clusters.txt29 Jan 2009: 5.3 -55.7 Terzan 3 6.18 -24.8 NGC 5466 8.55 21.9 NGC 288 9.88 17.2 NGC 7089 10.14 -18.9 NGC 6426 -
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. -
New Page 1
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). -
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. -
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. -
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 -
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). -
Mon. Not. R. Astron. Soc. 000, 000–000 (2009) Printed ...
https://people.ast.cam.ac.uk/~wyatt/bwmm09.pdf19 Jun 2009: Recentsurveys have shown that 4% of stars exhibit 24 µm excess and 16% exhibit 70 µmexcess. ... Thisrun starts with an initial disc mass of 35 M and has 24 Mat the time of the LHB. -
arX iv:0 911. 3426 v1 [ astr o-ph .SR ...
https://people.ast.cam.ac.uk/~wyatt/pgdm09.pdf19 Nov 2009: The majority of SUNS and DEBRIS tar-gets also have photometry at 24 and 70 µm from the MIPS(Multiband Imaging Photometer and Spectrometer) instru-ment on the Spitzer space telescope, ... 90. -60. -30. 0. 30. 60. 90. 0 3 6 9 12 15 18 21 24. -
survey07_rev2.dvi
https://people.ast.cam.ac.uk/~wyatt/lwbm09.pdf21 Jul 2009: 1.50 -0.37 < 1.6GJ9809 M0 24.0 03 0.5 2.20 0.36 2.20 0.16 < 2.4. ... 2006), and excluding GJ526 at thisstage) makes the detection fraction to amount to 24.51.5 % in oursample of 50 M-dwarfs. -
Debris discs around nearby solar analogues
https://people.ast.cam.ac.uk/~wyatt/gwb09.pdf8 Jul 2009: All of our target stars have now been searched with Spitzer for de-bris discs, using Multiband Imaging Photometer for Spitzer (MIPS)at 24 and 70 μm wavelengths. -
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. -
/astro/data/upsand1/mpayne/PLANETESIMAL_DRIVEN_MIGRATION/plots/plot_31…
https://people.ast.cam.ac.uk/~wyatt/pwt09.pdf3 Sep 2009: 0.24), while its mass has further doubled to 0.4M.Only a very small amount of additional migration is observed. ... 0.24. Similarly, the mass of theouter-most body also increases significantly as the surfacedensityand the surface density ratio are -
Mon. Not. R. Astron. Soc. 000, 000–000 (0000) Printed ...
https://people.ast.cam.ac.uk/~wyatt/wbpc09.pdf25 Oct 2009: Rewriting equation 23 gives. Mlate = [1.471011 Imax/K]M 4/3? q13/3t1[(1e)13/3S(e)]1, (24). -
11626.dvi
https://people.ast.cam.ac.uk/~wyatt/swh09.pdf23 Jun 2009: June 23, 2009. Resolving the hot dust around HD69830 and η Corvi with MIDI andVISIR. R. Smith1, M.C. Wyatt1, and C.A. Haniff2. 1 Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge, CB3 0AHe-mail:rsed@ast.cam.ac.uk. 2
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