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. " The Arecibo Observatory is sponsored by the National Science Foundation. Any opinions, findings and conclusions or recommendations . expressed in this publication are those of the author(s) and do not necessarily reflect the views of the National Science Foundation."

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• The AO Optical Laboratories National Astronomy and Ionosphere Center (Arecibo

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... Us . ... Data . ... Retrieving HST Data . ... In order for FOS to have observed a target, that target must, naturally, have been located in the instrument aperture. ... An FOS Onboard target acquisition: Used either a Binary Acquisition (ACQ/BINARY), a Peakup or Peakdown (ACQ/PEAK), an interactive acquisition (INT ACQ), an early FOS Image (ACQ) or a firmware acquisitions (ACQ/FIRMWARE). ... The overwhelming majority of FOS target acquisitions used the onboard acquisition modes ACQ/BINARY and ACQ...

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• COS Instrument Handbook
• GHRS Instrument Handbook
• STIS Instrument Handbook

. [ Go back to Comet WWW site ] . Andrew A. Martis . martis @ sai.msu.ru .

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• Comet Center of SAI: Our observations

... НЕПРЕРЫВНОГО МАТЕМАТИЧЕСКОГО ОБРАЗОВАНИЯ . ... Кружок ?Олимпиады и математика? ... Московская математическая олимпиада . Заочный математический конкурс . ... Устные математические олимпиады . Олимпиады по программированию . Математический праздник . Математические регаты . ... Математические бои . Олимпиада по геометрии им. И.Ф.Шарыгина . ... Программа ?Math in Moscow? Научные конкурсы . Творческий конкурс . ... График олимпиад . ... XXVII Математический праздник . ...

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• Moscow Center for Continuous Mathematical Education - Independent University of

... Институт прикладной математики им. М.В.Келдыша . БАЛЛИСТИЧЕСКИЙ ЦЕНТР . О Центре . ... Баллистический Центр Института прикладной математики им. М.В.Келдыша РАН . Баллистический центр (БЦ) ИПМ им. М.В. Келдыша создан по предложению С.П. Королева и М.В. Келдыша в 1965 году. На него были возложены работы по баллистико-навигационному обеспечению (БНО) управления полетом пилотируемых кораблей и автоматических космических аппаратов научного и народно-хозяйственного назначения. ...

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Next: NICMOS/HST H-band (F160W) Images Up: NICMOS Science Previous: HST NICMOS Observations of . ... Observations of P . ... The NICMOS team has devised a comprehensive program of observations of the Galactic Center. ... Data in hand give a first look at variability and a detailed look at the search for the tip of the main sequence will be discussed where NICMOS has demonstrated adequate sensitivity and photometric precision to identify likely O8-B1 stars at the Galactic Center. ...

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• NICMOS/HST H-band (F160W) Images of the 30 Dor Starburst Cluster

... 10.09.2001 . ... CXO , NASA Explanation: Why would the center of our Galaxy flicker? Many astronomers believe the only credible answer involves a black hole . ... This short flicker therefore provides additional evidence that a black hole does indeed reside at our Galaxy's center . ... Publications with keywords: black hole - Galactic Center - Sgr A . Publications with words: black hole - Galactic Center - Sgr A . ... Journey to the Center of the Galaxy . ... Too Close to a Black Hole . ...

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• Астронет > Galactic Center Flicker Indicates Black Hole
• XWare > APOD

Russian SHAREABLE DATA CENTER Institute of Solar-Terrestial Physics SB RAS . ... The instruments engineer and technical support subdivision consists of the engineer support group: 4 senior engineers, 5 engineers and 14 staff members of service personnel. Head: Zavorin A. V. The main subdivision's instrument is the Incoherent Scatter Radar . The instruments engineer and technical support subdivision's main task is technical support of Irkutsk IS radar experiments. ...

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• East Siberian Center of Earth Ionosphere Research. Chirp ionosonde.
• Shareable Data Center "East Siberian Center for the Earth's Ionosphere...
• East Siberian Center for the Earth's Ionosphere Research. Modelling, secondary

ESAC Calibration management What does that mean ? ... 14 June 2006 Marcus G. F. Kirsch Marcus Kirsch , XMM-Newton European Space Astronomy Center Page 1 menu Ї X-ray calibration in the last century Ї Can we do better Ї Calibration management Ї Committee for X-ray calibration Ї Calibration mission scenario ESAC Marcus Kirsch , XMM-Newton European Space Astronomy Center Page 2 ...

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• http://xmm.vilspa.esa.es/calibration/documentation/epic_cal_meetings/200502/mk_xiat.pdf
• http://xmm.vilspa.esa.es/sas/6.5.0/doc/esrcselect.ps.gz
• http://xmm.vilspa.esa.es/sas/8.0.0/doc/rgslinepos.ps.gz

... 2001 September 10 . Galactic Center Flicker Indicates Black Hole . ... CXO , NASA . Explanation: Why would the center of our Galaxy flicker? Many astronomers believe the only credible answer involves a black hole . ... Only one known type of object can fit so much mass in so small a volume: a black hole . This short flicker therefore provides additional evidence that a black hole does indeed reside at our Galaxy's center . ... About APOD | ... NASA Technical Rep.: ...

