... The schedule after July 31 is tentative. Please send comments and corrections to efomalon@nrao.edu FRQ codes are L (1.6 GHz ), C (5.0 GHz ), K (22 GHz ) and B (1.6/5.0 GHz ) VLBA W062a2 PIC-A C Pent 301 Th:Oct-28 16:40 - 18:45 S2 Percentage of time 7.8 HALCA Observations for WB = WESTERBORK EXPNO SOURCE FRQ Corr DOY DY: DATE UT RANGE Record/copy W018f J1335+45 L Socr 148 Fr:May-28 16:00 - 02:50 VLBA W027b1 J1927 +73 L Socr 149 Sa:May-29 20:35 - 08:35 ...

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• In-Orbit Checkout/GOT Schedule

... Proposing for VLBI Time at Arecibo . ... Documentation (Field System, VLBA4 terminal, Mark 5 system) . ... In 2001, the Arecibo Observatory received its hybrid VLBA-MARK IV (VLBA4) data acquisition system, and currently NAIC commits Arecibo to support VLBI observing up to a maximum of 4% of the 305-m's observing time. ... Tracking Time (h:mm) . ... The inclusion of the 305-m Arecibo radio telescope can dramatically boost the sensitivity of VLBI observations, even with its limited source tracking...

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• WAPP - Snap Page
• ON/OFF (Position Switching)
• AstroWeb: Astronomy/Astrophysics on the Internet

Adaptive Resource Modelling for Autonomous Planning & Scheduling Andrew Carrel, Phil Palmer Surrey Space Centre, University of Surrey, UK 5th International Workshop on Planning and Scheduling for Space Baltimore, 24th October 2006 Contents Resources types in operations planning. The NEAT planner/scheduler. ... Neural network resource modelling. ... Adaptive Resource Modelling 2 IW PSS, October 2006 Planning with Resources User goals achieved by operations. ... NEAT manages resources effectively. ...

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• Spike for FUSE
• Spike for HST
• WFPC2 STAN

... Up: Description of program searchdup Previous: Program use . Input records are ordered per date of observation, and the list of known (observed) sources is cleared. Each record is compared in position to all the known sources. If the sky distance is less or equal to the specified one, the record is added to the list of observations for that source. If no known sources are within the specified radius, a new source is created, with the coordinates of the observation record. ...

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• Program parameters
• Radioastronomy reduction procedures
• Description of program searchdup

... 389Voges+ IX/29 ROSAT All-Sky Survey Faint Source Catalog (Voges+ 2000) ============================================================================= ROSAT All-Sky Survey Faint source Catalogue (RASS-FSC) Voges W., Aschenbach B., Boller Th., ... The sources have a detection likelihood of at least 7 and contain at least 6 source photons. ... 0 Extraction radius 141-146 A6 --- PrioFlags [01] priority flags (8) 147 A1 --- PHA [ABCDb] PHA range of best detection (9) 149-152 F4.2 --- VigFactor ?= ...

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• Variable radio sources
• Source Positions
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... LABORATORY OF RADIO ASTRONOMICAL OBSERVATIONS . Radio sources identification is one of the most important tasks of the current radio astrophysics. ... Optical idetification. ... Optical identifications of subsample of steep spectra radio sources from RC catalog using 6m SAO telescope of SAO RAS: optical observations. ... Astronomy Reports. ... Identification of radio sources with data of various radio catalogs allows one to construct continual spectrum of the object and its radio structure. ...

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• di_eks
• Observational data
• Instrumentation

... Each day a different image or photograph of our fascinating universe is featured, along with a brief explanation written by a professional astronomer. 2002 October 5 . X-Ray Cygnus A . ... Central in both pictures, the center of Cygnus A shines brightly while emission extends 300,000 light-years to either side along the same axis. Near light speed jets of atomic particles produced by a massive central black hole are believed to cause the emission. ... About APOD | ... NASA Technical Rep.: ...

