XMM-Newton Science Analysis System . ... Meta Index . This task fits a linear combination of real-valued image components to a Poissonian, integer-valued image. ... Fitting algorithm: . Constraints on the model components: . Truncated Poisson fitting: . ... Input Files . Output Files . Algorithm . ... Index . XMM-Newton SOC/SSC -- 2007-07-09 ...

Еще в разделе: (Показать все результаты (>25351) - xmm.vilspa.esa.es/ )

• Description

... The GHRS has the usual components of an astronomical spectrograph: entrance apertures, a collimator, dispersers, camera mirrors, and detectors. ... The collimator and camera mirrors are unexceptional and need no further description here (see ``The HST Focal Plane and the GHRS Apertures'' on page 73 for details). ... The first two first-order gratings, G140L and G140M, have their spectra imaged by mirror Cam-A onto detector D1, which is optimized for the shortest wavelengths. ...

Еще в разделе: (Показать все результаты (>21971) - www.stsci.edu/ )

• WFPC2 Drizzle Cookbooks
• CSPICE Routines: VPACK_C
• CSPICE Routines: VUPACK_C

Next: Format of the Up: Auxiliary Data Previous: Description of the . For convenience in table handling only values for single lines or doublets (most of the observed cases) can be entered. If higher multiplicities are actually needed small changes have to be made in the table and program format. Possibility for 50 different atomic transitions. N.B. : in case of doublets, columns 3, 5, 7, 9, and 11 refer to the reddest component, and columns 4, 6, 8, 10 and 12 to the bluest. ...

Еще в разделе: (Показать все результаты (>2497) - www.sao.ru/ )

• Instrument Description: CASPEC
• Session Parameters
• Multivariate Statistical Methods

... A technique allowing automatic representation by a relatively small number of independent parameters based on the principal component analysis of data sequences is presented. ... In recent years the spectrum of observed astronomical data can be characterized as greatly varied. ... In this instance, the problem of initial description and classification of newly-observed data becomes most urgent, especially if there is a lack of preliminary observational material and theoretical expectations. ...

Еще в разделе: (Показать все результаты (>1718) - www.adass.org/ )

• A Spectroscopy Exposure Time Calculator for IRAF
• ETCs and Observations Simulation at the VLT
• A Graphical User Interface for a Development Environment (GUIDE)

... Created: 23 February 2001 . ... SOFTWARE MAINTENANCE MANUAL . ... 9 January 2001 . ... Note: in the final document, the table of contents will be to third level] . The Software Maintenance Manual describes the procedures for installation and maintenance of the software for the Gemini Near-infrared Integral Field Spectrograph (NIFS). ... Section 19.4.3 of the document “Programmatic Requirements for Gemini Instrumentation Development” states the requirements for the Software Maintenance Manual . ...

Еще в разделе: (Показать все результаты (>1507) - www.mso.anu.edu.au/ )

• GSAOI Instrument Description Page
• GSAOI Component Supplier Links Page
• GSAOI Dwarf Galaxies Science Page

... CentralProcessor 0.11 documentation . ... The Central Processor Manager is the local monitoring and control agent for the Central Processor sub-system. ... At the moment the Central Processor Manager only controls the acquisition phase; that is, it only controls the ingest pipeline. ... In addition to the CP manager specific parameters, any parameters that begin with ice_properties are passed directly to the ICE Communicator during initialisation. ... string . ... Central Processor Manager . ...

Еще в разделе: (Показать все результаты (>11120) - www.atnf.csiro.au/ )

• cmodel (Model Image Generator) CentralProcessor 0.11 documentation
• User Parameters - Continuum Self-calibration CentralProcessor 0.11...
• Making a Fake Observation

Orbital data : INTERBALL AZ GSE and GSM cartesian coordinates, GSE cartesian velocity (once per 10 minutes). ... Magnetic field data from IMAP experiment. Magnetic fileld absolute value and magnetic field index (the difference between absolute value and model value), status flag. ... Counts of H+ and O+ ions are accumulated during one spin period by detectors D6 (antisunward looking), D8 (spin plane), D10 (sunward looking) of TRICS2 subsystem (1.0-30 keV). ... TRICS1, TRICS2, TRICS3 subsystems: . ...

