... radiusup: sources are ordered in order of increasing radius (see subsection 3.5 ). radiusdown: sources are ordered in order of decreasing radius (see subsection 3.5 ). rownumber: sources are ordered in order of increasing row number in the source table. expr: for this value, the task looks in parameter ncutsortexpression for an expression involving column names. This expression is evaluated and the sources are then ordered in increasing order of the resulting value. ...

Еще в разделе: (Показать все результаты (>31930) - xmm.vilspa.esa.es/ )

• Parameters

Target Acquisition Reference Information . ... In almost all cases where an onboard acquisition will not work (because the object is in a crowded field, or is variable, or is a moving target), it is sufficient to use an early acquisition to get a WFPC2 or FOC image a few weeks in advance of the GHRS observation. ... Explicit BRIGHT and FAINT limits may be specified if you desire, although there is an increased risk of a failed acquisition unless you are confident of those fluxes. ... MAPs . ...

Еще в разделе: (Показать все результаты (>12535) - www.stsci.edu/ )

• Surface Brightness Parameters from Deconvolved PC Images of Elliptical Galaxies
• Ferrarese Ford: Surface Brightness Parameters from Deconvolved Images
• Constraints on Acquisitions and the STEP-TIME Parameter

In this gallery are many images of Low Surface Brightness Galaxies which have recently been discovered and analyzed. ... The central surface brightness of this galaxy is 24.28 . Malin 2 This galaxy is another huge disk galaxy with a scale length of 15 kpc and a redshift of 15000 km/a. The high surface brightness knot in one of its spiral arms actually has the same color, luminosity and H-alpha equivalent width as the entire Large Magellanic Cloud . ... Truly it is a Low Surface Brightness Galaxy. ...

Еще в разделе: (Показать все результаты (>316) - zebu.uoregon.edu/ )

The parameter brief (with its actual uncertainty sbrief) is the mean effective surface brightness in B-band , i.e. the mean surface brightness inside the effective aperture (the circular aperture enclosing one-half the total flux). It is expressed in mag arcsec -2 . ... 2) from the mean surface brightness "LV" inside the effective isophote (elliptical isophote enclosing one half the total flux) measured by Launberts&Valentijn (1989) . ... Effective radius . ... HyperLeda . ...

Еще в разделе: (Показать все результаты (>1914) - www.sao.ru/ )

• Mean astrophysical parameters from LEDA
• Nonlinearity
• Documentation: LEDA: parameter: bri25

The HyperNews Linux KHG Discussion Pages . Forum: The Linux Kernel Hackers' Guide . Re : Tunable Kernel Parameters? . Re : Increasing number of files in system (Simon Cooper) . Keywords: kernel tuning, file handles, Bus error . Date: Sat, 25 Oct 1997 11:25:44 GMT . From: Simon Cooper < simon.cooper@snc-net.demon.co.uk > . Sorry for the typo, my (Linux loader) lilo.conf entries are: . image=/vmlinux.safe [Newline] label=LinuxS [Newline] root=/dev/hda2 [Newline] .

Еще в разделе: (Показать все результаты (>7598) - www.arcetri.astro.it/ )

• Program parameters
• Determination of the Detector Parameters
• Where are the tunable parameters of the kernel?

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. ...

Еще в разделе: (Показать все результаты (>91) - selena.sai.msu.ru/ )

• http://selena.sai.msu.ru/Pug/Publications/m44_70_pugacheva.pdf

Old subtables of the extended ``HIPASS Bright Galaxy Catalog'' . ... Koribalski, Staveley-Smith, Kilborn, + HIPASS/ZOA teams 2004, AJ 128, 16 . The 1000 Brightest HIPASS Galaxies: HI Properties . ... The 1000 Brightest HIPASS Galaxies: The HI Mass Function . ... The 1000 Brightest HIPASS Galaxies: Newly Cataloged Galaxies . ... To download the gzipped ps-file click here . ... The Brightest Galaxies from HIPASS . Presented is the distribution of the 700 brightest HIPASS galaxies. ...

