Next: A box, to include Up: To produce a region Previous: To produce a region . select cursor and circle . When in the image window, the mouse now has a box shape with an arrow at the upper left corner. The mouse buttons act as follows: . LEFT - to move the center of the circle at the position of the arrow point. ... RIGHT - idle. center the circle at the point source by positioning the arrow point and clicking on the LEFT mouse button. A circle will appear at the arrow position. ...

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• *imcnts* - Radial Profile of an extended source at the field center
• Source Selection
• Spectral Extraction of Point Sources

Astronomy Picture of the Day . The Milky Way's Gamma-Ray Halo . ... Credit: D. Dixon ( UCR ), D. Hartmann ( Clemson ), E. Kolaczyk ( U. Chicago ), NASA Explanation: Our Milky Way galaxy appears to be surrounded by a halo of gamma rays . ... In this false color all-sky image centered on the Milky Way , the brown and green regions indicate brighter, known sources of gamma-rays. ... Publications with keywords: halo - Milky Way - gamma ray . Publications with words: halo - Milky Way - gamma ray . ...

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• The Center of the Circinus Galaxy in X Rays
• Астронет > The Center of the Circinus Galaxy in X Rays
• Астронет > The Milky Way's Gamma-Ray Halo

... November 5, 1997 . The Milky Way's Gamma-Ray Halo . Credit: D. Dixon ( UCR ), D. Hartmann ( Clemson ), E. Kolaczyk ( U. Chicago ), NASA . Explanation: Our Milky Way galaxy appears to be surrounded by a halo of gamma rays . Gamma rays are the most energetic form of electromagnetic radiation , with more than a hundred thousand times the energy of visible light, but known gamma-ray sources don't account for the diffuse distribution of this high-energy glow. ... About APOD > . ...

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• Solar Mystery Nears Solution With Data From SOHO Spacecraft
• The BD+40 region (Abstract)
• APOD: January 21, 1997 - Journey to the Center of the Galaxy

... OCR by H.Andernach 1/96, to be proof-read) This is the first of a series of papers presenting results of a 10-GHz radio continuum survey of the galactic plane region using the 45-m telescope at Nobeyama. ... Weak Nonthermal Sources: A comparison with the Bonn S-GHz survey reveals a number of weak nonthermal sources near the galactic plane. ... For this reason we conducted a survey of the galactic plane region at 10 GHz using the 45-m radio telescope at the Nobeyama Radio Observatory (NRO). ...

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• RATAN-600 NCP bright radio sources
• The Second EGRET Catalog of High-Energy Gamma-Ray Sources
• Source Positions

... 2008 November 9 . Two Black Holes Dancing in 3C 75 . Credit: X-Ray: NASA / CXC / D.Hudson, T.Reiprich et al. ... Explanation: What's happening at the center of active galaxy 3C 75? The two bright sources at the center of this composite x-ray (blue)/ radio (pink) image are co-orbiting supermassive black holes powering the giant radio source 3C 75 . ... At the cores of two merging galaxies in the Abell 400 galaxy cluster they are some 300 million light-years away. ... About APOD | ...

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• APOD: 2010 November 7 - The Center of Centaurus A
• APOD: 2001 November 6 - In the Center of Spiral Galaxy M83
• APOD: 2009 November 16 - M83's Center from Refurbished Hubble

... Meta Index / Home Page / Description / Specifying source region shapes . When radiusstyle =`contour', the task calculates the source region shape as an elliptical locus which approximates the contour of the PSF at a given flux value. ... Clearly, in order to calculate the shape of such a flux contour, it is necessary firstly to normalize the PSF to the source brightness and secondly to determine the flux level (in `brightness' units per pixel) at which to find the contour. ...

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• Specifying source region shapes and sizes

home resources > books . SEARCH ASP SITE: Match ALL words Match ANY word . ... Buy The Black Hole at the Center of our Galaxy at Amazon.com! Reviewed by Terrell Kent Holmes . In 1974 astronomers discovered a bright radio source at the center of the Milky Way Galaxy, in the direction of the constellation Sagittarius. It was an unknown quantity then, but astronomers now know that the object is a supermassive black hole causing a maelstrom of activity at the galactic center. ...

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• ASP: Resource Center
• ASP: Beacons in the Gloom
• ASP: Clubs and Organizations

Next: The Model Up: No Title Previous: Radiopulsars as Sources of . In this section, we study the evolution of stellar populations on a time-scale of 10 Myr for a starburst љ occurring under conditions similar to those in the Galactic Center (see Lipunov et al. (1995d)[ 126 ]). We estimate the expected number of X-ray transient љ sources (NS + MS star), super accreting BH, and BH + supergiant binaries, all as functions of time elapsed after the burst. ...

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• Discussion and conclusions
• Population synthesis of X-ray sources at the Galactic center
• Grants Center

... Classes . Files . ... File List . File Members . images . Regions . ... National Radio Astronomy Observatory 00023 //# 520 Edgemont Road 00024 //# Charlottesville, VA 22903-2475 USA 00025 //# 00026 //# $Id: WCConcatenation.h 20615 2009-06-09 02:16:01Z Malte.Marquarding $ 00027 00028 #ifndef IMAGES _ WCCONCATENATION _H 00029 #define IMAGES _ WCCONCATENATION _H 00030 00031 //# Includes 00032 #include images / Regions /WCCompound.h 00033 #include images / ...

