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Quasars and Galaxies at the Highest Redshifts
https://people.ast.cam.ac.uk/~rgm/presentations/20050922-Crafoord-Symposium.ppt8 Mar 2006: GOOD NEWS. The 1.0 to 1.8 micron IR sky is very dark between the OH lines which contain 95% of broad band background. ... THE NOT SO GOOD NEWS. The narrowest gaps are narrower than in the optical; filter widths of 0.1 per cent are needed compared with 1% -
The APM Sky Catalogues: Overview
https://people.ast.cam.ac.uk/~mike/apmcat/overview.html20 Apr 2012: The APM Sky Catalogues: Overview. Over the last few years we have used the APM facility to measure the first epoch Palomar O and E sky survey plates, with the aim of constructing a readily accessible Northern sky optical catalogue (see Gemini No. 37 -
Oxford Meeting
https://people.ast.cam.ac.uk/~rgm/presentations/20060412-SKA-Meeting_Oxford.ppt15 Apr 2006: Infrared OH Sky Observations: Mahaira etal, 1993, PASP. GOOD NEWS. The 1.0 to 1.8 micron IR sky is very dark between the OH lines which contain 95% of broad ... THE NOT SO GOOD NEWS. The narrowest gaps are narrower than in the optical; filter widths of -
Astronomy & Astrophysics manuscript no. aa ©ESO 2024April 9, ...
https://people.ast.cam.ac.uk/~wyatt/ylkw24.pdf9 Apr 2024: The new ALMA observa-tion is marked as a black circle, and the blue circle represents the fluxat the stellar position. ... Con-sequently, the broad structure of the Herschel observations seessmaller grains whose distribution is modified by radiation -
COHSI
https://people.ast.cam.ac.uk/~optics/cohsi/cohsi.htm16 Jun 2015: This new instrument configuration is called CIRPASS. COHSI was designed to suppress the nightsky airglow due to OH emission in the 1.0-1.8 micron region by filtering out the -
Quanz_et_al_ESA_white_paper_MIR_interferometry_revised
https://people.ast.cam.ac.uk/~wyatt/qabb22.pdf22 Mar 2024: Therefore, tackling a prime objective of exoplanet science and understanding how unique or common planets like our Earth are in our galactic neighborhood will require a new, dedicated approach. ... below). 15. 2.3 Timing for a space-based mid-infrared -
M. Pettini: Introduction to Cosmology — Lecture 9 RECOMBINATION ...
https://people.ast.cam.ac.uk/~pettini/Intro%20Cosmology/Lecture09.pdf6 Nov 2018: sources of noise in microwave satel-lite communications at Bell Laboratories in New Jersey.4 Their discoverywas announced alongside the interpretation of the CMB as relic thermalradiation from the Big Bang -
https://people.ast.cam.ac.uk/~wfcam/docs/onsky.txt
https://people.ast.cam.ac.uk/~wfcam/docs/onsky.txt19 Aug 2003: detectors will be being used in a new mains power environment, attached to a telescope, and may have noise properties different to those measured in the lab. -
The LCIR survey at Cambridge
https://people.ast.cam.ac.uk/~optics/cirsi/lcirs/16 Jun 2015: defining a large sample of candidate high redshift near-IR selected galaxies for follow-up spectroscopy with the new Gemini 8m and Magellan 6.5m telescopes, and. -
CIRSI software system specifications
https://people.ast.cam.ac.uk/~optics/software/overview.htm16 Jun 2015: Operating commands. Written in TCL scripting language, using both built-in TCL language features and new camera specific commands. ... This will translate the message containing the new position into the local telescope control language. -
https://people.ast.cam.ac.uk/~wfcam/docs/ukidss01.txt
https://people.ast.cam.ac.uk/~wfcam/docs/ukidss01.txt13 Dec 2002: will be tested using SSS will provide additional simple interface for quick queries power users will use SQL V2: more plotting access across super frames stacked frames (user-specified) new source -
WFCAM Pipeline Design
https://people.ast.cam.ac.uk/~wfcam/docs/glossary.html24 Jan 2003: pointing - a telescope slew to position with new guide star acquisition. -
mnr7957.tex
https://people.ast.cam.ac.uk/~wyatt/gwhd04.pdf19 Apr 2006: A new 850-µmimage shows that there is indeed such a debris disc, extending out to 55 au (15 arcsec)radius. -
CIRSI Exposure Time Calculator
https://people.ast.cam.ac.uk/~rgm/cirsi/signal_cirsi_help.html10 Nov 1998: New blocking filters New blocking filters shall be added to CIRSI in Oct 98. ... These new filters have predicted peak throughput of 90% in H compared with 52% for the blocking filters used in May/June 1998. -
INT Wide Field Camera Imaging Survey
https://people.ast.cam.ac.uk/~mike/casu/WFCsur/WFCsur.html18 Jan 2000: This new instrument offers unique opportunities for the UK/NL communities to execute high resolution, deep, wide field optical imaging surveys. ... give an indication of when new data will be available for download. -
CIRPASS data reduction cookbook for data taken at the Gemini…
https://people.ast.cam.ac.uk/~optics/cirpass/datared/cookbook_gemini.phpsure that update is also set to yes for dogemini so that the new entries are written to the data when the task is run. -
CMASF (San Juan, Argentina)
https://people.ast.cam.ac.uk/~dwe/AstSurv/pepe.html6 Oct 2000: Maximun priority is given to the zone -3º to -9º the same zone observed in San Fernando for the Astrophotographic Catalogue in order to computes proper motions using new measures of ... In 1991 the original declination glass circle was changed for a -
Cosmic dust fertilization of glacial prebiotic chemistry on early ...
https://people.ast.cam.ac.uk/~wyatt/wrll24.pdf22 Mar 2024: Science (New York, N.Y.) 233,869–72 (1986). [21] Maurette, M., Brack, A., Kurat, G., Perreau, M. & -
User manual - Images
https://people.ast.cam.ac.uk/~optics/software/user/image.htm16 Jun 2015: The command will not create a new image if an existing image has the same name. ... Note that new images can be initialised to any value when they are created with the imcreate command. -
https://people.ast.cam.ac.uk/~optics/cirsi/ing/proposals_public/2001/2…
https://people.ast.cam.ac.uk/~optics/cirsi/ing/proposals_public/2001/2001a/patt2.sty16 Jun 2015: 3.0 Sept 1996 Richard McMahon (IoA) [rgm@ast.cam.ac.uk] %% Conversion to Latex substyle %% %% 3.1 July 1997 Bill Martin and Vik Dhillon (RGO) %% Released to community for new ... AAO) %% Increased space for Section 14 - Related Applications %% %% 3.5
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