... The results of the follow-up spectroscopy of 187 emission-line galaxy (ELG) candidates from the Case objective-prism survey with the 6m telescope are described. ... Significant fraction ( 23%) of the observed Case galaxies do not show emission lines in blue. ... Observations and data reduction . IPCS observations and data reduction . CCD observations and data reduction . ... Accuracy of data, comparison with independent measurements . ...

... Team . ... GRB mini-workshop 2006 . ... 6-meter telescope BTA: . The monitoring of gamma-ray burst afterglows and the study of their host galaxies . Monitoring of core-collapse supernovae and investigation of their host galaxies . ... Supernovae and gamma-ray bursts . ... Are some GRB host galaxies lying in galaxy clusters? ... Supernovae and gamma-ray bursts (Within the scope of the international program "Astronomy in Prielbrusiye") . ... The physics of gamma-ray bursts in the SWIFT era . ...

... 2011: . ... The measurements of the apparent diameter of a long-period variable star R Leo, a cold pulsating giant in the last stage of evolution, the scales of which are hundreds of times larger than the Sun were conducted at the 6-m BTA telescope. ... The discovered effect explains the observed anomalously large values of the pulsar slowdown indices, as well as the known differences in the estimates of their ages with the ages of the corresponding supernova remnants. ... Archive . ...

The project of the informational system creation on the problem of evolution of radio galaxies, as a part of the "Big Trio" project aimed on studing of distant radio galaxies, is designed. This system allows a user to operate with simulated curves of spectral energy distributions (SED) to estimate ages and redshifts by photometry data. Authors use SEDs of several models for different types of galaxies. ... The HTTP and e-mail access is organized to this system. ...

... 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 ...