... 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 . ...

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• Initial parameters of compact stars
• Initial Distributions of Binary Parameters

... 2009) 0 Fig.1 · Max-Planck-Institute for Radioastronomy, Bonn , VLBI ESO, COMPONENTS PARAMETERS FROM INTERFEROMETRY · Following S.Kraus et al. ... Using i=105o , we obtain v sini = 32 km/s. BEST MODEL FIT 1OriC 1 · Mass, M · Luminosity, log L · Radius, R · Teff, K · log g · Equatorial rotation velocity, km/s · Magnetic field , G · The time of life, yrs 35.8 5.20 10.0 37000 4.01 5.4 500-1500 150 000 1OriC 2 10.0 4.69 8.2 30000 3.60 96.2 moves to MS 1 OriC ...

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Next: CAL_getBoresightMatrix Up: Routines of the Calibration Previous: List of CCF Components Contents . ... The CAL functions CAL_getBadPixelList & CAL_getBadPixelMap use the CAL state variable temperature only to check that the current operating temperature is consistent with the CCF constituent BadPix . ... Used CAL State Variables . List of CCF Components used . ... Next: CAL_getBoresightMatrix Up: Routines of the Calibration Previous: List of CCF Components Contents Michael Smith 2011-09-20 ...

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• EPIC Related CAL Routines
• OM Related CAL Routines
• Mirror Related CAL Routines

The following tasks belong to the category ROTATION-CURVES: . ... It overlays radial HI velocities (i.e. 'tilted ring' circular velocities) on velocities in XV diagrams and lets you adjust the tilted ring parameters to get a better fit. ... reswri . RESWRI derives the kinematical parameters from the observed velocity field by fitting tilted-rings to the velocity field and fits harmonic terms after convergence of the ROTCUR part of code. ... ROTCUR . ...

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• Casda Upload Utility CentralProcessor 0.11 documentation
• User Parameters - Continuum Self-calibration CentralProcessor 0.11...
• cmodel (Model Image Generator) CentralProcessor 0.11 documentation

... solve : find optimum fit in a grid of model spectra . ... It initiates an optimisation by starting with a grid of theoretical spectra, defined by model or read_grid , a set of starting parameters and an observed spectrum. ... The parameters to be optimised include: T eff , log g , n A , v sin i , v rad being effective temperature, surface gravity, an abundance variable, rotation velocity and radial velocity for one or two stars, and R 2 / R 1 being the relative radius of the second star, if present....

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• Armagh Observatory

... The HST uses an onboard model of its orbit to perform in real-time various control functions relating to spacecraft operations and observation support. ... New coefficients for the ephemeris are updated every other day, and are archived as FITS keywords for each HST observation data set. Using these coefficients,an observer can perform a variety of calibration and characterization calculations relating to the orbital position and velocity of the telescope. ...

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• TwoFitlines: An Spectrum and Line Analysis Tool
• Application of the Minimum Determination Algorithm to the Study of the Fine
• A Computer-Based Technique for Automatic Description and Classification of

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 . ...

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• Documentation: LEDA: parameter: vvir
• Edition of the Table Containing the Cloud Model
• Multivariate Statistical Methods

CIMA is more than just the observing tool - in fact, the observing tool is just a part of a bigger package called the CIMA software package. ... There is also a another package called the CIMA WAPP software which contains the WAPP software, the special Tcl/Tk interpreter used by CIMA and support libraries. ... All CIMA software components recognize the following general options that are part of the CIMA version selection system: . ... The select_cima script can be used to set up a default version. ...

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• AGES Database Search
• Orbits in the period / acceleration plane
• Submitting New Observing Modes to AO

... Bojan Nikolic web pages (r. 329) . ... We present a Bayesian approach to calculating the coefficients that convert the outputs of ALMA 183 GHz water-vapour radiometers into estimates of path fluctuations that can be used to correct the observed interferometric visibilities. ... Inference of Coefficients for Use in Phase Correction . ... Simulating Atmospheric Phase Errors, Phase Correction and the Impact on ALMA Science . ... Copyright 2005 -- 2016, Bojan Nikolic feedback welcome ...

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• Structure of Active Galactic Nuclei in a model with the radial magnetic field
• Data Format Session at 2001 IAU WG Meeting
• Determination of the relative orientation between radio and dynamical reference

Irregular phenomena in the Earth Pole oscillation process and temporal variations of geopotential Valery Bondarenko, Vadim Perepelkin s The observed irregular phenomena in the Earth Pole oscillation process are very variety. ... These phenomena indicated in the IERS data are the "abnormal" fluctuation of the Earth Pole coordinates which owing to changing of the geodynamical parameters gives negative result in interpolation and forecast of the first approximation mathematical model. ... Fig. ...

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• Phase light curves of young binary systems
• Catalogue of double stars

... In recent years, substantial information concerning the Io torus has been published. ... Explaining the observed steady state rotation of the torus seems to be difficult. The angular velocity of the torus must be in accordance with the celestial mechanics laws, of the same orders as Io's one. ... We wish to straighten out the situation describing the main geometric and kinematic features of the Io torus using a steady state model based on some of Alfven's ideas [Alfven, 1981]. ...

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• Geomagnetic Kp Index
• TCV [Oulu]
• Auroral arcs [Oulu]

... To plot the data (and model, here xitau.model), I have read the model, computed the model values for the ASTROMETRY, and used Plot|ASTROMETRY to produce the ASTROMETRY plot widget. ... First, plot the data and with Util|Ellipse and the mouse buttons interactively define an apparent ellipse to fit your data as best as you can. ... Under Util|Orbit, there is a Thiele-Innes procedure to estimate the orbital elements using your apparent ellipse and Kepler's laws! ... Back to tour page . ...

