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29 Jan 2009: Fe/H]=-0.41+/-0.20 with a tail to -1.52. LMC-like [Fe/H] distribution? Kinematics. Ibata, Wyse, Gilmore, Irwin, Suntzeff 1997.

6 Mar 2009: uJy. Y. 1.02. 0.10. 60. 20.3. 20.9? 19.6. 20.2? J. 1.25. ... 0.18. 60. 19.9. 20.9? 19.2. 20.2? H. 1.65. 0.30. 60. 19.0.

13 May 2009: CASU Analysis of RAL VIRCAM data. 20-6-2006. 20-6-2006 [pdf]. ... Example WFCAM FITS header (based on INT CIRSI data). 30-06-2003. 20-06-2003 [fits].

14 May 2009: General Lecturing:. Given a very great number of lectures including seminars, conference reviews and paper presentations, popular lectures, including (for >20 years) talking to groups of local schoolchildren on general astronomy. ... Ph.D Awarded:

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

10 Apr 2009: 0. 20. 40. 60. Dec. 250 200 150 100RA. Orphan Stream: 17 < g < 19 => 20 < BHB distance (kpc) < 50. ... 2. 3. 4. log(. g). 0. 20. 40. 60. Dec. Orphan Stream: 17 < g < 19 => 20 < BHB distance (kpc) < 50.

28 Sep 2009: About 20 nights of data are still missing and Andy Adamson is investigating these.

26 Jun 2009: NAW said there is a GREAT meeting in Nice from November 19-20 and another small WG meeting about ground-based wide-field spectroscopic requirements at the IoA July 7-8.

29 Jan 2009: PRINT, 20!dpi/4., FORMAT=’(F30.18)’ Formatted printingt=STRING( $ print (1,2)1,2, FORMAT=’("(",I1,",",I2,")")’). 2. 2 File manipulation.

14 May 2009: SPIE, 290, 159 (1981). 20. Wright, J.F. and Mackay, C.D., The Cambridge Charge--Coupled Device (CCD) System'. ... Optical aperture synthesis on the INT. Gemini, Newsletter of RGO, No 20, 2.

8 Jul 2009: Thedisc is observed to be larger than the radius of 20 au inferred fora black-body SED (Zuckerman & Song 2004), suggesting some. ... excess is predicted to increase only slightly dur-ing such events and the dusty episode would last 20 Myr (Boothet al.

30 Mar 2009: nm. Using a special interference filter centred on 975.5 nm with a bandwidth of 20 nm, they could search between hydroxyl lines for so-called Lyman-α radiation.

3 Sep 2009: 0.01. 0.1. 1. 10. 5 10 15 20 25 30 35 40 45 50. ... Mou. ter /. ME. arth. Simulation Time. No BinaryBinary, a=20 AU, e=0.5.

12 Feb 2009: tcol = r1.5 M-0.5 (ρrdrDmax/Mtot) (12q-20)(18-9q)-1[11.25(e/I)2]-0.5/G(q,Xc). This can be solved to give:. ... Emission efficiency Qem=Qabs 1 for λ<D and (λ/D)n for λ>D (although there are emission features, e.g., 10 and 20 µm features of silicates

21 Jul 2009: For a statistical analysis, we combine these datawith our prior SCUBA and MAMBO-2 observations of 20 other M-dwarfs. ... This correction amounted to between 5% and 20%of the integrated flux density.

28 Jan 2009: The planets: van de Kamp (1982) proposed 2 planets of 0.5 and 0.7MJ in orbits of 12 and 20 years.

19 Jun 2009: have gas giants (planets with masses equal to orgreater than Saturn) within 20 AU which Marcy et al. ... LHBs is<12% (assuming that Saturn mass planets within 20 AUare required for an LHB).

23 Jun 2009: B 44.2 34.3 1.20 73840 Cal42.2 26.8 0.65 116870 Cal46.1 39.2 0.75 η Corvi Sci46.6 42.4 1.15 107218 Cal. ... 13.7 12.5 10 6.7Wavelength, um. 010. 20. 30. 40. Pix. el.

15 Sep 2009: sample (20 stars total) only weak constraints could be derived. Similarly, a submillimeter.

25 Oct 2009: S2d = 0.54e5/3(1 e2)4/3. (20). 2.4.3 Where do collisions occur, and at what velocity? ... have used the in-clination distribution function given by equation 2.20 of Krivov etal.

19 Nov 2009: 0. 20. 40. 60. 80. 100. 120. 0 0.2 0.4 0.6 0.8 1. ... 20. 30. 40. 50. 60. 70. 80. 90. 100. 2000 3000 4000 5000 6000 7000 8000 9000 10000.