... This step is done mostly interactively and uses some basic ad-hoc IDL procedures, mainly for testing and checking of the consistency of the results.Once the observations have been selected and the count spectra extracted, the available spectra of each background level are accumulated. ... Average QUALITY such that QUALITY =0|1 Exposure times are added and the total is written in the EXPOSURE keyword of the header of the output FITS file. Finally, the CCFs are built from these templates. ...

... HST switched to 2-gyro mode operations 18 months ago, in anticipation of this eventuality. ... NICMOS was not available for scheduling this week; observations will resume next week. ... Jane Charlton, The Pennsylvania State University . ... Abstract . ... Two new `bullets' for MOND: revealing the properties of dark matter in massive merging clusters . ... Photometric Imaging of Asteroid 2 Pallas . ... Systemic and Internal motions of the Magellanic Clouds: Third Epoch Images . ... Past weeks: . ...

Organization of the Data Processing in the Interball Project. ... Interball Data Archive contains data produced during Interball mission: raw data, data files produced by express-analysys and preprocessing systems, orbit and attitude data files, key physical parameters, Magion-4,5 subsatellites data files and other types of data. Express-analysys data is available for Interball participants within 1 day after telemetry session, level 1 processed data - within 2 weeks. ... Attitude data files . ...

... Of the 4 buttons in the bottom part of the configuration screen, three deals with power level adjustments: the 'Power control' button brings up the power control window where You can adjust the power levels of the different parts of the IF/LO system, the 'Power levels' button brings up the power level monitoring window (which also can be run outside CIMA as the 'powerwin' program), and the 'Adjust Mock power' button which adjusts the power levels on the Mock spectrometer (but nowhere else). ...

... CentralProcessor 0.11 documentation . ChannelSelTask selects a subset of channel space. ... This is a legacy task which was used for early BETA debugging with notably contaminated spectrum. ... As for all tasks, parameters are taken from keys with tasks. name .params prefix (not shown in the table below) where name is an arbitrary name assigned to this task and used in tasklist (this allows us to run the same task more than once with different parameters). ... Parameter . ... ChannelSelTask . ...

... Accelerating black holes, spin-2/3fields and C-metric . A TOPOLOGICAL EXTENSION OF GENERAL RELATIVITY TO EXPLORE THE NATURE OF QUANTUM SPACETIME, DARK ENERGY AND INFLATION . EFFECTIVE THEORY FOR QUANTUM GRAVITY . TESTS OF GENERAL RELATIVITY AND ALTERNATIVE THEORIES OF GRAVITY USING GRAVITATIONAL WAVE OBSERVATIONS . ... THE MASS OF THE OPPENHEIMER-SNYDER-BLACK HOLE: ONLY FINITE MASS QUASI-BLACK HOLES . ... NEUTRINO MASS AND THE STANDARD MODEL . Neutrino masses and flavor mixing . ...

Klimov,S.I., V.V.Kopeikin, V.V. Krasnosel`skikh, A.M.Natanzon, A.E.Reznikov, M.P.Gough, S.P.Kingsley, T.A.Lachlan-Cope, H.G.Muller, L.J.C.Woolliscroft. ... Space Res., (1990), v.10, No.3-4, (3)35-(3)38. Grard,R., C.Nairn, A.Pedersen, S.Klimov, S.Savin, A.Skalsky, J.G.Trotignon. ... Space Sci., (1991), vol.39, No.1/2, pp.89-98. ... Res. ... Space Res., (1991), vol.11, No.9, pp.( ... Space Res., vol.11, No.9, p.(9)15-(9)18, 1991. ... Adv. space Res., v.11, No.9, p.19-34, 1991. ...

Quick guide for ChaMPlane Database Searching sources by coordinates [left panel ]: select the coordinate (e.g RA=337.3831880 , Dec=61.2185250 , Radius=2 ) [right panel ]: display the results Browsing by ObsID [left panel ]: list available observations by ObsID [middle panel ]: list available data product for the selected ObsID [upper right panel ]: list the data by srcid [lower right X-ray source ID is defined as XS + x-ray ObsID + energy band + CCD ID + source number. ...