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1 - 20 of 32 search results for KaKaoTalk:vb20 200 |u:people.ast.cam.ac.uk where 0 match all words and 32 match some words.

  1. Results that match 1 of 2 words

  2. Other NIR spectrographs

    https://people.ast.cam.ac.uk/~optics/cirpass/docs/other_nirspec.html
    16 Jun 2015: ISAAC (LW). 8m VLT UT1. 2-5. 1500,700,450,200 (lres). 8000,4000,2500,1250 (mres). 41.5.

  3. Observing guide for CIRSI (WFIRC) at LCO du Pont ...

    https://people.ast.cam.ac.uk/~optics/cirsi/cirsi.guide.html
    16 Jun 2015: pc, computer room 200.29.61.153 bodega2.lco.cl bodega2 # Yerko Aviles pc # 200.29.61.154? ... 139 remote.lco.cl remote # # Visitor Laptops # 200.28.111.145 visitor1.lco.cl visitor1 200.28.111.146 visitor2.lco.cl visitor2 17).

  4. MGB thesis Chapter 5

    https://people.ast.cam.ac.uk/~optics/tech/mgb_phd/chapter5.htm
    16 Jun 2015: The trolley is set to scan at 200 Hz and forms the main peak in the data.

  5. Other IFUs

    https://people.ast.cam.ac.uk/~optics/cirpass/docs/other_ifu.html
    16 Jun 2015: software. PIFS. type. slicer. telescope. Palomar 200 inch. wv range. 1-2.5 micron, 1-5 micron.

  6. 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: 13. -5. 199. 200. 12. -4. 200. 201. 11. -3. 201.

  7. Observing guide for CIRSI (WFIRC) at LCO du Pont ...

    https://people.ast.cam.ac.uk/~optics/cirsi/cirsi-guide-lco-0.6.html
    16 Jun 2015: pc, computer room 200.29.61.153 bodega2.lco.cl bodega2 # Yerko Aviles pc # 200.29.61.154? ... 139 remote.lco.cl remote # # Visitor Laptops # 200.28.111.145 visitor1.lco.cl visitor1 200.28.111.146 visitor2.lco.cl visitor2 17).

  8. CIRSI LCO 100" Observing Notes - 1999 April/May

    https://people.ast.cam.ac.uk/~optics/cirsi/ociw/lco1999may/cirsi_lco_notes_1999may.html
    16 Jun 2015: Cannot connect to 200.28.111.133. This probable means that you started the NT-Camera Control before you startup up Pixcel on CIRCC.

  9. 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.

  10. 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

  11. 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

  12. Chapter 4 - Controls Reference

    https://people.ast.cam.ac.uk/~optics/cirsi/docs/pixcel/20010508/chapter4.htm
    16 Jun 2015: Base Electronics base pixel value, typically 200-1000 and is updated periodically.

  13. MGB thesis Chapter 2

    https://people.ast.cam.ac.uk/~optics/tech/mgb_phd/chapter2.htm
    16 Jun 2015: 1.05. 150 - 300. Indium Gallium Arsenide (InGaAs). 0.7. 1.7. 77 - 200.

  14. https://people.ast.cam.ac.uk/~optics/dazle/sky-data/ukirt_sky_ramsey_e…

    https://people.ast.cam.ac.uk/~optics/dazle/sky-data/ukirt_sky_ramsey_etal.dat
    16 Jun 2015: 196 1.29700 3408.63 197 1.29850 3794.42 198 1.29990 4543.59 199 1.30140 4584.77 200 1.30280 4085.07 201 1.30420 3724.87 202 ... 75750 202.051 199 1.75880 511.795 200 1.76010 1403.21 201 1.76140 4458.84 202 1.76270 12575.5 203 1.76400 13281.0 204 1.76530

  15. Chapter 2 - Operating the software

    https://people.ast.cam.ac.uk/~optics/cirsi/docs/pixcel/20010508/chapter2.htm
    16 Jun 2015: Base Electronics base pixel value, typically 200-1000 and is updated periodically.

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

    https://people.ast.cam.ac.uk/~wyatt/blrf15.pdf
    14 Sep 2015: There are modulations in the raw flux data at the 200 ppmlevel which are visible by eye. ... 5. Time (BJD-2454833). No. rma. lize. d f. lux. 190 200 210 220 230 240.

  17. https://people.ast.cam.ac.uk/~optics/cirsi/ociw/lco1999may/eric/reduct…

    https://people.ast.cam.ac.uk/~optics/cirsi/ociw/lco1999may/eric/reduction_manual
    16 Jun 2015: It is approximately the size of one chip, i.e., 200 arcsec on a side.

  18. MGB thesis Chapter 3

    https://people.ast.cam.ac.uk/~optics/tech/mgb_phd/chapter3.htm
    16 Jun 2015: [Chapter 3: Camera. Outline. This chapter describes the near infrared camera built for COAST. It examines the properties required from the camera system, the range of devices available and the factors involved in the choice of detector. The design,

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

    https://people.ast.cam.ac.uk/~wyatt/pw15.pdf
    14 Sep 2015: A /. yr-1. 108. 106. 104. 102. 100. a / au0 50 100 150 200. ... 0.2. 0.4. 0.6. 0.8. r / au0 50 100 150 200.

  20. MGB thesis Chapter 4

    https://people.ast.cam.ac.uk/~optics/tech/mgb_phd/chapter4.htm
    16 Jun 2015: The exposure times were 50, 100 and 200 milli-seconds. Results. Signal (e. -.

  21. arX iv:1 503. 0207 3v1 [ast ro-p h.E P] ...

    https://people.ast.cam.ac.uk/~wyatt/kmmg15.pdf
    10 Mar 2015: for material uniformlydistributed around a circular narrow ring at 200 au, with thein-clination derived from the 70µm PACS image. ... models the inner edge is around 30 au, and theouter edge around 200 au.

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