M1 image More About M1 Nice Color Picture . ... M16 image More About M16 HST image . ... M31 image More About M31 Nice Color Picture . ... M42 image ; M43 image More About M42/43 Nice Color CCD Picture . M51 image More About M51 Color Image of M51 M51 Supernova . M57 image More About M57 Nice Color CCD Picture Very Deep M57 Image . ... M81 image More About M81 M81 Supernova Ultraviolet Image of M81 More about Ultraviolet Imaging . M82 image More About M82 M82 False Color M82 True Color . ...

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• Astronomy Plus CCD Images of Galaxies
• Astronomy HyperText Book: Stellar Evolution
• THE HUBBLE LAW JAVA APPLET

Current status of the source finding service: HALTED . ... Also fixing a bug preventing the sorting of output source lists. 13/6/2012 - v1.6, r15987 - Improved Gaussian fitting, performance improvements, use of casacore-1.4.0 and a few bug fixes. ... A major part of the ASKAP software development is to produce an effective source-finding tool to automatically process the images and cubes that come out of the pipeline imager. ... Please report any bugs or problems via the Redmine ticket system . ...

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• Research
• Duchamp Source Finder
• The HIPASS Bright Galaxy Catalog

CATS home ] [ Back to CATS list ] [ ftp ] . ... Received 1999 November 5; accepted 2000 February 10 Since radio sources with Ultra Steep Spectra (USS; alpha -35ddeg, we selected only sources with angular sizes Theta Comparison with spectrally unbiased samples at similar flux density levels, shows that our spectral index, flux density, and angular size selections do not affect the angular size distribution of the sample, but do avoid significant contributions by faint foreground spiral galaxies. ...

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• THE TEXAS SURVEY: Optical identifications
• MIT-GB catalog
• THE MOLONGLO REFERENCE CATALOGUE/1Jy. III

Information and Resources . ... Two of the most commonly-used browsing tools are Gopher and World-Wide Web (and its clients, such as NCSA Mosaic or Lynx). ... You can use Gopher to access STEIS by typing the following command (Figure 9.3 shows the results): . ... The World-Wide Web (sometimes referred to as WWW or W3) is a hypertext-oriented way of navigating through the Internet and finding information. ... Figure 9.6 shows the Lynx interface. ... Figure 9.5: - Using Mosaic to Read WWW Home Pages . ...

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• The Spitzer discovery of a galaxy with infrared emission solely due to AGN
• Herschel Key Program Heritage: a Far-Infrared Source Catalog for the Magellanic
• Local astronomers find gigantic halo around neighboring galaxy - By MEGHA

... This thread illustrates a step-by-step recipe to perform EPIC sources detection. ... However, some users - in particular SAS novices - may find useful to perform each individual step of the source detection algorithm, to achieve a better control and understanding of its outcomes. ... The event list MOS.evt is assumed to have been already cleaned for high-background intervals, following, e.g. , steps 3. to 5. in the edetect_chain thread . ... An example of MOS background map is shown in Fig.3. ...

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• EPIC source finding thread: edetect_chain
• General Comments
• Source image

Next: *imcnts* - Find counts Up: Regions and Source Parameters Previous: *isoreg* - A region . ... xi xspatial # Load the spatial package xs imcnts # Run the task to count photons source image file : xdata$rp110590.qp # Input file , use complete filename source region descriptor: c 6930 9390 240 # Circle at 6930 9390 # with radius of 240 pixels background image file or cts/pixel: xdata$rp110590.qp # From the same file bkgd region descripton: a 6930 ...

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• Where to Find Example/Test Code
• *imcnts* - Find counts in an extended region, after removing an embedded point
• The AstroStat Slog source detection

... Are HVCs a common feature of star forming galaxies? ... Consider the typical properties of the smallest HVCs (compact HVCs) found in HIPASS: . Distance . HI Mass . ... At 5 kpc . meager objects ~116 solar masses . ... 1.15 x 10 4 solar masses . ... Putman et al. (2003) found none to 10 7 solar masses. 2% of Sculptor to 3 x 10 6 solar masses by de Blok et al. (2001) found none. ... High velocity gas around other galaxies can be identified from maps and dynamics: . ... 2003) . ...

