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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

10 Mar 2015: LMC, SMC, the HI stream and the new satellites. Credit: V.

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

16 Jun 2015:

16 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.

16 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.

16 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

16 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

16 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

16 Jun 2015: New features. Now works on windows98 with vxd driver. Hawaii 2K devices supported.

16 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.

16 Jun 2015: Default values for new sections. [INFRARED] LINEAR=none FLIP_V=FALSE FLIP_H=FALSE ASSEMBLE=FALSE ROTATE_ORDER=0,90,180,270 ROTATE=FALSE SHIFT=0 CONSTANT=0 SUBTRACT=FALSE

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.

16 Jun 2015: Once multiple dithers have been mosaiced the dead lense and the calibration fibers are removed form the image and the table extension is updated to reflect the new fiber to lense

16 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.

16 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

16 Jun 2015: Filters that were loaded when CIRSI was shipped to LCO:. 0 Dk Dark position; metal plate 1 Jc New Carnegie J replacing Z 2 Jg J(Gemini consortium specification) 3 Hs

16 Jun 2015: Enter. PCIDeviceId=0x826e. if you have a new card, ie:. It says PCI Digital Camera Interface on the top left of the card.

16 Jun 2015: READY - Camera is able to start a new sequence, or has just finished one. ... To return the current value of a parameter send the name of the parameter, to set a new value send the name and the value separated by a space.

16 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.