... Chapter 4: Solar System Targets > 4.2 Target Identification . ... The following information is required to identify and classify each target. ... For example, separate targets should be defined if you plan to take spectra of several different surface features on a planet, or if you plan to observe the same feature with different timing constraints. ... Description . PLANET . If the target is the center of a planet, enter PLANET followed by its name (e.g., PLANET JUPITER , PLANET SATURN ). ...

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• Stellar Photometry
• Surface Brightness Profiles
• CSPICE Routines: SURFPT_C

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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• VLA 404 compact sources
• First results from follow-up spectroscopy with the NOT
• Procedures to Follow

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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• Naomi McClure-Grffiths

... 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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• Radio sources identfification
• Search for distant radio galaxies in SAO

... Asteroid 23593 images obtained using the Faulkes Telescope North at Haleakala, operated by Las Cumbres Observatory. ... My main project was to search through archive images of the Subaru telescope looking for and identifying asteroids. ... Two of the known asteroids were asteroid 23593 and asteroid 71250. ... The pictures below were taken with the Faulkes telescope and show the asteroid 23593 in its state at 11/08/2015 ten years after I identified it in the Subaru telescope's image archive. ...

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• EVOLUTION MODELS
• Principal Areas of Research
• Armagh Observatory Preprint No. ???

... ATNF Home . ... About ATNF overview . ... Australia Telescope Steering Committee . ... Australian Square Kilometre Array Pathfinder . Murchison Radio-astronomy Observatory . ... Parkes radio telescope . Australia Telescope Compact Array . ... Parkes | ... Visiting Parkes radio telescope . Visiting Australia Telescope Compact Array . ... Parkes radio telescope webcam . ... The follow up 21cm synthesis observations on the galaxies found by this survey are essential for a number of reasons. ...

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• GRAPHICS general subroutines
• Gas follows stars in resonance-ring galaxies
• ATNF Observer's help - what's new/broken/of interest

... 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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... This space is called the torus.) ... Prove that the following spaces are homeomorphic: (a) the set of lines in Rn+1 passing through the origin; (b) the sphere S n with identi ed diametrically opposite points (every pair of diametrically opposite points is identi ed); (c) the disc Dn with diametrically opposite points of the boundary sphere S n-1 = @ Dn identi ed. III.4. ... Prove that S n+m-1 \ S n-1 Rn Ч S m-1 where S n-1 S n+m-1 is standard: S n+m-1 = {(x1 ; : : : ; xn+m ) | ...

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• http://www.mccme.ru/dfc/2008/reports/Chelkak_Report10.pdf
• http://www.mccme.ru/tg2007/talks/Onishchik.pdf
• Conference "Flows on surfaces, symbolic dynamics and dynamics in moduli spaces"

Blackholes2 Forum Message . ... Holostars: Black Holes Without Event Horizons . ... Its name derives from the fact tht information is preserved in such a black hole, and must be a contraction of hologram and star. ... The exterior metrics and fields of the charged holostar are equal to the Reissner-Nordstroem black hole solution. ... 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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• Testing Convex Surfaces. - an Astronomy Net ATM Forum Message
• Telescope Types - an Astronomy Net General Forum Message
• You Followed The Apology With The Same Foolish Insult - an Astronomy Net

Astronomy Picture of the Day . ... 21.10.1999 . ... Credit Copyright: Louis Strous ( LMSAL ), SOHO - MDI Consortium, ESA , NASA Explanation: The Sun rotates on its axis about once every 27 days. ... Just follow the sunspots . ... It shows the Sun's visible surface for most days of August 1999 so that the same sunspots appear many times as the solar rotation carries them across the face of the Sun . ... October 1999 . ... 1999 2000 . ... Publications with keywords: Sun - solar rotation - sunspot . ...

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• Астронет > Follow The Spots
• Spirit Pan from Bonneville Crater s Edge
• Астронет > Spirit Pan from Bonneville Crater s Edge

... We suggest simple method of the selection of distant galaxies based on their radio properties. ... RC0015+0503a , RC0015+0503b , RC0015+0501 , RC0034+0513 , RC0038+0449 , RC0042+0504 . ... RC0105+0501 , RC0110+0500 , RC0117+0503 , RC0126+0502 , RC0133+0459 , RC0135+0450 , RC0137+0539 , RC0143+0505 , RC0152+0453 , RC0154+0459 , RC0159+0448 . ... RC0209+0501b , RC0213+0516 , RC0226+0512 , RC0250+0512 . ... RC0302+0456 , RC0308+0454 , RC0311+0507 , RC0318+0456 , RC0355+0449 . ...

