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 . ...

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• Designated Observatory Registry

... Galaxy Evolution home . Cavendish Astrophysics . ... Cosmological evolution of star-forming galaxies . The origin and evolution of radio sources . ... Radio sources are among the most powerful of the family of Active Galactic Nuclei (AGN). ... The overall properties of radio sources are well predicted by analytical models of self-modifying evolution of the radio source which we have developed, and many of the more unusual structures observed can be reproduced using computational models. ...

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• Galaxy Evolution: Publications submitted
• Galaxy Evolution: Regulation of the ISM and Star Formation
• Galaxy Evolution: Radio sources and their environments

... 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. ...

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• http://xmm.vilspa.esa.es/sas/7.0.0/doc/ommag/ChangeLog
• http://xmm.vilspa.esa.es/sas/5.4.1/doc/ommag/ChangeLog
• http://xmm.vilspa.esa.es/sas/6.0.0/doc/ommag/ChangeLog

... Files . ... File List . File Members . casa . ... The copyright details 00005 ** follow. ... 1024 is 10 (2^10 == 1024) */ 00077 #define LOG1024 10 00078 00079 /* these are for getting the memory statistics */ 00080 static int pageshift ; /* log base 2 of the pagesize */ 00081 static int pagesize _; 00082 00083 /* define pagetok in terms of pageshift */ 00084 #define pagetok (size) ((size) ... Generated on Fri Sep 3 2010 13:06:55 for casacore by 1.7.1 ...

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• Gravitational lensing and modified Newtonian dynamics
• VSOP Observing Schedule
• lbaops:tidnotes:fileprep [ATNF VLBI Wiki]

... use frames summary class fields routine details file attributes . ... AUTHOR: Craig B. Markwardt, NASA/GSFC Code 662, Greenbelt, MD 20770 craigm@lheamail.gsfc.nasa.gov UPDATED VERSIONs can be found on my WEB PAGE: http://cow.physics.wisc.edu/~craigm/idl/idl.html . PURPOSE: Compute confidence limits for chi-square statistic . ... CALLING SEQUENCE: DELCHI = MPCHILIM(PROB, DOF, [/SIGMA, /CLEVEL, /SLEVEL ]) . ... result = mpchilim( p , dof , sigma= sigma , clevel= clevel , slevel= slevel ) . ...

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• GLSFit.pro (JWST Pipeline routines in IDL)
• Comments
• WFPC2 Instrument Handbook Update

. 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

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Stellarium 0.12.3 . ... FileљStructure . FileљList . ... core . modules . Meteor.hpp . ... 46 љ Meteor ( const StelCore *, double v); . ... 64 љ Vec3f position; . 65 љ Vec4f color; . ... 67 љ : position( Vec3f (pos[0], pos[1], pos[2])), color(color) {} . 68 љ VERTEX_ATTRIBUTES( Vec3f Position , Vec4f Color); . ... 75 љ Vec3d obs; // observer position in meteor coord. system . ... 88 љ double xydistance; // distance in XY plane (orthogonal to meteor path) from observer to meteor . ...

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• Stellarium: core/modules/Landscape.hpp Source File
• Stellarium: core/StelSkyDrawer.hpp Source File
• Stellarium: core/StelApp.hpp Source File

... Readability |Check number: 1 | Description: Header existence for each |Evaluation (always/often/sometimes/| |source file and for each method, class, |never) : | ... Description: Naming conventions existence |Evaluation (always/often/sometimes/| |(variables start with lowercase, then |never) : | ... limited and commented |(always/often/sometimes/ | ... Description: Error message are formated : when an|Evaluation | error or an exception is raised, report the |(always/often/sometimes/ | ...

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• http://www.eso.org/~rsiebenm/FTP/PR13/HAWKiGraal_sciopsCRE.pdf
• ESO - Science Announcements
• ESO - Librarians' Professional Resources

... THE DETAILS . ... proj> : This is just your project number (i.e. a9999) and it is used both for making the executable file name (a9999.exec) and for knowing the name of your .sls set-up files (assumed to be a9999.sls). start_lst(hh:mm) : The is the LST at which your observations will start. ... You tell the program which .sls file to use for a given observation by the target object's priority number -- a priority of 2 selects the "b" set-up file, while all other priorities select the "a" set-up file...

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• CIMA Configuration Files
• Details of Rotang
• SPECTRAL LINE APPENDICES

... The fourth catalogue of radio sources observed at 408 MHz with the Molonglo radiotelescope is presented. A total od 1349 sources is listed to a limiting flux density of 0.2 Jy, the catalogue being largely above 0.25 Jy. ... Those sources for which hogh-frequency or optical data are available are classified into two lists, one of Cloud members and the other of 'unidentified nonthermal sources', presumably not Cloud members. ... 1973), AuJPS, 1973, n.28, p.1-?? ... 1974), AuJPS, 1974, n.33, p.1-44 . ...

