S. Kumar University of North Carolina Chapel Hill, United States shrawan@email.unc.edu Descent of line bundles to GIT quotients of flag varieties Let G be a connected semisimple complex algebraic group with a maximal torus T and let P be a parabolic subgroup containg T . ... The following theorem is our main result. Theorem. Let L() be a homogeneous ample line bundle on the flag variety X = G/P . ... h) G of type E7 : 12P i) G of type E8 : 60Q. -2 -2 +n -1 -1 + n , ni Z 1 ...

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• http://www.mccme.ru/tg2007/talks/Kac.pdf

... The European HST Archive has been moved to ESA's European Space Astronomy Centre ( ESAC ), Spain, where most of ESA's Space Science Archives are located and operated from. ... The Space Telescope European Coordinating Facility (ST-ECF), jointly operated by ESA and the European Southern Observatory ( ESO ) was, until the end of 2010, the European HST science facility, supporting the European astronomy community in exploiting the research opportunities provided by the Hubble Space Telescope. ...

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Radio data are displayed in the following format: . After the title with name of cluster under examination and with line about kind of data under one, e.g. Radio data [ optical data ] [ radio source identifications ] [ radio spectra (1.0 or 1.1) ] . ... The first line contains the number of radio sources associated with the cluster (these are just those sources with entries in sections 'Radio galaxy', 'Radio source' and 'Radio spectrum' below). ... Radio sources in cluster: 2 # . ...

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• Emission-line galaxies
• Relevant Standards - Apache HTTP Server
• Values, Variables, and Literals

... The orbits as follows are considered: INTERBALL Tail Probe (IB_TAIL) & Auroral Probe (IB_AUR), GEOTAIL (NASA/ISAS), and POLAR (NASA). ... The situation investigation aim is to select the following favourable spatial positions (FSP) : . ... FSP3 : That part of the FSP1 & FSP2 time intervals, which corresponds to the magnetic conjugations of the any couple of the considered spacecraft. ... The polar diagram plot . ... The geocentric distance (GCD) of the 4 spacecraft as a function of the time. ...

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• The TAIL 1996/1997 campaign
• INTERBALL IB_TAIL landing point coordinates
• Submission of questions

... Character codes are given in hexadecimal when available for the Postscript symbol set and HP's math -8 symbol set. ldots; \ldots three dots on the baseline cdots; \cdots three dots on same level as a minus sign vdots; \vdots three vertical dots ddots; \ddots diagonal dots (top left to bottom right) dotfill; \dotfill like cdots but fills column in an array thinsp; \, thin space sp; \: medium space emsp; \; thick ...

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• Definition Lists
• Character Entity Set(s)
• Sorting on a specific part of a field

Program: HELP Purpose: Display purpose lines or categories or complete documentation of tasks (subroutines and general items). ... SUBJECT=4: DOCUMENT= Give name of doc. to print: [return to menu] Send this document to a printer selected with PRINTER= The '*' character can be used as a wildcard, f.i. DOCUMENT=*gauss* prints all documents with 'gauss' in its name. ... For the subjects 4 and 5 (print documentation and purpose lines from documentation) a document name is wanted. ...

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• Language Extensions
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TUI supports the following offsets: . Object Arc offset by a given amount on the sky (i.e. along the arc of a great circle). ... Arc offsets are useful for moving a different portion of your object or a different nearby object onto the boresight . ... Object Arc XY this is identical to an Object offset except that it has been rotated to align along the instrument x-y axes. ... This is just like the Calibration XY offset, except that it is typically cleared when you slew to a new object. ...

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• MCP Menu documentation
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These observations are aimed at fully charactering FORS1 photometric system (UBVRI zero-points, color-terms and extinction coefficients) for the Tektronix 2048x2048 pixel CCD (24µm px) . To this aim, the two Landolt/Stetson photometric fields SA95 and SA101 will be observed on a number of epochs and at different airmasses during February and March 2007. ... SA101 . ... OBs for SA101 have to be observed during evenigh twilight (exceptions are expected for the second half of March) . ...

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• DFS Department internal procedure for issue of documentation
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• the Technical Archive procedure for issue of documentation

... solar system . ... Solar eclipse travelogue: Sulawesi delivers a spectacular eclipse . ... Observe the Solar System . ... Tour the Solar System . ... Do the paths of totality during solar eclipses follow a pattern that repeats after a certain period? ... RELATED TOPICS: SOLAR ECLIPSE . Total eclipses follow a period known as the saros, which is 18 years and 11 1/3 days long. ... Get instant access to subscriber content on Astronomy.com! ... Join Astronomy for America's 2017 total solar eclipse! ...

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• Surprise recovery of meteorites follow asteroid impact | Astronomy.com

... Circles are used to depict the source positions. ... A optional ID label can also be displayed alongside the circle, corresponding to the row num- ber of that source in the input source list. ... These circles are in fact DS9-type regions, which can be written out to a le for future use (for example, when running a later DS9 session) by setting withregionfile to true, and specifying the desired le name via the regionfile parameter. ... This is a text le containing region descriptions for each source...

