... The Figure shows the parallactic angle in relation to the source position at (RA,DEC), the zenith of the telescope at (LST,AoLatitude), the hour Angle HA, and the azimuth direction AZ (in the picture the source has already transitted). ... Now suppose that a second feed was placed 1 beam width away from the central horn parallel to the azimuth arm. ... Figure 1. shows the parallactic angle rate versus azimuth angle for declinations 8 through 28 (spaced 1 degree steps from Arecibo's latitude). ...

... Version 3.4.5 - 2005-06-28 (CB) ------------------------------- Ammended routine ommagnitude_mod in mssllib to set default polynomial coefficents to 1.0 and 0.0 (fixes SPR 3483 - mssllib version 2.43.12 has this fix) Also replaced source-list file in test directory with a more recent one to fix problem of negative magnitudes which cause a test-failure on one system. ... Adds a new column for the former correction. ... Version 2.2.2 2002-02-15 (CB) DEPEND file ammended to fix SPR 2757. ...

... You are here: start ТЛ lbaops ТЛ tidnotes ТЛ fileprep . ... VLBI Schedule . ... Observer's Wiki . ... lbaops:tidnotes:fileprep . Tidbinbilla schedule file preparation . ... SNAP file modifications . ... Dowload the .skd and .sum files for the experiment from the pub/people/vlbi directory of the FTP site ftp.atnf.csiro.au and put them in pcfs40:~/sched_prep. ... The SNAP file needs quite a bit of modification. ... lbaops/tidnotes/fileprep.txt ТЗ Last modified: 2015/12/18 16:39 (external edit) . ...

. Comment on J2250+1419 . Resolved: the source is extended, with about 0.15 Jy correlated flux density observed with the shortest VLBA baselines. It was not detected at 2.3 GHz by Preston et al. (1985). Augusto, Wilkinson & Browne (1998) find it partially resolved with MERLIN at 5 GHz. See Figure 3. VLBApls home page . Last modified: 16 Oct 2000

Next: Catalog Construction Up: Observations and Analysis Previous: Source Detections . ... It was assumed that the highest signal gives the most likely position of the source. ... Comparing the summed map with the maps from the individual energy ranges, the one which produced the smallest error box was chosen to represent the source position, as long as was greater than 4, a level chosen to reflect a reasonable degree of confidence in the detection. ...

do mod_pw (must be run from LRP account) . ... SU 0nnnn01 PC: xxxx cycle: 5 orb: 6 st.stat: scheduling in SPSS: Y cw_stat: S orient: Y type: GO/WFI pws.stat: planned S: Y proc_err: N lrp _state: ready LRP : 97073A ----------------------------------------------------------------------- QSP order_num: ( NONE ) week_id: ( NONE ) exe_time: ( NONE ) USC 1996.001:00:00:00 1997.054:00:00:00 M:c C:17-Feb-1997 N:FGS23GS Comment : Visit was unschedulable or had no FGS23 GSs when ...

... Galaxy Evolution home . ... The origin and evolution of radio sources . Radio sources and their environments . ... We are investigating how this interaction effects galaxy evolution in general as well as the feedback effect of the radio source on its host galaxy and AGN. ... One direct observational manifestation of this interaction is the existence of extended regions of emission-line gas which show a clear spatial relationship to the radio source itself. ...

The Astronomical Society of Australia has been asked by STANDARDS AUSTRALIA to compile a list of "designated" optical observatories that are valuable resources for (i) research, (ii) education and (iii) community use. The ASA is the final arbiter of whether any particular observatory is so designated. ... Upon receipt of your application form, your observatory will be entered on a list of "Pending Designated Observatories" on the ASA Home Page. ... It will be emailed for you. ... Email . ...

... astro-ph . ... Statistical Characterization of the Chandra Source Catalog . ... The first release of the Chandra Source Catalog (CSC) contains ~95,000 X-ray sources in a total area of ~0.75% of the entire sky, using data from ~3,900 separate ACIS observations of a multitude of different types of X-ray sources. ... In addition to these traditional catalog elements, for each X-ray source the CSC includes an extensive set of file-based data products that can be manipulated interactively. ...

October 30-31, 1992 . ... Modified images of the October 30-31, 1992 event. (a) - This NRH image is adapted to show a very bright loop-like source over AR 7321 near the SW-limb identified with the X1.7 soft X-ray LDE event peaked on 30d at 17:30 UT (see the GOES-7 soft X-ray plot also at the upper right corner). ... Here and hereafter, the white features are radio filaments. (c) - This modified NRH image shows some large scale microwave blob chains and structures. ...

. 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.

... Scheming arXiv:astro-ph abstracts almost an year never offered me an occasion that the fit of the Poisson distribution is tested in different ways, instead it is taken for granted by plugging data and (source) model into a (modified) ? ... Abstract: goodness-of-fit tests based on the Cramer-von Mises statistics are given for the Poisson distribution. ... 2 statistic for testing the goodness of fit in astronomy and this D statistics is considered as a two sided test approximately distributed as a ? ...

