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
• VV29 = Arp 188 = The Chainsaw Galaxy

... You are here: start €Ё lbaops €Ё lbaapr2011 €Ё v255n . ... VLBI Schedule . ... Observer's Wiki . ... lbaops:lbaapr2011:v255n . ... Setup v255n.5cm: . ... IFP#1-LO 6642 - 6658 MHz USB RCP . ... Setup v255n.5cm-icrf: . ... Ftp: ftp://ftp.atnf.csiro.au/pub/people/vlbi/v255/v255n . ... For Hobart the LOs should be set to 468 MHz (IFP#1) and 810 MHz (IFP#2) for the 4 x 16 MHz setup and 810 MHz for the 2 x 16 MHz setup. ... lbaops/lbaapr2011/v255n.txt €§ Last modified: 2015/12/18 16:38 (external edit) . ...

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• lbaops:tidnotes:fileprep [ATNF VLBI Wiki]
• lbaops:lbanov2011:v255p [ATNF VLBI Wiki]
• lbaops:lbajul2011:v255o [ATNF VLBI Wiki]

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. ...

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• Large_Scale Emitting Chains

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 ...

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• Discovery and Analysis of 21 ѕ®m Feature Sources in the Magellanic Clouds
• Comments
• Appendix: Recipe File XML Format GPI Data Pipeline 1.0 documentation

. 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.

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• Database of Optical Constants -- Level: welcome

. Comment on J2346+0930 . See Figure 4 for an image of each component. The source was detected at 2.3 GHz by Preston et al. (1985) (correlated flux density 40 mJy) with much higher resolution. VLBApls home page . Last modified: 16 Oct 2000

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... 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). ...

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• http://www.naic.edu/~phil/misc/srctrkbyha.html
• pulsedPwrIntoAlfa
• RF observing program

ChangeLog for omsource ====================== Version 1.9.5 - 2004-01-27 (CB) -------------------------------- Ammended code so that the logger list is cleared when delete list button clicked. (fixes SPR 3230). Version 1.9.4 - 2004-01-22 (CB) -------------------------------- Modified observation information display dialogue to show dates as a MJD. (fixes SPR 3226). ... Gui improved. ... Version 1.1.8 - 2002-12-05 (CB) -------------------- Fixed some minor bugs. ... Improved user interface. ...

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• http://xmm.vilspa.esa.es/sas/5.4.1/doc/omfchain/ChangeLog
• http://xmm.vilspa.esa.es/sas/6.5.0/doc/elcplot/ChangeLog
• http://xmm.vilspa.esa.es/docs/documents/CAL-SRN-0228-1-0.ps.gz

... 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. ...

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• Index of /~jsy1001/resources
• Index of /~jsy1001/resources/oifitslib
• Index of /~jsy1001/resources/exchange

... 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 = @ ...

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

... 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 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. ...

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• Source Detections
• Source Positions
• USS radio sources

... Posts tagged ?Power? ... Continue reading ?how to trace?? ... Category: Cross-Cultural , Data Processing , High-Energy , Misc , Quotes , Uncertainty | Comment . ... Tags: arXiv , Chandra , CXC , Optical , Peter Edmonds , positional coincidence , positional error , Power , progenitor , question for statisticians , significance , Supernova , Type Ia , White Dwarf , White Dwarf binary , X-ray . Category: arXiv , Astro , Data Processing , News , Objects , Optical , Stat , Uncertainty | ...

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• The AstroStat Slog Blog Archive tests of fit for the Poisson distribution
• The AstroStat Slog Cressie
• The AstroStat Slog kriging

... 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. ...

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• newsarchive [SAI Virtual Observatory - Wiki]
• volinks [SAI Virtual Observatory - Wiki]

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 ); . ...

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• Stellarium: core/StelModule.hpp Source File
• Stellarium: core/StelVideoMgr.hpp Source File
• Stellarium: scripting/ScreenImageMgr.hpp Source File

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 ] . ...

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• NEdit
• LWN: Driver porting: Zero-copy user-space access
• Spectral energy distribution

... May 13, 1997 . Optical Transient Near GRB970508 Shows Distant Redshift . ... Explanation: The GRB distance scale controversy may have just ended with a flash . ... Most importantly, continued scrutiny showed that this optical transient had absorption lines with a redshift of about 0.8 - the distance scale of galaxies and quasars . ... Above is a "negative" image of the GRB970508 field , located near the north celestial pole, taken hours after the initial flash of gamma rays. ... About APOD > . ...

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• APOD: 2001 June 7 - NGC 253: X-Ray Zoom
• Open Source Convention
• APOD: 2007 February 24- X-rays and the Eagle Nebula

... But where visible light pictures show the nebula divided into three parts by dark, obscuring dust lanes, this penetrating infrared image reveals filaments of glowing dust clouds and newborn stars. ... This impressively sharp color image shows off the galaxy's beautiful blue spiral arms. ... Also visible in the above image of the Martian North Polar Cap are red areas of rock and sand, white areas of ice, and dark areas of unknown composition but hypothesized to be volcanic ash. ...

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... 172 ] Briefly, the count rate at the detector from a source at a redshift z is . ... Figure 55 shows the ``Green functions'' for the double compact binary merging rate   evolution assuming no collapse anisotropy. ... Another way that diverse peculiarities in the - distribution induced by the sources evolution could arise is connected with a possible non-monotonic character of the star formation rate in galaxies. ... 22 ] Figure  56 shows two-dimensional cuts through the parameter space. ...

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• Conclusions
• Sources in the LMC: comments to the Table 2
• DHTML Kitchen: Tabs

On January 23, 1998 the space probe NEAR was on its way to its closest approach to Earth. Shortly before this, a so-called sunglint event was scheduled: by re-orienting its solar panels in order to reflect sunlight onto Earth's surface, the probe would shine for a few minutes brighter than any star in the sky. ... However, we were able to record a series of images of the space probe shortly before the sunglint event, and we have assembled them into a movie. ...

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• FIRPO Help 1
• NEAR recorded on 23 January 1998(frame 1)
• mod_expires - Apache HTTP Server