From Jose Vicente Perea jose.perea@sciops.esa.int Wed Aug 5 15:32:11 2015 From: Jose Vicente Perea jose.perea@sciops.esa.int ( SAS Builder ) Date : Wed, 5 Aug 2015 15:32:11 GMT Subject : [ sas-uploads ] ebkgreg-0.2.tgz Message-ID : 201508051532.t75FWBxv007955@sasbld01.net4.lan Package: ebkgreg-0.2.tgz - 79182 B MD5: 35da5416b2e63279c64ef39e7efb17a3 ...

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• [sas-uploads] eboxdetect-4.25.tgz
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The FITS archive & data processing pipelines . ... The archived data are broad band images (BBI) and long-slit spectra (LSS) plus their associated template and calibration files. The data in HFA can enter into the HyperLeda processing pipeline and the results can be freely downloaded. ... Definition of the file system (structure of the archive) . ... The coordinate systems must be updated when the data (pixel data, other keywords, related tables) are altered (eg. rebinning of the image). ...

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• Non-standard keywords
• Averaging and Merging Frames
• HyperLEDA documentation

... Whatever the dimension of the input set is, there will be always at most one profile axis. ... The set has axes RA,Dec,Freq ! ... Italic font colour foreground move 35 225 text inset n3198h freq move 35 225-5 text profile 0 0 move 35 225-10 text ( profile in Freq at RA 0, Dec 0) move 35 225-15 text Integration possible in RA and Dec move 35 155 text inset n3198h RA 0 Dec 0 move 35 155-5 text profile 2 116 move 35 155-10 text ( profile from Freq 2 to ...

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• Tasks
• Event-driven Tasks and Graphical User Interfaces
• SM - Overloading Keywords

ASC-FITS-2.0.1: ASC FITS File Designers' Guide (Rots and McDowell) (1999 Jun) . ASC-FITS-REGION-1.0: FITS region document (McDowell and Rots) (1998 Mar) . ... CXC-DM-001 Introduction: Data Analysis with the Chandra Data Model (2001 Oct) . ... 1998 Feb 26: SDS-1.0: Data Product List: obsolete . ... 1998 Mar 09: SDS-10.0: (ASC-FITS-REGION-1.0) FITS region document: see ASC-FITS-REGION-1.0 . 1998 Feb 09: SDS-11.0: FITS function document (superseded by ASC-FITS-FUNCTION-1.2) . ...

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• zhtools
• Viewing the qpoe file.
• The AstroStat Slog Blog Archive different views

... Here we will look at line plots. We will go through steps, such as changing linestyles and symbols, you can use to modify your line plots. ... IDL> plot, num, line . ... IDL> plot, num, line, psym = 1 . ... IDL> plot, num, line, linestyle = 1 . ... Line Style . ... IDL> plot, num, line, linestyle=2, thick=3 . ... IDL> plot, num, line, psym = 8, symsize = 2.0 . ... IDL> plot, num, line, charsize=2.0, title='GHRS spectrum . ... IDL> plot, num, line, charsize=2.0, xcharsize=0.8, xtitle='wavelength' . ...

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• Incorrect COS ACQ/IMAGE coordinate keywords
• NICMOS Data Handbook
• Observatory Support FAQ List

Peremennye Zvezdy ( Variable Stars ) 26 , No. ... Our BVR CCD photometric study of the globular cluster NGC 7006 permitted us to find two new suspected RR Lyrae variables. A cluster chart is presented with the position of known and suspected variables marked. ... According to the Catalogue of Variable Stars in Globular Clusters (Clement et al., 2001), it contains 76 variables, most of which are RR Lyrae variables, the RR1 to RR0 ratio being 8:55. ... for suspected and some of known variable stars. ...

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• An Orion of a Different Color

... Does the time it takes different methods to create all the elements coincide with the universeт??s accepted age? ... Illinois Urbana-Champaign) Different kinds of stars create elements at different rates, all of which are consistent with the age of the universe. Get instant access to subscriber content on Astronomy.com! ... Registration is FREE and takes only a few seconds to complete. If you are already registered on Astronomy.com, please log in below. ...

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• What can astronomers tell us about the different colors on the surface of
• What determines the length of totality during a solar eclipse? | Astronomy.com
• Why do some stars appear to flash a variety of different colors when you look

Masses of asteroids 10 Hygiea and 152 Atala obtained by the dynamical method . ... Masses of asteroids 10 Hygiea and 152 Atala have been obtained by the dynamical method. ... m 152 = 1.34 0.27 (10 -11 Sun )]. ... Very Long Baseline Interferometry (VLBI), Small Solar System Body (SSSB), mass of asteroids 10 Hygiea, mass of asteroids 152 Atala, the dynamical method, perturbing asteroids, the additional acceleration, the Yarkovsky effect, elimination of erroneous observations, optical observations. ...

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• Keywords_122
• Keywords_146
• Keywords_65

... The polygons of different observatory . ... geographical (Greenwich geocentric) . coordinates of the polygon's corners, . or by the geographical coordinates . ... GGLat (deg) . GGLong (deg) . ... Polygon's corners . geographical coordinates . Back to the top . Polygon's corners geographical coordinates . ... The central point geographical . coordinates and extensions . ... GGLat extension (deg) . ... GGLong extension (deg) . ...

