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1. Обзоры препринтов astro-ph
Подписка на рассылку обзоров astro-ph на Subscribe.Ru . ... Предыдущий выпуск (N335) . ... Обсудить на форуме Scientific.RU . ... Подписка на рассылку обзоров на Subscribe.Ru . Обзоры препринтов astro-ph . ... Собственно обзоры препринтов. ... Ранее обзоры также были на Астронете и на Scientific.Ru . ... АНКи доступны на Астронете , а с 2006 по 2008 г. также на сайте Элементы.Ру . ... Ранее они также размещались на сайте Астронет и в архиве моих обозрений (кодировка KOI8) на сайте Scientific.Ru . ...
[ Сохраненная копия ]  Ссылки http://xray.sai.msu.ru/~polar/sci_rev/current.html -- 14.8 Кб -- 02.04.2016
[ Сохраненная копия ]  Ссылки http://astro.uni-altai.ru/astro-ph/ -- 13.0 Кб -- 09.04.2016
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2. List of currently available KP AZ.
Orbital data : INTERBALL AZ GSE and GSM cartesian coordinates, GSE cartesian velocity (once per 10 minutes). ... Magnetic field data from IMAP experiment. Magnetic fileld absolute value and magnetic field index (the difference between absolute value and model value), status flag. ... Counts of H+ and O+ ions are accumulated during one spin period by detectors D6 (antisunward looking), D8 (spin plane), D10 (sunward looking) of TRICS2 subsystem (1.0-30 keV). ... TRICS1, TRICS2, TRICS3 subsystems: . ...
[ Сохраненная копия ]  Ссылки http://www.iki.rssi.ru/ibelova/az_key.htm -- 14.8 Кб -- 12.05.1999
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3. The Current CIMA Versions
. The following is a list of the currently installed versions of the CIMA. The links refer to the CIMA version log page . Normal: version 3.0 - this is the next version of CIMA which has become the new default version --- NOTE that this version uses a new syntax for command file observations, uses new configuration files and needs source files with full velocity information . Old: version 2.2 - this is the old version of CIMA You can return to the main CIMA page by clicking here .
[ Сохраненная копия ]  Ссылки http://www.naic.edu/~cima/cima_versions.html -- 2.3 Кб -- 01.03.2012
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4. Description
Next: Generation from In-Orbit Data Up: EMOS_BACKGROUND Previous: EMOS_BACKGROUND Contents . Currently not used in the SAS, but may be in the future. ... Accessed by : . CAL_getParticleBackground() : Obtain background particle spectrum in PI channel space according to the model : . Attributes: . ... Columns: . ... SPECTRUM : . unmodulated PI background PI spectrum . ... Next: Generation from In-Orbit Data Up: EMOS_BACKGROUND Previous: EMOS_BACKGROUND Contents Michael Smith 2011-09-20 ...
[ Сохраненная копия ]  Ссылки http://xmm.vilspa.esa.es/calibration/documentation/CALHB/node678.html -- 6.8 Кб -- 20.09.2011
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5. Current star formation rate
... The star formation rate (SFR) of the current SF episode can be estimated from the total H luminosity. ... For the derived total flux F (H )=5.8 erg s -1 cm -2 we obtain a total H luminosity of 10 39 erg s -1 . ... The total mass of ionized gas can be obtained from the average mass density inside the H II region and its volume. An average mass density corresponding to the average electron density of 1 cm -3 within a volume with a diameter of 0.5 kpc yields a total ionized gas mass of 10 6 . ...
[ Сохраненная копия ]  Ссылки http://www.sao.ru/precise/Laboratory/Publications/2000/0822_AA_v0/node13.html -- 7.0 Кб -- 11.03.2000
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6. A matrix of tweets from #AAS225
... Users . ... Data Collection and Analysis . ... This particular part of the analysis has been disabled since the code is struggling to cope with the number of users seen this year, in particular the large contingent of people who have re-tweeted NASA. ... Order accounts: by user number (effectively random) by number of tweets (includes retweets) by number of followers by number of followers that also tweeted about AAS225 by number of friends that also tweeted about AAS225 . ... by user number . ...
[ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/~dburke/aas225/user-matrix.html -- 10.3 Кб -- 10.04.2016
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7. Terry Mosely's Bulletins
From: TerryMosel@aol.com Date: Tue, 31 Dec 2002 13:03:40 EST Subject: Another Bright Comet? NEAT! Hi all, Here's another comet which may reach unaided visibility in late January early Feb. ... Prof Mark Bailey gave me the following details: COMET C/2002 V1 (NEAT): Discovered by the 'NEAT' auto-search facility, this comet is currently predicted to be around 8th magnitude, and to reach mag 2 or brighter when near Perihelion. ... Orbital elements: C/2002 V1 (NEAT) T = 2003 Feb. ...
[ Сохраненная копия ]  Ссылки http://star.arm.ac.uk/nibulletin/2002-Dec-31.html -- 5.6 Кб -- 07.01.2003
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8. Data Mining from the EROS Survey: the Current Status
... Up: Distributed Data Systems, Data Mining . ... The EROS (Exp?rience de Recherche d'Objets Sombres) experiment is a French collaboration between astronomers and particle physicists to search for the baryonic dark matter of the Galactic Halo by gravitational microlensing. ... Cross-identification with stellar objects in other surveys (e.g. ISOGAL, DENIS, see Omont et al. 1999) will also certainly become another use of EROS data in the next few years. ... EROS collaboration) 1998, A&A, 337, L17 . ...
[ Сохраненная копия ]  Ссылки http://www.adass.org/adass/proceedings/adass99/P3-35/ -- 10.9 Кб -- 04.10.2000
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9. XWare > APOD
Astronomy Picture of the Day . Introducing Nova Velorum 1999 . 24.05.1999 . A bright nova was discovered Saturday that is currently visible to the unaided eye in southern skies. ... John U. Obs.), making it more luminous than many famous bright stars. The Keyhole Nebula . ... The dark dusty Keyhole Nebula gets its name from its unusual shape. Officially designated NGC 3324, the Keyhole Nebula is a smaller region superposed on the larger Eta Carina Nebula. ... Europe at Night . ...
[ Сохраненная копия ]  Ссылки http://www.astronet.ru/db/xware/apod.html?page=87&d=2001-09 -- 15.2 Кб -- 12.04.2016
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10. What work is currently being done to improve the flux calibration accuracy for
... What work is currently being done to improve the flux calibration accuracy for echelle modes? ... Starting early in Cycle 11, monthly offsetting for echelle modes was turned off to minimize these types of calibration problems. ... We are currently working on redetermining the echelle flux calibration so that it is self-consistent with the 2-D scattered light algorithm. Time dependence of the sensitivity - Sensitivity-monitor data for the echelle modes are currently under investigation. ...
[ Сохраненная копия ]  Ссылки http://www.stsci.edu/hst/stis/faqs/faq_ech_flux_calibration.html -- 20.9 Кб -- 10.04.2016
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11. MILT Description
... This is possible at modest cost due to the low moments of inertia of the telescope and enclosure. ... This same performance will be achieved in higher winds when the telescope enclosure is facing away from the wind, or by using wind screens. ... The telescope system (MILT) will be remotely operable with an on-site operator's assistance by an astronomer located at one of the ARC member instit