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201 - 210 of 734 search results for news |u:people.ast.cam.ac.uk

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  2. Quanz_et_al_ESA_white_paper_MIR_interferometry_revised

    https://people.ast.cam.ac.uk/~wyatt/qabb22.pdf
    22 Mar 2024: Therefore, tackling a prime objective of exoplanet science and understanding how unique or common planets like our Earth are in our galactic neighborhood will require a new, dedicated approach. ... below). 15. 2.3 Timing for a space-based mid-infrared

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

    https://people.ast.cam.ac.uk/~wfcam/docs/onsky.txt
    19 Aug 2003: detectors will be being used in a new mains power environment, attached to a telescope, and may have noise properties different to those measured in the lab.

  4. Quasars and Galaxies at the Highest Redshifts

    https://people.ast.cam.ac.uk/~rgm/presentations/20050922-Crafoord-Symposium.ppt
    8 Mar 2006: GOOD NEWS. The 1.0 to 1.8 micron IR sky is very dark between the OH lines which contain 95% of broad band background. ... THE NOT SO GOOD NEWS. The narrowest gaps are narrower than in the optical; filter widths of 0.1 per cent are needed compared with 1%

  5. M. Pettini: Introduction to Cosmology — Lecture 9 RECOMBINATION ...

    https://people.ast.cam.ac.uk/~pettini/Intro%20Cosmology/Lecture09.pdf
    6 Nov 2018: sources of noise in microwave satel-lite communications at Bell Laboratories in New Jersey.4 Their discoverywas announced alongside the interpretation of the CMB as relic thermalradiation from the Big Bang

  6. CIRSI software system specifications

    https://people.ast.cam.ac.uk/~optics/software/overview.htm
    16 Jun 2015: Operating commands. Written in TCL scripting language, using both built-in TCL language features and new camera specific commands. ... This will translate the message containing the new position into the local telescope control language.

  7. https://people.ast.cam.ac.uk/~wfcam/docs/ukidss01.txt

    https://people.ast.cam.ac.uk/~wfcam/docs/ukidss01.txt
    13 Dec 2002: will be tested using SSS will provide additional simple interface for quick queries power users will use SQL V2: more plotting access across super frames stacked frames (user-specified) new source

  8. Oxford Meeting

    https://people.ast.cam.ac.uk/~rgm/presentations/20060412-SKA-Meeting_Oxford.ppt
    15 Apr 2006: Infrared OH Sky Observations: Mahaira etal, 1993, PASP. GOOD NEWS. The 1.0 to 1.8 micron IR sky is very dark between the OH lines which contain 95% of broad ... THE NOT SO GOOD NEWS. The narrowest gaps are narrower than in the optical; filter widths of

  9. WFCAM Pipeline Design

    https://people.ast.cam.ac.uk/~wfcam/docs/glossary.html
    24 Jan 2003: pointing - a telescope slew to position with new guide star acquisition.

  10. CIRSI Exposure Time Calculator

    https://people.ast.cam.ac.uk/~rgm/cirsi/signal_cirsi_help.html
    10 Nov 1998: New blocking filters New blocking filters shall be added to CIRSI in Oct 98. ... These new filters have predicted peak throughput of 90% in H compared with 52% for the blocking filters used in May/June 1998.

  11. Cosmic dust fertilization of glacial prebiotic chemistry on early ...

    https://people.ast.cam.ac.uk/~wyatt/wrll24.pdf
    22 Mar 2024: Science (New York, N.Y.) 233,869–72 (1986). [21] Maurette, M., Brack, A., Kurat, G., Perreau, M. &

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