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CIRSI (Sackler) Camera
https://people.ast.cam.ac.uk/~optics/cirsi/16 Jun 2015: Las Campanas IR Survey(LCIRS), Gravitational Lensing,. The Institute of Astronomy has been particularly fortunate in being given a substantial donation for the development of new instruments, as part of the -
DES Satellites, Cambridge PR graphics
https://people.ast.cam.ac.uk/~vasily/des_pr/10 Mar 2015: LMC, SMC, the HI stream and the new satellites. Credit: V. -
DAZLE : The Dark Age Z(redshift) Lyman-alpha Explorer
https://people.ast.cam.ac.uk/~optics/dazle/16 Jun 2015: DAZLE : The Dark Age Z(redshift) Lyman-alpha Explorer. [ Internal Project pages ]. DAZLE is a narrow band imaging instrument developed by the Institute of Astronomy (Cambridge) and the Anglo-Australian Observatory with the singular aim of detecting -
IoA Instrumentation Group
https://people.ast.cam.ac.uk/~optics/16 Jun 2015: We are collaborating with Department of Astrophysics at the American Museum of Natural History (AMNH) to design a new Integral Field Spectrograph (IFS) for Exoplanetary Science. -
CIRSI (Sackler) Camera
https://people.ast.cam.ac.uk/~optics/cirsi/docs.html16 Jun 2015: LCO observing guide -- computer inventory, observing procedures, troubleshooting, etc. observing procedure at INT (including new TCS info), troubleshooting, etc. ... PixCel Manual -- PixCel Manual with added Chapter 0 describing new IR features. -
About the Instrumentation Group
https://people.ast.cam.ac.uk/~optics/about.htm16 Jun 2015: 2. HgCdTe arrays for making deep NIR surveys. As part of our spectroscopy program we are also designing new spectrographs for 8-m telescopes which employ digital and hardware OH suppression. -
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 -
https://people.ast.cam.ac.uk/~optics/cirpass/datared/fibcal.txt
https://people.ast.cam.ac.uk/~optics/cirpass/datared/fibcal.txt16 Jun 2015: in_outfi= fibpos_paschenJ.list Name of file to contain the new position informa in_noise= 10 background noise in image in_sigma= 10 sigma above background which indicates a line -
User manual- packages
https://people.ast.cam.ac.uk/~optics/software/user/package.htm16 Jun 2015: Package loading. The TCL system contains a mechanism for finding automatically searching and loading new packages to if a command is used which isn't in the currently loaded set. ... The system must be able to issue commands to the telescope to acquire -
CIRPASS - The Cambridge IR PAnoramic Survey Spectrograph
https://people.ast.cam.ac.uk/~optics/cirpass/cirpass-old.htm16 Jun 2015: With the advent of the new 1024. 2. arrays this restriction is removed and it is possible to do the OH suppression in software (digital suppression) by simply capturing the spectra -
Image manual pages
https://people.ast.cam.ac.uk/~optics/software/user/image_man.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 initialsed to any value when they are created with the imcreate command. -
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. -
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 DuPont Run; 2001 Apr 10-15
https://people.ast.cam.ac.uk/~optics/cirsi/ociw/20010410-dupont.html16 Jun 2015: CIRSI DuPont Run; 2001 Apr 10-15. TODO. find out who will help set up on the first night [done]. finalise targets and field centres [done]. prepare almanac WWW page [done]. exposure times; dither patterns [done]. make a nightly plan [done]. Richard G -
Data Analysis Package
https://people.ast.cam.ac.uk/~optics/cirpass/docs/datanaly.html16 Jun 2015: The essential tasks required at the telescope are:. display a reconstructed broad-band image (with the option to save this image into a new FITS file). -
LCO LCIR WWW Home Page
https://people.ast.cam.ac.uk/~optics/cirsi/ociw/lco1999may/lcir/16 Jun 2015: New Observing Log Summary This includes pointing specific information such as exposures, seeing and sky brightness estimate. -
CIRSI DuPont Run; 2000 Dec 13-17
https://people.ast.cam.ac.uk/~optics/cirsi/ociw/20001213-dupont.html16 Jun 2015: CIRSI DuPont Run; 2000 Dec 13-17. TODO. find out who will help set up on the first night [done]. finalise targets and field centres [done]. prepare almanac WWW page [done]. exposure times; dither patterns [done]. make a nightly plan [done]. Richard G -
Planning material CIRSI DuPont Run; 03-11 Nov 2000
https://people.ast.cam.ac.uk/~optics/cirsi/ociw/20001103-dupont.html16 Jun 2015: CIRSI DuPont Run; 03-11 Nov 2000. TODO. find out who will help set up on the first night [done]. finalise targets and field centres [done]. prepare almanac WWW page [done]. exposure times; dither patterns [done]. make a nightly plan [done]. Richard G -
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. -
User manual:Concepts
https://people.ast.cam.ac.uk/~optics/software/user/concepts.htm16 Jun 2015: Although this model provides a number of important safety features for the new user, you cannot forget to save changes to an image or lose data because of a crash, there ... Instead of loading an image changing it and then saving the result you must copy
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