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21 - 30 of 106 search results for TALK:PC53 20 |u:people.ast.cam.ac.uk where 0 match all words and 106 match some words.

  1. Results that match 1 of 2 words

  2. HAWAII SAM MICROCODE

    https://people.ast.cam.ac.uk/~optics/cirsi/SAM/cirsi_sam_microcode_22dec97.html
    16 Jun 2015: 1714 1500 2.20. 2000 and above 1714 2.35. (note intermediate rates all work.

  3. 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

  4. CIRPASS at Gemini-S Diary

    https://people.ast.cam.ac.uk/~optics/cirpass/World-tour/Gemini-S/diary.html
    16 Jun 2015: Saturday 20/7/02. We had planned to go straight from Tololo to La Serena but a power failure up at the telescope at 5am forces us to go back and ... Two policemen wander by and do nothing as if a group of mad British astronomers often repair their

  5. https://people.ast.cam.ac.uk/~optics/cirsi/ing/2000a/20000520.al

    https://people.ast.cam.ac.uk/~optics/cirsi/ing/2000a/20000520.al
    16 Jun 2015: AM on 2000 Sep 24; standard zone = 0 hrs W For the night of: Sat, 2000 May 20 --- Sun, 2000 May 21 Local midnight = 2000 May 20, 23 hr UT, or ... evening twilight: 12 13 Morning twilight: 5 47 GDT; LMST at morning twilight: 19 32 12-degr twilight: 21 56

  6. https://people.ast.cam.ac.uk/~rgm/magnitudes/vega_hl75.dat

    https://people.ast.cam.ac.uk/~rgm/magnitudes/vega_hl75.dat
    9 Oct 2015: The monochromatic flux reaching the Earth's atmosphere from Vega at 5556ang is 3.39-9 ergs cm-2 s-1 A-1 3.50-20 ergs cm-2 s-1 ... ergs cm-2 Jansky's (ang) s-1 A-1 s-1 Hz-1 3300.0 1.137 3.3812E-09 1.2282E-20 1.2282E03 9.0848E14 14.958

  7. CIRSI ING 2000A

    https://people.ast.cam.ac.uk/~optics/cirsi/ing/2000a/
    16 Jun 2015: Mon 15 May to Mon 22 May, 2000. 15-17 ITP4-ELAIS(Perez-Fournon) [ Proposal ]. INT pointings18-20 PATT(INT/00A/P10)-SA57(Ellis) [ Proposal ]. 21-22 ITP3- XMM(Barcons) [ Proposal ].

  8. Mon. Not. R. Astron. Soc. 000, 000–000 (0000) Printed ...

    https://people.ast.cam.ac.uk/~wyatt/smw15.pdf
    15 Jan 2015: of 2π 102, and semimajoraxis chosen randomly and uniformly between 2.20 ap and. ... 105. 2x105. 3x105. 4x105. 5x105. 6x105. 7x105. 0 20 40 60 80 100.

  9. Next Generation Very Large Array Memo No. 6Science Working ...

    https://people.ast.cam.ac.uk/~wyatt/ihmg15.pdf
    24 Oct 2015: AU,corresponding to the gravitational radius of 10–20 M stars (Lizano, 2008;Keto, 2002). ... An angular resolution between 20–40 mas is therefore requiredto resolve these objects at the distance of 5 kpc.

  10. Mon. Not. R. Astron. Soc. 000, 1–14 (2002) Printed ...

    https://people.ast.cam.ac.uk/~wyatt/pw15.pdf
    14 Sep 2015: Instead, we run simulations withaplt = 20, 30, 40 and 50 au (noting that the inner peak ofthe observed surface density profile is at 50 au, and thatthe planet’s initial semimajor ... Conversely, we find thatplanets with initial semimajor axes of 20 and

  11. /astro/p7scch2/AUMic/paper/figures/all.eps

    https://people.ast.cam.ac.uk/~wyatt/wlke15.pdf
    16 Jun 2015: There is also an NW-SEasymmetry, with the NW side brighter than the SE side in-terior to 20 au. ... 37.5 – 42.5 r 00. 0.03 0.015 M1. 1.5 103 20 0.02.

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