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1. http://www.stsci.edu/ftp/observing/status_reports/old_reports_97/hst_status_07_03_97
HUBBLE SPACE TELESCOPE DAILY REPORT #1912 PERIOD COVERED: 0000Z (UTC) 07/02/97 - 0000Z (UTC) 07/03/97 Daily Status Report as of 184/0000Z 1.0 ACTIVITIES SCHEDULED AND ACCOMPLISHED: 1.1 Completed Four Sets of WF/PC-2 6253 (Pure Parallel Archive Program) The WF/PC-2 was used to execute a pure parallel program taking ultraviolet observations running concurrently with prime science observations. ... The observations were completed as scheduled, and no anomalies were reported. ...
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Ссылки http://www.stsci.edu/ftp/observing/status_reports/old_reports_97/hst_status_07_03_97 -- 7.6 Кб -- 03.07.1997
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2. Siding Spring Survey
T he Siding Spring Survey (SSS) is a Near-Earth Object search program that utilises the 0.5-m Uppsala Schmidt Telescope at Siding Spring Observatory, N.S.W., Australia. ... The mission of the Siding Spring Survey is to contribute to the inventory of near-earth objects (NEOs), or more specifically, the potentially hazardous asteroids (PHAs) and comets (PHOs) that may pose a threat of impact and thus harm to civilization. ... Based on the CSS Mission page . ... Siding Spring Survey Main Page . ...
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Ссылки http://www.mso.anu.edu.au/~rmn/ -- 11.4 Кб -- 23.12.2011
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3. X--ray Quiet PMS Candidates
... There are several explanations for these X--ray quiet PMS stars. To examine the explanations, it is proper to divide the PMS stars into three groups: those bluer than R - I = 0.7, those redder than the X--ray sources (R - I > 1.25) and those with colors similar to the X--ray sources. ... A total of 26 of the non--X--ray detected PMS candidates had spectra taken. ... Between V=14 and V=16, I find 25 stars which are X--ray sources and estimate 19 non--X--ray PMS stars. ...
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Ссылки http://hea-www.harvard.edu/~swolk/thesis/optical/node10.html -- 7.7 Кб -- 02.10.2012
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4. Small scale distribution in Molecular Clouds
... The presence of small scale fluctuations of density (or of optical properties) in the spatial distribution of the dust would have important consequences for the modelling of molecular clouds because the UV light penetration and therefore the physical and chemical processes depend strongly on their structure (cf Boiss? ... We have developed methods to study in a direct way the amplitude of small scale variations of the extinction throughout translucent clouds ( mag). ...
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Ссылки http://www.mrao.cam.ac.uk/yerac/thoraval/thoraval.html -- 20.5 Кб -- 08.12.2003
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5. Armagh Observatory
... Armagh Observatory, College Hill, Armagh BT61 9DG, +44 (0)28 3752 2928 . ... Distributions of impact velocity on Phobos for the sample of Long Period comets (top), Jupiter Family comets (middle) and asteroids (bottom) used in our sporadic meteoroid flux model. ... 100 m as determined from spacecraft images is consistent with a 50/50 contribution from the two meteoroid populations in our model. ... Last Revised: 2014 November 20th . ...
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Ссылки http://star.arm.ac.uk/highlights/2014/660.html -- 6.0 Кб -- 20.11.2014
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6. Redshift Distribution
... The distribution of redshifts among the DXRBS FSRQs identified so far (Figure 3) is quite similar to that of the 1 Jy and S4 samples. ... A more thorough comparison will have to await completion of our survey and the convolution of the redshift distribution with the WGACAT sky coverage. As has already been mentioned by Hook et al. (1996), selecting flat-spectrum sources is an efficient way of finding high-redshift, radio-loud quasars. ...
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Ссылки http://www.eso.org/~ppadovan/survey/dxrbs_paper/node12.html -- 6.5 Кб -- 03.12.2003
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7. ADASS 2003 Conference Proceedings
... We employ Bayesian inference for the joint estimation of sources and background on ROSAT All-Sky Survey (RASS) data. ... Background maps were estimated in a single step together with the detection of sources without pixel censoring. ... The source probability is evaluated for single pixels as well as for pixel domains to enhance source detection of weak and extended sources. ... The spline fits the background component whereas count enhancements classify pixel (domains) with source contributions. ...