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• Input Files
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There are six possible ways of object description: . a) by number(s) . ... d) by list . e) by orbital elements . ... They should be introduced as year, month, day with tenth (e.g. 20021104.1). d) Computations are performed for all objects listed in the file whose path and name should be introduced into assigned data field. ... On pressing Edit file button user has a possibility to look through the list of object elements or their coordinates and velocities to add or to change it. ...

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• Conference WPLTN-2012 | Conference page
• Statistics of diacritical characters in Minor Planets Names

... This function can also be used for particular types of subtypes or kinds: KIND (0) integer KIND (0.0) floating point number KIND (.FALSE.) logical variable KIND ("A") string of characters There is an intrinsic function SELECTED_REAL_KIND , which returns the kind of the type REAL that has a representation with (at least) the precision and the exponential range requested. ... With the choice SELECTED_INT_KIND (5) all integers between (but not including the limits) -100 000 and +100 000 are permitted. ...

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• ASA Carriage Control Characters
• Notation
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... Apache HTTP Server Version 2.4 . Apache > HTTP Server > Documentation > Version 2.4 > Miscellaneous Documentation . ... This page documents all the relevant standards that the Apache HTTP Server follows, along with brief descriptions. ... http://www.rfc-editor.org/errata.php - RFC Errata . ... This document summarizes the history of HTML development, and defines the "text/html" MIME type by pointing to the relevant W3C recommendations. ... HTML documents are SGML documents. ...

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• Using Apache With RPM Based Systems (Redhat / CentOS / Fedora) - Apache HTTP
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Zodiacal Light Panorama . ... Credit Copyright: Miloslav Druckm ller (UM FSI, Brno Univ. of Technology ), Shadia Habbal ( IfA, Univ. of Hawaii ) Explanation: Sweeping from the eastern to western horizon, this 360 degree panorama follows the band of zodiacal light along the solar system's ecliptic plane . ... In the mosaic projection, the plane of our Milky Way Galaxy runs at an angle , crossing the horizontal band of zodiacal light above the two horizons. ... NASA Official: Jay Norris. ...

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• Zodiacal Light Panorama
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... At 22:42:27 UT 26/07/09, the Burst Alert Telescope (BAT) on board of the SWIFT multi-wavelength space observatory triggered and located GRB 090726 gamma-ray burst event. ... About half an hour after the BAT trigger, the first images were obtained with the SAO RAS Zeiss-1000 telescope in four BVRI filters (see Fig.1). ... The spectrum of the optical transient was obtained with the SAO RAS 6-m BTA telescope 1.54 hours after the burst, using the SCORPIO instrument in the spectroscopic mode (Fig.2). ...

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... The following coordinates may be useful, but please contact us for up-to-date details if you plan supporting observations of this field. 22h 32m 56.22s -60d 33' 02.69" J2000 Equinox Note: PA_V3 = 230.5D, which corresponds to U3 ORIENT=50.5D. 22h 33m 37.67s -60d 33' 28.95" J2000 Equinox The position of the QSO has been determined with estimated errors less than 40 milli-arcseconds to be: 22h 33m 37.5883s -60d 33' 29.128" J2000 Equinox . ... Visit the Hubble Deep Field South main page . ...

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• Notation and Model
• CSPICE Routines: REPMOT_C
• Beginner's IDL - Line Plots

... In the above example, the second region uses the global coordinate system (PHYSICAL by default). ... Supported systems include: name description ---- ----------- PHYSICAL pixel coords of original file using LTM/LTV IMAGE pixel coords of current file FK4, B1950 sky coordinate systems FK5, J2000 sky coordinate systems GALACTIC sky coordinate systems ECLIPTIC sky coordinate systems ICRS currently same as J2000 LINEAR linear wcs as defined in file In addition, two mosaic coordinate ...

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• *display, xdisplay* -- Displaying an image in detector coordinates
• Image with sky grid overlaid
• *imcnts* - Use of the Sky Coordinate System

... This program was created for correlating chosen regions in the series of fts images. ... Chosen regions' . ... In this section the program counts the integral for each region of the grid for each image. ... As a matter of fact, the integral is total brightness of the region and it is counted by 'int_tabulated' IDL function. ... In addition, the program will show the count of the regions which correlate with the corresponding region (the brighter region means the bigger count) and its contour. ...

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• Data bases of Natural Satellites. Documentation. Manual
• jg0025

Follow-up astrometry and recoveries are made with the ANU 40 inch (1.0-m) f/8 reflector at Siding Spring Observatory (IAU code 413). ... A routine follow-up of 2003 WY153 on 2003 Dec 15 became much more than routine when a faint object with unusual motion vector was found close to the target asteroid. ... During routine astrometry with the 1.0-m to improve the orbit of the Apollo asteroid 2004 CB, the asteroid was found on March 30 to have a short tail! ... Siding Spring Survey Main Page . ...

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• Observational Techniques: Units and Coordinates Notes
• Naomi McClure-Grffiths

... Sfit . ... In addition, the variety of possible forms in which observed spectra might be presented (LORES normalised, HIRES fluxed, OPTICAL, ULTRAVIOLET), it is demanding to ensure every mode is operational at once. ... SLV . CHISQ . LORES . ... AMOEBA . ... GENETIC . ... HIRES . ... FLX . ...

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• Armagh Observatory
• Follow up from the Second Cross-Border Schools Science Conference |
• The Faulkes Telescope follow-up of archive image asteroids