... Team . ... GRB mini-workshop 2006 . GRB workshop 2009 . ... GRB host galaxies are not peculiar objects. ... At present, long GRBs are identified with explosions of (probably) usual massive stars at the end of their evolution, i.e. massive (core-collapse) supernovae (CC-SNe). Thus, now GRBs are identified with 1) regions of the forming of massive stars (with massive star-forming) in host galaxies and 2) with explosions of short-living massive stars in the same galaxies - CC-SN/GRBs. ...

... SAO RAS . ... In 2016, a leading center of the Russian ground-based observational astronomy, Special Astrophysical Observatory of the Russian Academy of Sciences, is celebrating its 50th anniversary. The Observatory organizes an international conference "Multi-spin galaxies 2016", as a part of the festivities. ... Afanasiev Victor (SAO RAS, Russia) . ... Mapelli Michela (INAF - Padova, Italy) . Moiseev Alexei (SAO RAS, Russia) - chair . ... Karachentsev Igor (SAO RAS, Russia) . ... Russia), . ...

Detailed identifications of the FIRST (and NVSS) radio sources are carried out for 26 rich Abell clusters of galaxies in the framework of the announced project (A.G.Gubanov et al. 1997, in ``Problems of modern Radio Astronomy'', XXVII Radio Astronomy conference, St.Petersburg, V.1, P.168). ... Identification of radio sources in clusters of galaxies"). Identifications are performed for all radio sources within Abell radius of cluster of galaxies (3 Mpc for the Hubble constant of 50 km/s/Mpc). ...

... In LABORATORY OF RADIO ASTROPHYSICS OF SPECIAL ASTROPHYSICAL OBSERVATORY OF RAS . ... History . ... Current problems of the group research interests: . study for cosmic microwave background, . study of radio galaxies (identification, evolution, statistical investigation of population), . investigation of the RATAN-600 antenna, . observations in the survey mode with RATAN-600 and their analysis, . creation of the software for data analysis. vo @ sao.ru ( Oleg Verkhodanov ) ...

... Corresponding gates in each row are connected in parallel at both edges of the array. ... Other gates. ... otherwise indicated, 45 kpixels/sec and standard voltages using a dual slope CDS circuit (8 µs integration time) Minimum Format Pixel Size Imaging Area Dark current (MPP), 20° C equivalent Readout noise Front Back Full Well signal Output gain CTE per pixel Typical 512 x 512 pixels 24 µm x 24 µm 12.3 mm x 12.3 mm 50 pa/cm2 5 electrons 7 electrons 350,000 electrons 1.5 µV/ electron 0 ...