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6 Mar 2009: Last modified: Fri Mar 6 09:52:24 GMT 2009.

29 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

29 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

29 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.

13 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].

20 Jul 2009: 7. VISTA update Raw data has been received via Garching for up to and including June 24.

14 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

30 Nov 2009: within 24 hours of the final bit of data being taken.

7 Jun 2009: takes 24 hours from observing finishing for the data to be transferred, verified and ingested here).

26 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

14 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.

12 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.

15 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).

19 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.

8 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.

12 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.

3 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

21 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.

25 Oct 2009: Rewriting equation 23 gives. Mlate = [1.471011 Imax/K]M 4/3? q13/3t1[(1e)13/3S(e)]1, (24).

19 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.

23 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