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2001B information
https://people.ast.cam.ac.uk/~optics/cirsi/ociw/2001b/16 Jun 2015: Moon. Jul 27; 1449-1149. Aug 02; 20 06 40, -22 13.3. ... Moon. Aug 25; 16 19 02, -18 45.6. Aug 30; 20 43 50, -20 49.3. -
About the Instrumentation Group
https://people.ast.cam.ac.uk/~optics/about.htm16 Jun 2015: IOA Instrumentation Group. Welcome. The Astronomical Instrumentation Group is currently building two fast-track NIR instruments which will provide much improved performance over instruments currently available. COHSI is a spectrograph for low -
Specific Parameters for [FeII] 1644 nm Filters Thickness: 1.12 ...
https://people.ast.cam.ac.uk/~optics/cirsi/technical/feii_ocli.htm16 Jun 2015: Bandwidth (77K). Short Slope. Long Slope. Peak Transmission. 1. 1637.6. 20.40. ... 0.86. 0.83. 77.1. 2. 1637.7. 20.34. 0.87. 0.83. 77.5. 3. 1637.8. -
https://people.ast.cam.ac.uk/~optics/cirsi/ing/2000a/20000619.al
https://people.ast.cam.ac.uk/~optics/cirsi/ing/2000a/20000619.al16 Jun 2015: AM on 2000 Sep 24; standard zone = 0 hrs W For the night of: Mon, 2000 Jun 19 --- Tue, 2000 Jun 20 Local midnight = 2000 Jun 19, 23 hr UT, or ... JD 2451715.458 Local Mean Sidereal Time at midnight = 15 42 22.2 Sunset ( 2326 m horizon): 21 20 GDT; Sunrise -
Index
https://people.ast.cam.ac.uk/~optics/util/myindex.htm16 Jun 2015: Up. Prev. Next. Index. This list is generated automatically from the page TITLE field. -updated 09:17:31 Jan,. URL http://www.ast.cam.ac.uk/optics/util/myindex.htm - Revised: 25 Jan 97. We are part of the Institute of Astronomy , which is part of -
COHSI
https://people.ast.cam.ac.uk/~optics/cohsi/16 Jun 2015: IFU Commissioning on UKIRT March 19, 20 & 25-29, 1998. -
https://people.ast.cam.ac.uk/~optics/cirsi/ing/2000a/20000519.al
https://people.ast.cam.ac.uk/~optics/cirsi/ing/2000a/20000519.al16 Jun 2015: AM on 2000 Sep 24; standard zone = 0 hrs W For the night of: Fri, 2000 May 19 --- Sat, 2000 May 20 Local midnight = 2000 May 19, 23 hr UT, or ... evening twilight: 12 08 Morning twilight: 5 48 GDT; LMST at morning twilight: 19 29 12-degr twilight: 21 55 -
COHSI
https://people.ast.cam.ac.uk/~optics/cohsi/cohsi.htm16 Jun 2015: Commissioning on UKIRT March 19, 20 & 25-29, 1998. -
Top Hits by year
https://people.ast.cam.ac.uk/~rgm/publications/tophits.html27 Jul 2015: Top 20 papers sorted by citation count per decade. 2010: [2000: [1990: [1980: [1970: [1960: [1950: [1940: [1930: [1920: [1910: [1900: [Top 20 papers sorted by citation count per year. -
CIRSI-Technical Characteristics and Expected Astronomical Performance
https://people.ast.cam.ac.uk/~optics/cirsi/cirsi_brief.html16 Jun 2015: 5.5' x 5.5'. 20.9' x 20.9'. 30.9. 0.42. INT. Prime f/3.3. ... NICMOS. MCT 256x256. 0.04-0.20. -. -. -. Notes:. (1) Survey Power is the product of the collecting area in m2 times the field of view in degrees, neglecting any losses due -
CIRSI - LCO Base WWW Page
https://people.ast.cam.ac.uk/~optics/cirsi/ociw/lco1999may/16 Jun 2015: CIRSI - LCO WWW Home Page. Important Note on location of this WWW pages. This is the CIRSI base WWW Homepage at LCO and has the location /home/www/users/rgm on andy.lco.cl. Access is currently restricted by IP number to LCO, OCIW, and IOA. Password -
CIRPASS software specification
https://people.ast.cam.ac.uk/~optics/cirpass/docs/soft_spec.html16 Jun 2015: Last modified: Thu Apr 17 11:44:20 2003. -
The LCIR survey at Cambridge
