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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.
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