... 13-Aug-2014 12:13 106K lk_20140815_0905.tar.. 15-Aug-2014 09:06 106K lk_20140901_0823.tar.. 01-Sep-2014 08:23 103K lk_20141016_1324.tar.. 16-Oct-2014 13:25 103K lk_20141211_1708.tar.. 11-Dec-2014 17:08 103K lk_20150430_0315.tar.. 30-Apr-2015 03:15 103K lk_20150430_0420.tar.. 30-Apr-2015 04:20 103K lk_20150818_1511.tar.. 18-Aug-2015 15:11 104K lk_20151113_1903.tar.. 13-Nov-2015 19:04 105K lk_20160314_0610.tar.. 14-Mar-2016 06:11 105K . ...

Next: Comments on Individual Sources Up: Sample Identification Previous: Sample Identification . In Figure 2, we show the spectra of the optical counterparts to 85 of 97 observed X-ray/radio sources. ... Positional information for all 85 sources for which we announce identifications herein are given in Table 3, including information from WGACAT, the PMN and Green Bank surveys, the NVSS and our ATCA survey. ... Of the 85 newly identified sources, 59 are FSRQs, and 22 are BL Lacs. ...

Stellarium 0.12.3 . ... 51 љ virtual void update ( double ) {;} . ... 54 љ virtual double getCallOrder ( StelModuleActionName actionName) const ; . ... 63 љ QString insertSkyLayer (StelSkyLayerP l, const QString& keyHint=QString(), bool show= true ); . ... 98 љ bool loadSkyImage ( const QString& id , const QString& filename, . ... 136 љ void showLayer ( const QString& id , bool b); . ... 153 љ QString insertSkyImage ( const QString& uri, const QString& keyHint=QString(), bool show= true ); . ...

... See also changes and comments in configure.in # prefix = @prefix@ exec_prefix = @exec_prefix@ DESTDIR = CFITSIO_LIB = ${DESTDIR}@libdir@ CFITSIO_INCLUDE = ${DESTDIR}@includedir@ INSTALL_DIRS = @INSTALL_ROOT@ ${CFITSIO_INCLUDE} ${ CFITSIO_LIB } ${ CFITSIO_LIB }/pkgconfig SHELL = / bin /sh RANLIB = @RANLIB@ CC = @CC@ CFLAGS = @ CFLAGS @ SSE_FLAGS = @SSE_FLAGS@ FC = @FC@ LDFLAGS = $( CFLAGS ) DEFS = @ DEFS @ LIBS = @ ...

... Articles | ... Forums . ... 230 deg . 49 deg . ... 130 deg . ... More Info . ... 210 deg . ... 168 deg . ... 249 deg . ... 195 deg . ... 271 deg . ... 110 deg . ... 338 deg . ... July 15 . 247 deg . ... 224 deg . ... 340 deg . ... July Phoenicids (PHE) . ... August 10 . 341 deg . ... 339 deg . ... 307 deg . ... 334 deg . ... 335 deg . ... 286 deg . ... 327 deg . ... 262 deg . ... 102 deg . ... 153 deg . ... 117 deg . ... December 2 . ... 123 deg . ... 100 deg . ... www.astronomy.net . ...

... Download the code document. A new version will be released soon with a more detailed document. An X-ray source detection algorithm, optimally designed to detected faint extended sources, making use of Voronoi tessellation and Friend-of-Friend technique. ... This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License. Download sweepline.py . ... ROSAT 400d . ROSAT MACS . ROSAT WARPS . ROSAT REFLEX . ... XMM XCS . ...

Appendix B. The SPIcam routine, m2test . ... modified from dofocus. macro m2test . ... echo "USAGE: m2test <start> <initial focus step> <number of exp. pairs>" . break . end . if ($EXPTIME > 30) . echo "exposure time is $EXPTIME" . ... echo "too short to be reliable" . ... focus = $1 . ... npairs = $3 . findex = 0 . ... focus = $focus - $findex * $step . echo doing focus = $focus (exp. ... focus $focus . findex = $findex + 1 . ... comment "m2test $1 $step $npairs" . ...

Home - News - Download - Documentation - Search - FTP . About NEdit . ... Download . Get NEdit . ... nedit man page . ... Mirror Sites . ... Christian Denat . ... Back ] . ... Select word/line/file ( modified ) . ... Project macros ( modified ) ( new ) . ... Find definition ( new ) ( new ) . Find definition dialog ( new ) ( modified ) . ... Trace IF / ELSE / END IF ( modified ) ( new ) . Fold C/C++ ( modified ) ( modified ) . ... Element functions ( modified ) [ Back ] . ...