Еще в разделе: (Показать все результаты (>499) - www.iki.rssi.ru/ )

• INTERBALL-TAIL KP list

grdvector - Plot vector fields from grdfiles grdvector compx . ... CYLINDRICAL PROJECTIONS: -Jc lon0 / lat0 / scale (Cassini) -Jj lon0 / scale (Miller) -Jm scale ( Mercator - Greenwich and Equator as origin) -Jm lon0 / lat0 / scale ( Mercator - Give meridian and standard parallel) -Joa lon0 / lat0 / azimuth / scale (Oblique Mercator - point and azimuth) -Job lon0 / lat0 / lon1 / lat1 / scale (Oblique Mercator - two points) -Joc lon0 / ...

Еще в разделе: (Показать все результаты (>490) - xray.sai.msu.ru/ )

• Change of Binary Parameters: Mass, Semi-major Axis and Eccentricity
• Other parameters of the evolutionary scenario
• Restrictions on the Scenario Parameters

Find Similar Abstracts (with default settings below ) . ... Also-Read Articles . ... Parameters of the 41 Dra system components . ... 00/2001 . ... Stars: Binaries, Binaries: Fundamental Parameters, Binaries: Individual . ... 61B Based on spectral and speckle-interferometric observations of the system 41 Dra, model atmosphere parameters of the system components have been derived: component Aa - T eff = 6500K, lg g = 3.99, R = 1.87 R solar , component Ab - T eff = 6500K, lg g = 4.11, R = 1.61 R solar . ...

Еще в разделе: (Показать все результаты (>1082) - jet.sao.ru/ )

• проект SCORPIO-2: parameters
• comedi_get_cmd_generic_timed
• SCORPIO-2 project: description

Table 5.3 Parameter Notation and Units Parameters of the TC93 Electron Density Model Estimated Value Description Outer axisymmetric component n1 h1 ( cm-3 kpc ) h1 ( kpc ) A1 ( kpc ) F1 0.0165 0.88 20 0.4 Nominal electron density , n1; scale height , h1 Scale height Reference radius Fluctuation parameter Inner axisymmetric component n2 h2 A2 F2 ( cm-3 ) ( kpc ) ( ...

Еще в разделе: (Показать все результаты (>5463) - www.naic.edu/ )

• http://www.naic.edu/~tghosh/thesis-jf/chap_6/Table6.2.pdf
• Index of /~phil/hardware/vertex/hagenDocmemos/klaus/ATA1A/parameter
• WAPP File Format Page

The VLTI Calibrator Selector Tool is a tool intended to assist in the selection of suitable interferometric calibrators for VLTI observations with MIDI and AMBER. It uses a model of the VLTI and its instruments to assess the fringe visibility, given the observed bandpass, the geometry, spectrum, and coordinates of the target and the time at which the observations are to be made. ... The tool offers an HTML/Java based interface and consists of two pages. ... The quality flag depends on LDD_chi2. ...

Еще в разделе: (Показать все результаты (>66847) - www.eso.org/ )

• HSTPOLSIM (V2.00) --- November00 --- HSTPOLSIM (V2.00)
• Health Check Monitor: Users Guide
• Quality Control: Daily health check monitor

hstpolsim -- Produce simulated polarization input data frames for HST instruments . ... inint = "" [name] . ... Name of the HST instrument for which simulated polarization images are to be produced. ... Name of the instrument specific polarizing filter for simulated images (ignored for SPECIAL instrument). filtname = "" [name] . Name of the instrument specific colour filter for simulated images. ... The header parameter FILTER provides the filter name and POLANG the polarizer angle. ...

Еще в разделе: (Показать все результаты (>263) - www.stecf.org/ )

• HSTPOLIMA (V1.00) --- April99 --- HSTPOLIMA (V1.00)
• HSTPOLPOINTS (V1.00) --- May99 --- HSTPOLPOINTS (V1.00)
• POLIMPLOT (V1.00) --- April99 --- POLIMPLOT (V1.00)

. The description of the instrument is divided into the following sections: . Optical Design . Cryogenics and Mechanics . Electronics and Software . Determination of Detector parameters . Some photos of the instrument . Other high resolution images .

