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MNRAS 000, 1–11 (2015) Preprint 9 November 2018 Compiled ...
https://people.ast.cam.ac.uk/~wyatt/khhw18.pdf9 Nov 2018: In total the datacomprise four years of photometry for roughly 200,000 dis-tinct stars. -
INT Wide Angle Survey
https://people.ast.cam.ac.uk/~rgm/wfcsur/1 Nov 2000: 07 50.0 20 30. 200, 22. 1. o. x1. o. vi. -
https://people.ast.cam.ac.uk/~optics/cirpass/datared/BINTABLE.txt
https://people.ast.cam.ac.uk/~optics/cirpass/datared/BINTABLE.txt16 Jun 2015: 13. -5. 199. 200. 12. -4. 200. 201. 11. -3. 201. -
Chapter 1 - Installation
https://people.ast.cam.ac.uk/~rgm/cirsi/pixcel/pixcel_19990428_help/chapter1.htm23 Jan 2000: IBM or 100% compatible 200 MHz or better Pentium PC. Hard disk with at least 100 Mbytes of free space (a lot more if you are storing images on this disk). -
Hard XMM sources
https://people.ast.cam.ac.uk/~xmmssc/internal/xsrc_select/xsrc_hard2.html20 Mar 2002: 0.49. 0.20. A 1837. 200. 2001-02-22. -
Educational and Outreach talks and activities for Carolin Crawford ...
https://people.ast.cam.ac.uk/~csc/newcv/2015talks.html24 Jul 2019: Mar. 40. Solar Eclipses. Year 8 at Harlow Academy. Mar. 200. -
Difference imaging
https://people.ast.cam.ac.uk/~wfcam/docs/reports/subtract2/index.html11 Jun 2004: These subsections are roughly 1000 x 1000 pixels in size centred at (1024,2048) with the intensity scaled linearly from the average "sky" level to cover the range /-200 counts in -
Chapter 4 - Controls Reference
https://people.ast.cam.ac.uk/~rgm/cirsi/cirsi_pixel_ir_docs_19981101/chapter4.htm15 Nov 1998: Base Electronics base pixel value, typically 200-1000 and is updated periodically. -
1906.08797
https://people.ast.cam.ac.uk/~wyatt/smkb19.pdf20 Nov 2019: temperature, and 40 K for the modified blackbody (theblackbody function is divided by 0.9 beyond 200 µm)of the disk. ... 230.02 mag 1J 1.2 5.420.03 mag 5H 1.6 5.280.04 mag 5KS 2.2 5.200.02 mag 5. -
ESO Public Surveys Proposal Form Phase 1 1 Title: ...
https://people.ast.cam.ac.uk/~rgm/vhs/v4/PS-VHS-v4p1.pdf5 Jun 2007: a factor of 200:1 based onthe well established space densities of the foreground L and T dwarfs. ... Observing efficiency % per tile 73.3 76.1 - - 69.9. Time for 8,200 sq deg = 5467 tiles of 1.5 sq degTotal Elapsed Hours - - 373 - 391. -
Microsoft PowerPoint - wyattpub
https://people.ast.cam.ac.uk/~wyatt/wyatt_kobe06.pdf24 Apr 2007: Spiral structure at 200 AU implies planet at 150 AU• Same structure seen in Saturn’s rings (Charnoz et al. ... Numerical integrations of star, migrating planet, 200 planetesimalsgiving capture probabilities for 3:2 resonance:. -
MASS AND TEMPERATURE OF THE TWA 7 DEBRIS DISK ...
https://people.ast.cam.ac.uk/~wyatt/mkw07.pdf3 Jul 2007: 2006). b >0.0096 60c Kalas et al. (2006). Eri. K2 3 730 200 40 1.5 850 0.1 85 Sheret et al. ... 2004)GJ 842.2. M0.5 20.9 200 25 4.6 850 28 5 13 Lestrade et al. -
Draft version March 24, 2022Typeset using LATEX twocolumn style ...
https://people.ast.cam.ac.uk/~wyatt/hycd22.pdf22 Mar 2024: 6 Hull et al. 200 100 0 100 200Position along major axis (au). -
Submitted to ApJ 16 July 2006, Accepted 3 October ...
https://people.ast.cam.ac.uk/~wyatt/wsgb07.pdf2 Nov 2006: belt width isdr = 0.5r; planetesimal strength is Q?D = 200 J kg. ... kg m3, e = 0.05, e/I = 1,Q?D = 200 J kg. -
arX iv:1 009. 0248 v1 [ astr o-ph .SR ...
https://people.ast.cam.ac.uk/~wyatt/sgbr10.pdf2 Sep 2010: 0.5. 1-50. 51-100. 101-150. 151-200. 201-250. 251-300. 301-350. 351-400. 401-450. 451-500. -
ApJ accepted, 7 November 2005Preprint typeset using LATEX style ...
https://people.ast.cam.ac.uk/~wyatt/wyat06.pdf19 Apr 2006: ac-count and 200 dust particles were produced with exactlythe same positions and velocities as the parent popula-tion. ... for the librationparameters to be fitted for each particle, and the meanparameters for each population of 200 dust grains to -
MNRAS 000, 1–21 (2016) Preprint 23 September 2016 Compiled ...
https://people.ast.cam.ac.uk/~wyatt/mdwk16.pdf23 Sep 2016: 4 L. Matrà et al. -200 -100 0 100 200. -60-40-20. ... 1. CO J=2-1N. E. -200 -100 0 100 200Stellocentric distance (AU). -
MNRAS 000, 1–16 (2022) Preprint 6 July 2023 Compiled ...
https://people.ast.cam.ac.uk/~wyatt/bwmd23.pdf11 Jul 2023: Rrk = Σirki=ick. ni4(Dk Di). 2 πvrelV. , (11). 100 200 300 400 500k-i. ... 0.08. 0.10. Vol. atile. Fra. ctio. n. 0 Myrs 10 Myrs 100 Myrs 200 Myrs. -
Hard XMM sources
https://people.ast.cam.ac.uk/~xmmssc/internal/xsrc_select/xsrc_hr2-err_gt0_b14.html28 Mar 2002: 0.901.79. A 1837. 200. 2001-02-22. Y. 2.0. -2.1. 20.6. 0. 22.4. ... 0.220.28. A 1837. 200. 2001-02-22. Y. 4.1. 0.3. 17.7. -2. 19.5. -
Educational and Outreach talks and activities for Carolin Crawford ...
https://people.ast.cam.ac.uk/~csc/newcv/2011talks.html24 Jul 2019: Oct. 200,180. X-ray Astronomy. Talk to the National Federation of Astronomical Societies.
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