... 88, Jan. 1983, p. 1-15. l. A survey of extragalactic radio sources made using driven declination scans is reported covering an area of about 0.07 sr to a limiting flux density of 35 mJy. The fast-scan survey was carried out at a galactic latitude greater than 17 deg with the NRAO 91-m telescope operating at 4.755 GHz, and the 480 sources detected were reobserved at 1.4 GHz with the National Astronomy and Ionosphere Center 305-m telescope at Arecibo. ...

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• NVSS radio survey
• The 7C(G) survey
• WSRT deep surveys

. 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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chandra_acis_ao9.par ; generate an ACIS spectrum for a source using a DEM , ; and optionally rescale the DEM to produce the same ; counts as a ROSAT / PSPC observation ; ;calling sequence ; .run initale ; @chandra_acis_ao9.par ; ;(LL/VK; modified from chandra_acis_ao5.par, Feb04) ;(LL ... density [cm^-3] T_components = [6.9, 7.4] ;log(T[K]) components in the EM EM_components = [5.1d12, 6.1d12] ;Emission Measure [cm^-3] obs_rate = 0.1 ; ROSAT / ...

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• The AstroStat Slog Blog Archive [ArXiv] component separation methods
• The AstroStat Slog Blog Archive tests of fit for the Poisson distribution
• The AstroStat Slog ICA

... 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. ...

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• News Results
• VSOP Observing Schedule
• casacore: components/ComponentModels/FluxStandard.h Source File

. XMM-Newton Science Analysis System . omatt (omatt-2.46.2) [xmmsas_20080701_1801-8.0.0] . Meta Index / Home Page . The position-angle of the major-axis of each source computed by omdetect ( PA ) is modified by omatt so that the angle is measured anti-clockwise from the North Pole. XMM-Newton SOC/SSC -- 2008-07-02

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• Change history

... 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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... 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 . ...

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• FIRPO Help 1
• mod_expires - Apache HTTP Server
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... 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

... 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

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. ... Status as a designated observatory will be reviewed every 2 years based on calendar year annual reports submitted in January. ... phone: 02 6125 0268 . ... Registry Number . ... Number of nights . ...

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• Designated Observatory Application
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... Galaxy Evolution home . Cavendish Astrophysics . Cavendish Laboratory . ... Cosmological evolution of star-forming galaxies . The origin and evolution of radio sources . Radio sources and their environments . ... Publications . ... Submitted . ... Calendar . ... Paul Alexander . P.Alexander@mrao.cam.ac.uk . ...

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• Galaxy Evolution: The origin and evoltuion of radio sources
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• Astrophysics Group members - E Waldram

... I need to take a closer look at the data. lbn SEFD, gain, and tsys vs za (ps) . ... The rotation angle is scaled to the maximum gain over the entire dataset and lbw gains are multiplied by .95 to match the lbn values. 26jul00 : processing : x101 /lb/ Aug00 /lbnjul00/26jul00.pro , plotting : x101 /lb/ Aug00 /lbnjul00/26jul00plt.pro 02aug00 : processing : x101 /lb/ Aug00 /lbnaug00/02aug00.pro , plotting : x101 /lb/ Aug00 /lbnaug00/02aug00plt.pro 03aug00 : processing : x101 /lb/ ...

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• Index of /~phil/hardware/vertex/sharemegsvertex/ocu/pcr/mscv51/source
• Index of /~phil/hardware/vertex/sharemegsvertex/lcu/pcr/c600/source
• RF observing program

We present observations of the spiral galaxy M33 with Spitzer at 24, 70, and 160 ЮМm. ... We compare the morphology of M33 at far-infrared wavelengths with other standard SF indicators such as HЮБ and radio continuum using a Fourier filtering technique to separate the diffuse emission components from compact sources. We find that the infrared emission at 24 and 70 ЮМm follows closely the structure of the ionized gas, indicating that it is heated largely by hot, ionizing stars. ... citations = 45 . ...

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• Far-infrared Source Counts at 70 and 160 Microns in Spitzer Deep Surveys
• The 24 Micron Source Counts in Deep Spitzer Space Telescope Surveys
• Hubble Operations Computing Environment

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/cmd/rotate.py Source File

. 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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• Optical constant database - Level: measurement/paper
• Database of Optical Constants -- Level: welcome
• Database of Optical Properties -- Level: subsubsubpage

You can also see this page in Russian with using KOI8 (X Windows) or CP1251 (MS Windows) Cyrillic coding. The Laboratory supports the space TV experiments, mainly in the planetary exploration missions. ... Image Co-registration . ... PHOBOS mission - Martian satellites investigations. Phobos on the Martian limb, the image from Phobos-2 probe from 02/28/89. ... Russian Space Bulletin. ... Last modified at June,26 1997 Alexey Kuzmin: akuzmin@mx.iki.rssi.ru . Back to IKI home page ...

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• Geomagnetic Indices Kp, ap, Ap, Cp and C9
• Plasma source [Oulu]
• Geomagnetic Kp Index

... Modifiers -----------------+------+----------- dict_name | text | not null dict_init | ... dict_initoption | ... not null dict_comment | ... Indexes: "pg_ts_dict_pkey" primary key, btree (dict_name) select * from pg_ts_dict; dict_name |dict_init| dict_initoption |dict_lexize| dict_comment ---------------+---------+-------------------------------------------+-----------+------------------------------ simple | ... 17158 |/usr/local/pgsql/share/contrib/english.stop| 17159 |English Stemmer. ...

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• Zen: sncat design
• Index of /groups/cluster/CEP/RADVEL

... 24-Jan-2006 16:10 . 2.7M . ... 08-Sep-2007 12:16 . ... 16K . ...

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• Index of /~inest/ASCOM/Developer Resources
• Index of /~inest/astrolib/Sun/kursoviki/Model2000/AtmModel
• Index of /~inest/astrolib/Sun/kursoviki/Model2000/AtmModel/UV

. Name . Last modified . Size . Description . Parent Directory . - . Automatically Generate a Photo Gallery from a Directory of Images_ Updated.mht . 2012-06-27 13:05 . 285K . PHP_ imagecopyresized - Manual.mht . 2012-06-27 14:40 . 540K .

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• Linux System Administrators' Guide 0.4
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• Simon's links to Grid resources on the WWW

... Thus the FTE described below must be added to the AOF FTE budget. ... Activity Scientist overview of changes (R7M) Observing preparation tool ( section 15.1) Instrument Control Panel ( section 15.2) Modification of AOF / Hawk-I acquisition template ( section 15.3) Site quality monitoring and display ( section 15.5) Exposure Time Calculator ( section 15.6) Modification Observing Tool (OT3) ( section 15.8) TOTAL FTE effort 1 0.1 0.3 0.3 0.3 0.2 0.3 2.5 ...

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• list of DFS Department documentation templates
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• Identifications and Efficiency