XMM-Newton Science Analysis System Page: 1 omfastshift July 9, 2007 Abstract Corrects FAST mode event list coordinates for spacecraft drift. ... Parameter Mand Type Default Constraints set yes string none OM Fast Mode Event List Intermediate File (output of OMPREP) thxset yes string none OM Tracking History Data Auxiliary Intermediate File (output of OMPREP) nphset yes string none OM ODF Non-Periodic Housekeeping le interpolate no boolean T Linearly interpolate s/c drift over FAST mode time slices? ...

Please enter the lightcurve file name and period search parameters: . Lightcurve file: . ... Apply the Heliocentric correction and convert all dates to Terrestrial Time (TT)? ... Also, the Heliocentric correction cannot be applied to such lightcurves. ... This period search service is also available at the mirror sites: Mirror 1 , Mirror 2 , Mirror 3 , Mirror 4 . You may download the latest source code distribution and install the period search service at your own web server. ...

... As described in "Tabular Storage of STIS Data" on page 20-5 , raw time-tagged Sdata are stored in an event table which contains separate columns for the x and y pixel coordinates and the arrival time of each detected photon event. ... Generate a series of ACCUMulated images from user specified time intervals of data and then process the image(s) with calstis . ... The default behavior for inttag is to accumulate all events from the table, writing the results as one image set in the output FITS file....

Next: *upspecrdf, downspecrdf* - Transform Up: Spectral Analysis Previous: *grid_plot* - Plot Results . The conversion of count rate to flux depends on the intrinsic spectrum of the source, so xflux must be used in conjunction with fit . Fit generates a table of the best fit intrinsic spectrum ( _int.tab extension). xflux uses this table to calculate either the integrated flux between two energy limits or the flux density at a specific energy. ... This produces ``..._obs.tab'' file. ...

... User Guide ] Task: ellint Purpose: Integrate a Miriad image in elliptical annuli. ... The integration is done separately for each image plane in the region included. ... They are the outer radius (arcsec) of the annulus; number of pixels in the annulus; the average (median) in the annulus; the rms of the annulus; the sum in the annulus normalized by the volume of the primary beam (if there is one); the cumulative sum for all annuli so far. Key: in Input image name. xyz images only. No default. ...

... CALIBRATE/LINE Calculate coefficients for wavelength calibration . CENTER/.. Compute center of line . CONVERT/TABLE Make image from table values . EXTINCTION/SPECTRUM Correct 1-D image for extinction . IDENTIFY/GCURSOR Identify table entries from graphic display . IDENTIFY/LINE Equate X positions to wavelengths . INTEGRATE/GCURSOR Integrate line interactively . MODIFY/GCURSOR Change data in line interactively . ... SEARCH/LINE Search calibration lines . ...

... Next: The PROS Big Up: Software Systems Previous: Data Reduction Software . ... The srcinten task provides PROS users with a tool to compute count rates for point sources in the ROSAT High Resolution Imager (HRI). ... Corrected upper limits are cited at locations where the count rate falls below the source detection threshold. ... Srcinten is a new PROS task that computes and applies the above correction factors to the net counts in a user-specified aperture. ...

ALMA | ... In this section, we explain why we need to correct phase fluctuations and ALMA's strategy to do this. Rapid fluctuations will be corrected with water vapour radiometers (WVRs). The Cavendish Astrophysics Group was also a leading contributor to the ALMA prototype WVRs, which were put through their paces in tests at the Submillimeter Array (SMA). ... The Cavendish Astrophysics Group in partnership with the Onsala Space Observatory built two prototype WVRs for the ALMA project. ...

... The data was taken over many days with the same source in more than one file. ... You want to convert the data to kelvins (this is galactic work) and then average all the scans for each source. ... input each onscan, average, and then scale to kelvins . place all of the averaged scans in an array, when done with the file, store this array in an idl save file for this day. ... Average together scans of the same source and then baseline them. input all of the daily save files into a single array . ...

Next: Evolution of Magnetic Rotators Up: ``Ecology'' of Magnetic Rotators Previous: The equilibrium period . The evolution of NS in binaries must be studied in conjunction with the evolution of normal stars. ... Figure: Tracks of NS on the period ( p ) - gravimagnetic parameter ( Y ) diagram: track of a single NS (vertical line) and of a NS in a binary system (looped line). ... Another version of the evolutionary track of a NS formed in the process of mass exchange within a binary system is: . ...

