... Meta Index / Home Page / Description / Using odfbrowser / Graphical User Interface (GUI) The toolbar contains buttons, that allow the user to filter information and to configure and run the programs on the selected exposures. If you hover your mouse over one of those buttons, some text will pop-up, that gives you additional information about the button. Some buttons will only become active once you selected one or more exposures. XMM-Newton SOC/SSC -- 2005-08-16 ...

... GUIDE'' (Graphical User Interface for a Data Environment) is an interactive IDL widget-based package that enables users to retrieve selected sets of satellite instrument data and perform various types of graphical analyses on them, without writing a specialized program. GUIDE simplifies the task of laying out multiple plots on a page by (1) using a page-editor to define and laying out multiple ``panels'' which contain the ``plot objects'', and (2) integrating data retrieval functions. ...

The Hubble Deep Field South (HDFS) is a Director's Discretionary program on HST in Cycle 7 to image, similarly to the Hubble Deep Field (North), a typical field at high galactic latitude in four wavelength passbands as deeply as reasonably possible. ... In addition to the WFPC2 field, HDFS will include a STIS field containing a QSO at z=2.25 identified by Hewett and Boyle. ... 30 Orbits F814W . 30 Orbits F606W . 30 Orbits F450W . ... 1 primary orbits with STIS/50CCD to image the QSO field . ...

... distributed/updated files; VCAL directory managed . ... export to qcweb: all files (ex hdr/fits) in $DFO_LOG_DIR/<date>; all files (ex hdr/fits, ex ps) in $DFO_PLT_DIR/<date> . ... The final directories on the DFOS systems are: $DFO_CAL_DIR/$DATE for calib data, $DFO_SCI_DIR/$DATE for science data, $DFO_PLT_DIR/$DATE for graphical information, and $DFO_LOG_DIR/$DATA for pipeline logs, association logs, trending logs, and ABs. ... 2.14 move the ABs, AB logs and processing logs to $DFO_LOG_DIR/<DATE> ...

Next: Discussion Up: Second priority candidates Previous: The random selected sample . To improve the efficiency for the selection of BCGs among the second priority candidates we introduced additional selection criteria using the APM (Irwin [ 1998 ]) database. ... The second priority candidates classified as BCG/H II based on their slit spectra all have rather blue colours according to the APM database (APM ). ... One BCG of the four newly found is classified in the APM as stellar. ...

The Network Time Protocol (NTP) is used to synchronize the time of a computer client or server to another server or reference time source, such as a radio or satellite receiver or modem. ... Information on the NTP architecture, protocol and algorithms can be found in the following articles and reports, which are available online . Mills, D.L. Internet time synchronization: the Network Time Protocol. ... Mills, D.L. Network Time Protocol (Version 3) specification, implementation and analysis. ...

... example, note below the dramatic speedup in searching a 1 Gb file using an AND filter, even when one of the columns (pha) has no index : time fundisp \ huge.fits'[idx_activate=0,idx_debug=1,pha= 2348 4000 4000 1]' \ x y pha x y pha ---------- ----------- ---------- 3999.48 4000.47 2348 3999.48 4000.47 2348 3999.48 4000.47 2348 3999.48 4000.47 2348 3999.48 4000.47 2348 ... Currently, indexed filtering only works with FITS binary tables and raw event files. ...

slitless -- Extract a spectrum from a direct/GRISM image pair slitless image grism output PARAMETERS . ... A two dimensional direct image to be used to select an object. grism . A two dimensional GRISM image containing slitless spectra of objects present in the direct image. output . ... Toggle whether or not a background estimate is subtracted from the extracted object spectrum. mingood = INDEF . Pixels of the grism image with values smaller than this are ignored. maxgood = INDEF . ...

Program: SCANAID Purpose: Add IRAS data with respect to a reference point (ADDSCAN) Category: IRAS File: scanaid.c Author: T. Prusti Keywords: INIRDS= Input IRDS OUTSET= Output set [Scans not stored in a set] Set to contain the selected detector scans. ... SHOW= Control plotting of scans [Plot final result] N(one), A(ll), O(ne by one) plotting can be chosen in addition to the default to show the ADDSCAN result only. ... Otherwise the plot y-scale will vary from scan to scan. ...

... Denmark: ftp://ftp.dmi.min.dk/pub/Data/WDCC1/indices/kp-ap/ . Germany: ftp://ftp.gfz-potsdam.de/pub/home/obs/kp-ap/ . ... we do not guarantee the correctness of the international sunspot number R; these values are published separately (Brussels, Belgium) The following scientific and format documentation is adapted from ftp://ftp.ngdc.noaa.gov/STP/GEOMAGNETIC_DATA/INDICES/KP_AP/kp_ap.fmt The subscript p means planetary and designates a global magnetic activity index. ...

... The numbers of three types of compact binaries containing accreting NSs and BHs, which are most interesting from the point of view of their observational appearances, have been calculated as a function of time: i) X-ray transient source containing a NS in an eccentric orbit around a main sequence Be-star (the observed prototype: A0535+26), ii) BH The evolution of the selected types of X-ray binaries during the first 10 million years after the starburst onset is presented in Fig. ...

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