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  1. Results that match 1 of 2 words

  2. Index of /~vasily/sdss/subaru

    https://people.ast.cam.ac.uk/~vasily/sdss/subaru/
    2006-05-23 14:24. 10K.
  3. Index of /~vasily/data/Auriga

    https://people.ast.cam.ac.uk/~vasily/data/Auriga/
    Index of /vasily/data/Auriga. 2022-05-20 21:48. 5.8M. 2022-05-20 21:48. 2.5M. 2022-05-20 21:48. 2.0M. 2022-05-20 21:48. 4.9M. 2022-05-20 21:48. 1.2M. 2022-05-20 21:48. 2.1M. 2022-05-20 21:48. 1.3M. 2022-05-20 21:48. 7.3M. 2022-05-20 21:48. 12M.
  4. Index of /~vasily/data/catalogues

    https://people.ast.cam.ac.uk/~vasily/data/catalogues/
    2024-03-19 06:24. 1.8M. ... 2024-03-19 06:24. 564.
  5. PowerPoint Presentation

    https://people.ast.cam.ac.uk/~phewett/SandES2017/Lec2017_24.pdf
    24 Nov 2017: Structure and Evolution of Stars 1. Structure and Evolution of StarsLecture 24: Extreme and some Fun Stars. •
  6. INT Wide Angle Survey

    https://people.ast.cam.ac.uk/~rgm/wfcsur/
    1 Nov 2000: 162426. van P. field. 16 24.0 26 34. -. 1. o. x1. o. ... u'. 3560. 600. 600. 24.3. 25.2. 7.0. 26.5. 27.4. 9.2. g'.
  7. Processing state of WFC data night by night

    https://people.ast.cam.ac.uk/~xmmssc/xid/nights_status.php
    2. 2000-06-24. 2. WFS-nonXID. 0.083/0.005/0.020/15. ... 15. 2001-01-24. 7. ITP-AXIS. 0.081/0.005/0.021/19.
  8. WFCAM simulations

    https://people.ast.cam.ac.uk/~wfcam/docs/reports/simul/index.html
    3 Sep 2007: Passband. H. Magnitude zero-point. 24.8. Magnitudes. Sky brightness. 13.6. Mags/arcsec2. Magnitude limits. ... imcore_conf. only (Figure 23) and median magnitude difference (Figure 24) were made.
  9. CASU analysis of WFCAM commissioning data - III Microstep Offsets

    https://people.ast.cam.ac.uk/~wfcam/docs/reports/commissioning3/index.html
    24 Feb 2005: 06 -0.05 1052:1049:3 0.25 11.32 0.02 11.52 -0.23 0.19 -0.08 -0.09 1050:1049:4 0.24 11.32 0.02 ... Jim Lewis (jrl@ast.cam.ac.uk). Last modified: Wed Feb 16 14:10:24 2005.
  10. L93 The Astrophysical Journal, 570:L93–L96, 2002 May 10 �� ...

    https://people.ast.cam.ac.uk/~wyatt/jhkg02.pdf
    19 Apr 2006: 24(40 AU) in ground-based, near-infrared, coronagraphic images.They estimated the disk position angle as , inclination50 1027 deg, and minimum dust mass 0.4 M. ... Trilling &2. Brown (1998) report an H-band disk surface brightness thatfalls below 24 mag
  11. CASU analysis of WFCAM commissioning data - I

    https://people.ast.cam.ac.uk/~wfcam/docs/reports/commissioning/index.html
    2 Nov 2006: Z Y J H K Overall zero-point (count/s) 22.8 22.7 23.0 23.4 22.6 WFCAM (e-/s) 24.4 24.3 24.6 25.0 ... 24.2 [assumes above gain measures ok] UFTI (e-/s) ---- ---- 24.5 24.7 24.2.

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