Next: Setting Up Your Account Up: ATCA Bin Mode Observations Previous: Pulsar bin-mode observations . We now mention a few bin-mode specific tasks. Pulse profiles - PSRPLT: Task psrplt produces a pulse profile (amplitude against bin number). It can also produce a greyscale with axes of bin number and frequency and the greyscale intensity being pulsar amplitude. De-dispersion, rebinning and timing correction - PSRFIX: Task psrfix performs three related functions. ...

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• Parameters Specific to the VLA
• Special Concerns for Specific Observatories
• INFORMATION AND ADVICE ON SPECIFIC TOPICS

... In spite of the good potential possibilities, some of the station "Dnepr" design characteristics did not allow us to apply the usual special IS radar measurement methods. ... Thus for IS signal measurements at the "Dnepr" station, we have developed special methods for recording and processing IS signals in order to determine plasma ionospheric parameters. ... Equations (4-5) from the basis for data post processing to obtain ionosphere parameters. ...

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. Lines are sorted character by character, starting at the first character in the line. You can also sort the contents of a file on a specific part of each line. Each line of text is a series of fields - words and other characters - separated from each other by a delimiter character - the spaces between the words. Changing the field delimiter . Defining the sort field . Sorting on several fields . Sorting on a specific part of a field .

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• Running commands at a specific time
• Sorting on a specific part of a field
• Mail commands

Next: TAP 26 Up: Results Previous: Results . While the bulk of these stars were located in the Orion OB1a and OB1b fields, two stars of particular interest were monitored from our Mount Stony Brook Observatory. One of these stars was TAP 26 (NTTS 041559+1716, HBC 376). This star, located in Taurus, had a measured rotational period which was inconsistent with its . The other star was P1724, located near Orion OB1d, for which x--ray periodicity had been observed. TAP 26 . P1724 . ...

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• TAP 26
• Results
• No Title

... Apache HTTP Server Version 2.2 . Apache > HTTP Server > Documentation > Version 2.2 . ... This document explains how to install, configure and run Apache 2.0 under Microsoft Windows. ... Version 1.3 of the Apache HTTP Server is the first version which includes a port to a (non-ASCII) mainframe machine which uses the EBCDIC character set as its native codeset. Warning: This document has not been updated to take into account changes made in the 2.0 version of the Apache HTTP Server. ...

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• Please be more specific....
• LASG - Product specific information - NetMAX
• LASG - Product specific information - TurboLinux

Astronomy Discussion Forums . ... A Number Is A Very Specific Thing . ... Post Message | ... Posted by Harvey on October 9, 2002 16:41:15 UTC . ... When you use the word 'number', you are introducing a specific kind of symbol that is known within the context of mathematics. ... You know what - harvey1 - October 9, 2002 - 20:53 UTC . ... www.astronomy.net . ... Forum posts are Copyright their authors as specified in the heading above the post. "dbHTML," "AstroGuide," "ASTRONOMY.NET" & "VA.NET" . ...

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. Comedi Documentation . Prev . Next . comedi_maxdata_is_chan_specific -- maximum sample depends on channel . #include <comedilib.h> . int comedi_maxdata_is_chan_specific (comedi_t * device, unsigned int subdevice); . If each channel of the specified subdevice has different maximum sample values, this function returns 1. Otherwise, this function returns 0. On error, this function returns -1. Prev . Home . Next . comedi_range_is_chan_specific . Up . comedi_get_maxdata

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• comedi_range_is_chan_specific

... Calibration and Performance Control for the VLT Instrumentation . ... The ESO VLT CCD Detectors Software . ... The Observatory Monitoring System: Analysis of Spacecraft Jitter . ... O. M. Smirnov and O. Yu. Malkov . ... NICMOS Calibration Pipeline: Processing Associations of Exposures . ... NICMOS Related Software Development at the ST-ECF . ... The Data Handling System for the NOAO Mosaic . ... IRAF Data Reduction Software for the NOAO Mosaic . ... Data Format for the NOAO Mosaic . ...

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• Zero-Points of FOS Wavelength Scales
• Specifics on a XML Data Format for Scientific Data

... User Portal . ... Science Users Information > Observing with ESO Telescopes > Phase 2 Preparation > Phase 2 Instrument Table . ... Phase 2 Instrument Table . ... Manuals and Tutorials . ... Calibration Plan . ... The P2PP Tool (version 3) . ... Phase 2 Users Workshops . ... If one instrument has special requirements, this is visualized in the relevant row of the table. A summary table of the main characteristics of all instruments is available here . Instrument . ... FAQ . ... User Manual . ...

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• Common DFO tools: architecture
• DFOS: Frequently Asked Questions
• How to create QC web pages

What if we could determine if a given star is likely to host a planetary system like our own by breaking down its light into a single high-resolution spectrum and analyzing it? ... The dark bands result from specific chemical elements in the star s outer layer, like hydrogen or iron, absorbing specific frequencies of light. By carefully measuring the width of each dark band, astronomers can determine just how much hydrogen, iron, calcium, and other elements are present in a distant star. ...

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• http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B8D9A152A-46CE-4B6B-9DCA-1AB63CCDD610%7D
• http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B3919D44E-3672-48A4-800E-F150D095D4A6%7D

... Comparative study of Tl-2201 single crystals with different temperatures of superconducting transition by means of specific heat method. Abstract: . The comparison studies of the specific heat of Tl-2201 single crystals with the different oxygen concentration have led to the conclusion that the doping by oxygen, resulting in lowering of T c and increasing of number of paramagnetic centers, leads to diminishing of antiferromagnetic correlations contribution to the specific heat. ...

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• X-Ray Structural Analysis
• Cadmium sulfide (CdS)
• Laboratory of Optical Strength and Diagnostics of Crystals (LOSDS)

In order to calculate the line profile of a given absorption line for atomic species Z with a wavelength LAMBDA (in Angstroms) and a microturbulent velocity VT (in km/s). ... mode . ... 1) The input model may contain