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1. An Unexpected Flare from the Crab Nebula
... An Unexpected Flare from the Crab Nebula . ... Credit Copyright: NASA , DOE , Fermi LAT , R. Buehler ( SLAC , KIPAC ) Explanation: Why does the Crab Nebula flare? ... As recently as one month ago, gamma-ray observations of the Crab Nebula by the Fermi Gamma Ray Space Telescope showed an unexpected increase in gamma-ray brightness, becoming about five times the nebula's usual gamma-ray brightness, and fading again in only a few days. ... Publications with keywords: Crab Nebula - gamma ray . ...
[ Сохраненная копия ]  Ссылки http://www.astronet.ru/db/xware/msg/1251798 -- 16.7 Кб -- 23.05.2011
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2. APOD: 2011 May 23 - An Unexpected Flare from the Crab Nebula
... 2011 May 23 . An Unexpected Flare from the Crab Nebula . ... As recently as one month ago, gamma-ray observations of the Crab Nebula by the Fermi Gamma Ray Space Telescope showed an unexpected increase in gamma-ray brightness, becoming about five times the nebula's usual gamma-ray brightness, and fading again in only a few days. ... The above image shows how the Crab Nebula normally appears in gamma rays, as compared to the Geminga pulsar, and how it then appeared during the recent brightening. ...
[ Сохраненная копия ]  Ссылки http://www.sai.msu.su/apod/ap110523.html -- 6.2 Кб -- 03.02.2013
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3. S.P. Korolev RSC Energia - International Space Station
... S.P. KOROLEV ROCKET AND SPACE CORPORATION ENERGIA . ... OAO RSC "Energia" . ... Company's History . ... History . ... ISS Russian Segment . ... ISS 45/46 . ... check for the following onboard the ISS RS: a capability to demonstrate the action of physical laws of dynamics of reactive and gyroscopic forces on ellipsoid (Letauschaya Tarelka device) rotating in the unsupported medium in microgravity, with video record of its behavior in the station module; . ... 2015 JSC "S.P. Korolev RSC "Energia" . ...
[ Сохраненная копия ]  Ссылки http://www.energia.ru/en/iss/researches/education/27.html -- 27.4 Кб -- 10.04.2016
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4. Comments
... Dead time corrections are not considered explicitly in the current version of this task, as it is expected that the EXPOSURE attribute, written to the spectral file by evselect (see also Julian Osborne's proposal regarding exposure-type attributes available on the SOC web server), should take into account dead time effects. arfgen calls the task attcalc internally. ... Note that the intermediate event dataset also contains attributes used to initialise the CAL in the subsequent call by attcalc . ...
[ Сохраненная копия ]  Ссылки http://xmm.vilspa.esa.es/sas/6.0.0/doc/arfgen/node37.html -- 8.4 Кб -- 18.03.2004
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5. http://www.stsci.edu/instrument-news/handbooks/nicmos/c13_accuracy.doc2.html
... In Table 14.1 we list a provisional summary of our calibration goals for Cycle 7 and Cycle 7-NICMOS. ... The present knowledge of photometric calibration does not yet permit a definitive projection of the ultimate accuracies which may be obtainable with NICMOS. ... Perforce our existing calibration data for Camera 3 have been obtained with it out of focus and therefore the estimates for its in-focus performance remain extrapolations. ... Breathing and dewar motion are approximately equal effects. ...
[ Сохраненная копия ]  Ссылки http://www.stsci.edu/instrument-news/handbooks/nicmos/c13_accuracy.doc2.html -- 6.5 Кб -- 07.08.1997
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6. Chapter 11. Specifying OpenGL Environment Variable Settings
Chapter 11. Specifying OpenGL Environment Variable Settings . ... Several antialiasing methods are available and you can select between them by setting the __GL_FSAA_MODE environment variable appropriately. ... To see the available values for __GL_FSAA_MODE along with their descriptions, run: nvidia-settings --query=fsaa --verbose . The __GL_FSAA_MODE environment variable uses the same integer values that are used to configure FSAA through nvidia-settings and the NV-CONTROL X extension. ...
