... 539R We present the results of a radio continuum survey at 21 cm wavelength or the GAlactic plane between 357 <l <95.5 and |l| < 4d caried out with the Effelsberg 100-m radio telescope. ... Contour maps are shown with a sensitivity of 125 mK Tb (or 61.6 mJy/beam area) at an angular resolution (HPBW) 9.4'. ... We present the results of a radio continuum survey at 21 cm wavelength orthe Galactic plane between 95.5 < l < 240 and -4 < l < +5o with the Effelsberg 100-m radio telescope. ...

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... Дни открытых дверей к юбилею САО РАН (12-14 апреля 2016 г.) . Международная конференция "Dark Ages and White Nights (Spectroscopy of the CMB)" (20-24 июня 2016 г.) . ... Международная конференция MULTI-SPIN GALAXIES - 2016 (26-30 сентября 2016 г.) . Международная астрономическая конференция "Физика звезд: от коллапса до коллапса" (3-7 октября 2016 г.) Архив . ... Подробнее.. ... 10.02.16 . ... БТА в реальном времени . ... Цейсс-1000 в реальном времени . ... Последнее обновление: 22/03/2016 ...

After a couple of visits by Steve Larson and Ed Beshore in late 2003 and early March 2004 to deal with various hardware issues and to install the new survey code, regular surveying commenced in mid-March 2004. ... However, the initial results are most satisfying and new objects have been found from the very first night. ... UA Media Release . ... Fellow Uppsala observer Rob McNaught was observing NEOs with the 1.0-m at Siding Spring as part of our regular program of follow-up observations. ...

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... Graduated from Moscow State University in 1970 and till now in permanent staff of the Sternberg Astronomical Institute, Moscow State University. ... Member, Euro-Asian Astronomical Society . ... Jointly with Dr. V.Konnikova, I teach a course in Radio Astronomy at the Astronomy Division , Physics Department of Moscow State University . ... Astronomical Meetings . ... Net Search: MetaCrawler . ... Moscow State University . ... Rudnitskij, Georgij M. Page last updated November 25, 2015. th . ...

The oral histories on this Website are the transcripts from audio-recorded, personal interviews with many who pioneered outer space and the Moon, and with those who continue the excitement of space exploration. ... The date of each interview is noted on the first page. If available, the Biographical Data Sheet provided background information for the Oral Historian to prepare for the interview. ... John V. Becker Oral History Interviews . ... Return to JSC Oral History Website . ...

... I ported the changes to stsci.sphere and resolved the 2to3 compaibility problems. ... I finished up converting the stsci.sphere package to run under Python 2 and 3, then converted the stsci.imagestats and stsci.imagemanip packages. ... I was able to run the test case for stsci.sphere to completion, so I checked the code in. ... I fixed the last remaining problem with the stsci.* packages and checked it in and moved onto updating the pysynphot package. ... Archive for 2015 . ...

2014 May version . ... Green D. A., 2014 , Bulletin of the Astronomical Society of India, 42 , 47-58. ( .pdf , or arXiv.org:1409.0637 ) If you make use of the detailed version of the catalogue, then plaese also cite: . Green D. A., 2014, `A Catalogue of Galactic Supernova Remnants (2014 May version)' , Cavendish Laboratory, Cambridge, United Kingdom (available at "http://www.mrao.cam.ac.uk/surveys/snrs/" ). ... Copyright D. A. Green 2014. 25872nd access to this version of the catalogue. ...

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The 2dF QSO Redshift Survey (2QZ) . ... Before jumping into all the finer details of teh survey, a brief non-astronomer's guide to redshift surveys is available. ... The primary scientific aims of the QSO survey are: (1) to obtain the primordial fluctuation power spectrum out to COBE scales, (2) to determine the rate of QSO clustering evolution in the non-linear and linear regimes and hence obtain new limits on the value of and the bias parameter, (3) to apply a powerful geometric method to measure . ...

We present results from a search for 21 cm associated HI absorption in a sample of 29 radio sources selected from the Australia Telescope 20 GHz survey. Observations were conducted using the Australia Telescope Compact Array Broadband Backend, with which we can simultaneously look for 21 cm absorption in a redshift range of 0.04 < z < 0.08, with a velocity resolution of 7 km/s . ... Australia Telescope National Facility . ... Australia . ...

Next: Particle Background Rejection Up: Detection Efficiency Previous: Front Illumination . ... The method requires that the CCD substrate be etched from the rear towards the depletion layer boundary. The device can be illuminated through this rear surface, which has a much thinner dead layer than the electrode side. ... The corresponding detection efficiency data are presented in Figure 7, and compared with the predicted data for a 20 m thick depletion layer. ...

Estimating the NEO Population and Impact Risk: Past, Present and Future . ... Since most of the risk resides in the largest impactors, finding that fraction of the largest bodies, and that none of them has a significant chance of impacting in the next century or so, "retires" more than 90 % of the impact risk, including most of the risk of a globally catastrophic impact event. ... In the mid-size range, from ~150 m to ~1 km, the main risk is from tsunami generated by an ocean impact. ...

... In this program there will be no charts in which to compare starfields or conduct magnitude comparison star photometry. The latter information will hopefully be made available once an event has been sanctioned by the IAU as being a bonifide event. ... NOTE: The Astronomical Society of the Pacific has just come out with a further scaled down version of the Digitized Sky Survey that is currently available (10X version). ...

... Public . Science . ... Science Users Information > Observing with ESO Telescopes > Public Surveys . ... Public Surveys . Publications with ESO Data . ... Large Programmes . ... Public Surveys Programmes . ... Public Surveys Phase 2 . ... Here we present the Public Survey projects and give information on the mechanisms that ESO has set in place to manage them, to ensure their legacy value and their usefulness for the astronomical community at large. ... ESO Public Surveys Phase 2 workshop . ...

The Mars Flag has a different design on the reverse side. obverse side of flag . ... The orbit lines on the obverse cross the Sun on the lower half of the flag and appear to go behind the Sun on the upper half of the flag. The reverse side has the orbits lines continuing around the Sun on the upper half of the flag. ... The Mars Flag reverse side is a continuation of the obverse side and not just a different design on the back and not a mirror image of the obverse. Main Flag Background Color . ...

ChASeM33 . The Chandra ACIS Survey of M33 - . The Chandra ACIS Survey of M33 (ChASeM33) is a very deep X-ray survey of the nearest face-on spiral galaxy, M33, using the superb spatial resolution of the Chandra X-ray Observatory . In order to understand motivation and scope of the survey, it is useful to know that it is in spiral galaxies that much of the drama of the present universe plays out: stellar birth and death, the recycling of matter from interstellar gas to stars and back again. ...

... Christmas is a home and family celebration, and therefore those who live away try to get back home. Everyone is buying Christmas presents for friends and relatives; parents try to present their children with everything they want. A Christmas tree stands in the everybody's living-room at Christmas. ... On Christmas Eve, when children are asleep, their parents come into their bedrooms and leave the presents near their beds or under the Christmas tree. ...

... Next: Colophon Up: Data Modeling and Previous: Robust Estimation and . ... In considering future software needs, I present five projects to enhance the astronomer's research effectiveness, and note that large telescope projects and information databases will also challenge software developers. ... The ADASS conferences are intended to foster discussions between astronomers and software developers so that the computational needs of researchers are understood and met. ...