System for high-accuracy determination of ephemeris and time corrections (SVOEVP) GLONASS A.Yu. ... 3 Purpose of SVOEVP The system for high- accuracy determination of GLONASS ephemeris and time corrections ( SVOEVP ) is intended for provision of high- accuracy solutions of user navigation and time determination problems: in real time by refining SVOEVP adaptive parameters of S/C GLONASS motion model and measurements model, by calculating SVOEVP calibration corrections for user ...

... CentralProcessor 0.11 documentation . ... These parameters govern all processing used for the calibrator observation. ... The dynamic flagging step can also optionally include antenna or baseline flagging. Then the bandpass table is calculated with cbpcalibrator , which requires MSs for all beams to be given. ... Second amplitude threshold applied when flagging 1934 data [hardware units - before calibration] . ... Name of the CASA table used for the bandpass calibration parameters. ...

... we show that the comparison between the calculated and observed numbers of the most ``fragile'' (from the point of view of the binary evolution scenario )   galactic binary types (such as X-ray low-mass X-ray binaries (LMXB), cataclysmic variables (CV),   Be-stars   with compact companions, relative number of visible binary radiopulsars   with normal and compact secondary components) impose certain constraints on the feasible initial ... Phenomenological Kick Velocity . ...

Observed maximum rotation velocity uncorrected for inclination effect. This quantity is calculated from 21-cm line widths at different levels and/or rotation curves (generally in H_alpha). ... These data are characterized by some secondary parameters: telescope, velocity resolution, level of the 21-cm line width and bibliographic reference. ... we start from a standard sample (a set of measurements giving a large and homogeneous sample). ... HyperLeda . ...

... dataset . ... Used only if withrmfset is set to true . ... dataset flat psf . The origin of the detector map: if set to dataset , then the user must specify the name of that dataset, and the table name of the map though detmaparray . If it is set to flat or psf , then the parameters detxoffset , detyoffset , detxbins and detybins define the detector map grid. ... If true , the raw detector map and the bad pixel lists are filtered using the DSS information stored in the spectrum dataset. ...

... Basic Observables: Zero-differenced phase and code ionosphere-free combinations of global GNSS network stations, corrected by P1-C1 satellite code biases (cc2noncc), daily observations with 30 seconds sampling rate Sites coordinates : IGb08 reference frame coordinates and velocities Displacements: solid tides, ocean loading, pole tide loading (IERS 2010) Geometric model : Receivers antennas eccentricities, absolute receiver and ...

GHRS Instrument Handbook 5.0 115 Index 116 GHRS Instrument Handbook 5.0 A Accumulation Mode 13, 19, 34, 43--45 CENSOR 44 details 95--96 CENSOR, see also noise rejection COMB 15, 44 DOPPLER 44 FP­SPLIT 14, 30, 43, 44 high signal­to­ noise methods 107 parameter summary 44 STEP ­PATT 15, 44, 92, 114 STEP ­ TIME 44 substepping 19 acquisition parameters ACQ/PEAKUP, see acquisition ...

... We demonstrate through numerical simulations that model parameters estimated with our technique are essentially bias-free, even when the average number of counts per bin is 1. ... The IW technique avoids such biases by estimating through successive iterations, where for each iteration, j, , and the best-fit parameters are determined by minimization of . ... In our sample, we find that the minimum values and best-fit parameters converge after about 6 iterations. ...

THE PARAMETERS INVOLVED IN HAPKE'S MODEL FOR ESTIMATION OF THE COMPOSITION OF THE EJECTA LUNAR TERRAINS. ... In the previous papers we were estimated the surface roughness of the ejecta lunar terrains by means comparison of the local phase function and the average integrated lunar indicatrix. ... The Hapke's theoretical model of the lunar surface reflection. ... For THE PARAMETERS INVOLVED IN HAPKE'S MODEL: S.G. Pugacheva, V.V. Shevchenko a low-albedo lunar surface parameter Bo = 1. ...

The determination of the detector parameters is based on sets of images of a spatially uniform-illumination scene (flatfield frames) and without any illumination (dark frames), putting a plug in place of the filter, taken at a series of exposure times. ... We interleave before and after each exposure time in the series of flatfield frames a set of reference images at an exposure time of 1 sec to determine the possible temporal variation of the illumination level. ...