. Pulkovo Observatory of Russian Academy of Sciences is situated . near Saint-Petersburg. It was founded in 1839. 196140, Saint-Petersburg, Pulkovskoye chaussee 65/1 . English version . Russian version . This page has been accessed times since May 1, 1999.

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• Pulkovo NEO Page: Apparent Close Approaches to the Stars
• Pulkovo NEO Page: Ephemeris Support

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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... Members . ... The ATM's of Boston was founded in 1934 by a group of persons interested in assisting others in the art of optical polishing the craft of telescope making, and to learn together about the science of astronomy and the use of astronomical instruments. ... Mr. Jones introduced the club to Dr. Harlow Shapley at Harvard College Observatory. ... Regular shop activities resumed with the help of these "professional amateurs" and the club grew to 180 members. ... Club Newsletters . ...

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Establishment and Observation of Space Debris Laser Ranging Zhang Zhongping, Zhang Haifeng, Wu Zhibo, Li Pu, Meng Wendong, Chen Juping, Chen WanZhen Shanghai Observatory, Chinese Academy of Sciences Contents: Introduction Establishment of laser ranging to space debris system Observation results Summary Introduction Large amount of space debris around the earth currently. ... Laser ranging (LR) is a kind of real-time measuring technology with meter or sub-meter precision for space-debris observation. ...

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• Keywords_39

. Comment on J1146-3328 . The derived position here is about 20" from that of the PMN survey position (Griffith & Wright 1993). The source is only detected on the shorter baselines and is probably resolved, although some smearing may be caused by the large position offset. VLBApls home page . Last modified: 16 Oct 2000

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. Helical jets from one supermassive black hole caused by a very closely orbiting companion (see blue dots). The third black hole is part of the system but farther away and therefore emits relatively straight jets. Roger Deane (large image); NASA Goddard (inset bottom left; modified from original).

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• http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B70AA544F-A8B9-41BD-BFFF-ED8DAB103C63%7D
• http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B0A7C857B-A1F2-4C94-A29C-9FE17DB0CDE0%7D
• Want to discover Planet X? You'll need these three tools | Astronomy.com

... Astrophysics Group . Graduate Research Opportunities 2016 . Available research projects/areas . ... Astrophysics Admissions Form . ... This includes active participation in the development of new instruments as well as the use of ground and space observatories. ... Further details are available at the following web site: http://www.mrao.cam.ac.uk/research/extragalactic-group-2/ . ... Our research group has a wide range of expertise in the development of receivers for radio astronomy. ...

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• Cavendish Astrophysics - Projects
• VLSS Image Service (14 MAy 2004)
• Modelling absorption and emission of radiation by interstellar dust Bojan

. Other Relevant Links . Number counts have been illustrated earlier in the talk. QSO Clustering and Large-Scale Structure , Scott Croom et al . QSO Evolution and the Luminosity Function , B.J. Boyle et al . | Front page | . | << - Contamination | QSO close pairs - >> | . Robert J. Smith, ">rsmith@mso.anu.edu.au Last modified: Fri Sep 24 11:39:02 EST 1999 .

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• Dunk Proceedings - 2dF QSO Redshift Survey (Close Pairs)
• Dunk Proceedings - 2dF QSO Redshift Survey (Redshift distribution)
• Dunk Proceedings - 2dF QSO Redshift Survey (Front Page)

Trace: benchmark . start : benchmark . ... SAI VO Projects . ... AstroSearch . AstroDB . AstroKeywords . ... Help on Wiki search . ... benchmark.txt Last modified: 2011/12/27 17:19 by karpov Back to top . SAI VO | Astronet | SAI MSU | ...

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• astro-ph
• saivo:newsarchive [SAI Virtual Observatory - Wiki]
• people:sergeykarpov:paper-arxiv-2007-adass [SAI Virtual Observatory - Wiki]

... All rights reserved. ds. The IRAF Client Display Library (CDL) Michael Fitzpatrick IRAF Group 1 , NOAO 2 , PO Box 26732, Tucson, AZ 85726 Abstract. The Client Display Library is a new interface that allows host (non­IRAF) C or fortran programs to display images or draw into the graphics overlay using the XImtool image server and image viewers which emulate the XImtool client protocol such as SAOtng, SAOimage, and IPAC Skyview. ... The IRAF Client Display Library (CDL) 203 Figure 2. ...

