Next: Feed Polarisation Up: Calibration Previous: Calibration Index . RPFITS files do not contain any information as to whether the telescope calibration was in units of Kelvin or Janskys. On reading the data a default value is set depending on the telescope and frequency of observation. ... ASAP>scans = scantable('2004-11-23_1841-P484.rpf', unit='Jy') # Or in two steps ASAP>scans = scantable('2004-11-23_1841-P484.rpf') ASAP>scans.set_fluxunit('Jy') . ...

. 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

... HST . ... Data . ... HST Overview . ... Program Information . ... Post-Observation . ... Retrieving HST Data . ... The page is divided into quadrants: summaries of the observation, the calibration, the image statistics, and OMS (or jitter) data. ... The Observation Summary in the upper left quadrant contains information from keywords which characterize an exposure, such as the proposal ID, instrument, target and its location, grating, observation mode, exposure time, wavelength information, etc. ...

... The task accepts two sources lists: the observation source list and the exposure source list. ... List of selected sources. This le contains a table, called SRCLIST, with the following columns: Name Type Description SRC NUM Integer Source ID from observation source list RA Double RA from exposure source list DEC Double Declination from expoure source list RATE Real Count rate from observation source list COUNTS Real Number of source counts, from exposure source ...

... O.B Slee , Australia Telescope National Facility, CSIRO, Sydney bslee@atnf.csiro.au ----------------------------------------------------- ... ----------------------------------- 1- 8 A8 --- Name IAU name 9 A1 --- nFlag Flagged '*' or '#' 11- 12 I2 h RAh Right Ascension B1950 (hours) 14- 15 I2 min RAm Right Ascension B1950 (minutes) 17- 20 F4.1 s RAs Right Ascension B1950 (seconds) 22 A1 --- DE- Declination B1950 (sign) 23- 24 I2 deg DEd Declination ... Dulk, G.A. Slee, O.B. 1972, Aust. ...

... 1998, ApJ , 503, 467 % Observed energy levels (6,7,8): from the line list of Thomas Neupert, 1994, ApJS, 91, 461 % Observed energy levels (level 9): from the line list of Young, Landi Thomas, 1998, A , 329, 291 % Observed energy levels (level 15): from the line list of Brosius, Davila Thomas, 1998, ApJS, 119, 255 % Observed energy levels (level 37): from the line ...

... This page contains "templates" for PmWiki's (:pagelist:) directive. ... page). (:if false:) [[#default]] (:template first {=$Group}:) :[[{=$Group}/]] /: (:template each:) : :[[{=$Group}/{=$Name}]] [[#defaultend]] (:ifend:) (:pagelist group={$Group} fmt=#default count=6:) . Site / . ... if false:) [[#count]] (:template defaults wrap=inline list=normal :) (:template last:) {$$PageCount} [[#countend]] (:ifend:) Number of pages in the {$Group} group: (:pagelist group={$Group} fmt=#count :). ...

... Things to think about ­ INTMIT, deconvolution Lister Staveley-Smith ­ X-ALFA March 15, 2003 1 HIPASS Bright Galaxy Catalog (BGC) Koribalski et al. ... Arecibo beam Parkes beam HIPASS spectrum HIPASS J0620-57 = ESO161-G001/NGC 2222/NGC 2221 (ATCA observation) Lister Staveley-Smith ­ X-ALFA March 15, 2003 8 The ALFA advantage ­ an example ! Cosmic variance for HIPASS BGC dwarfs #10 Mpc cells Dwarf galaxies Lister Staveley-Smith ­ X-ALFA March 15, 2003 9 Cosmic Variance in HIPASS BGC Zwaan et al. ...

... Tonight's Sky . ... The Magazine . ... Star Atlas . ... An artificial comet holds secrets to Earths life . ... Astronomy for Kids . ... Observing springtime deep-sky objects with a large telescope . ... The planet has extreme temperature swings and perhaps active lava flows. ... A digital supplement to Astronomy magazine. ... Join TravelQuest International with Astronomy and Discover magazines on one of three great tour options surrounding this celestial spectacle . ... Astronomy Magazine . ...

... The scheduling routines assist in creating an observing list (stored in the startable) from scratch or from another list stored on disk, and computing the visibility of the stars in a specific night and array configuration. The date of observation is taken from the variable date , and the array name from the variable systemid . If these are not defined, defaults are used for date (the next night) and for array (NPOI). ... addstar , stars _char Add one or more stars to the startable. ...

