... Advises . Contact Advises . As an advise for amateurs we would like to underline: if it's possible, try to observe 3 asteroid positions per night and do not neglect to observe the Numbered Minor Planets in your telescope field of view as a "by product" of your observational programs. ... We think such estimations ought to be produced every morning after CCD observations of the moving celestial objects by observer himself. ...

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... 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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• A matrix of tweets from #AAS221
• A quick look at tweets from the #AAS221

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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• ENGAMPLE

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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• A visual tour
• VLTI Calibrator Selection Help Page

Alfa_ang is a GUI for the rotang routine. The purpose of this routine is to calculate the optimum rotation angle for ALFA given the RA and Dec of a source and the date and time of the observation. The routine also returns the azimuth and zenith angle of the telescope at the requested time, thus it can be used to find the correct rotation angle and azimuth for the Fixed Azimuth Drift Scan observing mode used by the AGES drift precursor observation. ... To run alfa_ang at Arecibo: . ...

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• ATOMS by Number
• AGES drift Observer's Log
• Spectral-Line Observing

... HST . ... Home . ... Data . ... HST Peer Review Process . ... WFPC2 Home . ... Instrument Home . WFPC2 History . ... Calibration . Calibration Home . Calibration Plan . ... Data Analysis . Data Analysis Home . Data Analysis Library . ... Bug in Pipeline Reduction of some Single-chip WFPC2 Images . Impact of November Safing Event on Repeats of Failed Observations . ... A bug has just been discovered in the pipeline calibration software for a small fraction of WFPC2 images. ...

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• Apertures
• HST Call for Proposals
• Phase I Target Naming Conventions

... POSITION= Give central position: [0,0] ANGLE= Give angle (deg), w.r.t North towards the East: GRIDOUT= New grid spacing of [spacing in longitude] rotated axis: POINTS= Give number of pixels on rotated axis: [Number of pixels on longitude axis] SLICES= Number of slices above and below slice [0,0] through new projection centre. Total number of slices cannot exceed 256. SPACE= Spacing between slices: [grid spacing in latitude] OUTSET= Give output set: PLOT= Create plot of slice? ...

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• VSOP Observing Schedule
• VSOP Long-Term Schedule
• Release of 22 Feb 1996

... The described algorithm is suitable for measurements of complex images of stars. ... a) the zero-based number of stars in the complex (multicentric) image, . b) set of preliminary coordinates - x i , y i , for all stars, index i is number of a star, . ... i - index of a star in the complex image; . ... These parameters are calculated by a nonlinear method of a least squares.The main output parameters of this algorithm are x i , y i ; where the index i is number of a star in the multicentric image. ...

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January - June 2010 . ... Number theory seminar . ... There is a weekly number theory seminar taking place on Thursdays at the Independent Universty of Moscow (11, Bolshoi Vlassievsky pereulok), room 308. ... Thursday 20 May 2010 . 18:00-19:30 . ... p-adic representations of Gal(\bar{Q_p}/Q_p) III . ... p-adic representations of Gal(\bar{Q_p}/Q_p) II . ... S. Rybakov (Poncelet Laboratory) . Representations of Gal(\bar{Q_p}/Q_p) in GL_n(\bar{F_p}) . ... Thursday 1 April 2010 2010 . ...

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• Labo J.-V.Poncelet: Dmitry R. Lebedev
• Young researchers' seminar in statistical physics
• Conference "Combinatorial Methods in Physics and Knot Theory" (February 2005)

XMM-Newton Science Analysis System Page: 1 omregion November 22, 2004 Abstract Calculates evselect region les for an OM source 1 Instruments/Modes Instrument Mode OM FAST 2 Use pipeline processing yes interactive analysis yes 3 Description This task takes an OM OSW source list and a source number and produces evselect region les for the source and its associated background. ... Intermediate source region le for use by evselect 2. ...

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• http://xmm.vilspa.esa.es/sas/6.1.0/doc/regionstats.ps.gz
• http://xmm.vilspa.esa.es/sas/6.1.0/doc/eregionanalyse.ps.gz
• http://xmm.vilspa.esa.es/sas/6.1.0/doc/omsrclistcomb.ps.gz

... Time calculated from Fermi GBM Trigger Time = 14:12:08.67 ( Connaughton, GCN 9230 ). 1% coincident with our start zero image time. 3x3 degrees around Swift XRT position . ... SUBJECT: GRB 090424 : MASTER-Net prompt optical limit DATE: 09/04/25 20:29:42 GMT FROM: Vladimir Lipunov at Moscow State U/Krylov Obs E. Gorbovskoy, V. Lipunov, V.Kornilov, A.Belinski ... Our observations results: ---------------------------------------------------------------------- Fermi GRB Trigg.* ...

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... Images obtained using the Faulkes Telescope South, operated by Las Cumbres Observatory. ... The Faulkes Telescope Project and Las Cumbres Observatory Global Telescope Network had kindly given us the opportunity to use these telescopes and the observatory had booked us four sessions of controlling the telescope in order for us to make some observations on NEOs. ... Just before our first observing session on Friday, we were given a tour of the observatory building and its telescopes, by John McFarland...

