... 77, 1995 R. A. Shaw, H. E. Payne, and J. J. E. Hayes, eds. Simulation of HST PSFs using Tiny Tim J. Krist Space Telescope Science Institute, 3700 San Martin Dr., Baltimore, MD 21218 Abstract. ... The most recent ver­ sion, V4.0, includes new mirror zonal error maps and revised aberrations, significantly improving the PSF models. ... Introduction Tiny Tim is a stand­alone program for simulating HST PSFs as viewed with the on­board imaging cameras (WF/PC­1, WFPC2, FOC, COSTAR/FOC). ...

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• Interactive Fitting of EUVE Emission Line Spectra

... Science . ... Science Users Information > Science Activities > APEX Science Verification > SHFI . ... Observing Facilities . ... Observing with ESO Telescopes . ... Telescope Time Allocation . ... ESO Data . ... The Science Verification (SV) observations of the APEX Swedish Heterodyne Facility Instrument were observed in March 2008. ... A selection of the APEX-1 proposals listed below have been observed during the week of joint SV observations in March 2008, and later during the ESO time of period...

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• FORS1 Photometric System Characterization
• ESO - European ALMA Regional Centre
• ESO - ALMA

... ATNF Home . About ATNF . ... About ATNF overview . ... Australia Telescope Steering Committee . ... Australia Telescope User Committee . ... Australian Square Kilometre Array Pathfinder . Murchison Radio-astronomy Observatory . ... Parkes radio telescope . Australia Telescope Compact Array . Mopra radio telescope . ... Australia Telescope Online Archive (ATOA) . ... Visiting Parkes radio telescope . Visiting Australia Telescope Compact Array . ... Parkes radio telescope webcam . ...

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• ATCA 25th Anniversary: Accommodation
• casacore: measures/Measures/MCuvw.h Source File
• casacore: measures/Measures/MCFrequency.h Source File

Next: References Up: A Method of Integrating Previous: Description of algorithm . In April 1996 the described method was included in the software of automatic data acquisition complex "Continuous". ... The measuring of sensibility by observing at the wave lengths of 1.38cm and 2.7cm. The measuring of sensibility by observing at the wave lengths of 3.9cm and 7.6cm. wave lengths. The measuring of sensibility by observing at the wave lengths of 13.0cm and 31cm. wave lengths. ...

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• The C Preprocessor

... New Mexico State University is seeking a technical and computer-oriented person as a Support Astronomer for nighttime astronomical observing at Apache Point Observatory (APO) with the Astrophysical Research Consortium (ARC) 3.5m Telescope. б  . ... Paper/email documents will not be accepted. ... TELESCOPE OPERATIONS SPECIALIST . ... Responsibilities include nightly operation of the 3.5m telescope and instruments, Quality monitoring the data streams and system performance and observing efficiency. ...

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• coordConv
• lsst.tcc: include/tcc/telMod.h Source File
• Spectrograph Interface Control

Name Last modified Size Description . Parent Directory - drvrsmem.h 2012-11-30 14:35 6.4K fitsio.h 2012-11-30 14:35 103K fitsio2.h 2012-11-30 14:35 57K longnam.h 2012-11-30 14:35 20K . Apache/2.4.6 (Linux/SUSE) Server at www.astro.louisville.edu Port 80

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• Index of /software/sbig/archive/xmccd-4.2.1/xmccd-4.2.1/libcfitsio/include
• Moore Observatory's XmCCD Supporting Software
• Transit Finder

... These Frontier Fields will combine the power of HST with the natural gravitational telescopes of high-magnification clusters of galaxies. ... We are soliciting gravitational lensing maps for the last four Hubble Frontier Fields clusters (MACSJ0717.5+3745, MACSJ1149.5+2223, AbellS1063, and Abell 370) based upon the exceptionally deep HST FF imaging and other new ancillary data. ... For the full set of proposal instructions and requirements, see the FY16 Frontier Fields Lensing Map Call for Proposals....

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• Projects and Papers
• Convolving data models with PSF models
• Flat Fielding GPI Data Pipeline 1.0 documentation

... Liyong Liu (NAOC) . Site testing on seeing conditions of the astronomical observatories over China are briefly reviewed, including Xionglong station of NAOC, Gaomeigu station of Yunnan Observatory, Delingha station of Purple Mountain Observatory. ... PDF [3.0€аMB] October 8, 09:55 10:20 . ... In this paper, we will review the site survey activities in the past years, and present the site-testing results on the Oma site, including cloud cover, seeing, water vapor, transparency and sky brightness. ...

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Main Sections LabIR main page . Instrument page . Documentation . ... Special Sections Software Page . ... Tirgo Page . ... The activities of the group started at the end of 70's with the building of FIRT: the photometer of the National Infrared Telescope ( TIRGO ). ... FIRT: the photometer of the National Infrared Telescope ( TIRGO ). ... NICS , the NIR camera/spectrometer for the Telescopio Nazionale Galileo . ... Please select the LabIR Main Page or an item in the left menu. ...

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• CHIANTI atomic database
• Infrared astronomy

Stellarium 0.12.3 . ... Plugins . ... FileљStructure . FileљList . FileљMembers . plugins . Satellites . src . Satellite.hpp . ... 20 љ #ifndef _SATELLITE_HPP_ . 21 љ #define _SATELLITE_HPP_ 1 . ... 86 љclass Satellite : public StelObject . ... 88 љ friend class Satellites ; . ... 96 љ Satellite ( const QString& identifier, const QVariantMap& data); . 97 љ ~ Satellite (); . ... 105 љ return "Satellite" ; . ... 161 љ bool operator<( const Satellite & another) const ; . ...

