Search
Search Funnelback University
- Refined by:
- Date: 2015
21 -
70 of
91
search results for news |u:people.ast.cam.ac.uk
Fully-matching results
-
Appendix E - Batch files
https://people.ast.cam.ac.uk/~optics/cirpass/Software/PixCel/PixCel_install_floppy_281100/ir_app.htm16 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 -
CIRSI Project Review
https://people.ast.cam.ac.uk/~optics/cirsi/cirsi-prog-rev-0397.htm16 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. -
Chapter 1 - Installation
https://people.ast.cam.ac.uk/~optics/cirsi/docs/pixcel/20010508/chapter1.htm16 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. -
DAZLE Bibliographic WWW Page
https://people.ast.cam.ac.uk/~optics/dazle/bibliography/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. -
CIRSI (Sackler) Camera
https://people.ast.cam.ac.uk/~optics/cirsi/pubs.html16 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: -
DAZLE – the design Introduction DAZLE, the Dark Ages ...
https://people.ast.cam.ac.uk/~optics/dazle/info/DAZLE%20design%20concept.htm16 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 -
Rockwell PICNIC array
https://people.ast.cam.ac.uk/~optics/tech/hawaii/picnic.htm16 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. -
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. -
Infrared Installation
https://people.ast.cam.ac.uk/~optics/cirsi/docs/pixcel/20010508/ir_config.htm16 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. -
https://people.ast.cam.ac.uk/~optics/fits/year2000_announcement.txt
https://people.ast.cam.ac.uk/~optics/fits/year2000_announcement.txt16 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 -
SPIRAL phase A: A prototype IFS for the AAT
https://people.ast.cam.ac.uk/~optics/spiral/papers/spie.htm16 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 -
New Page 1
https://people.ast.cam.ac.uk/~optics/people/cdm_CV_130509.htm16 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. -
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 -
COHSI
https://people.ast.cam.ac.uk/~optics/cohsi/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 -
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 -
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 -
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). -
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 -
MGB thesis Chapter1
https://people.ast.cam.ac.uk/~optics/tech/mgb_phd/chapter1.htm16 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 -
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. -
CIRPASS TECHNICAL STUDY
https://people.ast.cam.ac.uk/~optics/cirpass/hdf.htm16 Jun 2015: 1996) New Astronomy, 1, 177. Maihara et al. (1993) P.A.S.P., 105, 940. -
fellowships_2015
https://people.ast.cam.ac.uk/~phewett/HPeiris_fellowships_2015.pdf30 Sep 2015: While you may have many ideas and projects from your PhD to continue in your first postdoc, don’t let this stop you from developing new collaborations with people at your -
HAWAII SAM MICROCODE
https://people.ast.cam.ac.uk/~optics/cirsi/SAM/cirsi_sam_microcode_doc_27may98.html16 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. -
Observing guide for CIRSI (WFIRC) at LCO du Pont ...
https://people.ast.cam.ac.uk/~optics/cirsi/cirsi-guide-lco-0.6.html16 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). -
3CD8ACD5-01E7-18B8
https://people.ast.cam.ac.uk/~optics/dazle/info/science.pdf16 Jun 2015: this regime can we expect to discover and open up new astrophysics in the early universe. ... Either result would be very important and open up new parameter space in observational cosmology. -
MGB thesis Chapter 4
https://people.ast.cam.ac.uk/~optics/tech/mgb_phd/chapter4.htm16 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 -
Project Reassessment Start Date
https://people.ast.cam.ac.uk/~optics/cirsi/docs/review/webreview.htm16 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 -
This is the text of the SAM microcode that ...
https://people.ast.cam.ac.uk/~optics/cirsi/SAM/cirsi_sam_microcode_code_27may98.html16 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 % -
https://people.ast.cam.ac.uk/~optics/cirpass/Software/drivers.list
https://people.ast.cam.ac.uk/~optics/cirpass/Software/drivers.list16 Jun 2015: PGDRIV 0 /PGMF PGPLOT metafile (new format, experimental) Std F77! PPDRIV 1 /PPM Portable Pixel Map file, landscape! -
Sofwate engineering / style manual
https://people.ast.cam.ac.uk/~optics/software/softeng.htm16 Jun 2015: im_ - Pointer to an image created with new(). h_ - Handle. -
Infrared Installation
https://people.ast.cam.ac.uk/~optics/cirpass/Software/PixCel/PixCel_install_floppy_281100/ir_config.htm16 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. -
Chapter 2 - Operating the software
https://people.ast.cam.ac.uk/~optics/cirsi/docs/pixcel/20010508/chapter2.htm16 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. -
CIRSI INT Observing Guide
https://people.ast.cam.ac.uk/~optics/cirsi/cirsi.guide.ing.html16 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. -
Observing guide for CIRSI (WFIRC) at LCO du Pont ...