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• OYSTER Lab
• The Hierarchical Stellar Systems Model Format
• Astroclimatology of Paranal

... Computing the true count rates for digital data. ... The following equation is used to find the count rate. x = ( raw counts / sample time ) . ... True count rates for digital data are corrected by using the first equation for a point source and the second for an extended source. a = ( y - pre_amp - darkrate ) / ( highvolt x pt_effic ) . ... True photocurrents (count rates for analog data) are corrected by the first equation for point sources and the second equation for extended sources. ...

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• Analysis of in B-Type Stars
• Fine Guidance Sensor Instrument Handbook
• Systematic Uncertainties Special Cases

... Fitting the observed dependence includes calculations of the polarization cross-sections averaged over particles orientation and size distribution, their normalization and the comparison of obtained dependencies with Serkowski's curve representing observational data for a chosen star. ... Variations of the polarization factors with wavelength are shown in Fig. 16 for homogeneous spheroidal particles with PF orientation. ... The distinction between prolate and oblate spheroids is also clearly seen. ...

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• Project summary
• Rayleigh and Rayleigh-Gans-Stevenson approximations
• Polarization properties (transmitted radiation)

True Color Image Gallery: Galactic SNR | Magellanic Cloud SNR . ... parameters were derived from bright shell at N . Abundance of O-like element was set to zero asumming Typ1 I SN( Hughes et al., 1995 ). source=(xswabs * xsvraymond) . reduce chi^2 = 7.41398 . ... DataSet 1: 153 data points -- 144 degrees of freedom. Statistic value = 1067.61 . ... DataSet 3: 90 data points -- 76 degrees of freedom. ... Back to SNR J0519.5-6902 Index . Chandra Supernova Remnant Catalog . ...

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• Spectral Analysis
• Rotation Periods of ZAMS Stars
• Comments on: chi-square distribution [Eqn] By: Alex By: vlk By: aneta By: aneta

... Two such triple stars with low mass components, GJ 900 and KUI 99, have been observed during the last six years at the 6 m BTA telescope (Zelenchuk). ... Fig. ... The relative positions of the AB pair changed linearly during the period 2000­2004, showing a mean value of 48 mas/yr (Fig. ... Orbital solutions for the outer pair were proposed by Baize [1], Heintz [4] and Soderhjelm [10]. ... The apparent ellipses of the KUI 99 AC and KUI 99 AB pair are shown in Fig. ... P. Baize: Astron. Astrophys. ...

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• The spectrograph design and the observing procedure
• Absorption bands identified with DIBs
• Optimization of spectroscopic observations

... Contacts . 2012: . ... We refined the fundamental parameters of the components, the orbital periods, and the conditions of photospheric heating of the secondary component by the ultraviolet radiation of the hot component. ... The observations of the star clusters associated with ultra-luminous x-ray sources (ULXs) in four galaxies on the 6-meter and VLT telescopes have shown that all the ULXs are located within 200pc of very young star clusters (younger than 5 million years). ... Archive . ...

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• IRAS01005+7910
• Galaxy sector, archive 2006
• Multi-Spin Galaxies ? 2016

makeasn -- Group images in "associations" makeasn *cal.fits . ... The output are calnicb type "associations" tables. These tables contain the names of the images in each group, and the relative offset of the images in pixels. These files can be used to co-add iamges either with calnicb or with asncombine. ... In addtion, the observing time as well as the relative orientation of the imgages can be used as a criterion for an images to be included in a group. ...

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• ALIGNASN (Nov98) --- nictools --- ALIGNASN (Nov98)
• HSTPOLSIM (V1.00) --- April99 --- HSTPOLSIM (V1.00)
• MAKEPRFCORR (Nov98) --- nictools --- MAKEPRFCORR (Nov98)

THE RELATIVE MONTHLY MEAN SUNSPOT NUMBER ON APRIL 2013 HAS MADE W apr.= ... THE INTERNATIONAL DAILY VALUE OF RELATIVE SUNSPOT NUMBER FOR 2013, APRIL ACCORDING DATA OF 70 SOLAR OBSERVATORIES HAS MADE 1.. 53 m 6.. ... Weekly Bulletin on Solar and Geomagnetic Activity Highlights on 29.04 - 05.05.2013 , Forecast on 06.04 - 13.05.2013, Carrington Rotations 2136 (17,78.04.2013) SUNSPOT-FORMING ACTIVITY OF THE SUN CHANGED FROM THE AVERAGE TO THE HIGH LEVELS. ... Class E(1-8A) AR RII/IV CME X / opt. ...

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• http://www.izmiran.rssi.ru/services/saf/archive/en/2015/obzor20150622.en.txt
• http://www.izmiran.rssi.ru/services/saf/archive/en/2015/obzor20150629.en.txt
• http://www.izmiran.rssi.ru/services/saf/archive/en/2015/obzor20151116.en.txt

The problem of solar wind data correlation for the observations onboard several spacecraft is very important for three points of view: . ... This problem is studied now in detail by systematic determination of ion flux and ion velocity data correlations by INTERBALL-1 (IKI group), WIND and IMP 8 (both - MIT group). ... Solar wind plasma correlation lengths from IMP 8, WIND and INTERBALL-1. ... Correlation of solar wind observations onboard several spacecraft: INTERBALL-1, IMP 8 and WIND data. ...

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• Space Research Institute (IKI) Seminar
• Magion History
• Wave complex KEM-3