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• Stellarium: core/modules/Meteor.hpp Source File
• Stellarium: /home/aw/devel/stellarium/trunk/plugins/Pulsars/src/Pulsars.hpp
• Stellarium: /home/aw/devel/stellarium/trunk/plugins/Oculars/src/Oculars.hpp

... Iowa Robotic Telescope | ... Talon is based on OCAAS, a software suite developed by software engineer Elwood Downey ( Clear Sky Institute ) for use at the University of Iowa ?s first remote facility (the ATF, or Automated Telescope Facility). ... XObservatory : Telescope Control Interface . ... This program calls upon and coordinates much of the interrelated portions of the Talon architecture, and forms the primary control panel for the telescope, dome, and peripheral systems when used locally. ...

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Over the coming weeks an international team, including Simon Jeffery , Vincent Woolf and Amir Ahmad of the Armagh Observatory, will use over fifteen different telescopes to make over one hundred nights of observations of just one star to learn about its internal structure. ... Although the approach has been used before, this may be the first time that a global asteroseismology project has tried to measure both light and spectrum variations at the same time for any star apart from the Sun. ...

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• Simon's Software - howto 1-3
• Armagh Observatory
• Software Store - Programmers Notes

... Bojan Nikolic web pages (r. 329) . ... We present a Bayesian approach to calculating the coefficients that convert the outputs of ALMA 183 GHz water-vapour radiometers into estimates of path fluctuations that can be used to correct the observed interferometric visibilities. ... Inference of Coefficients for Use in Phase Correction . ... Simulating Atmospheric Phase Errors, Phase Correction and the Impact on ALMA Science . ... Copyright 2005 -- 2016, Bojan Nikolic feedback welcome ...

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• OptInt PmWiki : Include Other Pages | Attach
• OptInt PmWiki : Include Other Pages | Edit
• OptInt PmWiki : Include Other Pages | History

... CIMAFITS is the name for the Arecibo FITS-file format. ... This is a list of (fairly) up-to-date documents describing CIMA and CIMAFITS: . The CIMA version history log which is the most up-to-date page listing all changes made to the different versions of CIMA . ... The CIMA user's log which chronologically lists changes made to CIMA that may be relevant to an observer. The CIMA engineering log which lists engineering changes made to CIMA that probably are of less interest to an observer. ...

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• Pulsar Astronomy at the Arecibo Observatory
• WAPP File Format Page
• REU Science Area

... An OBJECT column gives the name of the object observed (usually a star name). ... In critical cases, it is common practice to measure sky on two or more positions around a target object, and these positions must be identified. ... A general treatment of this problem requires a column called OBJECT, bearing the usual name of the object (as in the star tables); a column labelled STARSKY, to distinguish between star+sky, star alone, or sky alone; and additional columns to identify the sky position. ...

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• Line parameter measurements
• Input Data and Preprocessing
• Reduction of long-slit spectra

NMW survey overview . Access image archive . ... The New Milky Way survey aims to detect bright (V<13.5) optical transients near the Galactic plane using an automated wide-field (8x6 deg.) system capable of surveying the whole Milky Way area visible from the observing site in one night. ... All images obtained during the transient search survey are available online (please use the image archive access form ). ... Images per field: . ... Images per night: . ... Milky Way imaging time: . ...

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Diamond's Stealth 64 Video VRAM is the perfect choice for graphics and video performance. ... The Diamond Stealth 64 Video continues our award-winning tradition, delivering the best price / performance multimedia accelerators available. ... 64-bit graphics performance . ... Designed around a solid 64-bit graphics engine, the Stealth 64 Video VRAM provides unparalleled performance in any environment. ... The Stealth 64 Video VRAM includes hardware to accelerate video playback on the Windows desktop. ...

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• Stealth 64 Video 3200
• Stealth 64 VRAM Data Sheet
• Image: Another view. Myself included.

Next: NICMOS/HST H-band (F160W) Images Up: NICMOS Science Previous: HST NICMOS Observations of . ... Observations of P . ... The NICMOS team has devised a comprehensive program of observations of the Galactic Center. ... Data in hand give a first look at variability and a detailed look at the search for the tip of the main sequence will be discussed where NICMOS has demonstrated adequate sensitivity and photometric precision to identify likely O8-B1 stars at the Galactic Center. ...

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• STScI NICMOS Software
• AstroAsciiData

This mosaic of image swaths from Cassini's Titan Radar Mapper, taken with the synthetic-aperture radar (SAR), features a large dark region several hundred kilometres across that differs in several significant ways from other potential lakes observed on Titan. It is not as dark to the radar as many lakes (including the lakes seen here), and the nature of the margin is unusual. ...

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• When using my astronomy software or looking at various books, I notice that not
• Observing springtime deep-sky objects with a large telescope | Astronomy.com
• Springtime observing for small telescopes | Astronomy.com

CURRENT SHEET ENERGETICS, FLARE EMISSIONS, AND ENERGY PARTITION IN | SIMULATED AND OBSERVED SOLAR ERUPTIONS | ... We investigate coronal energy flow during a simulated coronal mass | ejection (CME), and compare observable characteristics of the simulation| |to observed eruptions. ... in the energy equation. ... flowing out the sides of the current sheet, the energy flowing out the | lower tip of the current sheet, and the energy flowing out the upper tip| |of the current sheet. ...

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• TESIS - Telescopes for EUV Spectral Imaging of the Sun