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• Public Events Organised by Armagh Observatory September to November 2002
• Latest News
• Weather November 2008

Next: Program use Up: Description of program searchdup Previous: Description of program searchdup . Parameter input is done with a graphic user interface. ... Input file: Name of the input catalog file. It has to be formatted, one record per source/observation, according to the format used in the Arcetri observations and source archives. ... Minimum number of observations per source Source with less than this number of independent observations are not included in the output file . ...

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• Conference registration - IGM@50: Is the Intergalactic Medium driving Star
• Next VLT Instrument Ready for the Astronomers (PR Photos 05a-c/00)

ARCSAT ID NUMBER: AS04 DESCRIPTIVE TITLE: Stellar Environments of the Nearest Red Dwarfs PI: Michele Silverstein (GSU) OBSERVER(S): Michele Silverstein (GSU), Todd Henry (GSU) and Tiffany Pewett (GSU) UNCERTIFIED/UNTRAINED OBSERVERS: COLLABORATORS: Wei-Chun Jao (GSU) and Jen Winters (GSU) CONTACT INFORMATION: (PI/OBSERVER email/phone) silverstein@astro.gsu.edu (404-413-6024), thenry@astro.gsu.edu (404-413-6054) TIME REQUESTED: 1. NOVEMBER 10 - NOVEMBER 16 2. ...

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• Procedure for Part Numbering Convention: Larry Carey, 2005
• Plug-plate coordinate system
• Guider Mechanical Commands

... This is a preliminary summary of the event on November 24, 1996, considered during the INTERBALL Workshop in Kiljavanranta, Finland, February 1998. ... Pronounced plasma sheet thinning (Bz decrease) . ... Particle burst observed inside the Polar Cap and in tail lobes . A short burst of particles detected by the Auroral Probe particle detectors during the Polar Cap crossing at 21:45 UT, almost simultaneously with the Tail Probe detectors registration of the particle burst inside the North Lobe. ...

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• STDA files
• Interball Workshop Programme
• Satellite position in the SE and GSM coordinate systems

New reduction of minor planets photographic plates obtained with Pulkovo Normal Astrograph A.A. Berezhnoy Pulkovo Observatory of RAS, Saint-Petersburg, Russia Minor Planet observations at Pulkovo Periodical observations of 14 bright asteroids named Selected Minor Planets (SMP) were performed at Pulkovo since 1948 within the international framework started by works of B.V. Numerov and D. Brouwer. ... 108 133 113 74 124 67 97 88 14 84 64 5 20 19 Epochs (YYYY.MM) 1200 Mean values of total obs. ...

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• http://www.puldb.ru/laza_gao/PUB/iau248_1.pdf
• Pulkovo Database of Observations of Visual Double Stars

... 2005 November 3 . Possible Pluto Moons . Credit : H. Weaver ( JHU / APL ), A. Stern ( SwRI ), and the HST Pluto Companion Search Team , ESA , NASA . ... This year, the Hubble Space Telescope may well have detected two further members of the Pluto system . Provisionally designated S/2005 P1 and S/2005 P2, the two potential new moons are seen orbiting in a counterclockwise direction about 44,000 kilometers (27,000 miles) from Pluto in these deep Hubble images recorded only three days apart. ...

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• APOD: 2004 November 14 - Leonids Above Torre de la Guaita
• APOD: 2014 November 16 - Leonids Above Torre de la Guaita
• APOD: 2000 November 26 - Leonids Above Torre de la Guaita

... Estimation of source coordinate time series from analysis of VLBI sessions. ... Conventions Cut-off elevation angle: 5є Terrestrial datum: NNR/NNT constraints to VTRF2008 stations without breaks (in total) For the sources : T L(2011) NNR Yes No s [ mas ] 2000 2000 Dip. ampl. [ mas /yr] 6.4 ±1.5 6.5 ±1.5 a (є) 263 ±11 263 ±11 d (є) -20 ±12 -23 ±12 Constraining each source to the ICRF2 position using very loose constraints (s=2as) is equivalent to apply loose NNR ...

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• Pulkovo NEO Page: Estimation of Accuracy of the Observations
• Pulkovo NEO Page: Ephemeris Support
• Catalogue of double stars

... Sun images . ... Active areas . February : 2016 . ... The following regions with sunspots can be now observed on the Sun's surface . Group number . ... Group length (in degrees) . ... Beta . ... Coordinates and other characteristics of active regions are issued for February 09, 2016 00:31 UT The following H-alpha plages without spots can be currently observed on the Sun's surface . ... Coordinates and other characteristics of active regions are issued for February 09, 2016 00:31 UT . ...

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• Sunspots and active regions February 10, 2010
• Sunspots and active regions February 10, 2014
• Sunspots and active regions February 01, 2013

Natural Satellites Service. ... Apparent Encounters . of the Tycho-2 Catalogue stars and the main natural planetary satellites . ... Suggestions . ... Here we present the precalculated circumstances of the apparent encounters of the stars of the Tycho-2 Catalogue with the main satellites of Saturn (S1-S8) for the period from November 2004 to February 2010, and with the Galilean satellites of Jupiter for the period from November 2004 to October 2010. ...

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• jg0026
• jo0053
• jg0036