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• THE TEXAS SURVEY: Published
• VLA 404 compact sources
• NVSS radio survey

... This gives a nice opportunity to check the quality of the FIRPO photometry against that of TIRGO. ... The values are Program POLYFIT V 10/Jul/90 ( A.Richichi ) - 24-Aug-1997 13:38:25 File : diff_temp_jc.dat Pol. degree: 1- N = 10- [ 2786.00- 4095.00 ] - [ 0.00- 1194.00] 1 -.10304E+01 0.26412E+00 2 0.29958E-03 0.74406E-04 sdev: 0.16063E+00 chi2 :0.24486E+01 Program POLYFIT V 10/Jul/90 ( A.Richichi ) - 24-Aug-1997 13:42:59 File : diff_temp_hc.dat Pol. degree: 1- N = 10- [ 2786.00- ...

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• FIRPO Help 3
• Server-Wide Configuration - Apache HTTP Server
• SWXCS

... Next: The PROS Big Up: Software Systems Previous: Data Reduction Software . ... The srcinten task provides PROS users with a tool to compute count rates for point sources in the ROSAT High Resolution Imager (HRI). ... Corrected upper limits are cited at locations where the count rate falls below the source detection threshold. ... Srcinten is a new PROS task that computes and applies the above correction factors to the net counts in a user-specified aperture. ...

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• ADASS 2002 Conference Proceedings
• An Extragalactic Point Source Simulator for SIRTF Pipeline Testing
• A User Friendly Planning and Scheduling Tool for SOHO/LASCO-EIT

... 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 ) ...

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• http://www.astro.louisville.edu/software/sbig/archive/xmccd-4.2.1/xmccd-4.2.1/libcfitsio/libcfitsio-3.340/Makefile
• http://www.astro.louisville.edu/software/sbig/archive/xmccd-4.1/xmccd-4.1e/libcfitsio/libcfitsio-3.310/Makefile.in
• Moore Observatory Astronomical Software Resources

August 3, 1998 . ... An example of the EUV large-scale chains revealed by the modified TRACE EUV images. (a) - The original TRACE EUV (171 A) mosaic image of August 3, 1998. Some thin chains and threads are seen inside the active complexes A and B in the north-west and south-west sectors of the disk. Large-scale structures outside the complexes are hardy visible. (b) - The same TRACE image, but after a modification. ... Back to the page of the TRACE chains . ... Last update: 9 August 1998 . ...

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• http://www.izmiran.rssi.ru/~ichertok/CHAINS/ANNOUNC/921030.htm
• Large_Scale Emitting Chains

... 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 . ...

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• The NMW survey homepage

This service contributes to the International Service of Geomagnetic Indices (ISGI) of the IAGA . ... The Kp numbers of the previous month are available in tabular format . ... There are available also historical and current Kp and derived indices per anonoymos FTP (see below). ... U.S.A. FTP server: ftp://ftp.ngdc.noaa.gov/STP/GEOMAGNETIC_DATA/INDICES/KP_AP/ . monthly update) . ... contains the monthly Kp / ap tables in a simple text format readable for both humans and computers (*.tab). ...

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• IKI IPL home page

Databases (NSDC) of the Natural Planetary Satellites. ... NSDC: Database of astrometric observations of Natural Planetary Satellites . ... They are thoroughly looking for observations in different sources, creating their owndatabases which are then mostly inaccessible to other researchers. ... In the file "content" with explications, the reference is given to the data source as well as the bibliographic reference. ... Data sources. ... Why a specific bibliographic database for Natural satellites? ...

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... 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 ? ...

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• The AstroStat Slog Blog Archive Eddington versus Malmquist
• Comments on: The Banff Challenge [Eqn] By: hlee By: Paul B By: vlk By: brianISU
• The AstroStat Slog Goodness of fit

... Prev . Next . comedi_command_test -- test streaming input/output configuration . ... int comedi_command_test (comedi_t * device, comedi_cmd * command); . The function comedi_command_test() tests the command structure pointed to by the parameter command and returns an integer describing the testing stages that were sucessfully passed. In addition, if elements of the command structure are invalid, they may be modified. Source elements are modified to remove invalid source triggers. ...

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• The spectrograph design and the observing procedure
• NEdit.org
• Radio sources identfification

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" . ...

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• lsst.tcc: python/tcc/mov/checkSegment.py Source File
• lsst.tcc: python/tcc/mov/checkPos.py Source File
• lsst.tcc: python/tcc/mov/fullSlew.py Source File