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• Arecibo Galaxy Environment Survey (AGES)
• Pulsar Highlights - ALFA Finds Youngest Binary Pulsar Ever
• The Arecibo Zone of Avoidance Survey (ALFAZOA)

The Astronomy Net . Articles | AstroGuide | ... Forums . ... H ere you can find resouces to help understand perhaps the grandest of all sciences. ... Upcoming Sky Events . ... This site includes lists of manufacturers, vendors, software, etc. organized in the AstroGuide to help when you are looking to purchase your tools. ... Astronomy Articles . ... Are you interested in writing an article for the Astronomy Net? ... www.astronomy.net . ... dbHTML," "AstroGuide," "ASTRONOMY.NET" & "VA.NET" . ...

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• Finding Himalia, The Fifth Brightest Moon Of Jupiter - an Astronomy Net Article

... LABORATORY OF RADIO ASTRONOMICAL OBSERVATIONS . Radio sources identification is one of the most important tasks of the current radio astrophysics. ... Optical idetification. ... Optical identifications of subsample of steep spectra radio sources from RC catalog using 6m SAO telescope of SAO RAS: optical observations. ... Astronomy Reports. ... Identification of radio sources with data of various radio catalogs allows one to construct continual spectrum of the object and its radio structure. ...

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• The ROSAT Bright Survey: II. Catalogue of all high-galactic latitude RASS
• Bispectrum speckle interferometry and future long-baseline interferometry of
• Search for distant radio galaxies in SAO

Astronotes Armagh Planetarium's Stellar Blog! ... Armagh Planetarium . ... Our Galaxy . ... Other Galaxies . ... Space Flight . ... This week?s€а Carnival is hosted by the excellent We Are All in the Gutter (Looking at the Stars) blog .€а You can go straight to the Carnival by clicking here. ... Hello, IтАЩm Colin, welcoming you to Astronotes, the PlanetariumтАЩs official blog. Here you will find the latest news and views from the fascinating worlds of astronomy and space exploration. ...

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• ESO finds weird doomed planet from another galaxy | Astronotes
• Finding Your Way in the Milky Way | Astronotes
• How has Mars changed over billions of years? | Astronotes

home resources . SEARCH ASP SITE: Match ALL words Match ANY word . ... Books . Favorite Links . ASP Educational Resources . Your resource for unique education materials, ASP favorites, technical publications, and more.. ... Your purchases help support the education programs of the ASP. We feature our favorite new Astronomy books with short descriptions. Looking for archived Books of Note? ... Feature Book . ... Feature Link . ... Publications | ... education | resources | ...

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• ASP: The Universe At Your Fingertips Activities TOC
• ASP: Black Holes: An Introductory Resource List
• ASP: Astronomy Behind the Headlines

The HyperNews Linux KHG Discussion Pages . Forum: The Linux Kernel Hackers' Guide . Re : Linux SMP Scheduling (Angela) . Date: Mon, 16 Mar 1998 16:34:54 GMT . From: Felix Rauch < rauch@inf.ethz.ch > . The definition of NO_PROC_ID can be fount by, e.g., the following command: . find . -name "*.[ch]" -print | xargs grep NO_PROC_ID | grep #define . (assuming you are in the Linux-source-directory). This will show that NO_PROC_ID is defined as follows: . #define NO_PROC_ID 0xFF .

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• Where to find libext2 sources?
• About this Book
• Positions

... galaxies . ... space flight . ... Hubble Space Telescope finds source of Magellanic Stream . New observations reveal most of the gas was stripped from the Small Magellanic Cloud about 2 billion years ago, and a second region of the stream originated more recently from the Large Magellanic Cloud. ... Astronomers using NASA s Hubble Space Telescope have solved a 40-year mystery on the origin of the Magellanic Stream, a long ribbon of gas stretching nearly halfway around our Milky Way Galaxy. ...