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• Trigonometry beyond 90 degrees
• STDA files

... AstroCC is a coordinate conversion utility for astronomy. It accepts an object designation or the coordinates of an object and calculates coordinates in alternative systems, and at different dates, times, and locations. It also provides lunar and bright planet coordinates to aid in planning observations. ... BJD values may also be retrieved from http://astroutils.astronomy.ohio-state.edu/time/utc2bjd.html which is based on Eastman et al. ... Coordinate data are obtained from SIMBAD. ...

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When Apache starts, it connects to some port and address on the local machine and waits for incoming requests. By default, it listens to all addresses on the machine, and to the port as specified by the Port directive in the server configuration. ... There are two directives used to restrict or specify which addresses and ports Apache listens to. ... Listen can be used to make a single Apache server listen to more than one address and/or port. ... Syntax: Listen [ port | IP-address:port ] . ...

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... Keywords: Proper Motions, Schmidt Plates, Astrometry, Guide Star Catalog, Palomar Sky Survey . In this paper we describe a program of determining proper motions from digitized scans of 1950's-era Palomar Sky Survey (POSS) Schmidt Plates and 1980's-era Palomar Oschin Schmidt `Quick V' plates that were taken for the Hubble Space Telescope ( HST ) Guide Star Catalogue. ... Arrows indicate the magnitude and direction of the proper motion for the stars. ...

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• Representations of Celestial Coordinates in FITS
• Proposed FITS Keywords and Column Headers for ALEXIS Mission Data Files
• ADASS 2003 Conference Proceedings

Databases (NSDC) of the Natural Planetary Satellites. ... NSDC: Database of astrometric observations of Natural Planetary Satellites . ... They are thoroughly looking for observations in different sources, creating their owndatabases which are then mostly inaccessible to other researchers. ... In the file "content" with explications, the reference is given to the data source as well as the bibliographic reference. ... Data sources. ... Why a specific bibliographic database for Natural satellites? ...

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... For given geographical longitude and time zone show the current data and time, Universal data and time, current local star time. ... Accept 10 different data formats (data&time, data with decimal day of month, data with decimal day of year, decimal year, some Julian dates), calculate from any formate to others, show day of week. Current data and time direct insertion function is exists. ... Calculate angular distance between two points at the sky by its equatorial coordinates. ...

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• Fast search through RTT150 data archive

This document describes changes from the original TCC to version 1.0 of the current TCC. ... The new TCC uses one socket per device (e.g. axis controller or mirror); the old TCC allowed multiple axes to be controlled by one LAT stream. ... The new TCC also communicates with hardware controllers via TCP/IP instead of LAT; this has the potential to reduce the use of terminal servers at APO. ... Set and Show ExpTime . ... Show Database (the new TCC does not use a central repository to store data) . ...

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• TUI:Telescope:User Catalogs
• TUI:Telescope:Offset Types
• M1 Airflow Lab Tests

asncombine -- Process and combine images in one or two NICMOS associations asncombine association . ... set to yes to include error planes in co-added images error. background . ... This is useful to use different background subtractions for different images. fheader . set to yes in order to multiply the background by the value of keyword "factor" in the image header. ... Set to yes to use quadrants statistics save in the image header from previous runs of asncombine. regquad1 . ...

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• Space Telescope-European Coordinating Facility
• ST-ECF Grism Spectrum Software for NICMOS Grism Data

The first persistent Web agent that we have created on Actor Prolog is a program that collects information about research groups that develop Prolog and projects in the field of logic programming. The agent looks through a given list of Web sites and calculates some attributes of the sites: the date of recent modification, total size, the number of figures, the number of outside links, the number of error links, the number of given keywords, etc. ... http://www.cplire.ru/Lab144/space/prolog.html . ...

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• Atmospheric influence on the different radioengineering systems functioning.

Scale-heights of the Galactic disk subsytems with different ages and metallicities . V.Marsakov & Yu. ... It is based on the fact, that all stars cross the disk plane several times during their Galactic orbital period. ... We have used our representative sample of nearby disk F2-G2 stars Marsakov & Shevelev (1995) in which fundamental stellar parameters was determined on the basis of published date on uvby-photometry, proper motion and radial velocities. ... Marsakov V.A., Shevelev Yu.G. Bull. ...

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• Vertical Structure, figures

. Previous slide . Next slide . Back to first slide . View graphic version .

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• Clearing the library. Note the different floor levels. There were at least 4
• The sculpture is accepted
• Things are very different for small planets

... Each day a different image or photograph of our fascinating universe is featured, along with a brief explanation written by a professional astronomer. 2004 April 1 . April Fools Day More Intense On Mars . Image Credit: Mars Exploration Rover Mission , JPL , NASA . Explanation: Today, April 1st, astrophysicists have announced a surprising discovery - April Fools Day is more intense on Mars! ... Happy April Fools day from the editors at APOD! ... About APOD | ...

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• APOD: 2004 March 25 - An Orion of a Different Color
• Zen: tp search en
• APOD: 2011 July 1 - VAR!