... The J, H and K bands are characterized by a bright background, such a background is mainly due to the emission of atmospheric lines and of thermal radiation. ... If the source cover a large fraction of the slit, spectra off-source must be observed to adequately sample the sky background. ... The on chip integration time (time spent in each position of the slit) must not exceed 40 seconds in J and H bands and 60 seconds in K band. ... We suggest a sequence of 10 for each elementary integration time. ...

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• Radioastronomy reduction procedures
• FIRPO Runs

... The analysis and reduction of the STIS flanking fields proceeded in similar fashion as for the imaging of the Main STIS Field. ... The DARK calibration reference file used in the CALSTIS data reduction steps was constructed using a 'delta-dark' image appropriate for the epoch of the flanking field observations. ... DRIZZLE drop-size used for the flanking fields was a "pixfrac" of 0.8. ... For information on the data reduction, please read first the technical information for the Main WFPC2 Field . ...

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• HDF-S Sydney Meeting Follow-up Notes
• HST Primer for Cycle 22
• NICMOS Data Handbook

Next: Photometry Up: Data files Previous: Astrometry Contents . Spectroscopy data files have the extension .vel . ... Available symbols are (0), x (1), * (2), triangle up (3), triangle down (4), square (5), diamond (6), pentagon (7), star (8) and circle (9). ... A 2428890.9305 -16.8 1.8 A 2428918.6569 +54.2 4.4 B 2443477.748 +145.0 5.0 B 2443478.743 -199.0 5.0 B 2443497.646 +179.0 5.0 B 2443498.673 -169.0 5.0 B 2443501.689 -201.0 5.0 C 2422984.4 -10.5 1.6 C 2425125.5 +5.9 0.6 . ...

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• ESO - Science Announcements
• ESO - Newsletter December 2015
• ESO - Newsletter January 2016

... This step is done mostly interactively and uses some basic ad-hoc IDL procedures, mainly for testing and checking of the consistency of the results.Once the observations have been selected and the count spectra extracted, the available spectra of each background level are accumulated. ... Average QUALITY such that QUALITY =0|1 Exposure times are added and the total is written in the EXPOSURE keyword of the header of the output FITS file. Finally, the CCFs are built from these templates. ...

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• How to reprocess ODFs to generate calibrated and concatenated EPIC event lists
• XSPEC session thread
• Procedure

For solar wind dials without any explanatory text, see this page . ... There are three logs, one for each condition index ( K P , Solar Wind ,and NOAA/SEC .) ... More about the solar wind's recent behavior can be found on my Current Solar Wind Conditions page. ... Other items of interest include NOAA/SEC Current Conditions , my composite current Auroral Images page, Windows on the Universe: Space Weather , and Public Outreach Index, Department of Space Physics and Astronomy, Rice University . ...

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... The 209 candidates were selected from our first and second priority samples introduced in Paper IV. Of 169 first priority candidates, 141 objects appeared in our list as new ones. 28 objects were listed in the NED as galaxies or objects from various catalogs with known redshifts and some of them already had information on emission lines in earlier publications. ... The ``random selected sample'' was created to access the fraction of BCGs in the second priority list and contains 43 objects. ...

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• Data reduction
• Selection method
• Emission-line galaxies

... The clock correction system described here refers the Parkes clock to UTC(NIST) and to UTC as defined by the BIPM. The data to make these corrections in TEMPO are stored in two files: . ... To checkout the repository, do the following on any ATNF machine: cd $CVSHOME cvs co soft_atnf/atas/clkcorr Ensure that the executables are up-to-date: cd $CVSHOME/soft_atnf/atas/clkcorr make Then follow the procedure outlined below to generate the clock correction files required by TEMPO: . ...

