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61 - 70 of 363 search results for KaKaoTalk:vb20 200 |u:people.ast.cam.ac.uk where 0 match all words and 363 match some words.

  1. Results that match 1 of 2 words

  2. Debris discs around nearby solar analogues

    https://people.ast.cam.ac.uk/~wyatt/gwb09.pdf
    8 Jul 2009: e. upto approximately 200 au radius for stars at 12–15 pc distance. ... For five precise (G2 V) solar analogues,the fitted disc radii are 100–200 au (Krivov et al.

  3. LOCAL HEATING IN THE GALACTIC CENTER WESTERN ARC N. ...

    https://people.ast.cam.ac.uk/~wyatt/mtpf03.pdf
    19 Apr 2006: Dust emissionpeaks are resolved with source sizes of 200 to 500 (1.7 104 to4.3 104 AU).

  4. L141 The Astrophysical Journal, 532:L141–L144, 2000 April 1q 2000. ...

    https://people.ast.cam.ac.uk/~wyatt/ftpk00.pdf
    19 Apr 2006: Compared to the fullextent of the mid-IR–emitting size of the disk (200 AU), therelatively small values of the dust FWHM sizes suggest thatthe mid-IR emission is sharply peaked ... extends out to at least a radius of 100 (200 AU) fromthe star in the

  5. PDF/48/aa5873-06.pdf.url

    https://people.ast.cam.ac.uk/~wyatt/lwbd06.pdf
    14 Dec 2006: 2004), we estimate for the firsttime the detection rate of cold debris disks around field M-dwarfs with ages between 20 and 200 Myr. ... al. 2005), the Castor moving group(200 Myr), the Ursa Maj moving group (500 100 Myr asrevised by King et al.

  6. Searching for Saturn's Irregular Satellite Swarm with Spitzer

    https://people.ast.cam.ac.uk/~wyatt/kwss11.pdf
    29 Jun 2012: Stansberry. OFF ON IE IW. -600 -400 -200 0 200 400 600offset (Saturn radii). ... 400. -200. 0. 200. 400. offs. et (. Sat. urn. radi.

  7. https://people.ast.cam.ac.uk/~rgm/wfcsur/int_ao.txt

    https://people.ast.cam.ac.uk/~rgm/wfcsur/int_ao.txt
    1 Mar 1998: Name of PI and affiliation Names of CoIs with affiliation Postal and email address of PI Summary of proposal (max 200 words) List of targets with filter passbands & exposure times Page

  8. VIRCAM Pipeline: vircam_tfits.c Source File

    https://people.ast.cam.ac.uk/~wfcam/docs/vista/vircam_manual/vircam__tfits_8c-source.html
    10 Apr 2013: vircam_tfits.c. 00001 / $Id: vircam_tfits.c,v 1.13 2007/10/25 17:34:01 jim Exp $ 00002 00003 This file is part of the VIRCAM Pipeline 00004 Copyright (C) 2005 Cambridge Astronomy Survey Unit 00005 00006 This program is free software; you can

  9. Hard XMM sources

    https://people.ast.cam.ac.uk/~xmmssc/xidops/xidobs/ukirt0210/versn_200203/xsrc_hard3.html
    20 Mar 2002: 0.42. 0.24. A 1837. 200. 2001-02-22. ... 0.46. 0.39. A 1837. 200. 2001-02-22.

  10. 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).

  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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