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• January 2006 resources | Astronomy.com
• Resources for red-star fans | Astronomy.com
• Study finds heat is source of "Pioneer anomaly" | Astronomy.com

... Chandra Observation of LMXB in M84 . We present characteristics of the X-ray point source population in the M84 field as observed by Chandra ACIS-S. We find the galactic sources in M84 follow the stellar light profile, which imposes similar formation histories for stars in both single and binary systems. After correcting for incompleteness in the source detection, we find a log N-log S similar to that of the elliptical galaxy NGC4697. ...

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• Introduction
• Effect of sources evolution on
• Population synthesis of X-ray sources at the Galactic center

These pages collect together references to many pictures of the solar system that can be found on the Net. ... Since I originally compiled this list the number of relevant images has grown tremendously. ... http://www.jpl.nasa.gov/pictures/ . ... ftp://dftnic.gsfc.nasa.gov/images/gifs/ . ... http://www.jpl.nasa.gov/galileo/images.html . http://www.jpl.nasa.gov/magellan/images.html . ... http://nssdc.gsfc.nasa.gov/image/planetary/ . ... NASA Image Access Homepage (Planetary Photojournal) . ...

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• Galileo Finds Giant Iron Core in Jupiter's Moon Io
• "Exploration" as a Classroom Resource

... 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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• Finder Documentation
• Galaxy Evolution: Radio sources and their environments
• Galaxy Evolution: Cosmological evolution of star formation

Next: Identifications and Efficiency Up: THE DEEP X-RAY RADIO Previous: Source Classification . ... For some sources which did not have NVSS positions before the time of optical observations, arcsecond positions from the Texas survey (Douglas et al. 1996) and NED (typically based on VLA data) were used. ... All X-ray/radio sources without counterparts on the survey plates were imaged at either the KPNO 0.9m or the CTIO 0.9m telescopes. ... Previously Identified Sources . Sample Properties . ...

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• VISTA finds hidden feature of Milky Way | ESO
• The Browne & March? Effect
• Finding well-hidden galaxies | ESO

... 2001 December 19 . Finding Dark Matter . ... Explanation: Where is dark matter ? Galaxies rotate and move in clusters as if a tremendous amount of unseen matter is present. ... In the above frame from a computer simulation of our universe , a 300 million light-year slice shows dark matter in gray and galaxies as colored circles. The red box indicates the location of a rich cluster of galaxies , while the green box shows a more typical cross-section of our universe . ... About APOD | ...

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• Planetary Picture List
• APOD: March 22, 1999 - An Infrared Galaxy Gallery
• Finding Out About (FOA) Bookmarks

... Table of Contents - Index - PS reprint - PDF reprint . ... All RXTE telemetry will be archived in a hierarchical database consisting entirely of FITS Binary Tables. We describe an interactive tool, the XTE Data Finder (XDF). ... Our basic design contains a three level hierarchy: Master Index, Subsystem Index, and Data Table. ... The Master Index acts as an observation catalog with references to Subsystem Indices, while the latter contain configuration information and references to the Data Tables. ...

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• How to Piece Together Diffracted Grating Arms for AXAF Flight Data
• Star Finding and PSF Determination using Image Restoration
• An Extragalactic Point Source Simulator for SIRTF Pipeline Testing

Comment on J2246-1206 . In contrast to the jet pointing to the NE in our image, the 5 GHz VLBI image of Shen et al. (1998) shows no indication of extended emission above the 20 mJy/beam level. Hong et al. (1999) find a jet component to the SE and identify that with a "superluminal" component possibly ejected in 1992. A 15 GHz image from the USNO database, taken nearly at the same epoch as the image of Hong et al. (1999) does not show any component at this position angle. ...

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