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• APOD: September 12, 1997 - The Center of NGC 6251 is Glowing
• APOD: 2008 December 11 - At the Center of the Milky Way
• APOD: 2004 June 29 - In the Center of NGC 6559

... This paper presents an overview of the CENTERFIT image centering algorithm library currently under development in the IRAF system. ... The centering algorithms employed by these applications must satisfy a wide range of efficiency and accuracy requirements, and function robustly on data sets spanning a broad wavelength, resolution, and signal-to-noise regime. This paper presents an overview of CENTERFIT, a library of 1-D and 2-D centering algorithms currently under development in the IRAF system. ...

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• ADASS 2002 Conference Proceedings
• Prototypical Operations Support Tools for NASA Interferometer Missions:
• The SIRTF Science Center Is Alive And Well And Living In Pasadena

Physical and dynamical parameters of particles in outbursting Comet 17 P/Holmes . ... The time depending offset between the center of brightness and center of mass of the comet nucleus has been determined on the ground of positional observations of the comet. ... The motion of these particles allowed subsequent offset between the center of brightness and center of mass of the comet nucleus to be obtained from positional observations. ... comet, dynamical model, outburst, brightness. ...

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• (Untitled)
• IAA VLBI Analysis Center
• IAA EOP Service

Next: CCD observations and data Up: Observations and data reduction Previous: Observations and data reduction . Spectra obtained in the IPCS mode with the grating B1 (600 grooves/mm) cover the range of 3600 - 5500 ? ... Sky spectrum was accumulated simultaneously in the aperture of the same size displaced by 20'' along the current azimuth direction. ... Next: CCD observations and data Up: Observations and data reduction Previous: Observations and data reduction root . ...

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• SAO 6m observations
• Observations and reduction
• XID: Cross-Association of ROSAT/Bright Source Catalog

SXG Data Center . ... Sky visbility This utility permits to find the sky region that will be accessible for obsevation by the main telescopes of SXG. Observation opportunity programm This utility permits to find the the observation opportunity of given source ( RA, DEC ) during given MJD interval by the telescopes of SPECTRUM-XG directed along X-axis. Mask of the Earth/Moon This utility permits to find the sky region that will be blocked by the Earth/Moon for observation by SPECTRUM-XG . ...

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• GRANAT Home Page

Program: PLATE Purpose: snips raw data from tape(s) to custom plate Category: IRAS Author: Do Kester File: plate.src Keywords: INSTRUME= give instrument identification [] a combination of observation mode SURVEY SPLINE AO PO FLASH UNKNOWN and band number 12 25 60 100 LRS BPHF 1 2 3 4 ( 2 letters suffice ) PO is an alias for AO; AOs, POs and UNKNOWNs are collectively known as pointed observations. ... Only scan(snip)s which pertain to the same area and instrument can be stored in the same IRDS. ...

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• http://www.atnf.csiro.au/computing/software/gipsy/sub/irpl_userinfo.shl
• The ``HIPASS Bright Galaxy Catalog'' (version-4)
• selfcal

... Inst Data Fit allows one to determine various parameters needed for instrument data files, including: scale, orientation and the position of the rotator with respect to the instrument. ... Run Inst Data Fit. ... Specify all fields above the "Fit Scale and Orientation" button New Rot_Inst_ang . ... Modified the instructions so that new scale and orientation values are applied to the instrument block before measuring center-of-rotation data (to solve a problem brought to light by SPICam). ... R.O. ...

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• Spectrographic time budget
• TUI:Guiding:User's Guide
• Rotation range

... Dept. for Astrometry & Space Geodynamics . ... Dept. for Physics of Stars&Galaxies . Dept. for Space Plasma Physics . ... Laser station . ... 2016,MNRAS, 2016MNRAS.tmp.. ... 2016,MNRAS, Vol.455 ,is.1,p.357-369. ... 2016,MNRAS, Vol.456 ,is.1,p.181-191. ... WASP- 22, WASP-41, WASP- 42 and WASP- 55. ... 2016,MNRAS, Vol.456 ,Is.1,p.990-1002. ... GNSS stations System.NET network , which send their observations to IGS and EPN through the Operational center of MAO NAS of Ukraine . ...

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• Achievements - Page 4
• Observational Sites
• Activity - Page 2

... CfA Home . HCO Home . SAO Home . ... Welcome to CfA . CfA History . ... Laboratory Astrophysics . Extreme Astrophysics . ... 617) 495-7210 . ... 617) 495-7044 . ... 617) 495-7265 . ... HEA Research . ... HEA Home Page . CFA/HEA Home Page . ... High Energy Astrophysics Division (HEAD) . Chandra X-ray Center . ... Chandra Cluster Cosmology Project . Chandra Multiwavelength Project (ChaMP) . ... Chandra-Planck Clusters Project . ... CfA Virtual Observatory Project . ...

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• Champlane Observation: Magellan/IMACS June 6-9, 2005
• Chandra Images for J0454.4-6713
• GX339-4