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• APOD: October 1, 1996 - BATSE's Biggest Gamma Ray Burst (Yet)
• Open Source Convention
• APOD: 2000 October 6 - X-Rays From Sirius B

... News Latest News News Archive Newsletter Quarterly Status Report . ... Data Analysis SAS News What is SAS? ... Calibration & Background Calibration Background Analysis . ... Back to Background Analysis Page . The XMM-Newton Extended Source Analysis Software package (XMM-ESAS) is developed at the NASA/GSFC XMM-Newton Guest Observer Facility (GOF) in cooperation with the XMM-Newton SOC and the Background Working Group. ... http://xmm.esac.esa.int/sas/current/doc/esas/index.html . ...

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• Correction of non-point-source time series:
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home education > resources . SEARCH ASP SITE: Match ALL words Match ANY word . ... Astronomy Education Bibliography . ... Astronomical Pseudo-Science . ... Astronomy of Many Cultures Resource Guide . ... Black Holes: An Introductory Resource List . ... Astronomy Education Review . Space Science Education Resource Directory . ... This is a selected list of resources for those who want to examine with a skeptical eye some of the claims at the fringes of science that seem connected to astronomy. ...

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• ASP: Astronomical Pseudo-Science: A Skeptic's Resource List
• ASP: The Astronomy of Many Cultures: A Resource Guide
• ASP: Multicultural Astronomy: The Astronomy of Non-western Cultures: A Resource

This Directory contains mean hourly, mean daily and mean monthly values of cosmic ray intensity recorded by World Network NM stations to the end of 2011. ... CD is created in WDC for STP, Moscow and IZMIRAN. ... This directiry contains catalogue Corrected for pressure and verificated data in WDC for STP, Moscow . This directiry contains catalogue Corrected only for pressure but Original data in WDC for STP, Moscow . ... 20 May - 22 July 1972, M., 1975 6. 27 March - 22 July 1972, M., 1975 7. ...

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... ESO Science Newsletter October 2015 . 08 Oct 2015 . ... This newsletter is a summary of recent ESO Science Announcement items. Follow the links or visit ESO Science Announcements to read more. ... A detailed report on the outcome of the ALMA Early Science Cycle 3 Proposal Review Process is available . ... Read more . ... 17 Sep 2015: . ... Science Operations 2015: Science Data Management . ... You are receiving this newsletter because you subscribed to the ESO Science Newsletter. ...

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• The Cross-correlations
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• Sample Identification

lsst.tcc љ 1.2.2-3-g89ecb63 . ... Files . ... include . ... telMod.h . ... 6 љ #include <string> . ... 24 љ explicit TelMod (std::string const &filePath) { . ... 86 љ void loadPath (std::string const &filePath); . ... 112 љ std::vector<std::string> getTermNames () const ; . ... 145 љ std::ostream & operator<< (std::ostream &os, TelMod const &telMod); . ... double getTerm(std::string const &termName) const . ... std::vector< std::string > getTermNames() const . ... TelMod(std::string const &filePath) . ...

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• lsst.tcc: python/tcc/cmd/offset.py Source File
• lsst.tcc: python/tcc/mov/checkPos.py Source File
• lsst.tcc: python/tcc/util/runningStats.py Source File

... 00001 /* Example code for FITS-based optical interferometry exchange format 00002 00003 $Id: exchange.h ,v 1.6 2003/04/07 10:20:28 jsy1001 Exp $ 00004 Definitions of data structures, function prototypes 00005 00006 00007 Release 5 7 ... structures */ 00017 /* NB must allow for final null when dimensioning character arrays */ 00018 00020 typedef struct _element { 00021 char tel_name [17]; 00022 char sta_name [17]; 00023 int sta_index ; 00024 float diameter ; 00025 ...

