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Educational and Outreach talks and activities for Carolin Crawford ...
https://people.ast.cam.ac.uk/~csc/newcv/2010talks.html24 Jul 2019: May. 24. Big numbers, stars and black holes. Talk to KS2 pupils at St James the Great School, Southwark as part of the Southwark Splash project. -
CIRSI ING 2000A
https://people.ast.cam.ac.uk/~optics/cirsi/ing/2000a/16 Jun 2015: WFS WFC June 24-29. ELAIS WFC June 30, July 1-2(ITP). Planning information. -
2001B information
https://people.ast.cam.ac.uk/~optics/cirsi/ociw/2001b/16 Jun 2015: Aug 10; 02 20 09 9 24.2. -
WFS Pipeline Processing
https://people.ast.cam.ac.uk/~mike/casu/WFCsur/pipeline.html4 Jun 1999: Photometry. approximate photometry at the 10% level can be obtained by using the following default CCD zero-points: U = 22.4, B = 24.5, V = 24.4, R = 24.4, I = ... The renormalised CCD gain is approximately 3.12 so to convert to photons/s magnitude zero -
Index of /~phewett/Vivienne_Spectra/RMpro/Work
https://people.ast.cam.ac.uk/~phewett/Vivienne_Spectra/RMpro/Work/2019-10-19 10:24. 31K. -
WFCAM Pipeline Design
https://people.ast.cam.ac.uk/~wfcam/docs/glossary.html24 Jan 2003: On 24 Jan 2003, 15:49. -
CIRPASS data reduction cookbook for data taken at the Geminiโฆ
https://people.ast.cam.ac.uk/~optics/cirpass/datared/cookbook_gemini.phpAndrew J. Dean. <ajd@ast.cam.ac.uk>. Last modified: Mon Mar 24 11:03:08 2003. -
Summary
https://people.ast.cam.ac.uk/~optics/cirpass/summary.bak16 Jun 2015: Last modified: Wed Nov 24 12:12:20 1999. -
Research
https://people.ast.cam.ac.uk/~nmadhu/Nikku_Madhusudhan/Research.html27 Aug 2022: First statistical retrieval method for exoplanetary atmospheres (Madhusudhan & Seager, 2009, ApJ, 707, 24). โข -
Cambridge XMM XIDOPS WWW Page
https://people.ast.cam.ac.uk/~xmmssc/xidops/xidobs/obsplan/20041224/24 Dec 2004: XMM XID Observing Resources: 2004 Dec 24-26 run. ... Last modified: Fri Dec 24 17:06:56 2004. -
WFS Status
https://people.ast.cam.ac.uk/~mike/casu/WFCsur/wfsj0801.html24 Nov 2000: 41 39 00 j2000 U g' r' i' z wfsj08014019_019 08 00 24.8 38 59 00 j2000 wfsj08014019_020 08 00 24.4 39 19 00 j2000 wfsj08014019_021 ... j2000. For summary of fields passing DQC criteria click here. Last modified: Fri Nov 24 08:50:18 2000. -
Astrometric distortions
https://people.ast.cam.ac.uk/~mike/casu/WFCsur/distortion.html4 Jun 1999: The INT handbook gives k1 = 24.7 "/mm and k3 = -9.202e-05 "/mm3. ... Last modified: Fri Jun 4 18:24:01 1999. -
CIRSI - LCO Base WWW Page
https://people.ast.cam.ac.uk/~optics/cirsi/ociw/lco1999may/16 Jun 2015: Last modified: Wed Nov 24 12:44:25 1999. Maintained by Richard G. -
MNRAS 000, 1โ17 (2022) Preprint 28 June 2022 Compiled ...
https://people.ast.cam.ac.uk/~wyatt/mcjm22.pdf22 Mar 2024: ๐กvis =. ๐๐ฮ๐. 3๏ธ2ln(2)๐. ๐ฮ๐2๐. (24). With this definition, the steady-state surface density ( ยค๐+/(3๐๐)) isindependentofฮ๐,andmatchesthesurfacedensityobtainedsolvingthe radial viscous evolution and the -
The STARS Web Pages
https://people.ast.cam.ac.uk/~stars/archive/data.html11 Dec 2003: 20. Ne. , 16 -. 24. Mg, 17 - r, 18 - L, 19 -. , 20 -. , 21 -. , 22 -. , 23 - k. ... Edd. , 30 - w.l. 23 is the square of the radius of gyration; 24-26 are homology invariants; 30 is the convective velocity times the mixing length. -
WFC - CCD Characteristics
https://people.ast.cam.ac.uk/~mike/casu/WFCsur/gain.html20 Apr 1999: 25.6. 25.7. 25.6. 24.9. #2. 23.8. 25.6. 25.6. 25.6. 25.0. #3. -
https://people.ast.cam.ac.uk/~vasily/sdss/dropouts/dropouts.txt
https://people.ast.cam.ac.uk/~vasily/sdss/dropouts/dropouts.txt3 Jun 2011: 200.76777495 3.7214707 25.29 24.61 23.14 23.00 19.97 4 140.21862225 30.4611002 23.07 23.08 22.58 20.84 19.00 5 ... 85138 51.536387 24.02 23.72 23.09 21.47 20.74. -
WFS Status
https://people.ast.cam.ac.uk/~mike/casu/WFCsur/wfsjpleiades.html16 Dec 2000: Nominal grid centre: 03 47 00.00 24 00 00.0 J2000 Pleiades RA step size : 30.00 arc mins Dec step size : 20.00 arc mins Filters: I Z Nominal ... Exposures: 600s, 1200s Nominal 3 degree x 3 degree grid Passbands wfsj03472400-iz01 3 49 18.07 24 49 13.0 -
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. -
The STARS Web Pages
https://people.ast.cam.ac.uk/~stars/archive/descript.html9 Oct 2003: in the code). There is one more possible output (. fort.24. ),
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