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• Solar Energy
• The Galaxy Gallery Page VII: Infrared Imaging
• Low Surface Brightness Galaxy Gallery

Next: *xexamine* examine Up: *display, xdisplay, xexamine* - Previous: To display other sizes . The following command will display a .qp file in the original detector coordinates. In this case a ROSAT PSPC image is used so it is also blocked to a reasonable size: . xp> xdisplay ``xdata$rp110590.qp[block=30, key=(detx, dety)]'' . ... xp> xdisplay ``xdata$rp110590.qp[block=15, key=(detx, dety)] [1:512,1:512]'' . ...

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• QPOE Files
• Who is tweeting about #AAS225
• zhtools

Download Izmccd (~2.7 MB). Solution of problems at identification of star field. ... 2) Scale is not correct. ... In this case algorithm of identification will revise all values of scale from twice smaller up to twice greater. ... There should be more than value of the field "Number of stars in frame". ... The star field is considered identified if number of the identified stars more or equally to this value. It is necessary to set value from 4 up to value of field "Number of stars in frame". ...

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ARNICA (ARcetri Near Infrared CAmera) is the imaging camera for the near infrared bands between 1.0 and 2.5 m that Arcetri Observatory has designed and built as a general facility for the Tirgo telescope. The scale is 1 arcsec per pixel, with sky coverage of more than 4 arcmin times 4 arcmin on the NICMOS 3 (256 X 256 pixels, 40 m side( detector array. ... Arnica progress report : performance and technical results obtained in the last years at Tirgo , Not , and Vatt . ... Arnica and Longsp data: . ...

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• Relevant Standards - Apache HTTP Server
• Arcetri Star-formation Group Research Topics
• SWXCS

... The package AMPLE (Adaptable Minor Planet Ephemerides) is dedicated to solving a number of problems concerning minor planets with the aid of IBM-type personal computer. ... Obtaining selection of orbital elements and/ or photometric parameters of minor planets in conformity with imposed restrictions. ... The orbital elements of all minor planets used in AMPLE for 2015 have been determined in IAA on the ground of available observations in the catalogue of observations of the Minor Planet Center. ...

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• ENGAMPLE

The database contains references to the papers, data files and links to the Internet resources related to measurements and calculations of the optical constants in the wavelength interval from X-rays to radio domain. ... References to some useful books and reviews on the subject (e.g. the classical handbooks edited by E.D.Palik) and links to Internet collections of optical constants and personal WWW pages with related software were also placed in the database. You have arrived at our welcome page. ...

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• intro3e
• The 2175? feature
• The Stellar Content and Distance to the Nearby Blue Compact Dwarf Galaxy

Day 2 BREAK­OUT GROUPS SUMMARY: Medium Deep: . ... Modes o Trish: Talk to P­ALFA about pulsar modes o Steve: Leapfrog mode (follow same short track for several minutes, then jump back, doing on/offs with stop and stare mode) o Jon: Multi­drift mode (e.g. 25 repeats) . Science: o Mary: HVCs (ultra compact & low surface density) o Kristine: Nearby Galaxies o Jon: Targeted Environments o Jess & Steve: Mass function at different distances (past Virgo) o Erik: Continuum HI Absorption Ultra­Deep: . ...

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• http://www.naic.edu/vscience/schedule/tpfiles/LazarustagP2863tp.ps
• http://www.naic.edu/vscience/schedule/tpfiles/PeektagA2586tp.pdf
• http://www.naic.edu/vscience/schedule/tpfiles/LazarustagP2863tp.pdf

... Content Model: Optional list header (LH), followed by one or more terms (DT) and definitions (DD). A definition list is a list of terms and corresponding definitions. Definition lists are typically formatted with the term on the left with the definition following on the right or on the next line. ... The definition list element can take the COMPACT attribute, which suggests that a compact rendering be used, and is appropriate if the list elements are small and/or the entire list is large. ...

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• Unordered Lists
• The Structure of HTML 3.0 Documents
• List Header

Astronotes Armagh Planetarium's Stellar Blog! ... Stars . ... Space Flight . ... Some 13.7 billion years ago, a mere millionth of a second after the Big Bang, the first hydrogen and helium nuclei condensed out of a hot, dense soup of quarks and gluons. ... In the very last few kilometres some of the light was scattered by a myriad of water droplets (containing hydrogen nuclei which had existed almost since the Big Bang) slowly descending through the air following a rainshower. ...

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