... 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. ...

. Comment on J2249+1136 . Resolved: this "head-tail" radio galaxy is extended, although 0.15 Jy correlated flux density is observed with the shortest VLBA baselines. See Figure 3. VLBApls home page . Last modified: 16 Oct 2000

... 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. ...

... ATNF Home . ... About ATNF overview . ... Australia Telescope Steering Committee . ... Murchison Radio-astronomy Observatory . ... Parkes radio telescope . ... Mopra radio telescope . ... Visiting Parkes radio telescope . ... Parkes radio telescope webcam . ... For example, modified Newtonian dynamics (MOND) has no relativistic extension, and so makes no firm lensing predictions, but galaxy-galaxy lensing data can be used to empirically constrain the deflection law of a MONDian point-mass. ...

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 . ...

... See also changes and comments in configure.in # prefix = /usr/local/src/xmccd-4.1d/ libcfitsio / libcfitsio -3.310 exec_prefix = ${prefix} DESTDIR = CFITSIO_LIB = ${DESTDIR}${exec_prefix}/lib CFITSIO_INCLUDE = ${DESTDIR}${prefix}/include INSTALL_DIRS = ${prefix} ${CFITSIO_INCLUDE} ${ CFITSIO_LIB } ${ CFITSIO_LIB }/pkgconfig SHELL = / bin /sh RANLIB = ranlib CC = cc CFLAGS = -g -O2 -Dg77Fortran -fPIC SSE_FLAGS = FC = gfortran LDFLAGS = $( CFLAGS ) ...

... 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 . ...

Last modified on November 25, 1996 by A. Richichi . Performance of the 1.23 mirror / November 1996 . Dear FIRPO friends, this is a report after my direct experience with the 1.23 mirror, and after Leonardo has reduced most of the photometry collected by VC/ChL in September. ... However, what is worrying is that I got the feeling that it is now much more difficult to find the sources in the eyepiece of the main mirror. ...

... 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 ? ...

Next: Code II: Unknown Up: Image Restorations of High Previous: Construction of Algorithms . ... The positions of the designated point sources ( ) must be given as well as initial amplitudes for and . ... The integrated flux of the point sources ( ) plus that of the distributed emission ( ) is constrained to equal that of the observed image ( ). ... This is investigated in Fig. 1 where all emission derives from point sources but only one - the brightest - is designated as such. ...