https://people.ast.cam.ac.uk/~optics/cirsi/lcirs/16 Jun 2015: SSA22 22 17 54.0 00 14 34. NICMOS 22hr 22 20 17.2 -24 43 27. -
Hawaii / Picnic interface ver 3
https://people.ast.cam.ac.uk/~optics/cirsi/documents/CIRSI_wiring_amp55.htm16 Jun 2015: DPLUS. 20. R. 20. Chips 13. DGND. 21. S. 21. Chips 13. ... DPLUS. 20. j. 20. Chips 24. DGND. 21. k. 21. Chips 24. -
Observing Plan
https://people.ast.cam.ac.uk/~optics/cirsi/ociw/DuPontObservingPlans/20010410/16 Jun 2015: RA:15:03:52 Dec:-12:40.4. set:. rise : 19:48. [8:20. 18:11? :? :? 19:49. ... RA:15:57:18 Dec:-16:45.3. set:. rise : 20:27. [8:22. 18:16? :? :? 19:48. -
IOA DuPont time material
https://people.ast.cam.ac.uk/~optics/cirsi/ociw/DuPontIoaTimeSchedule/16 Jun 2015: IOA DuPont time material. Scheduled Dates. 1999. 2000. 20-22, Jan [3 nights] [Observer(s): Andrew Firth ]. 17-19, Feb [3 nights] [Observer(s): Andrew Firth ]. 19-23, Mar [32 nights] -
Observing Plan
https://people.ast.cam.ac.uk/~optics/cirsi/ociw/20001213-dupont-obsplan/16 Jun 2015: RA:12:02:36 Dec:5:56.0. set:. rise : 2:03. [2:20. 9:10? :? :? 22:15. -
Observing Plan for Semester ????
https://people.ast.cam.ac.uk/~optics/cirsi/ing/2000a/cirsi_almanac_plan.html16 Jun 2015: Mon May 22. TBA. [UT of first science observation:?:? 7.20. 02:08. ... 0.4 dark hours after end of twilight and before moonrise. 20:19:49 -20:54.3. -
CIRPASS at Gemini-S picture gallery index
https://people.ast.cam.ac.uk/~optics/cirpass/World-tour/Gemini-S/Pictures/16 Jun 2015: Last modified: Fri Sep 20 12:09:51 2002. -
HAWAII SAM MICROCODE
https://people.ast.cam.ac.uk/~optics/cirsi/SAM/cirsi_sam_microcode_22dec97.html16 Jun 2015: 1714 1500 2.20. 2000 and above 1714 2.35. (note intermediate rates all work. -
design study report
https://people.ast.cam.ac.uk/~optics/cirpass/design-study-a.htm16 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 -
Observing guide for CIRSI (WFIRC) at LCO du Pont ...
https://people.ast.cam.ac.uk/~optics/cirsi/cirsi.guide.html16 Jun 2015: Keep the peak counts below about 8K (you could put the telescope somewhat out of focus, eg 20 units, if necessary). ... Run Filter Chip1 Chip2 Chip3 Chip4 Comment 7614 H (?) 4300 2300 2300 4000 Filter used on Nov 19/20, 20/21 7615 Hl (?) 1200 700 600 -
CIRPASS at Gemini-S Diary
https://people.ast.cam.ac.uk/~optics/cirpass/World-tour/Gemini-S/diary.html16 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 -
https://people.ast.cam.ac.uk/~optics/cirsi/ing/2000a/20000520.al
https://people.ast.cam.ac.uk/~optics/cirsi/ing/2000a/20000520.al16 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 -
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: Keep the peak counts below about 8K (you could put the telescope somewhat out of focus, eg 20 units, if necessary). ... Run Filter Chip1 Chip2 Chip3 Chip4 Comment 7614 H (?) 4300 2300 2300 4000 Filter used on Nov 19/20, 20/21 7615 Hl (?) 1200 700 600 -
Craig Mackay
https://people.ast.cam.ac.uk/~optics/people/cdm_pub_list_130509.htm16 Jun 2015: SPIE, 290, 159 (1981). 20. Wright, J.F. and Mackay, C.D., The Cambridge Charge--Coupled Device (CCD) System'. ... Optical aperture synthesis on the INT. Gemini, Newsletter of RGO, No 20, 2. -
https://people.ast.cam.ac.uk/~rgm/magnitudes/vega_hl75.dat
https://people.ast.cam.ac.uk/~rgm/magnitudes/vega_hl75.dat9 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 -
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 ]. -
Mon. Not. R. Astron. Soc. 000, 000–000 (0000) Printed ...