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• http://www.stecf.org/conferences/adass/adassVII/reprints/schallers.ps.gz
• Space Telescope-European Coordinating Facility
• ADASS '97 Program Information

SWIRL DISTRIBUTION ON THE LUNAR SURFACE: LOCATIONS ANTIPODAL TO THE YOUNG BASINS? ... There are two main classes of hypothesises of the swirl origin: formation of the swirls in the regions antipodal to large impact basins (1), and formation of the swirls in result of cometary impacts (2). ... The Orientale basin is youngest. ... Fig. ... On the other hand, there are two cases of absence of correlation between swirl areas and regions antipodal to impact basins (for small swirl formations). ...

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• http://selena.sai.msu.ru/Symposium/ant.doc

... New version of code is here . ... The observational data of some globules are placed in new section of DOP. ... The original graphic library with optical properties of non-spherical particles with different shapes and structure is available. ... New section about optical properties of particles with non-Rayleigh inclusions is added. ... Two new sections are added. Optical properties of porous particles and Database of interstellar extinction and polarization curves . ...

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• INTAS project 99/652
• UGC4332
• Database of Optical Properties -- Level: subpage

Supernova 1987A in LMC . One day in 1987, an astronomer by the name of Ian Shelton was making observations of the Tarantula Nebula in Large Magellanic cloud at Las Campanas Observatory, and he noticed something strange on his image. ... SN 1987A got as bright as 2.7, the only other recent SN even to come close was 1885A in M31 which got up to mag 6. ... Mag 4.5 . ... IAUC 4318 2/25/87 Type II? ... IAUC 7354 2/1/00 New structure in the inner ring . ... IAUC 7360 2/7/00 HST observation of new spot . ...

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• Our Observing Site
• Extragalactic Novae - 1999.
• Extragalactic Novae - 2000.

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This general purpose telescope enclosure offers simple access to the sky for small instruments. Its truss roof rolls back on the steel I-beams and tracks that extend to the north of the building. A chain drive attached to the underside of the trusses provides the power that makes opening the observatory simple. Heavy steel pins secure the roof when it is closed. ...

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• Moore Observatory Astronomical Software Resources
• ImageJ for Astronomy
• Roll Roof Facility at Moore Observatory

... Today this year's largest group of sunspots will cross the Sun's central meridian. ... The next day, the number of spots in the group reached five, and the day after, on June 2nd, it was possible to count thirteen sunspots on solar disk, which had been clear prior to this. ... This year's two most powerful active areas, which passed across the solar disk at the beginning of May, 2009, are set to appear in the Sun's eastern sector in two days, on June 6th. ...

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• The CORONAS-PHOTON has registered the formation of the Sun's southern belt of
• The Russian TESIS Observatory will observe two solar eclipses from space
• TESIS team

... Exposure Time Calculator (ETC) . Survey processing . ... VISTA is a 4-m class wide field survey telescope for the southern hemisphere, equipped with a near infrared camera (1.65 degree diameter field of view at VISTA's nominal pixel size) containing 67 million pixels of mean size 0.34 arcsec and available broad band filters at Z,Y,J,H,K s and a narrow band filter at 1.18 micron. A wide field visible camera, if constructed, could also be used on VISTA. ... Tile . ... ESO VISTA Public Surveys . ...

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... Dept. for Astrometry & Space Geodynamics . ... Dept. for Physics of Stars&Galaxies . ... Dept. for Physics of Planetary Systems . ... Science . ... All Pages . ... Research of the stars with planets which pass apparent star disk (transiting exoplanets). The transit method based on a detection star brightness decrease during a passing of planet in front of its disk. Observed brightness system decries when planet pass star disk and its volume depend of the relative sizes star and planet. ...

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• Internet telescope

... Characterize how our impression of large scale structure has changed over the last 25 years. ... Examine the implications of Modified Newtonian Dynamics on small and large scale phenomenon which is observed. ... Critically summarize research being done on the Hubble Deep Field as it pertains to galaxy formation and evolution. Critically summarize our attempts to dynamically infer the value of the mass density of the Universe from studieds of large scale streaming motions. ...

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• CCD Astronomy Magazine Article Page 5
• Low Surface Brightness Galaxy Gallery
• Physics 410/510 Observational Cosmology

... Department Number . ... Astro Space Center . ... Telephone Number . 7(495) 333 3366 . FAX Number . 7(495) 333 2378 . ... amalin@lukash.asc.rssi.ru . ...

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• Lukash Vladimir Nikolaevich, Astro Space Center (ASC)
• Mikheeva Elena Vladimirovna, Astro Space Center (ASC)
• Kompaneets Dmitrij Alexandrovich, Astro Space Center (ASC)