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81 - 100 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. https://people.ast.cam.ac.uk/~vasily/sdss/dropouts/dropouts.txt

    https://people.ast.cam.ac.uk/~vasily/sdss/dropouts/dropouts.txt
    3 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

  3. https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_030417.txt

    https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_030417.txt
    5 May 2003: JRL to ponder. The tape systems will be Ultrium LTO-2 with a native capacity of 200 GB.

  4. Prochaska atomic data

    https://people.ast.cam.ac.uk/~rfc/atomdat.html
    22 Mar 2005: O I  922.200  2.45e-4 3.21e6  M03. O I  921.857  1.08e-3 1.00E7  M03.

  5. Educational and Outreach talks and activities for Carolin Crawford ...

    https://people.ast.cam.ac.uk/~csc/newcv/2016talks.html
    24 Jul 2019: Jul. 200. Astronomical research at Cambridge. Four talks to Chinese high-school students attending the CUKDC courses.

  6. The APM Facility: Overview

    https://people.ast.cam.ac.uk/~mike/casu/apm/apm_intro.html
    30 Nov 1998: A standard 200 Mhz Pentium-pro PC running linux is used to both control the microdensitometer and perform all the on-line data analysis. ... By using a flying spot'' sampling rates of 200 KHz are readily attained.

  7. Educational and Outreach talks for Carolin Crawford in 2008 ...

    https://people.ast.cam.ac.uk/~csc/newcv/2008talks.html
    24 Jul 2019: Mar. 200. Black holes for beginners. Talk to yr7 students at Sawston Village College as part of the CU Science Roadshow.

  8. VizieR Search Page

    https://people.ast.cam.ac.uk/~rgm/apmcat/cds/VizieR.html
    18 Jun 2001: Maximum Entries per table:. 10. 20. 50. 100. 200. 1000. 9999.

  9. NAME: write_wfcdqc_dbd PURPOSE: produce a dbd file so that ...

    https://people.ast.cam.ac.uk/~xmmssc/xidops/docs/idl/write_wfcdqc_dbd.html
    19 Feb 2001: Default is 200 OUTPUTS: db: string, name of output database. EXAMPLE: write_wfcdqc_dbd,'dbase',maxentries=200 DEPENDENCIES: RESTRICTIONS: UNTESTED CALLED PROCEDURES AND FUNCTIONS: astrolib functions MODIFICATION HISTORY: 18-Feb-2001

  10. The Electronics

    https://people.ast.cam.ac.uk/~mike/casu/pds/pdselec.html
    18 Aug 1999: The new electronics to control the two axes are essentially identical and are built on a single commercial prototyping card connected to the isa bus of a 200 MHz PC.

  11. Educational and Outreach talks for CS Crawford in 2007 ...

    https://people.ast.cam.ac.uk/~csc/newcv/2007talks.html
    24 Jul 2019: Institute of Physics lecture at Hertfordshire University. Nov. 200. The Planets.

  12. Hard XMM sources

    https://people.ast.cam.ac.uk/~xmmssc/internal/xsrc_select/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.

  13. Data Aquisition

    https://people.ast.cam.ac.uk/~mike/casu/pds/pdsupg.html
    18 Aug 1999: It was been decided to replace the entire system with a single 200 MHz PC running Linux, similar to the new APM system.

  14. Useful Material and Other Surveys

    https://people.ast.cam.ac.uk/~rgm/wfcsur/other_surveys.html
    11 May 2000: m. 05.72. s. , 34. o. 16' 47.5''. 57.4, 67.3. 200.4, 46.0.

  15. Draft version March 10, 2020Typeset using LATEX twocolumn style ...

    https://people.ast.cam.ac.uk/~wyatt/edhm20.pdf
    10 Mar 2020: 0.1 0.3 1.0 3.0 10.0Age [Gyr]. 200. 0. 200. 400. 600.

  16. arX iv:1 408. 4116 v1 [ astr o-ph .EP ...

    https://people.ast.cam.ac.uk/~wyatt/kw14.pdf
    22 Aug 2014: 2/2 as our like-lihood function. Chains with an ensemble of 200 “walkers” areinitialised with parameters that vary randomly1% from theχ2 fitting results, and then run for 50 steps as ... 6 shows that a typical warmcomponent would haveTwarm = 200

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

    https://people.ast.cam.ac.uk/~rgm/vhs/v4/PS-VHS-v4p0_fjc.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

  18. MNRAS 000, 1–14 (2018) Preprint 8 January 2019 Compiled ...

    https://people.ast.cam.ac.uk/~wyatt/mybf19.pdf
    8 Jan 2019: Weoriented the disc such that the gap is narrowest towardsω 100 (PA 200). ... m. 1] NE. SW. SW-NE. 0 50 100 150 200. Deprojected distance [au].

  19. MNRAS 000, 1–12 (2015) Preprint 12 May 2016 Compiled ...

    https://people.ast.cam.ac.uk/~wyatt/mmsw16.pdf
    17 May 2016: The presented im-ages are the median of 200 iterations. We observe a noise level of. ... Moreover, the value of Ṁ ishighly dependant on Q?D which could vary between 200 and 10.

  20. Other NIR spectrographs

    https://people.ast.cam.ac.uk/~optics/cirpass/docs/other_nirspec.html
    16 Jun 2015: ISAAC (LW). 8m VLT UT1. 2-5. 1500,700,450,200 (lres). 8000,4000,2500,1250 (mres). 41.5.

  21. Hard XMM sources

    https://people.ast.cam.ac.uk/~xmmssc/internal/xsrc_select/xsrc_hr3-err_gt0_b14.html
    28 Mar 2002: 5. 56.2. 14h0m39.85s. -11d5m48.2s. 48.24. 0.5. 1.6. 1.7. 0.200.26. -0.340.20. 0.420.24. ... 0.853.08. A 1837. 200. 2001-02-22. Y. -1.7. -1.8. 20.7. 0. 22.6.

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