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• Follow up observations
• Other deconvolution tasks
• Pulsar group | Main / ANDSATNF

. Home . Structure of Data . Description . Catalog . Publications . VO . ЮБ 2000 . 23:56:37.5 . ЮД 2000 . +61:24:02 . l . 116.420 . b . -0.776 . diameter . 4.0' . (m - M) 0 . 12.2 0.17 . distance . 2750 220 pc . E(B - V) . 0.49 0.02 . log(t) . 8.2 0.05 . SAO 1-m, BVRI observations (777 measurements) VOTable . 2MASS data VOTable . IPHAS IDR data VOTable . Developed by the Team . Send us your questions or feedback

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• SAI OCL Catalog King 20
• SAI OCL Catalog Koposov 12
• SAI OCL Catalog King 18

... At 22:42:27 UT 26/07/09, the Burst Alert Telescope (BAT) on board of the SWIFT multi-wavelength space observatory triggered and located GRB 090726 gamma-ray burst event. ... About half an hour after the BAT trigger, the first images were obtained with the SAO RAS Zeiss-1000 telescope in four BVRI filters (see Fig.1). ... The spectrum of the optical transient was obtained with the SAO RAS 6-m BTA telescope 1.54 hours after the burst, using the SCORPIO instrument in the spectroscopic mode (Fig.2). ...

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• LSFVO: SCORPIO project
• Optimization of spectroscopic observations

... Astrophysics Group . Graduate Research Opportunities 2016 . Available research projects/areas . ... Astrophysics Admissions Form . ... This includes active participation in the development of new instruments as well as the use of ground and space observatories. ... Further details are available at the following web site: http://www.mrao.cam.ac.uk/research/extragalactic-group-2/ . ... Our research group has a wide range of expertise in the development of receivers for radio astronomy. ...

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• AMI-Planck Follow-up Observation Database
• OptInt PmWiki : MROIFastTipTilt / Doc Man
• Links for NST IB Physics B `Classical Dynamics'

... This class is designed to be an up to date summary of the last 10-20 years of observations relevant to Cosmology. ... Theory today is bombarded by a vast array of observational data but there remains no clear and preferred model for the origin and evolution of structure in the Universe. ... The inflationary paradigm and the nature of the Dark Matter - Inflation solves a lot of problems that are inherent in the standard Big Bang Model. ... Kinds of Dark Matter and Observational Constraints . ...

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• The Galaxy Gallery Page VII: Infrared Imaging
• THE HUBBLE LAW JAVA APPLET

... Proposing for VLBI Time at Arecibo . ... Documentation (Field System, VLBA4 terminal, Mark 5 system) . ... In 2001, the Arecibo Observatory received its hybrid VLBA-MARK IV (VLBA4) data acquisition system, and currently NAIC commits Arecibo to support VLBI observing up to a maximum of 4% of the 305-m's observing time. ... Tracking Time (h:mm) . ... The inclusion of the 305-m Arecibo radio telescope can dramatically boost the sensitivity of VLBI observations, even with its limited source tracking...

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• The Mock Spectrometer
• ALFA Sky Angle Tracking
• Arecibo Observatory L-Wide Band Receiver

Astronomy Discussion Forums . Forums: . ... Discussion Forums . ... Follow Up . Forum List | Follow Ups | Post Message | ... Login to Post . ... www.astronomy.net . About Astronomy Net | Advertise on Astronomy Net | ... Unless otherwise specified, web site content Copyright 1994-2016 John Huggins All Rights Reserved . Forum posts are Copyright their authors as specified in the heading above the post. "dbHTML," "AstroGuide," "ASTRONOMY.NET" & "VA.NET" . ...

