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Other NIR spectrographs
https://people.ast.cam.ac.uk/~optics/cirpass/docs/other_nirspec.html16 Jun 2015: ISAAC (LW). 8m VLT UT1. 2-5. 1500,700,450,200 (lres). 8000,4000,2500,1250 (mres). 41.5. -
Observing guide for CIRSI (WFIRC) at LCO du Pont ...
https://people.ast.cam.ac.uk/~optics/cirsi/cirsi.guide.html16 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). -
MGB thesis Chapter 5
https://people.ast.cam.ac.uk/~optics/tech/mgb_phd/chapter5.htm16 Jun 2015: The trolley is set to scan at 200 Hz and forms the main peak in the data. -
Other IFUs
https://people.ast.cam.ac.uk/~optics/cirpass/docs/other_ifu.html16 Jun 2015: software. PIFS. type. slicer. telescope. Palomar 200 inch. wv range. 1-2.5 micron, 1-5 micron. -
https://people.ast.cam.ac.uk/~optics/cirpass/datared/BINTABLE.txt
https://people.ast.cam.ac.uk/~optics/cirpass/datared/BINTABLE.txt16 Jun 2015: 13. -5. 199. 200. 12. -4. 200. 201. 11. -3. 201. -
Observing guide for CIRSI (WFIRC) at LCO du Pont ...
https://people.ast.cam.ac.uk/~optics/cirsi/cirsi-guide-lco-0.6.html16 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). -
CIRSI LCO 100" Observing Notes - 1999 April/May
https://people.ast.cam.ac.uk/~optics/cirsi/ociw/lco1999may/cirsi_lco_notes_1999may.html16 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. -
CIRSI INT Observing Guide
https://people.ast.cam.ac.uk/~optics/cirsi/cirsi.guide.ing.html16 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. -
New Page 1
https://people.ast.cam.ac.uk/~optics/people/cdm_CV_130509.htm16 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 -
design study report
https://people.ast.cam.ac.uk/~optics/cirpass/design-study-a.htm16 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
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