Еще в разделе: (Показать все результаты (>8422) - www.arcetri.astro.it/ )

• Program parameters
• Determination of the Detector Parameters
• IBIS: Technical Description

Hourly values of parameter foF2 (F2 layer critical frequency) The description of letters in the tables of parameter foF2 A blanketing. ... C non-ionospheric (equipment). D above upper frequency range of equipment. E below lower frequency range of equipment. F frequency spread. ... K particle E layer. L no sufficiently defined cusp between F layers. ... N superimposed layers. O measurement refers to o component. ... Q range spread. R attenuation near critical frequency. ...

Еще в разделе: (Показать все результаты (>10034) - www.wdcb.ru/ )

• http://www.wdcb.ru/stp/data/ionosphere/NP-7/Readme.doc
• Index of /stp/data/Images_of_f-plots/TABL/Tables of different Parameters/M3000
• Index of /stp/data/Images_of_f-plots/TABL/Tables of different Parameters/fo Es

... Co-ordinate systems description . Directories structure . The file names' construction . The file set description . ... The orbital information for each month is presented in the separate directory. The INTERBALL orbital data are located on the STDA server, for each month in the separate subdirectory, which name consists from the year (YYYY) and month (MM) numbers. The Parent Directory of the Tail Probe orbital data is http://www.iki.rssi.ru/da/interball/tail/orbit/ . ...

Еще в разделе: (Показать все результаты (>1300) - www.cosmos.ru/ )

• PhSRM
• Magnetic mapping file description
• OFO IKI / Test Calibration Facilities

The data in the Table on p. 5788 – 5789 embrace estimated parameters for 128 binary systems in near Earth, Mars crossing, main belt and Trojan orbits (more than 90% of corresponding objects are marked in the Table "Minor planet lightcurve parameters" as undoubtedly binary and in other cases as suspected binary). ... The data were presented by P. Pravec (Astronomical Institute, Academy of Sciences of Czech Republic) (see Pravec, P., Harris, A. W., 2007. Binary Asteroid Population. ...

Еще в разделе: (Показать все результаты (>468) - www.ipa.nw.ru/ )

... This is possible at modest cost due to the low moments of inertia of the telescope and enclosure. ... This same performance will be achieved in higher winds when the telescope enclosure is facing away from the wind, or by using wind screens. ... The telescope system (MILT) will be remotely operable with an on-site operator's assistance by an astronomer located at one of the ARC member institutions. ... Mean Wind Speed . ... Offsets > 10 deg: 1 arc sec rms max . ... 5 sec max, tracking to tracking . ...

Еще в разделе: (Показать все результаты (>714) - www.apo.nmsu.edu/ )

• lsst.coordConv: coordConv::FK4CoordSys Class Reference
• lsst.coordConv: coordConv::Coord Class Reference
• lsst.coordConv: coordConv::OtherCoordSys Class Reference

OptInt PmWiki : Pm Wiki / Page Directives . ... attachlist NAME:) shows a list of attachments of the group or page NAME. (:attachlist ext=xxx:) specifies an extension for filtering by type of file. (:attachlist *:) shows the uploads directory and permits browsing of all uploaded files by directory ( will not work if $EnableDirectDownload is set to 0 ). (:description text:) . ... If supported by the skin , each of these turns off the corresponding portion of the page. (:redirect PageName:) . ...

Еще в разделе: (Показать все результаты (>3394) - www.mrao.cam.ac.uk/ )

• Inference of Coefficients for Use in Phase Correction Bojan Nikolic web pages
• How to create a new tool in CASA Bojan Nikolic web pages (r. 329)
• DUST: dustiface.h File Reference

... 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 ...

Еще в разделе: (Показать все результаты (>272) - www.gao.spb.ru/ )

• Phase light curves of young binary systems

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 . ...

Еще в разделе: (Показать все результаты (>3874) - hea-www.harvard.edu/ )

• Using the PROS software
• Structure of the Spectral Package
• Model Spectra for Spectral-Fitting Program