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1. ICWG meeting, Iceland 2006 - Participants
... XMM-Newton SOC Home Page Conferences & Meetings . ... General User Support XMM-Newton Helpdesk Users Group . ... SOC Info XMM-Newton Contact Details How to get to ESAC ESA Research Fellowships ESAC Trainee Projects ESA Young Graduate Trainees . About XMM-Newton Image Gallery XMM-Newton Technical Details XMM-Newton SOC Overview XMM-Newton 10th Anniversary . ... Participants . ... XMM-Newton EPIC . ... 13-18 . ... XMM-Newton EPIC-MOS . ... XMM-Newton RGS . ... XMM-Newton . ... CfA, USA . ...
[ Сохраненная копия ]  Ссылки http://xmm.vilspa.esa.es/external/xmm_sw_cal/icwg/participants.shtml -- 24.8 Кб -- 10.04.2016
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2. PPTA Wiki | Meetings / Ppta3
... PPTA timeline . ... PPTA_MEETINGS . ... Meeting minutes . ... List of projects . PPTA tasks . ... Data release 2 discussion . Editing this wiki . ... Ppta3 . ... Aim: To highlight results from the Parkes Pulsar Timing Array (PPTA) project, to discuss astrophysical sources of gravitational waves and to discuss future issues . ... Data have been collected for the Parkes Pulsar Timing Array (PPTA) project over the past 4 years. ... Time . ... The Parkes data archiving project (only 10 minutes) . ...
[ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/research/pulsar/array/index.php?n=Meetings.Ppta3 -- 16.1 Кб -- 12.04.2016
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3. SMOV Status Planning Meeting Minutes 03/31/97
NOTE: The next meeting is April 2, 8:30 AM. STATUS REPORTS 1. ... WFPC2 Status - Proceeding nominally with Cycle 6 science and remaining SMOV monitors. ... NICMOS Status - Engineering Status - Following the 7042 Fine Alignment activities on Friday, the Filter Wheels were reconfigured to the nominal pre-positioning (FW1=F110M, FW2=FW3=F160W). ... STIS Status - Engineering Status - Over the weekend, a CCD motor temperature went slightly out of limits low. ... Go back to the Meeting Minutes Page ...
[ Сохраненная копия ]  Ссылки http://www.stsci.edu/smov/notes/0331smov.html -- 6.0 Кб -- 04.04.1997
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4. Astronomy HyperText Book: Stellar Evolution
... Stellar Evolution is driven entirely by the never ending battle between Pressure and Gravity . As imbalances are reached, the star is driven to find a new Energy source. ... Pressure and gravitational forces are equal, the star is stable and its core is sufficiently hot to fuse Hydrogen into Helium More about main sequence stars . ... The luminosity generated by the core fusion of Helium into Carbon is far greater than the shell luminosity associated with the fusion of Hydrogen into Helium. ...
[ Сохраненная копия ]  Ссылки http://zebu.uoregon.edu/textbook/se.html -- 4.8 Кб -- 16.12.1997
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5. "Stargazers" and National Science Standards
... The material in "From Stargazers to Starships" meets several important requirements of the national standards. Pages cited below are from National Science Education Standards National Academy Press, Washington 1995. ... For example: the sections on astronomy not only describe calendars and sundials (including their construction), but also the astronomy of the ancient Greeks, including two different ways in which ancient Greeks estimated the distance to the Moon. ...
[ Сохраненная копия ]  Ссылки http://www.iki.rssi.ru/mirrors/stern/stargaze/Standrds.htm -- 7.9 Кб -- 21.12.2007
[ Сохраненная копия ]  Ссылки http://www.cosmos.ru/mirrors/stern/stargaze/Standrds.htm -- 7.9 Кб -- 22.12.2007
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6. http://observ.pereplet.ru/images/GRB081102/grb_film.html
... GCN 8471 | ... TITLE: GCN CIRCULAR NUMBER: 8516 SUBJECT: GRB 081102: MASTER refind and final results DATE: 08/11/11 15:50:10 GMT FROM: Vladimir Lipunov at Moscow State U/Krylov Obs E. Gorbovskoy, V. Lipunov, V.Kornilov, A.Belinski, N.Shatskiy, N.Tyurina, D.Kuvshinov, P.Balanutsa Sternberg Astronomical Institute, Moscow State University A. Tlatov, A.Parkhomenko Kislovodsk Solar Station of the Pulkovo Observatory V.Krushinski, I.Zalognikh Ural State GCN Circ 8470, Lipunov et al., ...
[ Сохраненная копия ]  Ссылки http://observ.pereplet.ru/images/GRB081102/grb_film.html -- 8.2 Кб -- 01.10.2012
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7. HIDEEP and HIJASS Results
Next: HIMF Up: Minutes of the 1st Previous: HIPASS . ... HIDEEP is a deep, blind survey with Parkes over a small patch of sky. ... 9000 sec per beam . ... HIDEEP optical follow up: . ... HIDEEP galaxy properties: . ... HI column densities: . ... To figure out the actual HIDEEP sensitivity, you have to decide how to derive the limits on the column density when the beam is large (unresolved sources). ... In terms of your column density, you are assuming filled beam and then adopting an optical size. ...
[ Сохраненная копия ]  Ссылки http://www.naic.edu/alfa/ealfa/meeting1/minutes/hideep.html -- 8.4 Кб -- 08.05.2006
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8. ADASS 2002 Conference Proceedings
... Up: Web Services and Publications . ... We present the architecture, design, and implementation details of the ADASS XII web site. The web site was implemented in Zope, a high-performance application server, web server, and content management system rolled into one. ... The sitemap was created in the beginning to organize the constantly flowing and changing information of web sites. ... The unique Zope content management application divides web content from the site design. ...
[ Сохраненная копия ]  Ссылки http://www.adass.org/adass/proceedings/adass02/P2-7/ -- 10.7 Кб -- 12.03.2003
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9. ESO - Standard Star Catalogue Search Tool
... Science . ... Science Users Information > Observing with ESO Telescopes > Observing Tools and Services > Standard Stars Catalogues > Standard Star Catalogue Search Tool . ... Publications with ESO Data . ... ESO Data . ... This tool searches the standard star catalogues for standards that are within dX airmasses of the target at a given LST. ... In this case put the LST when the target was observed in the TargetLST box as before, and put the LST of the standard star observation in the StdObs LST box...
[ Сохраненная копия ]  Ссылки http://www.eso.org/sci/observing/tools/catsearch.html -- 32.5 Кб -- 10.04.2016
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10. Selection criteria
... An overall criterion for standard-star selection is the accuracy needed in the final results: if you need more accuracy, you will need more standard stars. ... While it is possible to get a rough estimate of the extinction by observing different standard stars at high and low airmasses, the relatively large conformity errors in most photometric systems, together with the low accuracy of some standards, make this method very inefficient (see Young [ 10 ], p.178). ...
[ Сохраненная копия ]  Ссылки http://www.sao.ru/precise/Midas_doc/doc/94NOV/vol2/node280.html -- 7.3 Кб -- 23.02.1996