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Ссылки http://www.adass.org/adass/proceedings/adass03/O3-3/ -- 19.8 Кб -- 13.08.2004
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8. Russian-Finnish Symposium, Program
... Professor Esko Valtaoja (Turku University, Director of Tuorla Observatory): "The problem of high-energy emission from AGN" . ... Associate Professor Harry Lehto (Tuorla): "Radio observations of GRS1915+105" . ... Dr. Alexander Riehokainen (Tuorla, Academy Researcher): "Multiwavelength observations of the Sun over a full activity cycle" . ... Ilona Torniainen (Metsahovi, PhD student): "Inverted-spectrum radio sources" . ... A Study of solar polar zone using eclipse data with RATAN-600 . ...
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Ссылки http://www.sao.ru/cats/~satr/RFSymp/papers.html -- 6.6 Кб -- 25.09.2006
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9. Main research and development work completed in 2009 and ready for
... Space Research Institute . ... Main research and development work completed in 2009 and ready for implementation . ... Development of the Northern Eurasia land cover map based on medium spatial resolution satellite data. ... The research and development has been completed of the first in Russia and in the whole world high-speed digital streams decoder for space and satellite channels with extremely high noise levels. ... Main research and development work completed in 2008 and ready for...
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Ссылки http://www.iki.rssi.ru/eng/niokr2009.htm -- 7.7 Кб -- 18.07.2011
[ Сохраненная копия ] Ссылки http://www.cosmos.ru/eng/niokr2009.htm -- 7.7 Кб -- 18.07.2011
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10. Contribution of Low Surface Brightness Galaxies
... ATNF Home . ... About ATNF overview . ... Australia Telescope Steering Committee . ... Parkes radio telescope . ... It has been argued in the literature that low surface brightness (LSB) galaxies might contribute a considerable HТљ I cross section. ... Figure 3: The column density distribution function ( left ) and HТљ I mass density ( right ) for high and low surface brightness galaxies. High surface brightness galaxies dominate the HТљ I cross section, especially for column densities . ...
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Ссылки http://www.atnf.csiro.au/pasa/16_1/zwaan/paper/node5.html -- 55.5 Кб -- 08.04.2016
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11. Effect of sources evolution on
... 172 ] Briefly, the count rate at the detector from a source at a redshift z is . ... Figure 55 shows the ``Green functions'' for the double compact binary merging rate evolution assuming no collapse anisotropy. ... Another way that diverse peculiarities in the - distribution induced by the sources evolution could arise is connected with a possible non-monotonic character of the star formation rate in galaxies. ... 22 ] Figure 56 shows two-dimensional cuts through the parameter space. ...
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Ссылки http://xray.sai.msu.ru/~mystery/articles/review/node98.html -- 16.9 Кб -- 29.03.1997
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12. LWN: Driver porting: completion events
... LWN.net Weekly Edition for March 18, 2004 . ... LWN.net FAQ . ... This article is part of the LWN Porting Drivers to 2.6 series . Completions are a simple synchronization mechanism that is preferable to sleeping and waking up in some situations. ... When your driver begins some process whose completion must be waited for, it's simply a matter of passing your completion event to wait_for_completion() : . ... void complete(struct completion *comp); void complete_all(struct completion *comp); . ...
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Ссылки http://mavr.sao.ru/hq/sts/linux/doc/porting_to_26/23993.html -- 11.9 Кб -- 28.12.2007
[ Сохраненная копия ] Ссылки http://www.sao.ru/hq/sts/linux/doc/porting_to_26/23993.html -- 11.9 Кб -- 02.10.2012
[ Сохраненная копия ] Ссылки http://jet.sao.ru/hq/sts/linux/doc/porting_to_26/23993.html -- 11.9 Кб -- 02.10.2012
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[ Сохраненная копия ] Ссылки http://jet.sao.ru/hq/sts/linux/doc/porting_to_26/23993.html -- 11.9 Кб -- 02.10.2012
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13. http://www.naic.edu/~pulsar/y2kws/first_announcement.txt
Current and Future Pulsar Science with the Arecibo Telescope A Y2K Workshop at Arecibo - March 12-14 2000 First Announcement - Invitation to Participate ================================================================================ Dear Colleague, We are pleased to officially announce our plans to hold a Pulsar Workshop at the Arecibo Observatory, Puerto Rico, on March 12-14 2000. ... Shared-room accomodation will be allocated either at the Observatory or at El Buen Cafe Hotel in down-town Arecibo. ...