The AstroGuide . ... AstroGuide Listing . ... See many more Astronomy Listings by: Category or Alphabet . The observatory consists of a dome containing a 17" f/15 classical Cassegrain reflector, a roll-off roof building containing a 12.5" f/6.5 Newtonian reflector, a classroom building with a darkroom, and two other buildings. ... Web Site . http://www.astrohbg.org/naylor_observatory.php . ... Unless otherwise specified, web site content Copyright 1994-2016 John Huggins All Rights Reserved . ...

In this gallery are many images of Low Surface Brightness Galaxies which have recently been discovered and analyzed. ... The central surface brightness of this galaxy is 24.28 . Malin 2 This galaxy is another huge disk galaxy with a scale length of 15 kpc and a redshift of 15000 km/a. The high surface brightness knot in one of its spiral arms actually has the same color, luminosity and H-alpha equivalent width as the entire Large Magellanic Cloud . ... Truly it is a Low Surface Brightness Galaxy. ...

This diagram illustrates the fact that the list marker box has no impact on the position of the principal list box. ... For the upper list, the list marker box (which contains a bullet) is outside and to the left of each list item principal box. For the lower list, the list marker box (which contains a bullet) is the first inline box inside each list item principal box. ... A label reads, "The left sides of the list item boxes are not affected by marker placement." ...

True Color Image Gallery: Galactic SNR | ... Data for each remnant are organized into the sections listed below. ... Chandra Counts and Fluxes: are given in 3 energy ranges. ... Other images are in narrow bands selected to illustrate the spectral morphology of that particular remnant and differ from remnant to remnant. Any image can be downloaded in GIF, PS, or FITS format. ... Survey Missions: Depending on the remnant; shows IR, visual and radio images. ... Chandra Supernova Remnant Catalog . ...

... SphericalTexturedPolygon Member List . ... AllSky enum value (defined in SphericalRegion ) . ... contains (const Vec3d &p) const (defined in SphericalPolygon ) . ... inline, virtual] . ... getIntersection (const SphericalPolygon &r) const (defined in SphericalRegion ) . ... getSubtraction (const SphericalPolygon &r) const (defined in SphericalRegion ) . ... getUnion (const SphericalPolygon &r) const (defined in SphericalRegion ) . ... setContour (const QVector< TextureVertex > &contour) . ...

. To run a command from the history list use a command from this table. To... Do this... Move up through the command history list ^P one command at a time. Move down through the command history list ^N one command at a time. Run the previous command. !! Run command number n ! n Run most recent command starting with ! string characters in string Run most recent command containing !? string characters that match string . Examples .

THE 75th NAME-LIST OF VARIABLE STARS. ... The 75th Name-List consists of two tables. ... the literature, taken from positional catalogues, including USNO A1.0/A2.0 and GSC, or determined by the authors); the range of variability (sometimes the column Min gives, in parentheses, the amplitude of light variation; the symbol ( means that the star , in minimum light, becomes fainter, than the magnitude indicated); and the system of magnitudes used ( P are photographic ...

Dr. Victoria I. Prokhorenko . ... Situation Analysis of The "PROGNOZ" Orbit for Solar- Terrestrial Space Experiments. ... Studies of Satellite Situations Mission. ... A Situation Analysis of the Orbits of the Tail and Auroral Probes in the "INTERBALL" Project. ... Specific Tasks of Multiple Scale Plasma Measurement in Regatta- Cluster System (co-authors S. Savin and L. Zelenyi)- In Book: Proceedings of an International Workshop on Space Plasma Physics Investigations by Cluster and Regatta. ...

List of publications . ... Moscow University Press. 160 pp. ... Shevchenko V.V. A Lunar Base. Moscow. ... Shevchenko V.V., Chikmachev V.I. Lunar Base - a Project of XXI Century. ... Shevchenko V.V., Pugacheva S.G., Dehktereva K.I. Brightness Characteristics of the Infrared and Visible Radiation of the Lunar Surface. ... Problems of Complex Research of the Moon. ... Solar System Research. ... Baydal G.M., Sizentzev G.A., Sotnikov B.I., Shevchenko V.V. Lunar Base Infrastructure and Lunar Resources. ...

... 1) Our CAS system will store the catalogues. ... Each catalogue should contain one or more tables. 2) The names of the catalogues should be unique, as well as the the names of tables of the SAME catalogue. ... 4) All the metadata about the CAS system, its tables, catalogues should reside in separate schema (currently "cas_metadata"). 1) The main system table of CAS is the table "catalog_list". ... short info (column "info") . ... 2) The second system table of CAS is the table "table_list". ...