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... Flux density at 1 GHz (/Jy): 160 . ... Radio: Limb-brightened to NE, with faint extension to the E. Optical: Brightest to the NE, with faint filaments outside the NE boundary. ... Fesen 1984, ApJ, 281, 658. ... ADS . ... 151 MHz observations (1'.2?3'.1) and Half-Mile Telescope at 1.4 GHz (2'.1?5'.4). ... Radio, IR, optical, UV and X-ray comparison, including VLA at 1.6 GHz (3".8?3".3 and 40''). ... 1988, ApJ, 335, 215. ... IR observations of shocked O 2 . ... Observations of shocked molecular...

... ATNF Home . ... About ATNF overview . ... Australia Telescope Steering Committee . ... Publications . Publications overview . ... Parkes radio telescope . Australia Telescope Compact Array . ... Publications & acknowledgements . ... The Australia Telescope Compact Array (/ Parkes radio telescope / Mopra radio telescope / Long Baseline Array) is part of the Australia Telescope National Facility which is funded by the Australian Government for operation as a National Facility managed by CSIRO. ...

NStars 1: photometric surveyse --- | ... There are a number of 2MASS sources which have (faint) counterparts on POSS II F (R) or N (I), but don't have an entry in the GSC 2.2. ... It is possible that some images might have no GSC counterpart due to proper motion taking the source outside the 6 arcsecond search radius between the palte-taking and the 2MASS observation. ... Figure a1.1: The (F-J)/(J-K) two-colour diagram for faint sources with GSC2.2 counterparts. ... Intermediate sample . ...

... 88, Jan. 1983, p. 1-15. l. A survey of extragalactic radio sources made using driven declination scans is reported covering an area of about 0.07 sr to a limiting flux density of 35 mJy. The fast-scan survey was carried out at a galactic latitude greater than 17 deg with the NRAO 91-m telescope operating at 4.755 GHz, and the 480 sources detected were reobserved at 1.4 GHz with the National Astronomy and Ionosphere Center 305-m telescope at Arecibo. ...

home education > resources . ... Resources . ... Astronomical Pseudo-Science . ... Black Holes: An Introductory Resource List . ... http://www.astrosociety.org/2012 . ... Fraknoi, A. "Dealing with Astrology, UFOs, and Faces on Other Worlds: Guide to Astronomical Pseudo-science in Classroom," Astronomy Edu cation Review, (2004): http://dx.doi.org/10.3847/AER2003022 . ... The Skeptic's Dictionary: An excellent source of brief reviews, references, and links on dozens of areas of pseudo-science. ...

... Columns RA_CORR and DEC_CORR are only passed to the output summary source lists, when srcmatch is used on only one source list. ... Additionally, the number of entries per row for a given column can also be retrieved from the FITS keyword TDIMi (i being the column index). srcmatch will pass on the columns RA_CORR and DEC_CORR (generated by eposcorr ) from the input X-ray source list to the summary output list, only if the number of input source lists is 1 . ...

lsst.coordConv љ unknown . ... Files . FileљList . ... include . coordConv . time.h . Go to the documentation of this file. 1 љ #pragma once . ... 3 љ #include " coordConv/site.h " . ... 5 љ namespace coordConv { . ... 15 љ double lastFromTAI ( double tai, Site const &site); . ... 22 љ double julianEpochFromTAI ( double mjdSec); . ... 36 љ double besselianEpochFromTAI ( double mjdSec); . ... Definition: time.cc:43 . ... Generated on Thu May 7 2015 10:42:46 for lsst.coordConv by љ 1.8.5 ...

The ChaMP announces a second release of processed optical and X-ray data. ChaMP X-ray Point Source Catalog , the basic parameters, photometry, and flux of 6512 ChaMP sources in 130 Chandra observations from Chandra Cycles 1 and 2 (Last Update 08/09/2006, Release Notes ) . ChaMP X-ray Products and Catalogs for Publicly released Chandra/ChaMP Fields . Full Field Images includes FITS and GIF images, source lists, and X-ray data products. ...

Next: USING THE AO-CONTROL GUI FOR SPECTRAL LINE OBSERVATIONS Up: Spectral-Line Observing at AO Previous: STANDARDS OF REST & . This is the list of objects you wish to observe. Ideally, it should be named 'src.list' and should be placed in your project area on the data-taking computer. The format for your source list is: . name RhRmRs.s DdDmDs.s b/j velocity # Any comments you have . Name: Your object name, usually given as one word (no spaces). ... Good target . ... Lousy Target . ...

... Browse on Line . ... To get this to work, add a macro menu item which calls open_include() . ... Oops. ) return } # # We have a filename ; now run through our list of paths see # if we can open the file . # include_path = $g_ include _path path_separator = : bpos = 0 epos = search_string( include_path , path_separator, bpos ) while( epos bpos ) { path_bit = substring( include_path , bpos , epos ) if( open_with_test (path_bit / ...