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1 - 10 of 33 search results for TALK:PC53 20 |u:people.ast.cam.ac.uk where 0 match all words and 33 match some words.

  1. Results that match 1 of 2 words

  2. 03Q4m2_casu_deliverables.xlsWP CASU WP name /sub task / 03Q4…

    https://people.ast.cam.ac.uk/~wfcam/docs/monthly_reports/03Q4m2_casu_deliverables.pdf
    1 Dec 2003: 2.2 data reduction specification document 20. Simon Hodgkin Page 1 1/12/03.

  3. 1 Acronyms and Abbreviations

    https://people.ast.cam.ac.uk/~wfcam/docs/esotemplates/Document%20Management%20Plan_JMD_V5.0_260302.doc
    25 Apr 2003: 2.0. 20/6/01. 3b. File Name Convention corrected from ‘FFFFF’ to ‘DDDDD’. ... Annex A: VISTA Document Numbering System 18. Annex B: VISTA Phase B Product Codes 20.

  4. 2.1 Example HDSTRACE of WFCAM container file

    https://people.ast.cam.ac.uk/~wfcam/docs/headers_0p6.doc
    14 Aug 2003: AMEND = 1.769 / Airmass at end of observation. TELRA = 20.0123456 / [h] Current telescope right ascension. ... TELDEC = 29.9876543 / [deg] Current telescope declination. GSRA = 20.0103456 / [h] Right ascension of guide star.

  5. 2.1 Example HDSTRACE of WFCAM container file

    https://people.ast.cam.ac.uk/~wfcam/docs/headers_1p1.doc
    31 Oct 2003: AMEND = 1.769 / Airmass at end of observation. TELRA = 20.0123456 / [h] Current telescope right ascension. ... TELDEC = 29.9876543 / [deg] Current telescope declination. GSRA = 20.0103456 / [h] Right ascension of guide star.

  6. Cambridge XMMSSC Internal pages

    https://people.ast.cam.ac.uk/~xmmssc/internal/
    10 Feb 2003: XMM Subaru Deep Survey (SDS) programme. Last modified: Mon Feb 10 20:16:49 2003.

  7. H:\ukirt\WFCAM\DOCUMENTS\Active\Science array tests.doc Document…

    https://people.ast.cam.ac.uk/~wfcam/docs/ScienceArrayTests.pdf
    8 Jan 2003: The result showed an extremely faint residual image in the first dark (20 seconds after saturation) aftersaturation at a level of 1.8E-4 of the saturation level. ... The situation is worse in channels 2and 4 (in this diagram) where the decay occupies

  8. https://people.ast.cam.ac.uk/~wfcam/docs/cat_with_compress.txt

    https://people.ast.cam.ac.uk/~wfcam/docs/cat_with_compress.txt
    6 May 2003: brightness (counts/pixel) SKYNOISE= 13.92 / Pixel noise at sky level (counts) THRESHOL= 20.89 / Isophotal analysis threshold (counts) MINPIX = 4 / Minimum size for images (pixels) CROWDED = 1 / Crowded field analysis

  9. https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_030924.txt

    https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_030924.txt
    26 Sep 2003: 3. Report from RAL camera design review meeting held 17-19th Sept PSB reported that the 3 day meeting, attended by 20-25 delegates, was very interesting.

  10. https://people.ast.cam.ac.uk/~wfcam/docs/wfcam01.txt

    https://people.ast.cam.ac.uk/~wfcam/docs/wfcam01.txt
    10 Jul 2003: MJI said that at S/N 5 20% photometry, you are normally at 50% completeness. ... PATT (AA): Skyprobe is still a possibility. 20% of WFCAM to non-UKIDSS (17 proposals).

  11. https://people.ast.cam.ac.uk/~wfcam/talks/ukidss_nov2003.txt

    https://people.ast.cam.ac.uk/~wfcam/talks/ukidss_nov2003.txt
    27 Nov 2003: Equatorial (good for VISTA) (iii) dec 20 degrees (X=1.0) - go overhead (iv) =100 stars on a chip 1.

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