https://people.ast.cam.ac.uk/~wyatt/smw15.pdf15 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. -
Next Generation Very Large Array Memo No. 6Science Working ...
https://people.ast.cam.ac.uk/~wyatt/ihmg15.pdf24 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. -
Mon. Not. R. Astron. Soc. 000, 1–14 (2002) Printed ...
https://people.ast.cam.ac.uk/~wyatt/pw15.pdf14 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 -
/astro/p7scch2/AUMic/paper/figures/all.eps
https://people.ast.cam.ac.uk/~wyatt/wlke15.pdf16 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. -
proceedings2.dvi
https://people.ast.cam.ac.uk/~optics/dazle/publications/5492-1022-dazle.pdf16 Jun 2015: 9.99 13325.2 20.5 75.7 13401.0 3.81 80 Clean window. 2.2. Narrowband Filters. -
Appendix XXX
https://people.ast.cam.ac.uk/~optics/cirsi/docs/review/appendix.doc16 Jun 2015: SHUTTER_OPEN_DELAY:. % Delay for address to settle%. [ADDS_20 HOLD RES_I _RES_T H1 _CONVT UP CAMA WR_RM] CONTINUE;. ... ADDS_20 HOLD RES_I _RES_T H1 _CONVT UP CAMA WR_RM] CONTINUE;. % Save highest byte on the stack%. -
Draft version January 19, 2015Preprint typeset using LATEX style ...
https://people.ast.cam.ac.uk/~wyatt/mmks15.pdf19 Jan 2015: 501. 0381. 3v1. [as. tro-. ph.E. P] 1. 5 Ja. n 20. ... that, for the planet-hosts, thebinary fraction is significantly lower than field stars forbinary semimajor axes <20 AU. -
https://people.ast.cam.ac.uk/~optics/cirpass/datared/list_xml.txt
https://people.ast.cam.ac.uk/~optics/cirpass/datared/list_xml.txt16 Jun 2015: GY-11 16:23:20.8 -24:17:21 2349.8-2601 16:23:49.8 -24:26:01 CRBR-14 16:23:17.3 -24:19:25 GY-10 ... 23:20.8 -24:17:08 2MASSW-J2049197-194432 20:49:19.74 -19:44:32.5 2MASSW-J2147446-264406 21:47:44.62 -26:44:06.6 2MASSW-J2206228-204705 -
Project Reassessment Start Date
https://people.ast.cam.ac.uk/~optics/cirsi/docs/review/review.doc16 Jun 2015: It is more suited to a shallow survey to H(20 as indicated by Figure 2.2.1a. ... Short wavelength cut-on (micron) 0.85 0.85. Read noise (e- at 77K) < 20 < 5. -
MNRAS 000, 1–14 (2015) Preprint 17 December 2015 Compiled ...
