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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: im_ - Pointer to an image created with new(). h_ - Handle.

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: 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

16 Jun 2015: 1996) New Astronomy, 1, 177. Maihara et al. (1993) P.A.S.P., 105, 940.

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 CIRPASS team and the new CIRPASS plug-plate system at cassegrain.

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: 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: What has to happen is that the configuration file being used has to be edited and then re-loaded into Pixcel with the new parameters in it.

16 Jun 2015: Transfer to another telescope therefore is simply a case of making a new fibre feed and making a new plate-holder unit to suit the new telescope. ... For a multislit system transfer to another telescope requires making a new collimator.

9 Oct 2015: v22 v21) 4(Mp/M)2ǫ21 v5pv3. Hence show that the new orbit has a semimajor axis with a corresponding ǫ2 thatsatisfies.

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 plot is updated with the pixels from the new image under the line selection. ... The histogram is updated with the data from the new image under the rectangle selection.

16 Jun 2015: vii) type 'cmd TCS USER "ENTER APERTURE 0 x y" where x & y are the new aperture 0 values. ... The boring command in section (vii) could be put into a script [rgm 20000614] (ix) NOW edit the CIRSILoadApertures script to have the new value of aperture 0.

16 Jun 2015: cubemean.c Assume new controler in place, loop1 not skipped Version 0.94 (November 2001) - Carine Babusiaux Add 2mass catalogue option in astrometry.pl (using 2mass.pl) Version 0.93 (20

16 Jun 2015: Then on the PLW window, go to Files->New Settings and click OK on the next few windows that pop up. ... In the Guider Control GUI, select Options->Timing and enter new rates (two sets of rates are written on the white board).

16 Jun 2015: Attempted to install new modes, but unsuccessfully 8/6/97 4.08: Installed Shutter control mode selection: type 2 = single line multiple repeat type 4 = normal type 8 = read-reset-read ... L H" % Chip 4 only % CHIPALL = "H H H H" % All Chips active %

16 Jun 2015: An ideal solution would be a dichroic filter at the output of the path compensator which would reflect infrared light to the new system while allowing visible light through to the

16 Jun 2015: The prime difficulty in moving in this direction has been the prohibitive cost of the new large arrays. ... Thus the new Keck spectra give much more promising indications of the merits of surveying for emission line galaxies in the near-infrared spectral