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• NIGHTCAL – New Version 0.7.2 Available To Download - an Astronomy Net Software
• Re: Re: RPM Package Available For XEphem 3.4? - an Astronomy Net XEphem Forum
• Re: RPM Package Available For XEphem 3.4? - an Astronomy Net XEphem Forum

Peremennye Zvezdy", . ... Max . Min . ... USNO-A2.0 0525-03498176 . ... Comm. ... USNO-A2.0 0525-03518699 . ... USNO-A2.0 0525-03528829 . ... USNO-A2.0 0525-03533089 . ... USNO-A2.0 0525-03553393 . ... USNO-A2.0 0600-44453902 . ... USNO-A2.0 0600-44469023 . ... 0.0008 . ... 0.0007 . ... 0.0007 Min II =14 m .36. ... 0.0005 Min II =15 m .66. ... A close pair of two stars: USNO-A2.0 0525-03533089 and USNO-A2.0 0525-03533312. USNO-A2.0 0525-03533089 varies. ... Comparison star . ...

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Posting Observations . ... You will need to subscribe to vsnet-acc (to allow you access to post your observations). ... VSNet has several different e-mail sigs, and sub sigs. ... These list are controlled by a software package called " Majordomo ", which allows you to subscribe and unsubscribe yourself from these list with an e-mail message (automated). ... Once you have subscribed to vsnet-acc (which will only send you a welcome message back and nothing else) you can post to the other list. ...

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. Grazing Incidence X-ray Reflectivity: Studies for the AXAF Observatory . X-Ray Reflectivity I: Reflectivity of Iridium Coatings . Density Measurements: Rutherford Backscattering Spectroscopy . AXAF Coating Process Selection Study: Reflectivity Measurements . Other Related Web Sites: . X-ray Interactions with Matter (Maintained by Eric Gullikson at LBL: atomic scattering factors, x-ray properties, calculate reflectivity, transmission, attenuation, etc. of X-rays) . Pat Slane's Home Page

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• Doug Burke's Perl/S-Lang pages: Datatype examples
• Doug Burke's Perl/S-Lang pages: General examples
• TRANSFERRING PROS 2.5 FILES

... International Astronomy Olympiad 2002 . ... The 7th International Astronomy Olympiad will be held on October 22-29, 2002 at the Special Astrophysical Observatory of Russian Academy of Sciences (SAO RAS) in North Caucasus. ... Authorized National Representative Astronomy Organizations (ANRAO) of the participating countries are authorized to form the teams of the Olympiad member-states. ... VII IAO . ... Information about the International Astronomy Olympiad 2003 will be known in the late 2002. ...

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• VI International Astronomy Olympiad: information available before
• Laboratory for Spectroscopy of Molecular Structures
• VIII International Astronomy Olympiad: information available before

Follow-up astrometry and recoveries are made with the ANU 40 inch (1.0-m) f/8 reflector at Siding Spring Observatory (IAU code 413). ... A routine follow-up of 2003 WY153 on 2003 Dec 15 became much more than routine when a faint object with unusual motion vector was found close to the target asteroid. ... During routine astrometry with the 1.0-m to improve the orbit of the Apollo asteroid 2004 CB, the asteroid was found on March 30 to have a short tail! ... Siding Spring Survey Main Page . ...

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• Naomi McClure-Grffiths Group
• Marc White - Astrophysicist - The Australian National University
• Student Briefing

... The technology needed to implement a Distributed Astronomical Data Archive (DADA) is available today (e.g., Fullton 1993). Query interface standards are needed, however, before the DADA information will be discoverable. ... These parameters would be used to index each dataset in each catalog. ... The technology is available today to perform cross-catalog queries, to fetch the data at the click of a mouse, quickly to add new observation catalogs, and to distribute the load across multiple machines. ...

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• Organizing Observational Data at the Telescope
• ADASS 2003 Conference Proceedings
• On-The-Fly Re-Calibration of HST Observations

Lab . Main page News People . ASA . Master . Master net Homepage . ... Lomonosov Moscow State University Sternberg Astronomical Institute . ... MASTER . ... Lomonosov (ShOK) . ... About Space Monitoring Laboratory, scientific directions, instruments, contacts . People, who work in lab . Latest news and news archive . ... All news ...

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• Ya.B. Zeldovich All-Moscow Seminar of Astrophysicists