https://people.ast.cam.ac.uk/~optics/cirsi/cirsi.guide.html16 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). -
Craig Mackay
https://people.ast.cam.ac.uk/~optics/people/cdm_pub_list_130509.htm16 Jun 2015: Moshut. Woodbury, New York : American Institute of Physics, 1998. (AIP conference proceedings ; 428), p.499. ... S. Young, and D. F. Buscher. A new photon counting spectrometer for the COAST. -
https://people.ast.cam.ac.uk/~optics/fits/year2000_agreement.txt
https://people.ast.cam.ac.uk/~optics/fits/year2000_agreement.txt16 Jun 2015: Readers should be altered as soon as possible to cope with the new format. ... Cases of DATE-OBS before 1900-01-01 should always be written with the new format. -
Craig D Mackay
https://people.ast.cam.ac.uk/~optics/people/cdm_career_summary.htm16 Jun 2015: I found a British company (now called E2V Technologies ) working on a new detector called the Charge Coupled Device (CCD). -
Automatically generated thumbnail gallery
https://people.ast.cam.ac.uk/~optics/cirpass/World-tour/LaPalma/Pictures/pics-lpo-2004b/Instrument%20construction/16 Jun 2015: The CIRPASS team and the new CIRPASS plug-plate system at cassegrain. -
Mon. Not. R. Astron. Soc. 000, 000–000 (0000) Printed ...
https://people.ast.cam.ac.uk/~wyatt/smw15.pdf15 Jan 2015: The dust detectoraboard New Horizons may soon detect dust in resonance. -
Appendix XXX
https://people.ast.cam.ac.uk/~optics/cirsi/docs/review/appendix.doc16 Jun 2015: QUAD_SEL= "H" % Latch new quadrant mask %. CHIP_SEL= "H" % Latch new chip mask %. _SELECT = "L L" % Don't change quad or chip select%. % -
PROVISIONAL FAINT STANDARDS
https://people.ast.cam.ac.uk/~optics/cirsi/calib/faint_stds.html16 Jun 2015: The new, definitive list of UKIRT standards will be published, more formally than the old, in due course. -
MGB thesis Chapter 6
https://people.ast.cam.ac.uk/~optics/tech/mgb_phd/chapter6.htm16 Jun 2015: New technologies being developed for space applications such as composite or thin metal mirrors could offer a solution. -
Other IFUs
https://people.ast.cam.ac.uk/~optics/cirpass/docs/other_ifu.html16 Jun 2015: status. commissioned WHT June and Sept 1999, foreoptics modified during 2000 to work with new WHT AO system, NAOMI. -
Chapter 3 - Operating the Camera
https://people.ast.cam.ac.uk/~optics/cirsi/docs/pixcel/20010508/chapter3.htm16 Jun 2015: Check the 'Override settings for.' to make changes to settings, or check 'Store as.' for the creation of a new setting. ... To create a new sequence of single or multi image acquisition, select the Sequence tab. -
Draft version January 19, 2015Preprint typeset using LATEX style ...
https://people.ast.cam.ac.uk/~wyatt/mmks15.pdf19 Jan 2015: 3 School of Physics, University of New South Wales, Sydney,NSW 2052, Australia. ... 4 Australian Centre for Astrobiology, University of New SouthWales, Sydney, NSW 2052, Australia. -
Project Reassessment Start Date
https://people.ast.cam.ac.uk/~optics/cirsi/docs/review/review.doc16 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 -
https://people.ast.cam.ac.uk/~optics/cirsi/ociw/DuPontIoaTimeProposals…
https://people.ast.cam.ac.uk/~optics/cirsi/ociw/DuPontIoaTimeProposals/cirsi-dupont-bulge-gilmore-proposal.txt16 Jun 2015: New L-band data are being obtained in an approved program at the South Pole facility. ... SCUBA data are being obtained and analysed, together with new high-resolution CO data. -
https://people.ast.cam.ac.uk/~optics/cirsi/ing/proposals_public/2001/2…
https://people.ast.cam.ac.uk/~optics/cirsi/ing/proposals_public/2001/2001a/int_2001a_cirsi_sur.log16 Jun 2015: It should NOT be used for NEW documents! New documents should use Standard LaTeX conventions and start with the documentclass command. -
Chapter 4 - Controls Reference
https://people.ast.cam.ac.uk/~optics/cirsi/docs/pixcel/20010508/chapter4.htm16 Jun 2015: New Select the New file icon to clear the image area to start a new image. ... Software toolbar. New file Select the New file icon to clear the image area to start a new image.
Search history
Recently clicked results
Recently clicked results
Your click history is empty.
Recent searches
Recent searches
Your search history is empty.