[ Сохраненная копия ]  Ссылки http://www.naic.edu/~phil/hardware/nvidia/doc/driverInstall/chapter-11.html -- 10.3 Кб -- 30.10.2009
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7. ADASS 2003 Conference Proceedings
... 314 Astronomical Data Analysis Software and Systems XIII, eds. F. Ochsenbein, M. Allen, & D. Egret (San Francisco: ASP), 812 . ... Abstract: The calculation of flux upper limits in the source-free ("background") regions of photon-limited images is complicated by instrumental and statistical modeling and requires non-trivial computational effort. ... The principal component in this is the time taken to pre-process and handle the 30 GB of RASS data rather than the calculation of each upper limit. ...
[ Сохраненная копия ]  Ссылки http://www.adass.org/adass/proceedings/adass03/P10-11/ -- 12.9 Кб -- 13.08.2004
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8. http://www.gao.spb.ru/english/personal/malkin/publ/zm135.pdf
... Several attempts to discover the FICN signal in VLBI nutation series made during last years failed. ... We investigated several VLBI CPO series by means of spectral and wavelet analysis. It has been shown that there are several periodic signals with close amplitude around the expected FICN period without any prevailing one that can be reliably associated with the FICN. ... DATA ANALYSIS We analyzed several CPO series obtained in IVS analysis centers by means of spectral and wavelet analysis. ...
[ Текст ]  Ссылки http://www.gao.spb.ru/english/personal/malkin/publ/zm135.pdf -- 144.9 Кб -- 02.01.2015
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9. mod_proxy_ftp - Apache HTTP Server
... Apache HTTP Server Version 2.4 . ... FTP support module for mod_proxy . ... Source File: . ... Thus, in order to get the ability of handling FTP proxy requests, mod_proxy and mod_proxy_ftp have to be present in the server. ... How can I access FTP files outside of my home directory? ... To log in to an FTP server by username and password, Apache uses different strategies. ... In order to allow both browsing the directories on an FTP server and downloading files, Apache looks at the request URL. ...
[ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/manual/fr/mod/mod_proxy_ftp.html -- 18.4 Кб -- 19.11.2015
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10. Time domain analysis
... As noted above, periodic signals are best analysed in the frequency domain while stochastic signals are usually more profitably analysed in the time domain. The analysis in the time domain often involves the comparison of two different signals while in the frequency domain analyses usually concern only one signal. The expectation value of the covariance function of uncorrelated signals is zero. ... In particular the ACF of a function with period P has the same value, P . ...
[ Сохраненная копия ]  Ссылки http://www.sao.ru/precise/Midas_doc/doc/94NOV/vol2/node240.html -- 3.7 Кб -- 23.02.1996
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11. I Expected More Sense Than That. - an Astronomy Net Exploration Forum Message
Astronomy Discussion Forums . ... I Expected More Sense Than That. ... Post Message | ... Posted by Richard D. Stafford, Ph.D. on November 8, 2002 04:14:05 UTC . ... You are missing the point - harvey1 - November 8, 2002 - 13:10 UTC . I hope Stafford doesn't mind my intruding his forum - mrsouza - November 8, 2002 - 14:55 UTC . ... www.astronomy.net . ... Forum posts are Copyright their authors as specified in the heading above the post. "dbHTML," "AstroGuide," "ASTRONOMY.NET" & "VA.NET" . ...
[ Сохраненная копия ]  Ссылки http://www.astronomy.net/forums/exploration/messages/155.shtml -- 15.4 Кб -- 09.04.2016
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12. ESO - I see unexpected boxy emission-like features in my REDL spectra - where
... Science . ... Science Users Information > Data Handling and Products > Data Reduction FAQ > I see unexpected boxy emission-like features in my REDL spectra - where do they come from? ... Observing with ESO Telescopes . ... ESO-MIDAS . ... ESO Data . ... The pipeline by default interpolates across the bad columns in the REDL CCD when it creates the master bias, but does not so when it processes the science data. This inconsistency can create boxy emission-like features as seen in the figure below. ...