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• G332.4-0.4
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... 2005: . ... Orbital period of an X-ray transient source in the system CI Cam. For the first time, the orbital motion of a compact component of the X-ray transient CI Cam has been found, the orbital period (19.41 days) and eccentricity (0.62) have been determined, masses of stars of the system have been estimated. The compact component of the system is most likely to be a white dwarf. Archive . ...

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• Ratan-600 observation schedule
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• Solar system sector, archive 2010

Magnetic field measurements onboard the Interball Tail spacecraft are carried out by the FM-3I instrument which consists of two flux-gate magnetometers covering two different ranges: [-200, +200] nT and [-1000, +1000] nT. Besides scientific goals, the FM-3I experiment data is used to perform the attitude control of the Interball Tail spacecraft. ... August 22, 1995 . ... October 18, 1995 . Top of the page . ... Back to the Interball Home Page . ...

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• ULF waves [Oulu]
• Pi B [Oulu]
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The Texas survey of radio sources covering -35.5{deg} < {delta} < 71.5{deg} at 365MHz . ... We present the Texas Survey of discrete radio sources between -35.5deg and 71.5deg declination (B1950), which was carried out at 365MHz with the Texas Interferometer during 1974-1983. ... The Texas Survey . ... The sources in the simpler model. ... Right Ascension 1950 . ... field separator . ... Some sources came from Version 6 of the Texas Survey ('TS6' in strp field) or Version 7 ('TS7' in strp field) . ...

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• RadioAstron Announcement of Opportunity - 1, english version
• Description of the RadioAstron project, english version
• RSOG Pre-Observation Products

... Previous: Filtering KPNO LaTeX Observing Proposals with Perl . ... The Planning and Scheduling Tool was designed allow the user easily to take advantage of all available resources of the four telescopes (LASCO's three coronagraphs and the EIT Telescope) to maximize the use of the telemetry downlink. The Planning Tool allows users to develop customized observing sequences while monitoring compression factors and on-board processing times to realistically work within the limits of the instruments. ...

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• An Extragalactic Point Source Simulator for SIRTF Pipeline Testing
• A New PROS Task for Calculating HRI Source Intensities or Upper Limits
• QPSIM: An IRAF/PROS Tool for Source Simulation

... Amazingly detailed, this false-color x-ray image is centered on the galaxy Cygnus A. Recorded by the orbiting Chandra Observatory, Cygnus A is seen here as a spectacular high energy x-ray source. But it is actually more famous at the low energy end of the electromagnetic spectrum as one of the brightest celestial radio sources. ... With brilliant Venus above the western horizon at sunset and Jupiter and Saturn high in the east by early evening, November's night sky is filled with bright planets. ...

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... The stars examined here were primarily culled from two lists of X--ray sources in Orion. ... The second region is two degrees in extent east--west and ten degrees north--south with Orionis being near the northern edge. ... In the end, two main regions were chosen for monitoring: stars near Orionis and stars northwest of the belt of Orion. ... The PSPC identified 22 sources within 15 of Orionis in addition to the sources listed in Table 1 , giving a total of 85 X--ray sources in the Orionis region. ...

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• Photometry
• ChASeM33 Source Catalog
• *qpsim* - Generate Simulated Event List

... Articles | ... Forums . ... 230 deg . 49 deg . ... 130 deg . ... More Info . ... 210 deg . ... 168 deg . ... 249 deg . ... 195 deg . ... 271 deg . ... 110 deg . ... 338 deg . ... July 15 . 247 deg . ... 224 deg . ... 340 deg . ... July Phoenicids (PHE) . ... August 10 . 341 deg . ... 339 deg . ... 307 deg . ... 334 deg . ... 335 deg . ... 286 deg . ... 327 deg . ... 262 deg . ... 102 deg . ... 153 deg . ... 117 deg . ... December 2 . ... 123 deg . ... 100 deg . ... www.astronomy.net . ...

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• For The Record - an Astronomy Net Exploration Forum Message
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• NASA-MSU Center for Educational Resources, CERES, AstroGuide Listing