Astronet Поиск по астрономическим сайтам English Russian
       
        Точная форма слов   О проекте   Сайты   Справка
Найдено документов: 388642 (183 сайтов) ---- Время поиска: 0.96сек.   

1 | 2 | 3 | 4 | 5 | 6 | 7 | 8 | 9 | 10 | След.

Показаны документы, содержащие фрагменты текста из документа
http://www.rochesterastronomy.org/novae.html.

1. Supernova 2009js in NGC 918
Supernova 2009js in NGC 918 . This page is devoted to information on Supernova 2009js in NGC 918 . Basic information on this SN, including the last reported brightness, on this Supernova can be found on the main page . Information on the original web pages for many of these images can be found on the updates and links web pages. Discovered independently by Lick Observatory Supernova Search (USA) and Koichi Itagaki (Japan). ... 2009/10/11.44 . 17.2 . ... Joseph Brimacombe . ...
[ Сохраненная копия ]  Ссылки http://www.sai.msu.su/mirrors/isn/sn2009/sn2009js.html -- 8.2 Кб -- 13.02.2011
[ Сохраненная копия ]  Ссылки http://www.rochesterastronomy.org/sn2009/sn2009js.html -- 8.4 Кб -- 19.04.2014
Похожие документы

2. Extragalactic Novae - 2002.
... This is a partial list of the Extragalactic Novae discovered in 2002. Current Novae can be found on the main page . Nova NGC 2403 2002 , ATEL 1638 , discovered 2002/12/30.124 by K. Hornoch . Found in NGC 2403 at R.A. = 07h37m38s.36, Decl. ... Nova M31 2002 6 , IAUC 7970 discovered 2002/08/04.13 by K. Hornoch . ... Nova M31 2002 5 , IAUC 7937 discovered 2002/07/22.5 by LOTOSS . ... Nova M31 2002 4 , IAUC 7937 discovered 2002/07/20.5 by LOTOSS ; Observatory G. Colombo . ...
[ Сохраненная копия ]  Ссылки http://www.sai.msu.su/mirrors/isn/sn2002/novae.html -- 19.7 Кб -- 05.02.2013
Похожие документы

3. A REVISED AND UPDATED CATALOG OF QUASI-STELLAR OBJECTS
... see also previos version 1991 VII/158 A REVISED AND UPDATED CATALOG OF QUASI-STELLAR OBJECTS ================================================================================ HEWITT A., BURBIDGE G.: 1993 Astrophys. ... A standardization of the files and their description was performed at CDS to allow automatic conversions to FITS tables. The paper contains a catalog of all known quasi-stellar objects (QSOs) with measured emission redshifts, and BL Lac objects, complete to 1992 December 31. ...
[ Сохраненная копия ]  Ссылки http://www.sao.ru/cats/doc/QSO2.html -- 12.3 Кб -- 18.03.2015
Похожие документы
Еще в разделе: (Показать все результаты (>3223) - www.sao.ru/ )

4. Saturn [Oulu]
... Saturn is the sixth planet from the Sun , and the second largest in the solar system . Saturn's most distinctive feature is its ring system . ... Saturn has an internal magnetic field with a dipole aligned with the rotation axis (Ness et al., ... The solar wind and Saturn's rings and satellites supply the particles that are trapped in the radiation belts. ... Between the inner and outer satellites orbits Titan, Saturn's largest moon (larger than the planet Mercury ). ... Res., ...
[ Сохраненная копия ]  Ссылки http://www.iki.rssi.ru/magbase/REFMAN/SPPHTEXT/saturn.html -- 5.1 Кб -- 21.12.2007
Похожие документы

5. FOS ISRs on RECOMMENDED REFERENCE FILES
Note : FOS Instrument Science Reports (ISRs) relating to Calibration Plans are listed in reverse numerical (approximately chronological) order. ... For a paper copy of a report, please send e-mail or call the STScI Help Desk. ... ISR Paper Copy . ... 113 Reference Guide and Complete History of FOS Calibration Reference Files and Tables (8/94) . ... 112 FOS Dead Diode Reference Files: A Quick Reference Guide to the Appropriate File for a Particular Date and Instrumental Configuration (8/94) . ...
[ Сохраненная копия ]  Ссылки http://www.stsci.edu/ftp/instrument_news/FOS/isrlis_rec.html -- 4.6 Кб -- 12.05.2000
Похожие документы

6. BLoCXS: Bayesian Low-Counts X-ray Spectral Analysis
... BLoCXS is a Bayesian code that uses Markov-Chain Monte Carlo and Data Augmentation techniques to analyze CCD-resolution X-ray spectra in the Poisson regime. BLoCXS can be used to . fit common emission models to low-counts spectra . identify narrow emission lines in low-resolution spectra . identify Gaussian emission lines (with fixed/unknown location and width) . compute profile posterior distributions, . simulate data from posterior predictive distributions, . ...
[ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/AstroStat/BLoCXS/ -- 3.6 Кб -- 10.04.2016