Еще в разделе: (Показать все результаты (>8357) - www.atnf.csiro.au/ )

• User Parameters - Preparation of the Science field data CentralProcessor 0.11
• User Parameters - Continuum imaging CentralProcessor 0.11 documentation
• Task parameter manipulation

... Guider functions . ... Guide Sensor Performance . ... Guide Sensor Sky Coverage/ Star Availability . Guide Star Selection Criteria . ... Guide fiber organization and reach at plug plate . ... Plug plate holes for guide stars are identical to those for science FO . ... FOV for each of 9 guide stars is 7.4 arcsec dia. (0.45 mm FO, Sumitomo IGN-05/10) . ... Selected guide stars must have no neighbor stars within TBD (5 arcsec) radius that have a brightness within TBD (5 mag.) of guide stars . ...

Еще в разделе: (Показать все результаты (>642) - www.apo.nmsu.edu/ )

• Echelle for Beginners
• Telescope Parameters

... The parameter y   characterizes the ratio between the gravitational and magnetic ``properties'' of a star and will, therefore, be called the gravimagnetic parameter . Two magnetic rotators having quite different magnetic fields, subjected to different external conditions but with identical gravimagnetic parameters, have similar magnetospheres, as long as the accretion rate is quite low ( ). ... For isolated rotators, the accretion rate  yr is assumed. ...

Еще в разделе: (Показать все результаты (>438) - xray.sai.msu.ru/ )

• The Effect of Relativistic Wind on Accretion Flow Parameters
• Initial Distributions of Binary Parameters
• Initial parameters of compact stars

Next: Coherent integration Up: Astrometry data reduction Previous: Introduction Contents . ... In order to increase the SNR for these data, we coherently integrate the complex visibility for typically 200 ms. The coherent integration is done using the COBRA procedure cohstrictor . In order to provide the necessary input file for this step, the following CONSTRICTOR parameters should be used. ... The .coh extension is standard for coherent integration. ... NumAv = 100. ... Pass on metrology data . ...

Еще в разделе: (Показать все результаты (>10924) - www.eso.org/ )

• Preparation of parameter file
• The Brightness of the Night Sky
• Stellar parameters from calibrations of spectral types

... Using the uvby -photometry and proper motion data for about 5500 F stars within 80 pc from the Sun, we have studied velocity ellipsoid parameters and obtained the following results. 1) The sizw of all wllipsoid semiaxes increase systematically for groups of stars with the decrease of both temperature (at constant metallicity) and metallicity (at constant temperature). ... As a result, each of the three parameters - temperature, metallicity and velocity dispersion - is an age indicator. ...

Еще в разделе: (Показать все результаты (>54) - ip.rsu.ru/ )

... Parameters of the Moon-perturbed orbit . ... From orbits consistent with this limitation and with the date of the launch October 1, 2000 as an example, an orbit was selected with apogee directed to the North Galactic pole at the begining and rotation of orbit plane was maximized. The initial state vector is given in the inertial coordinate system in epoch J2000.0. ... The orbit has initial perigee radius Rp=7000.0 km, initial apogee radius Ra=343000.0 km and initial period T=8.453 days. ...

Еще в разделе: (Показать все результаты (>134) - www.asc.rssi.ru/ )

• Results of measurements of SRT antenna parameters in Pushchino
• ОТЧЕТ

Proposal Identification No.: ... At mid-latitudes, OI 844.6 nm emission brightness is a potentially excellent proxy for [O], and recent improvements to its forward emission model warrant renewed effort to pursue ground-based sensing using this unique emission. ... To this end, we propose several observational campaigns, spanning a variety of seasonal conditions, using combined passive optical and incoherent scatter radar instrumentation. ...

Еще в разделе: (Показать все результаты (>2720) - www.naic.edu/ )

• http://www.naic.edu/~astro/aotms/backends/96-01.pdf
• http://www.naic.edu/vscience/schedule/tpfiles/KearnstagA1446tp.ps
• http://www.naic.edu/~gibson/galfa/igalfa/docs/poster_2011_ncur_newton_full.pdf

... IRAF supports two kinds of parameters, auto parameters and hidden parameters, which are treated differently. auto parameters are updated every time a task is run. ... Parameters for each task are contained in `parameter files' in the uparm sub-directory in `myiraf'. ... im > imhead.longheader=yes # explicitly setting <task.param>=<value> im > eparam imhead # Edit the parameter file to update one or more # parameters at the same time # see next section . ...

