! This is the full VLBA calibrator list. It should be treated with some caution. ! It contains entries from old VLBA calibrator lists for sources not in modern ! geodetic solutions (and probably suspect) and from fairly recent geodetic solutions ! by the Goddard geodetic group and by Leonid Petrov. There are likely to be small ! offsets between the different catalogs. For the best astrometric results, one of ! the individual GSFC or Petrov catalogs should be used. ! This is the header from Petrov's catalog:
srcid srcno ra dec x y srcname lev gl gb offset psf error ratio scale_src scale_bkg ac_ra ac_dec ac_srcname ac_gl ac_gb apmid core ratio _core ratio _pie ratio _clean error95_f1 error95_f2 15S [ Source ID] 5N [ Source number] 12N [RA by wavdetect in deg ] 12N [Dec by wavdetect in deg ] 9N [x by wavdetect in pixel] 9N [y by wavdetect in pixel] 22S [ Source name] 3N [level] 12N [Gl in deg ] 12N [Gb in ...
W Boson Properties Eric Torrence University of Oregon formerly Enrico Fermi Institute University of Chicago Eric Torrence Physics in Collision June 2001 Overview З Introduction З W Boson Production З Decay Branching Fractions З Electroweak Couplings З W Mass and Width З Conclusions All numbers from Moriond 2001 http://www.cern.ch/ torrence /talks/PIC01 Eric Torrence Physics in Collision June ... VRF Ebeam= 20 MeV? ... Eric Torrence Physics in Collision June 2001 ...
ST-ECF Instrument Science Report WFC3-2008-15 The TV2 ground calibrations of the WFC3 NIR grisms H. Kuntschner, H. Bushouse, J. R. Walsh, M. KЭmmel July 08, 2008 ABS TRACT Based on thermal vacuum tests (TV2; June - August 2007), the performance of the WFC3 near-IR G102 and G141 grisms has been assessed. ... The setup for G141 is identical. ... 10 ST-ECF Instrument Science Report WFC3-2008-15 Figure 5: Instrument efficiency of various orders for the WFC3 G141 grism as function of wavelength. ...
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Ссылки http://www.stsci.edu/hst/wfc3/documents/ISRs/WFC3-2008-15.pdf -- 1953.1 Кб -- 16.07.2008
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Ссылки http://www.stecf.org/documents/isr/WFC3-2008-15.pdf -- 1953.1 Кб -- 14.08.2008 Похожие документы
... 337, 275292 (2002) The correlation of line strength with luminosity and redshift from composite quasi-stellar object spectra S. M. Croom,1 K. Rhook,1 E. A. Corbett,1 B. J. Boyle,1 H. Netzer,2 N. S. Loaring,3 L ... We measure highly significant Baldwin effects for most broad emission lines (C IV 1549, C III] 1909, Mg II 2798, H ,H ) and show that they are predominantly caused by correlations with luminosity, not redshift. ... The correlations of log W with log(1 + z ) for each line. ...
Wed Jan 31 03:17:17 AST 2007 CIMA executive starting ... Wed Jan 31 03:17:17 AST 2007 STARTING NEW CIMA SESSION Wed Jan 31 03:17:17 AST 2007 Using CIMA version 2.2.14 'normal' from 2007-01-30 15:20 Wed Jan 31 03:17:17 AST 2007 bound to EXECUTIVE, /tmp/mailboxdefs.dtusr Wed Jan 31 03:17:17 AST 2007 online is 1 - remote is 0 Wed Jan 31 03:17:17 AST 2007 All entries in the log-file are timestamped in AST ( = UTC - 4 hours ) Wed Jan 31 03:17:17 AST 2007 CIMA session for project 'a2048' in 'line' mode for 'RT'