... It is surprising that given such deep eclipses in the visible light, the soft X-rays did not reveal any traces of the eclipse ... The vertical lines are the lines of night sky emission. The strongest vertical line is the emission H line. ...
... the proper identifications, and in some cases it was necessary to control visually the identifications using sky surveys images ... No emission or absorption lines deeper than ~ 2% are seen in any part of the optical spectrum, or only extremely week ...
... time), 2) directivity diagram (antenna pattern) of the detector (which chooses a particular sky region in particular sidereal time), and 3) known position on the sky the inhomogeneous distribution of the possible sources of SN signals, such as Galactic ...
... 1..281Colla+ B2 Sky Survey at 408 MHz (B2) (21.7d-40.3) BR_GALS BRGAL r few 1975CSIRO.. ... 85..329Pauliny-Toth A deep survey of selected regions for extragalactic sources at 4.85GHz EGRET1 GRO1 x n 1994ApJS...94.. ...
... time), 2) directivity diagram (antenna pattern) of the detector (which chooses a particular sky region in particular sidereal time), and 3) known position on the sky the inhomogeneous distribution of the possible sources of SN signals, such as Galactic ...
... identification of the source IGR J08390-4833 from the INTEGRAL all-sky survey ... of a new cataclysmic variable from integral all sky survey: IGR J08390--4833 ... A. IGR J08390-4833 is a new cataclysmic variable from the INTEGRAL all- sky survey ...
... at 0.96, 3.9 and 11.2 GHz in: New Horizons . from the Multi-Wavelength Sky Surveys. Symp.IAU N179, 1997,p. 103-105. ADS . ... P.19-23 . M.Naugol'naya . "New results of deep probing of the Moon at RATAN-600" . 1998. ...