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1. Previously Identified Sources
Next: Sample Properties Up: Sample Identification Previous: Comments on Individual Sources . Previously known serendipitous sources were selected by cross-correlating WGACAT with a variety of optical and radio catalogs, including the Ver?n-Cetty & Ver?n (1996) and Hewitt & Burbidge (1993) quasar catalogs, the 1 Jy (Stickel et al. 1994) and S4 (Stickel & K?hr 1994) radio catalogs, and the BL Lac catalog of Padovani & Giommi (1995b). ... Details of these 97 objects are given in Table 6. ...
[ Сохраненная копия ]  Ссылки http://www.eso.org/~ppadovan/survey/dxrbs_paper/node10.html -- 6.3 Кб -- 03.12.2003
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2. ISOGAL YSO Candidates (Abstract)
... The 7 and 15 um observations of selected fields in the Galactic Plane obtained with ISOCAM during the ISOGAL program offer an unique possibility to search for previously unknown YSOs, undetected by IRAS because of lower sensitivity or confusion problems. ... The main indications of the previous analysis are confirmed, but the criteria for selecting YSO candidates had to be revised to select only bright objects, in order to limit the contamination of the sample by Post-MS stars. ...
[ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/~lt/preprints/igysocand/abstract.html -- 3.0 Кб -- 11.09.2007
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3. A Technique for Determining Proper Motions from Schmidt Plate Scans at ST ScI
... Keywords: Proper Motions, Schmidt Plates, Astrometry, Guide Star Catalog, Palomar Sky Survey . In this paper we describe a program of determining proper motions from digitized scans of 1950's-era Palomar Sky Survey (POSS) Schmidt Plates and 1980's-era Palomar Oschin Schmidt `Quick V' plates that were taken for the Hubble Space Telescope ( HST ) Guide Star Catalogue. ... Arrows indicate the magnitude and direction of the proper motion for the stars. ...
[ Сохраненная копия ]  Ссылки http://www.adass.org/adass/proceedings/adass94/williamsonr.html -- 10.9 Кб -- 03.11.2000
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4. Select a circle around the central point source
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. ...
[ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/PROS/PUG/node62.html -- 5.9 Кб -- 01.10.2012
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5. Anatoly V. Zasov
... Field of research: Extragalactic astronomy. ... NASA Astrophysics Data System (ADS) Abstract Service . ... CADC Home Page . ... CCD Images of Galaxies . ... RUSSIAN LINKS . ... UA Astronomy Personal Home Page - Bill Keel . ... The Shape of the Rotation Curves of Edge-on Galaxies, by A.V.Zasov and A.V.Khoperskov, 2003. ... A Thickness of Stellar Discs, by A.V.Zasov, and D.V.Bizyaev, 2003 . Minimum Velocity Dispersion in Stable Stellar Disks, by A.V.Khoperskov, A.V.Zasov, and N.V.Tyurina, 2003 . ...
[ Сохраненная копия ]  Ссылки http://neptun.sai.msu.su/~zasov/ -- 11.1 Кб -- 05.05.2008
[ Сохраненная копия ]  Ссылки http://star.sai.msu.ru/~zasov/ -- 11.1 Кб -- 05.05.2008
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6. A gallery of interacting galaxies Bojan Nikolic web pages (r. 329)
... Bojan Nikolic web pages (r. 329) . Galaxy Evolution . This pages illustrates some of the galaxies with close pairs which we identified in our study of star formation in interacting galaxies selected from the Sloan Digital Sky Survey (Nikolic et al 2004, see the publication list ) . ... This is 10 out of 114 of all of the galaxies in the volume limited sample at redshift smaller than 0.03 and with the first companion within 30 kiloparsecs. A gallery of interacting galaxies . ...
[ Сохраненная копия ]  Ссылки http://www.mrao.cam.ac.uk/~bn204/galevol/interactgallery.html -- 9.0 Кб -- 04.04.2016
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7. Black Hole Mass Estimates of Radio-selected Quasars
The black hole (BH) masses in the centers of active galactic nuclei (AGNs) have been estimated for a sample of radio-selected, flat-spectrum quasars to investigate the relationship between BH mass and radio properties of quasars. ... In contrast to previous studies, we find no correlation between BH mass and radio power in these AGNs. We find a range in BH mass similar to that seen in radio-quiet quasars from previous studies. ... You can now find me in room 99 at Epping. ...
[ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/people/Matthew.Whiting/papers/html_abstracts/black_hole_mass_abs.html -- 3.5 Кб -- 26.12.2007
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8. http://www.naic.edu/vscience/schedule/tpfiles/TsaitagA2715tp.pdf
Proposal Identification No.: ... The previous proposal number is A2715. Proposal Type: General Category: Sub-Category: Observation Category: Total Time Requested: Minimum Useful Time: Prop osal Title: ABSTRACT: Regular Astronomy Spectroscopy Extragalactic 39 hours Hours HI Content of Mid-IR Bright, Low Metallicity Blue Compact Dwarf Galaxies We propose to measure the HI contents of 10 selected nearby metal-poor blue compact dwarf galaxies (BCDs) using ALFA on Arecibo Telescope. ...
[ Текст ]  Ссылки http://www.naic.edu/vscience/schedule/tpfiles/TsaitagA2715tp.pdf -- 49.6 Кб -- 18.03.2013
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9. Abstract
739 observed NEAs and new 2-4 m survey statistics within the EURONEAR network . ... Additionally we observed 40 survey fields spanning three nights covering 11 square degrees near opposition, using the Wide Field Camera on the 2.5 m Isaac Newton Telescope (INT), resulting in 104 discovered main belt asteroids (MBAs) and another 626 unknown one-night objects. ... We identify Near Earth Object (NEO) candidates among the unknown (single night) objects using three selection criteria. ...
[ Сохраненная копия ]  Ссылки http://star.arm.ac.uk/~dja/papers/abs13PSS.html -- 3.2 Кб -- 05.09.2013
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10. Observational data and reduction
... were entered in the atlas. ... In so doing lines were selected which yielded radial velocities close to the symbiotic velocity of MWC 560 (+35 km/s). ... The visible spectrum of MWC 560 is poor in absorption lines especially near the brightness maximum. In our atlas are visible only the blue-shifted components of , , NaI and FeII(42), interstellar lines NaI, a few diffuse interstellar bands (DIB) and telluric lines of and and, at length, traces of the spectra of the M giant. ...
[ Сохраненная копия ]  Ссылки http://mavr.sao.ru/hq/ssl/MWC560/node2.html -- 9.3 Кб -- 02.10.2012
[ Сохраненная копия ]  Ссылки http://www.sao.ru/hq/ssl/MWC560/node2.html -- 9.3 Кб -- 01.10.2012
[ Сохраненная копия ]  Ссылки http://jet.sao.ru/hq/ssl/MWC560/node2.html -- 9.3 Кб -- 01.10.2012
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11. Anatoly V. Zasov
... Field of research: Extragalactic astronomy. ... NASA Astrophysics Data System (ADS) Abstract Service . ... CADC Home Page . ... CCD Images of Galaxies . ... RUSSIAN LINKS . ... UA Astronomy Personal Home Page - Bill Keel . ... The Shape of the Rotation Curves of Edge-on Galaxies, by A.V.Zasov and A.V.Khoperskov, 2003. ... A Thickness of Stellar Discs, by A.V.Zasov, and D.V.Bizyaev, 2003 . Minimum Velocity Dispersion in Stable Stellar Disks, by A.V.Khoperskov, A.V.Zasov, and N.V.Tyurina, 2003 . ...
[ Сохраненная копия ]  Ссылки http://lnfm1.sai.msu.ru/~zasov/ -- 11.4 Кб -- 16.06.2006
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12. Source Positions
Next: Catalog Construction Up: Observations and Analysis Previous: Source Detections . ... It was assumed that the highest signal gives the most likely position of the source. ... Comparing the summed map with the maps from the individual energy ranges, the one which produced the smallest error box was chosen to represent the source position, as long as was greater than 4, a level chosen to reflect a reasonable degree of confidence i