https://people.ast.cam.ac.uk/~wyatt/rw15.pdf17 Dec 2015: MNRAS 000, 1–14 (2015) Preprint 17 December 2015 Compiled using MNRAS LATEX style file v3.0. Dynamical Constraints on Outer Planets in Super-Earth Systems. Matthew J. Read1? and Mark C. Wyatt11Institute of Astronomy, University of Cambridge, -
https://people.ast.cam.ac.uk/~optics/cirsi/ing/2000a/20000620.al
https://people.ast.cam.ac.uk/~optics/cirsi/ing/2000a/20000620.al16 Jun 2015: AM on 2000 Sep 24; standard zone = 0 hrs W For the night of: Tue, 2000 Jun 20 --- Wed, 2000 Jun 21 Local midnight = 2000 Jun 20, 23 hr UT, or -
Summary
https://people.ast.cam.ac.uk/~optics/cirpass/summary.bak16 Jun 2015: Last modified: Wed Nov 24 12:12:20 1999. -
https://people.ast.cam.ac.uk/~optics/cirsi/ociw/lcirs_standards.info
https://people.ast.cam.ac.uk/~optics/cirsi/ociw/lcirs_standards.info16 Jun 2015: Keep the peak counts below about 8K (you could put the telescope somewhat out of focus, eg 20 units, if necessary). ... The following standards are used: 9185 22 02 05.7 -01 06 02 J2000 NEAR SSA22 9104 01 03 15.8 -04 20 44 J2000 NEAR NOAO FIELD 9106 03 -
https://people.ast.cam.ac.uk/~optics/cirsi/ing/2000a/20000517.al
https://people.ast.cam.ac.uk/~optics/cirsi/ing/2000a/20000517.al16 Jun 2015: evening twilight: 11 59 Morning twilight: 5 49 GDT; LMST at morning twilight: 19 22 12-degr twilight: 21 54 GDT -- 6 22 GDT; night center: 2 08 GDT Moonrise: 20 -
https://people.ast.cam.ac.uk/~optics/cirsi/ing/2000a/20000612.al
https://people.ast.cam.ac.uk/~optics/cirsi/ing/2000a/20000612.al16 Jun 2015: evening twilight: 13 59 Morning twilight: 5 39 GDT; LMST at morning twilight: 20 54 12-degr twilight: 22 10 GDT -- 6 13 GDT; night center: 2 11 GDT Moonset : 5 -
https://people.ast.cam.ac.uk/~optics/cirsi/ing/2000a/20000616.al
https://people.ast.cam.ac.uk/~optics/cirsi/ing/2000a/20000616.al16 Jun 2015: evening twilight: 14 16 Morning twilight: 5 39 GDT; LMST at morning twilight: 21 10 12-degr twilight: 22 11 GDT -- 6 14 GDT; night center: 2 12 GDT Moonrise: 20 -
https://people.ast.cam.ac.uk/~optics/cirsi/ing/2000a/20000617.al
https://people.ast.cam.ac.uk/~optics/cirsi/ing/2000a/20000617.al16 Jun 2015: JD 2451713.458 Local Mean Sidereal Time at midnight = 15 34 29.1 Sunset ( 2326 m horizon): 21 20 GDT; Sunrise: 7 05 GDT Evening twilight: 22 46 GDT; LMST at -
https://people.ast.cam.ac.uk/~optics/cirsi/ing/2000a/20000618.al
https://people.ast.cam.ac.uk/~optics/cirsi/ing/2000a/20000618.al16 Jun 2015: JD 2451714.458 Local Mean Sidereal Time at midnight = 15 38 25.6 Sunset ( 2326 m horizon): 21 20 GDT; Sunrise: 7 06 GDT Evening twilight: 22 47 GDT; LMST at -
https://people.ast.cam.ac.uk/~optics/cirsi/ing/2000a/20000613.al
https://people.ast.cam.ac.uk/~optics/cirsi/ing/2000a/20000613.al16 Jun 2015: evening twilight: 14 03 Morning twilight: 5 39 GDT; LMST at morning twilight: 20 58 12-degr twilight: 22 10 GDT -- 6 13 GDT; night center: 2 12 GDT Moonrise: 18 -
https://people.ast.cam.ac.uk/~optics/dazle/f.clarke/cirpass-lines.txt
https://people.ast.cam.ac.uk/~optics/dazle/f.clarke/cirpass-lines.txt16 Jun 2015: 39 12726.1 20 12744.6 24 12749.3 45 12760.9 76 12776.0 32 12779.1 149 12798.0 57 12803.5 107 12824.8 25 12831.1 58 ... 2 8.25 15183.0 20 15236.8 90 15283.6 45 15328.2 177 15391.1 54 15427.9 163 15457.9 4 15496.6 17 15505.5 44 -
Observing and Proposal Material Blain/Gray Lensing Cluster proposal…
https://people.ast.cam.ac.uk/~optics/cirsi/ociw/DuPontIoaTimeProposals/16 Jun 2015: Last modified: Thu Apr 20 22:40:22 2000. -
SPIRAL spectrograph
https://people.ast.cam.ac.uk/~optics/spiral/spiral.htm16 Jun 2015: URL http://www.ast.cam.ac.uk/optics/spiral/spiral.htm - Revised: 20 Jul 97. We are part of the Institute of Astronomy , which is part of the University of Cambridge.
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