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• casacore: lattices/Lattices/LCEllipsoid.h Source File
• Source Fitting and Positions
• The HIPASS Bright Galaxy Catalog

... 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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EMBARGOED UNTIL: 9:20 AM CST, January 6, 1999 CONTACT: John Biretta Space Telecsope Science Institute, Baltimore, MD (Phone: (410) 338-4917; Internet: biretta@stsci.edu) HUBBLE DETECTS FASTER-THAN-LIGHT MOTION IN GALAXY M87 Astronomers reported today discovering clouds which appear to move many times faster than the speed of light, shooting out from the region of a black hole at the center of the M87 galaxy. ... It's an illusion created by the finite speed of light and rapid motion," Biretta said. ...

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• GRB 011030
• STScI Preprint #1225
• Herschel Key Program Heritage: a Far-Infrared Source Catalog for the Magellanic

... Home Observing Lincoln Center . ... AAA Fall Astronomy Class: Astronomy Basics тАУ October-November 2015 . ... This MonthтАЩs Sky тАУ April 2015 . This MonthтАЩs Sky тАУ May 2015 . This MonthтАЩs Sky тАУ June 2015 . ... Beyond New York City . ... Observing Resources for Amateur Astronomers - Part 1: Beginning Observers . ... A History of the First Forty Years of the Amateur Astronomers Association . ... 2016 Amateur Astronomers Association of New York Designed by Press Customizr Powered by . ...

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• lincoln center ? Amateur Astronomers Association of New York
• Franklin Lincoln Center 3 copy 2 ? Amateur Astronomers Association of New York
• Lincoln Center Observing Schedule ? Amateur Astronomers Association of New York

Recent observations of the Sculptor Galaxy by NASA's Nuclear Spectroscopic Telescope ARray (NuSTAR), combined with those from NASA's Chandra X-ray Observatory, suggest that the supermassive black hole at the center of NGC 253 has dozed off, or gone inactive, sometime in the past decade. ... This object, which appears as a blue spot near the hotter, central region of the galaxy, is either a black hole or a dense, dead star, called a neutron star, feeding off a partner star. ...

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• http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B7FB1DE71-9334-49A7-B8C1-938ACCA4A41F%7D
• http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BFB4C868E-684A-47DB-8F0C-AE88DAFC2A6D%7D
• Astronomers find source of most powerful cosmic rays | Astronomy.com

... Bad Astronomy . ... Bitesize Astronomy . ... Last week's Snack talked about how black holes can affect the environment around them in such a way as to be very bright . ... It's a common misconception that black holes always have matter swirling into them. ... As this matter gets closer and closer to the black hole it piles up and a large, fairly flat disk forms. This is called the accretion disk , because matter from this disk accretes (that is, falls in) on the black hole. ... 2008 Phil Plait. ...

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... This program was created for correlating chosen regions in the series of fts images. ... Chosen regions' . ... In this section the program counts the integral for each region of the grid for each image. ... As a matter of fact, the integral is total brightness of the region and it is counted by 'int_tabulated' IDL function. ... In addition, the program will show the count of the regions which correlate with the corresponding region (the brighter region means the bigger count) and its contour. ...

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• New sats of Uranus - Sources
• Trudy GAISH, vol. LXV, 1996, Abstracts in English
• New sats of Saturn - Sources

... Pre-university education . ... The NEICON consortium provides free test access to three platforms of electronic resources of McGraw-Hill Education company: . ... ACCESS ENGINEERING (www.accessengineeringlibrary.com ) is the largest platform in the area of technology and engineering science. It contains over 250 key items as well as interactive graphs, tables and video materials. ... ACCESS MEDICINE (www.accessmedicine.com) is the basic medicinal platform of McGraw-Hill Education. ...

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• Samara region
• Multiple access center "Interuniversity Mediacenter in Samara"
• Samara regional center of information in the field of Education and Research

... This paper describes the main algorithms used by the Einstein Level One processing to create the exposure masks and the background maps for Einstein IPC images, and how these algorithms were recreated in the IRAF environment. Our goal was to recreate the algorithms used by the Level One Processing to create exposure masks and background maps for Einstein Image Proportional Counter (IPC) data (cf. sections 2.5 and 2.7 of Harnden et al. ...

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• How to Piece Together Diffracted Grating Arms for AXAF Flight Data
• QPSIM: An IRAF/PROS Tool for Source Simulation
• ADASS 2003 Conference Proceedings

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• Project SUBMILLIMETRON

This WWW form allows the user to list selected portions of the NRAO/VLA Sky Survey (NVSS) radio source catalog. ... Until the completion of the survey the source catalog will NOT cover the entire region of the survey and care must be exercised in interpreting the results of a catalog search. ... The second parameter in the "Search radius" box or one of the optional items in a position list can be used to specify a region in which to look for other sources. ... An example of a position list entry is: . ...

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• Astrophysics Group Variability studies
• Astrophysics Group 7C(G)
• G189.1+3.0

... 3600 seconds of data with 1 second integrations. 32 bits were saved. 60 seconds of 1 millisecond integrations. 16 bits were saved. ... 3600 sec average of 1 second spectra shows any birdies (.ps) ( .pdf ) . ... Black in polA, red is polB. Top plot is band0, center plot is band1, bottom plot are both spectra with the 60 Mhz offsets of the mixers. ... The average spectra over each data set was computed and then used to normalize each spectra before computing the total power. ... Middle plot. ...

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• National Astronomy and Ionosphere Center (Arecibo Observatory)
• Thesis Figures
• Calibration Scans on Continuum Sources