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1. Modification of Source-axes position angles
. XMM-Newton Science Analysis System . omatt (omatt-2.46.2) [xmmsas_20080701_1801-8.0.0] . Meta Index / Home Page . The position-angle of the major-axis of each source computed by omdetect ( PA ) is modified by omatt so that the angle is measured anti-clockwise from the North Pole. XMM-Newton SOC/SSC -- 2008-07-02
[ Сохраненная копия ]  Ссылки http://xmm.vilspa.esa.es/sas/8.0.0/doc/omatt/node7.html -- 3.3 Кб -- 02.07.2008
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2. source comment
. Comment on J2243-2544 . The jet extends in the opposite direction to that shown by Shen et al. (1998) at 5 GHz with about 2 times higher resolution than our image. The structure we see is confirmed by the 2.3 and the 8.4 GHz images from the VLBA Calibrators database. VLBApls home page . Last modified: 16 Oct 2000
[ Сохраненная копия ]  Ссылки http://www.vsop.isas.ac.jp/VLBApls/J2243-2544.comment.htm -- 1.5 Кб -- 16.10.2000
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3. http://www.naic.edu/~phil/callbn/lbSefdGT_Aug00.html
... I need to take a closer look at the data. lbn SEFD, gain, and tsys vs za (ps) . ... The rotation angle is scaled to the maximum gain over the entire dataset and lbw gains are multiplied by .95 to match the lbn values. 26jul00 : processing : x101 /lb/ Aug00 /lbnjul00/26jul00.pro , plotting : x101 /lb/ Aug00 /lbnjul00/26jul00plt.pro 02aug00 : processing : x101 /lb/ Aug00 /lbnaug00/02aug00.pro , plotting : x101 /lb/ Aug00 /lbnaug00/02aug00plt.pro 03aug00 : processing : x101 /lb/ ...
[ Сохраненная копия ]  Ссылки http://www.naic.edu/~phil/callbn/lbSefdGT_Aug00.html -- 9.0 Кб -- 04.01.2002
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4. VSOP Observing Schedule
... VS experiment codes are VSOP Survey Observations VT Test/Calibration Observations --------------------------------------------------------------------- EXPNO SOURCE FRQ Corr DOY DY: DATE UT RANGE #TEL TELESCOPES V028a2 J1733-13 L Socr 156 Su:Jun-04 06:00 - 13:00 11 VLBA TI W030e2 J1733-13 C Socr 157 Mo:Jun-05 04:00 - 13:00 11 VLBA CD W031b VS01m W030e3 J1733-13 C Pent 157 Mo:Jun-05 13:00 - 20:00 4 HH CD UD KA W031B W030f1 J1911-20 C ...
[ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/pub/people/vlbi/vsop/www/short_000604.html -- 6.8 Кб -- 27.12.2007
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5. Hubble Operations Computing Environment
... Disk space . Access to SOGS through the firewall . ... The HST planning and scheduling computing environment primarily consists of the Unix "SOGS" cluster, which includes about 30 Sun machines and about 10 MacOSX machines. ... It has 659 Gb of disk space and uses RAID 5. ... The operational Assist and PMDB databases live on the server HAL9000 which is a Fire 480R. (Since Assist and PMDB are on the same server, cross-database queries are possible and this simplifies operations.) ... Fire V210 . ...
[ Сохраненная копия ]  Ссылки http://www.stsci.edu/ops/computing/workstation-list.html -- 5.7 Кб -- 22.03.2011
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6. NVSS radio survey
... The NVSS is being made as a service to the astronomical community, and the principal data products are being released into a directory accessible by anonymous FTP as soon as they are produced and verified. ... The large (4 deg x 4 deg) map cubes and total intensity only images and their associated multisource (u,v) data sets are stored as binary files in FITS format (see Grosbol et al. ... The source catalog derived from the available images is kept in directory CATALOG as CATALOG.FIT. ...
[ Сохраненная копия ]  Ссылки http://www.sao.ru/cats/doc/NVSS.html -- 7.9 Кб -- 30.09.1998
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7. Database of Optical Properties -- Level: subsubpage
. The page is under construction. Our table shows a classification of various light scattering methods, applicability to different scatterers and to their ensembles as well as the anzatz sources and recent reviews. In comments we briefly discuss different classifications, features, relationships, available codes, comparison works and recent reviews of the light scattering methods. To the top . Created by V.I. Last modified: 10/04/03, V.I.
[ Сохраненная копия ]  Ссылки http://www.astro.spbu.ru/DOP/3-REVS/survey.html -- 2.3 Кб -- 19.11.2010
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