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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: The device is operated via simple polled transfers. New device drivers that support full DMA access have recently been received by AstroCam for Windows 95. ... A new filter wheel is under construction now. 2.6 System Testing hardware and software.

16 Jun 2015: Before you install your software. If you are using a new PC with your system, it is strongly recommended you check your PC system is functioning correctly.

16 Jun 2015: DAZLE: Dark Ages Z Lyman-alpha Explorer. This is a collection of published work with a connection to issues relating to the DAZLE project. There are two lists, one covering the theoretical background and the other relevant observational results.

16 Jun 2015: CIRSI Publications. SPIE Proceedings.. CIRSI: Progress with the Cambridge Infra Red Survey Instrument. M.G. Beckett, C.D. Mackay, R.G. McMahon, I.R. Parry, R.S. Ellis, S.J. Chan, M. Hoenig. in 'Infrared Astronomical Instrumentation', 1998, Editor:

16 Jun 2015: In conjunction with the improved image quality now demonstrated with new 6.5-10 m telescopes, DAZLE will be the only instrument well suited to searching for early star-forming systems

16 Jun 2015: Rockwell PICNIC array. Martin Beckett 17 Nov 96. Rockwell has recently replaced the NICMOS 256x256 MCT array with a new device called PICNIC.

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.

16 Jun 2015: Parameters. The new parameters are in five groups at end of the pixcel.ini. ... RUN=0 to 9999999. A run number is inserted into the filename of each fits file written, the number is automatically incremented with each new sequence.

16 Jun 2015: Please note section 7 ("Transition") in the text, in which the IAU-FWG recommends that ".readers should be altered as soon as possible to cope with the new format." and ".FITS ... conformance to these new rules in order to be prepared for full

16 Jun 2015: The objectives of the phase-A study are to develop the construction techniques for a new type of fibre-fed spectrograph and to test it on the AAT by carrying out

16 Jun 2015: In addition a new detector system that allows the spectrum of the fringe pattern to be detected has been developed. ... Following that a new CCD system was built by CDM and used on the Anglo-Australian Telescope (AAT) in 1981.

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: 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: 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

16 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

16 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).

16 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

16 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

16 Jun 2015: The usual scheme is for actuators on the back of a thin mirror to bend it into a new shape to cancel the wavefront distortions introduced by the atmosphere. ... This has been possible because of the introduction of new detector technology but why was it