... Background scans are automatically loaded with the get_data procedure, but can be manually loaded, for example after computing the biases when the background has been zeroed before, using the following procedure. get_bgdata Backgroundtable created. ... We flag these data manually (just plot channel 11 and then use Util|Edit to flag; re-plot to check whether all the data has been flagged); when OYSTER averages point data, any data without valid background scans will be discarded. ...

... It automatically figures out the line-free emission and fits a polynomial baseline to that data. ... ASAP> scans.auto_poly_baseline(order=2,threshold=5) . ... Don't try and fit the edge of the bandpass which is noisier ASAP> scans.auto_poly_baseline(edge=(500,450),order=3,threshold=3) # Only fit a given region around the line ASAP> scans.set_unit('km/s') ASAP> msk = scans.create_mask((-60,-20)) ASAP> scans.auto_poly_baseline(mask=msk,order=3,threshold=3) . ...

. XMM-Newton Science Analysis System . dataconv (sas-1.479) [xmmsas_20080701_1801-8.0.0] . Meta Index / Home Page / Attributes . Subsections . CREATOR . DATE . HISTORY . XMM-Newton SOC/SSC -- 2008-07-01

. Please standby and you will be automatically connected to the new location of the unframed Supernova page. Or, click on the link above. If you have questions or problems, please email me at David Bishop dbishop@vhdl.org . Last modified: Mon Aug 27 12:40:15 EDT 2001

Next: CORRELATOR BOARDS Up: OBSERVING PROCEDURES Previous: Frequency Switching . ... Continuum sources in the list used for flux density calibration were selected in an ad-hoc fashion from a variety of places, but primarily from Kuehr et al (A&AS, 45, 367, 1981), the compendium of linearly polarized sources by Tabara & Inoue (A&AS, 39, 379, 1980), and an unpublished list of unconfused calibrator sources prepared from the NVSS survey by Jim Condon and Qi Feng Yin. ... Board 0 . ...

Top] [Prev] [Next] [Bottom] . ... Initial Data Processing / 11-2 . POSITION Mode Pipeline / 11-3 . TRANSFER Mode Pipeline / 11-7 . ... This chapter describes how FGS data are calibrated. Unlike the data from other HST instruments, FGS astrometry data are not calibrated automatically. Observers now require the assistance of the FGS team at STScI and the Space Telescope Astromety Team (STAT) at the University of Texas to process astrometry science data through the FGS pipeline. ...

... The name Discovery Date mag Size(m) Publication MASTER -Observatory --------------------------------------------------------------------------------------------------------------------------- HAZARDOUS ASTEROIDS : 7 MASTER HAZARD Asteroid 2015 UM67 2015 Oct 28.88218 16.9 940m MPEC 2015-V01 MASTER -SAAO automatically MASTER software 6 MASTER rediscovered HAZARD Asteroid 2011 QG21 2015 Aug 17.94764 17.2 300m MPEC 2015-Q28 ...

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Next: Overscan correction and Up: Processing the Data Previous: How the Data . The command REDUCE/CCD can process one or more science frame automatically provided: . the association table correctly describes the associations between the science frames and the calibration frames; . the CCD reduction table or the SC_... keywords contains the correct names of the master calibration frames; . ... REDUCE/CCD will first identify the association and reduction tables. ...

Next: Imaging Polarimetry with NICMOS Up: NICMOS Data Calibration and Previous: The Photometric Performance of . ... NICMOSlook and Calnic C . ... Extracting spectra from a large number of NICMOS grism images requires a convenient interactive tool which allows a user to manipulate direct/grism image pairs. ... NICMOSlook and Calnic-C are two programs that were designed to take advantage of the fact that the NICMOS grism mode typically consists of taking both a direct and a grism image. ...

INFRARED FOURIER-SPECTROMETER SICH-F . ... Instrument work regimes: 1) Inside. 2) Calibration at inside standard sources 2 - 4 times per a rotation. 3) Calibration at "free space" 2 - 4 times per a rotation. 4) Infrared radiation measuring 10 - 40 min. per a rotation. ... Spectrometer consists of the photodetector block and the block of signal processing and control. ... Diagnostic information and attach data will transfer by state telemetric channels. ... Detector temperature. ...

... QPOE event times are typically expressed in units of an on-board spacecraft clock. ... The conversion is automatically performed as part of the timing corrections in 8.7.2. The stand-alone task scc_to_utc allows conversion of an arbitrary spacecraft time to UTC. input files: xtimingdata$scc_to_utc.tab ti> scc_to_utc tbl_fname = xtimingdata$scc_to_utc.tab # ROSAT # conversion table input spacecraft clock time (1606720.) ...

Next: Analysis Tools for Nebular Emission Lines . ... Extracting spectra from a large number of NICMOS grism images requires a convenient interactive tool which allows a user to manipulate direct/grism image pairs. ... The direct image is used to locate objects of interest, to find the position of the appropriate spectra in the grism image, to determine the optimal extraction technique to use, and to calibrate the wavelength range of the extracted spectra. ... Figure 1: The NICMOSlook User Interface . ...

As usual: it depends! It depends on the operating system of your laptop! And then: I don't know and it's not my task to know, so please don't ask me. ... In the menu "Start" -> "(all) Programs" -> "Accessories" -> "System Tools" -> "System Information" . click on "Components" -> "Network" -> "Adapters" . ... Open a DOS-window by clicking on "Start" -> "Programs" -> "Command Prompt" and enter the command "ipconfig /ALL" . ... Here you can find a more detailed description. ...

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... Apache HTTP Server Version 2.2 . Apache > HTTP Server > Documentation > Version 2.2 > Programs . Available Languages: en | ... The following programs are simple support programs included with the Apache HTTP Server which do not have their own manual pages. ... You can find them after the configuration process in the support/ directory. log_server_status . ... This perl script will take a combined Web server access log file and break its contents into separate files. ...

This module provides information on server activity and performance. ... Compatibility: Available in Apache 1.1 and later. ... ExtendedStatus To enable status reports only for browsers from the foo.com domain add this code to your httpd.conf configuration file <Location /server-status> SetHandler server-status Order Deny,Allow Deny from all Allow from .foo.com </Location> . ... A machine-readable version of the status file is available by accessing the page http://your.server.name/server-status?auto . ...

Next: Sharing swap spaces with Up: Memory Management Previous: Creating a swap space . An initialized swap space is taken into use with swapon   . ... You can monitor the use of swap spaces with free   . It will tell the total amount of swap space used. $ free . ... The total column does not show the physical memory used by the kernel, which is usually about a megabyte. ... Sometimes a lot of swap space can be in use even though there is a lot of free physical memory. ...

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