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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 -
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. -
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. -
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. -
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 -
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 -
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
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