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Ссылки http://www.naic.edu/~pulsar/y2kws/first_announcement.txt -- 7.1 Кб -- 07.12.1999
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14. Geomagnetic Indices Kp, ap, Ap, Cp and C9
This service contributes to the International Service of Geomagnetic Indices (ISGI) of the IAGA . ... The Kp numbers of the previous month are available in tabular format . ... There are available also historical and current Kp and derived indices per anonoymos FTP (see below). ... U.S.A. FTP server: ftp://ftp.ngdc.noaa.gov/STP/GEOMAGNETIC_DATA/INDICES/KP_AP/ . monthly update) . ... contains the monthly Kp / ap tables in a simple text format readable for both humans and computers (*.tab). ...
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Ссылки http://www.iki.rssi.ru/magbase/REFMAN/KP_INDEX/index.html -- 13.1 Кб -- 14.10.2001
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15. research field
Main research interests: . 1) Structure and geometry of the circumnuclear medium of AGN, particularly through hard X-ray observations of obscured sources. ... 3) Physics of Ultraluminous Infrared Galaxies (ULIRGs): analysis of the AGN and starburst components through hard X-ray and infrared (with ground-based 3-5 micron spectroscopy, and with Spitzer in the 5-30 micron band) imaging and spectroscopy. ...
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Ссылки http://www.arcetri.astro.it/science/gal-agn/res_risaliti.html -- 2.1 Кб -- 14.08.2009
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16. Сазонов Сергей Юрьевич (ИКИ РАН)
Next: Сейфина Елена Викторовна (ГАИШ) Up: abstracts Previous: Ревнивцев Михаил Геннадьевич (ИКИ РАН) . Статистика активных ядер галактик и космический рентгеновский фон по данным обсерватории ИНТЕГРАЛ The recently completed INTEGRAL hard X-ray all-sky survey provides a sample of more than 100 nearby AGN selected without regard to absorption effects. ...
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Ссылки http://hea.iki.rssi.ru/conf/hea2007/abstracts/node64.html -- 3.6 Кб -- 19.12.2007
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17. Untitled Document
... Maintenance and Work Completed on M1: September 10, 1999 . Whiffles Installed on M2: September 10, 1999 . M1 Support System Maintenance: September 10, 1999 . M1 Temperature Sensor Work and Repair: September 10, 1999 . M1 Hex-cell Deterioration: September 14, 1999 . ... M1 Whiffle Mount and M1 Back, September 21, 1999 . ... Views of Secondary Mirror (Back): April 13, 2000 . ... Front Portals: June 8, 2001 . ... M2 and M3 Baffle Work: June 8, 2005 . ... M3 Work: November 7, 2007 . ...
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Ссылки http://www.apo.nmsu.edu/Telescopes/ARCprogress/defaultarchive.html -- 22.0 Кб -- 05.03.2014
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18. Stats
... Latest SNe . ... Statistics on Supernovae Discoveries . Discoveries by amateurs have been rising in recent years. ... And the next page shows the amateurs who have discovered a supernova: . ... All SNe since 1885. (external link) . The next pages relate to all supernovae discovered so far, their properties and their parent galaxies: . SNe distribution according to galaxies' morphological type. ... SNe distribution according to their magnitudes. All SNe distribution since 1885. ...
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Ссылки http://www.sai.msu.su/mirrors/isn/SNSTATS.HTM -- 6.7 Кб -- 20.12.2007
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19. Dynamic tests of the scientific equipment 'Contact' have been completed in SSAU
... Pre-university education . ... Facilities and equipment . ... SSAU History . SSAU roadmap . ... Contacts . ... The scientists of Samara State Aerospace University have completed dynamic tests of the first Russian university nanosatellite SamSat-218D created by SSAU students. ... It has already passed the whole set of tests and transferred to the Rocket and Space Centre Progress . ... The whole test cycle of the nanosatellite SamSat-218D (Module Contact-Nanosatellite") will be completed in July. ...
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Ссылки http://www.ssau.ru/engnews/11689/ -- 26.0 Кб -- 31.07.2015
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20. Vladimir Marsakov Abstracts
... It was found that the Sun lies 9?2 pc above the plane of hte Galactic disk in the direction of North Galactic pole and that F0-F9 stars contribute 0.0035 M /pc 3 to the density of the Galactic disk. ... We used this method to determine the scale height of the subsystem of F stars of the Galactic disk, Z 0 =160?10 pc. ... It is suggested that scale height of the metal-poor stars subsystem is due to the infall of the metall-poor intergalactic gas onto the disk. ...
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Ссылки http://ip.rsu.ru/~marsakov/abs/abst26.htm -- 4.4 Кб -- 02.02.2007
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