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41 - 50 of 350 search results for KaKaoTalk:vb20 200 |u:people.ast.cam.ac.uk where 0 match all words and 350 match some words.

  1. Results that match 1 of 2 words

  2. arX iv:a stro -ph/ 0504 086 v1 4 A ...

    https://people.ast.cam.ac.uk/~wyatt/srms05.pdf
    19 Apr 2006: higher surface brightness at r >200 AU compared to the r4 power law. ... but has slightlyhigher surface brightness at r > 200 AU compared to ther4 power law.

  3. Mon. Not. R. Astron. Soc. 000, 1–8 (2016) Printed ...

    https://people.ast.cam.ac.uk/~wyatt/ghmm16.pdf
    21 Jul 2016: A 200 km/svelocity range is shown around the stellar velocity in the heliocen-tric frame of 23.0 0.3 km/s (Torres et al. ... The wide-fit baseline yields a 10.5 sigma detection of 200.0 19.1 mK km/s.

  4. MNRAS 000, 1–17 (2023) Preprint 25 October 2023 Compiled ...

    https://people.ast.cam.ac.uk/~wyatt/ckkl23.pdf
    22 Mar 2024: 200. 0. 200. 400. µJy. /Bea. m. Figure 1. Naturally weighted ALMA 880𝜇m images of our BPMG M-dwarf sample. ... 0. 200. 400. µJy. /Bea. m. Figure 2. Naturally weighted ALMA 880𝜇m image of TYC 7443-1102-1.The stellar location is marked with a.

  5. MNRAS 000, 1–14 (2020) Preprint 8October 2020 Compiled…

    https://people.ast.cam.ac.uk/~wyatt/xkwy20.pdf
    8 Oct 2020: 2015).Assuming thepriors stated above,we ran LOFTI on the relative Gaia measurements until 200,000orbits were accepted, and plot the joint posterior distributions inFig. ... 160. 200. 240. []. 10 15 20. m [MJup]. m [MJup] = 1422.

  6. https://people.ast.cam.ac.uk/~rgm/wfcsur/jsc_ridos.txt

    https://people.ast.cam.ac.uk/~rgm/wfcsur/jsc_ridos.txt
    1 Mar 1998: Hence in total the project life-span would be 4 years, with a survey area of 100-200 square degrees in up to seven colour bands. ... Hence in total the project life-span would be 4 years, with a survey area of 100-200 square degrees in up to seven

  7. Hard XMM sources

    https://people.ast.cam.ac.uk/~xmmssc/internal/xsrc_select/xsrc_hr3-err_gt0.html
    27 Mar 2002: 0.853.08. A 1837. 200. 2001-02-22. Y. -1.7. -1.8. 20.7. 0. 22.6. ... 0.210.31. A 1837. 200. 2001-02-22. Y. -1.4. 1.4. 15.5. -1. 17.4.

  8. Graphics produced by IDL

    https://people.ast.cam.ac.uk/~vasily/sdss/orphan/orphan6.pdf
    10 Apr 2009: 2. 3. 4. log(. g). 4.0 3.9 3.8 3.7 3.6log(Teff). 300 200 100 0 100 200 300Radial velocity (Galactic frame). ... 0. 20. 40. 60. Dec. 250 200 150 100RA. Orphan Stream: 17 < g < 19 => 20 < BHB distance (kpc) < 50.

  9. Chapter 1 - Installation

    https://people.ast.cam.ac.uk/~rgm/cirsi/pixcel/pixcel_19990428_help/chapter1.htm
    23 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).

  10. Pixcel - Remote operation

    https://people.ast.cam.ac.uk/~rgm/cirsi/pixcel/pixcel_19990428_help/remote.htm
    23 Jan 2000: ALLOW=200.28.111.138. This is a comma separated list of machines which are allowed to connect to Pixcel.

  11. ESO Public Surveys Proposal Form Phase 1 1 Title: ...

    https://people.ast.cam.ac.uk/~rgm/vhs/v4/PS-VHS-v4p0.pdf
    5 Jun 2007: The Y-J colour is ESSENTIAL since the so called ’rare’ L and T dwarfs outnumberthe quasars by a factor of 200:1 based on the well established space densities of ... Observing efficiency % per tile 73.3 76.1 - - 69.9. Time for 8,200 sq deg = 5467

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