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21 - 30 of 365 search results for KaKaoTalk:vb20 200 |u:people.ast.cam.ac.uk where 0 match all words and 365 match some words.

  1. Results that match 1 of 2 words

  2. INT WFS Photometric Calibration Technical Note 1.0: Determination of…

    https://people.ast.cam.ac.uk/~xmmssc/xidops/xiddocs/int_wfs_tn_photometric_calibration.html
    24 Dec 2004: The full well on all devices is 200,000e- and the gain is around 3.5 for standard read out. ... 0.22 -0.30 14.3 15.4 15.6 15.7 15.9 139 73 80 96 200 40 40 40 40 40 0724-003 RUBIN 149 2 7

  3. Estimate of the Number of CPU Nodes to Execute ...

    https://people.ast.cam.ac.uk/~wfcam/ukreview/vircam_cpu_estimate.pdf
    29 Sep 2006: Data:. • Average of 200 Gb of science data per night (about 14 hours long). • ... Average night: 200 Gb/0.27 Gb = 740 images per night.

  4. Mark Wyatt

    https://people.ast.cam.ac.uk/~wyatt/
    15 Apr 2024: being accreted onto the Earth is in grains between 100-200 micron in size is understood in terms of the interplay between Poynting-Robertson drag and collisions, this result has not

  5. WSA Interface Control Document

    https://people.ast.cam.ac.uk/~wfcam/docs/wsaicd_draft2.html
    5 Mar 2003: noise level THRESHOL 200.0 e real [ADU] Detection threshold used SEEING 1.7 e real [pixels] Average stellar FWHM ELLIPTIC 0.05 e real Avg.

  6. CIRSI INT Observing Guide

    https://people.ast.cam.ac.uk/~optics/cirsi/cirsi.guide.ing.html
    16 Jun 2015: PLUS_5=5.300. MINUS_5=-5.400. ANALOGUE_IN=-0.30. VOUT_D=5.200. VOUT_C=5.200. VOUT_B=1.100. VOUT_A=1.300. ... 5.200. PLUS_25=23.400. PLUS_12=12.300. MINUS_12=-11.000.

  7. New Page 1

    https://people.ast.cam.ac.uk/~optics/people/cdm_CV_130509.htm
    16 Jun 2015: This involved using the One-Mile Radio Telescope of the Mullard Radio Astronomy Observatory to observe a sample of 200 bright radio sources in the 3C revised catalogue, at galactic latitudes

  8. PrimordialD_jun18.key

    https://people.ast.cam.ac.uk/~pettini/Primordial%20D%20Jun18
    5 Jul 2018: N(H I) = 2.5 1020 cm2. Fe/H = 1/200 solar. Very Metal Poor DLAs are the choice astrophysical environments for measuring the primordial abundance of deuterium.

  9. design study report

    https://people.ast.cam.ac.uk/~optics/cirpass/design-study-a.htm
    16 Jun 2015: A peak throughput of 20-24% is achievable. A Baranne spectrograph design with 0.19m of wavelength coverage and a multiplex gain of 200 (50 per spectrograph) looks feasible technically but ... A fully specified classical spectrograph with a wavelength

  10. CIRPASS data reduction cookbook SN1987a

    https://people.ast.cam.ac.uk/~optics/cirpass/datared/cookbook_sn1987a_old_200307.php
    imreplace.upper = 200. imreplace.radius = 0. imrep. imreplace.images = "badpix". imreplace.value = 1. ... imreplace.imaginary = 0. imreplace.lower = 200. imreplace.upper = INDEF. imreplace.radius = 0.

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

    https://people.ast.cam.ac.uk/~csc/newcv/2014talks.html
    24 Jul 2019: Mar. 350, 200. Your place in the cosmos. Talk to high school pupils from Finland. ... Mar. 200. The Northern Lights. Talk at Public Open Evening, IoA.

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