Next: ASTROMET/EDIT Up: Available Commands Previous: Available Commands . This command computes the astrometric transformation parameters for the input data set using a least-square fitting algorithm. The input data is assumed to be two MIDAS tables with fixed columns names. ... ASTROMET/TRANSFORM only computes the transformation parameters. ... R_A Real column containing the right ascension in degrees; . ... XCEN Real column to contain the X measurement; . ...

... dataset . Name of the event list dataset. ... The name of a dataset with a template image in its primary extension should be supplied to this parameter. ... If outputstyle =`sky', the template image is also necessary to specify the pixel dimensions and World Coordinates of the output. withdss . ... If attstyle =`binnedset' the user should supply to the present parameter the name of a dataset which contains a time series of the spacecraft attitude variation during the exposure. flatexpcubeset . ...

Welcome to the 10C Survey website! ... The first 10C Survey results from an area of 27 sq. degrees complete to 1 mJy and 12 sq. degrees complete to 0.5 mJy have now been released. ... The first results from the survey, which is the deepest extragalactic radio source survey of any significant extent (> 0.2 sq. degrees) above 1.4 GHz, including the deep 15.7-GHz source count are contained in AMI Consortium: Davies et al. ... For each field, deep and shallow areas have been defined. ...

... Apache HTTP Server Version 2.4 . ... Session encryption support . ... session_crypto_module . ... The session will be encrypted with the given key. Different servers can be configured to share sessions by ensuring the same encryption key is used on each server. ... The SessionCryptoPassphrase directive specifies the keys to be used to enable symmetrical encryption on the contents of the session before writing the session, or decrypting the contents of the session after reading the session. ...

Up: Sky Surveys . ... The object catalogue and compressed pixel data are stored online and are accessible via the WWW. ... small area (up to 15arcmin) pixel images with attached object catalogue, . ... The primary data format is FITS for both images and binary tables of object catalogues, which enables porting of the data into established software packages. ... In this way, it is possible to browse the data by clicking on objects in the image display or the catalogue list to highlight them in both. ...

... This section will deal with obtaining photons within specified regions of an image. Available regions are: Annulus Box Circle Ellipse Field -- entire field Irregular region based on intensity of map... i.e. region defined by contour levels. ... The imcnts task in the xray-spatial package sums the source and background counts in specified regions, and subtracts one from the other properly normalized. ... imcnts* - Find counts in an extended region, after removing an embedded point source . ...

... We discuss the Phase II instructions for patterns in this section in order to illustrate the options available, however, this is not an exhaustive description and is not the appropriate reference to use when preparing a Phase II proposal. ... OFFSET=SAM (default), (use SAMs; gyros for large moves with re-acquire); SAM-NO-REACQ, (use SAMs; do not attempt to re-acquire guide stars); SAM-NO-GYRO, (use SAMs; must use same or new guide stars). ... SAM, the default, will use guide stars whenever possible....

Next: Summary List of SCHED Up: THE SCHED INPUT FILES Previous: THE SCHED INPUT FILES Contents . The schedule file is the main, and perhaps only, input file that the user prepares. ... A large number of input parameters are available for the schedule file. ... Default: The value assigned by SCHED if the parameter is not given in the schedule file. ... SCHedule . ... Next: Summary List of SCHED Up: THE SCHED INPUT FILES Previous: THE SCHED INPUT FILES Contents Craig Walker 2014-04-14 ...

Next: Absolute visual magnitudes Up: Command line procedures Previous: Plot data from the Contents . Files containing stellar parameter data reside in oyster/starbase . Extensive photometric data is found in files spec_par.X , where X signifies the luminosity classes for dwarfs, giants, and supergiants, V, III, Iab , respectively. For subgiants, brightgiants, and the subclasses of the supergiants, limited data is in files spec_MV.IV , spec_MV.II , spec_MV.Ia , spec_MV.Iab , spec_MV.Ib . ...

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: . ...

The starting page - The catalogues page - The list of the PUL2 fields - The list of the Pul-3(Pul-3SE) fields - The list of the PUL_ERS fields . please read short description of the access form controls . ... catalogue number of star (Obligatory parameter) . ... Right Ascension (ICRF/Tycho-1) J2000 at the central epoch of obs. (hours, minutes, seconds) (Obligatory parameter) . ... Declination (ICRF/Tycho-1) J2000 at the central epoch of obs. (degrees, arcmin, arcsec) (Obligatory parameter) . ...