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1 - 10 of 30 search results for KaKaoTalk:vb20 200 |u:people.ast.cam.ac.uk where 0 match all words and 30 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. 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.

  4. 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.

  5. 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.

  6. 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).

  7. 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.

  8. 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.

  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. 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

  11. 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.

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