Еще в разделе: (Показать все результаты (>2260) - hea-www.harvard.edu/ )

• Editing Files and Parameters
• Chandra Images for SNR J0519.5-6902
• Listing and Printing Files, Parameters, and Tables

... Future seminars . P a s t seminars . Seminar council . The emission time of Gamma-Ray Bursts" . A. Sanin (IKI) . ... The three new parameters of cosmic gamma-ray bursts are introduced: the emission time, the peak energy of the emission time spectrum and the cosmological invariant parameter. ... Using this distribution the "collective estimation" of the best fitting redshifts for the group of long bright gamma-ray bursts detected by BATSE experiment was found. ...

Еще в разделе: (Показать все результаты (>718) - www.cosmos.ru/ )

• Multipoint correlations of the solar wind parameters observed by several
• Magnetic mapping file description
• Magnetic mapping

... 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. ...

Еще в разделе: (Показать все результаты (>1671) - www.adass.org/ )

• Recent Advances in Parameter Estimation in Astronomy with Poisson-Distributed
• TwoFitlines: An Spectrum and Line Analysis Tool
• In-Orbit Calibration of the Distortion of the SOHO/LASCO-C2 Coronagraph

In this chapter we will consider an example of visual expert system written on the Actor Prolog language. ... There are a lot of methods of oil field bed stimulation that increase output of the oil production: thermal, physical-chemical, gas, microbiological, and others. ... Fig. ... The Top-Most diagram consists of three blocks: the "Describe parameters of hydrocarbon field" block, the "Check adaptability of existed methods of oil production" block, and the "Display solution" block. ... Gas methods. ...

Еще в разделе: (Показать все результаты (>450) - www.cplire.ru/ )

• SYNCHRONIZATION OF DRIVE-RESPONSE SYSTEMS ON CONDITION OF A LARGE MISMATCH OF
• Project 4 - RFBR - Stepantsov, Determination of the space anisotropy of order

... Публикации и издания Публикации профессорско-преподавательского состава СГАУ Издания проф. Сосниной Т.Н. Biosphere: Analysis of Value Parameters . ... Besides, the ways of saving the use value and value properties of biosphere are analyzed. The expediency of transformation of two-criterion theory of value into the three- criterion theory of the balance of value, where the ecologic component performs the function of the key criterion has been founded. ... BIOSPHERE USE VALUE OF THE PRODUCT: MAIN . ...

Еще в разделе: (Показать все результаты (>323) - www.ssau.ru/ )

New reduction of minor planets photographic plates obtained with Pulkovo Normal Astrograph A.A. Berezhnoy Pulkovo Observatory of RAS, Saint-Petersburg, Russia Minor Planet observations at Pulkovo Periodical observations of 14 bright asteroids named Selected Minor Planets (SMP) were performed at Pulkovo since 1948 within the international framework started by works of B.V. Numerov and D. Brouwer. ... 108 133 113 74 124 67 97 88 14 84 64 5 20 19 Epochs (YYYY.MM) 1200 Mean values of total obs. ...

Еще в разделе: (Показать все результаты (>28) - www.puldb.ru/ )

• The Pul-3 astrometric catalogue (Second edition). Data access form.
• The Pul_ERS astrometric catalogue. Data access form

External influences on spin parameters for INTERBALL - AP . ... The main interest is that almost all kind of external influences to parameters of motion (eclipse, normalization, ROS) are presented in the one time interval. Three upper panels illustrate the spin velocity, the angle between kinetic moment and sun direction, and the nutation.All external events are represented on the lowest panel as blue, green and yellow columns. ...

Еще в разделе: (Показать все результаты (>584) - www.iki.rssi.ru/ )

• AZ Key parameters, 1998
• AZ Key parameters, 1997
• AZ key parameters, 1996