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1 - 10 of 109 search results for TALK:PC53 20 |u:people.ast.cam.ac.uk where 0 match all words and 109 match some words.

  1. Results that match 1 of 2 words

  2. About the Instrumentation Group

    https://people.ast.cam.ac.uk/~optics/about.htm
    16 Jun 2015: IOA Instrumentation Group. Welcome. The Astronomical Instrumentation Group is currently building two fast-track NIR instruments which will provide much improved performance over instruments currently available. COHSI is a spectrograph for low

  3. https://people.ast.cam.ac.uk/~optics/cirpass/datared/BINTABLE.txt

    https://people.ast.cam.ac.uk/~optics/cirpass/datared/BINTABLE.txt
    16 Jun 2015: 17. 18. 33. 1. 18. 19. 34. 0. 19. 20. 35. ... 1. 20. 21. 34. -2. 21. 22. 33. -1. 22. 23.

  4. https://people.ast.cam.ac.uk/~optics/cirpass/datared/list_xml.txt

    https://people.ast.cam.ac.uk/~optics/cirpass/datared/list_xml.txt
    16 Jun 2015: GY-11 16:23:20.8 -24:17:21 2349.8-2601 16:23:49.8 -24:26:01 CRBR-14 16:23:17.3 -24:19:25 GY-10 ... 23:20.8 -24:17:08 2MASSW-J2049197-194432 20:49:19.74 -19:44:32.5 2MASSW-J2147446-264406 21:47:44.62 -26:44:06.6 2MASSW-J2206228-204705

  5. design study report

    https://people.ast.cam.ac.uk/~optics/cirpass/design-study-a.htm
    16 Jun 2015: A slit length of 20 arcsec is 50 pixels so we have a total multiplex gain of 80 (for a limiting magnitude of J=23 there are 160 galaxies in a ... The analysis shows that despite the uncertainties in knowing e and t for the real instrument the uncertainty

  6. Other IFUs

    https://people.ast.cam.ac.uk/~optics/cirpass/docs/other_ifu.html
    16 Jun 2015: number of lenses. 2 IFU each with 20 fibres, or one with 300 fibres (ARGUS mode).

  7. CIRPASS software specification

    https://people.ast.cam.ac.uk/~optics/cirpass/docs/soft_spec.html
    16 Jun 2015: Last modified: Thu Apr 17 11:44:20 2003.

  8. CIRPASS TECHNICAL STUDY

    https://people.ast.cam.ac.uk/~optics/cirpass/hdf.htm
    16 Jun 2015: The galaxy sample was broken down into three magnitude bins: J < 20, 20 < J < 22, and J > 22. ... The bright galaxy sample (J < 20) requires somewhat larger aperture sizes than the fainter sample does.

  9. https://people.ast.cam.ac.uk/~optics/cirpass/Software/PixCel/PixCel_IR…

    https://people.ast.cam.ac.uk/~optics/cirpass/Software/PixCel/PixCel_IR_090101/PixcelD.SUP
    16 Jun 2015: gci2d.dll:"C:mgbsrcgci2capellac.cpp" ignore alloc_conflict in file gci2d.dll:"C:mgbsrcgci2pdcigrab.cpp" ignore alloc_conflict in module gci2d.dll ignore bad_address(20,18) in file

  10. CIRPASS assemblies May02

    https://people.ast.cam.ac.uk/~optics/cirpass/srm/CIRPASS%20assemblies%20May02.htm
    16 Jun 2015: Refrigeration Plant. This is the 220V 60 Hz version which will probably be used in Chile (with 20% reduced cooling capacity due to the unusual electrical supply at Gemini-S).

  11. Summary

    https://people.ast.cam.ac.uk/~optics/cirpass/summary.bak
    16 Jun 2015: Last modified: Wed Nov 24 12:12:20 1999.

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