... Iowa Robotic Telescope | ... Talon is based on OCAAS, a software suite developed by software engineer Elwood Downey ( Clear Sky Institute ) for use at the University of Iowa ?s first remote facility (the ATF, or Automated Telescope Facility). ... XObservatory : Telescope Control Interface . ... This program calls upon and coordinates much of the interrelated portions of the Talon architecture, and forms the primary control panel for the telescope, dome, and peripheral systems when used locally. ...

... The predicted magnetic conjugations correspond to the less then 5 deg relative geocentric angular distance of the two satellites magnetic footprints. ... Universal time) . ... the difference between two satellites corrected geomagnetic local times (see as well column 11) . ... the difference between two satellites corrected geomagnetic latitude (see as well column 12) . ... the satellite geographical latitude . ... the corrected geomagnetic local time . ... the corrected geomagnetic latitude . ...

Vertexing Tools Vertexing Tools Jan Strube University of Oregon Overview Overview · · · · · · Introduction The Algorithm ­ ZvTop Implementation in hep.lcd Introducing org.lcsim Present Status Summary and Outlook 2005-8-20 Jan Strube - Snowmass 2005 1 The Algorithm ­ ZvTop The Algorithm ­ ZvTop D. Jackson, NIM A388:247-253, 1997 D. Jackson, NIM A388:247-253, 1997 · Topological ... The position is the one found by the algorithm, but the tracks are not fitted. ...

MyMidiGui is an IDL wrapper for some of the MIA and EWS routines which was originally written to support MIDI data analysis during service mode observations on Paranal. Since the first release ( Version 0.2 ), MyMidiGui has been extensively revised and integrated into the OYSTER environment. This enables easier plotting and analysis of MIDI data with OYSTER after having been reduced using MIA+EWS. The MyMidiGui major version numbers correspond to the compatible versions of MIA+EWS . ...

... The files here will change whenever we have a new beta version that has had an error-free telescope run. ... A few things to note, however, about this "beta" edition: There is almost no error checking on the operation of the filter wheel. ... CCDops has better error checking than XmCCD, so if you have a Windows computer available, check your camera with CCDops when you use it for the first time. ... I have a built-in fixed delay to inhibit multiple requests too fast for the wheel. ...

Here is one CCD image of the SN. ST7 image format. Dark and flat corrected, Mar 19,1998 at.01.11 UT, yellow filter, temp -20c, 600s track and accumulate exposure (20x30s). The telescope used is 150/2063mm refractor. ... The next image was taken at 29.3.1998 01.27 UT, CCD ST-7, 600 s. Track and Accumulate exposure (15x40s.), no filter, dark and flat corrected, temp -20c, telescope used 2063/152 refractor. ... Back to Supernovae in NGC and IC galaxies . Back to Supernova 1998S images . ...

You can also see this page in Russian with using KOI8 (X Windows) or CP1251 (MS Windows) Cyrillic coding. The Laboratory supports the space TV experiments, mainly in the planetary exploration missions. ... Image Co-registration . ... PHOBOS mission - Martian satellites investigations. Phobos on the Martian limb, the image from Phobos-2 probe from 02/28/89. ... Russian Space Bulletin. ... Last modified at June,26 1997 Alexey Kuzmin: akuzmin@mx.iki.rssi.ru . Back to IKI home page ...

... Search PostgreSQL resources | ... Tsearch2 - is the full text engine, fully integrated into PostgreSQL RDBMS. Text Search is integrated into PostgreSQL 8.3 ! ... Download ispell dictionaries ready to use with tsearch2. ... chezh dictionaries , check also this article for more information. 61-tsearch-french-utf8.diff.gz - patch by Cedric Villemain, which adds utf8_french configuration (with snowball stemmer and list of french stop words) for fr_FR.UTF-8 locale . ... Text Search was sponsored by: . ...

... Robust Bandpass Removal Traditionally, the bandpass that is present in single­dish 21 cm spectra is re­ moved by observing in a ``signal­reference'' mode. ... Instead, a statistical estimate of the bandpass at the position and time that a particular spectrum---the target spectrum---was acquired is made from a set of earlier and later spectra observed by the same beam---these are the reference spectra. ... I b,p,c is a 1024­ channel flux density spectrum. ... References Barnes, D. G. 1998, this...

Sample page from NUMERICAL RECIPES IN FORTRAN 77: THE ART OF SCIENTIFIC COMPUTING (ISBN 0-521-43064-X) Copyright (C) 1986-1992 by Cambridge University Press.Programs Copyright (C) 1986-1992 by Numerical Recipes Software. ... 4.0 Introduction Integration of Functions Numerical integration, which is also called quadrature, has a history extending back to the invention of calculus and before. ... Isaacson, E., and Keller, H.B. 1966, Analysis of Numerical Methods (New York: Wiley), Chapter 7. ...