O-C for observatory with code - 046. September, 2004 . Compressed Ephemeris DE200/LE200 -------------- MP Obs Dynamical Time RA (O-C)cosDEC DEC (O-C) h m s " ' " " 4179 046 2004 9 10.858556 21 51 58.693 -0.35 -15 46 13.30 0.26 4179 046 2004 9 10.860276 21 51 58.588 -0.44 -15 46 14.86 0.45 4179 046 2004 9 10.861726 21 51 58.508 -0.41 -15 46 16.33 0.45 Mean of last 3 obs. ... 91042 046 2004 9 10.015486 1 59 29.878 -2.37 +12 30 33.76 0.81 ? ... Mean of last 6 obs. ...

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• http://www.accuracy.puldb.ru/200707/C094.HTM
• http://www.accuracy.puldb.ru/200308/C046.HTM
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Next: DISH : The Single Dish Environment in AIPS++ . ... We present the SDImager tool which is designed to be the single dish imaging component of DISH in AIPS++. ... Recent work has concentrated on developing an imaging tool for single dish on-the-fly (OTF) observations using the same imaging class library as used for synthesis imaging in AIPS++. ... The initial single dish imaging tool in AIPS++ provides a few tools to examine and image these types of observations. ...

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... HST . How are observations affected when only a single guidestar is acquired? ... Data . ... HST Overview . ... Retrieving HST Data . ... Target Acquisition . ... In this situation, the roll of the telescope is under GYRO control, which may allow a slow drift of the target on a circular arc centered on the single guidestar. ... To calculate the approximate magnitude of the drift of the target on the detector, you will need to find the distance of the target from the acquired guidestar. ...

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• STIS Instrument Handbook
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... Data archive . Observing . Currently search mode observations can be carried out using the PDFB3 , PDFB4 , BPSR and the analogue filerbank. ... J1412+0224_R; P 14:12:00 +02:24:00; d4_cfg srch_256_512; d4_frq 1369.0; d4_tcyc 10; rcvr MULTI; tobs 60; mode srchset; sr4_nsblk 2048; sr4_btc 1.0; sr4_nbit 8; sr4_nprod 1; sr4_tsmp 1000 . ... The first column J1412+0224_R and J1412+0224 gives the name of the calibrator source and of the pulsar (or candidate position) . ... Group . ... Pulsar Groups . ...

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The examples of the errors. ... Observations with ordinary values of the "Mean error of single observation" Obj Code DT RA (O-C) DEC (O-C) mag z h m s " ° ' " " ° 3907 761 1998 08 24.383673 3 17 44.739 0.28 +30 46 00.84 -0.08 15.8 18 3907 761 1998 08 24.409133 3 17 46.152 0.28 +30 46 10.85 0.12 15.8 11 3907 761 1998 08 25.392523 3 18 40.107 0.33 +30 52 27.69 0.04 15.4 15 Total mean value of 3 observations 0.297±0.017 0.027±0.058 Mean error of single observation 0.029 0.101 COMMENT. ...

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Arecibo Observatory . ... All participants will take part in a Hands-on Project at the single-dish school. Mentored by a member of the NAIC or NRAO staff, each of you will join a team of 3 or 4 participants to perform a short pre-planned research-style observation. ... Hence, while summer clothing is appropriate, a light sweater may be needed for the evenings, and also in the air-conditioned rooms, lecture theater and control room of the Observatory. ...

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SCSI=Small Computer System Interface. ... SCSI was ratified in 1986. ... 50 PIN IDC MALE at the controller & harddisk. 50 PIN IDC FEMALE at the cable. Pin . ... Data Bus 0 . ... Data Parity (odd Parity) . ... GND . Ground . ... Control/Data . ... Input/Output Note: Direction is Device relative Bus (other Devices). All odd-numbered pins, except pin 25, are connected to ground. Pin 25 is left open. ...

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• Radio survey for new compact HII regions
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... Simple X-ray Aperture Photometry Problem : Determine source intensity s and errors for an unresolved (point) x-ray source Know: · Number of counts , C, in source aperture (solid green ellipse) · Number of counts , B, in background aperture (dashed green elliptical annulus) · Areas As and Ab of source and background apertures · f = psf(x,y)dx dy over source aperture · g = psf(x,y)dx dy over background ... What happens if the single observation pdf 's are distinct? ...

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SCSI=Small Computer System Interface. ... SCSI was ratified in 1986. (at the controller & harddisk) . ... Data Bus 0 . ... Data Parity (odd Parity) . ... GND . Ground . ... Control/Data . ... Note: Direction is Device relative Bus (other Devices). All odd-numbered pins, except pin 25, are connected to ground. ...

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• IBIS: SolarNet Access
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The problem with double event patterns (M. Brusa, K. Dennerl ­ MPE) EPIC CAL/OPS meeting - MPE Classification of doubles SA S 2 Right SAS 3 Forward SA S 4 Left SAS 1 Backward readout direction split backward (SAS: ,,1 ) split left (SAS: ,,4 ) split right (SAS: ,,2 ) Forward/ Backward doubles : superposition of true doubles and false ... Double (1 ­ backward) - "detector representation" REV #84 Singles (blue) Dbackward (red) "Curved shape" wrt singles Singles vs. ... Al line Singles vs. ...

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The VLTI Calibrator Selector Tool is a tool intended to assist in the selection of suitable interferometric calibrators for VLTI observations with MIDI and AMBER. It uses a model of the VLTI and its instruments to assess the fringe visibility, given the observed bandpass, the geometry, spectrum, and coordinates of the target and the time at which the observations are to be made. ... The tool offers an HTML/Java based interface and consists of two pages. ... The quality flag depends on LDD_chi2. ...

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• Data Flow System overview
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... Galaxy Collisions: Simulation vs Observations . ... 14.05.2013 . ... Explanation: What happens when two galaxies collide? ... Since galaxies are mostly empty space, no internal stars are likely to themselves collide . ... Pictured above is a computer simulation of two large spiral galaxies colliding , interspersed with real still images taken by the Hubble Space Telescope . ... May 2013 . ... Publications with keywords: colliding galaxies . Publications with words: colliding galaxies . ...

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Next: Correlator Products . Previous: RSOG Post-Observation Products . ... Merged Correlator Input Log . Calibration and Flag files . SRT Amplitude Calibration Data . ... Phase Calibration (PCal) Data . ... DPC to Correlators . What: The RSOG produces the `merged' correlator input log file based on the Data Processing Logs supplied by the GTSs and on Executed Sequence of Events supplied by GOCG to produce a single correlator input log for all the GTSs for each observation. ...

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Back . Moveable feed-cabine #3 with secondary mirror (9*5.5m) is equiped by spectro-polarimetric radiometers complex in wavelenths range 1.38 - 30 cm. The single phase center multiband horns are used. All time it used with antenna "Southern Sector+ Flat mirror".

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.

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Next: First CCD Observations of Up: Highlights Previous: Origin of Stars Contents . Subdwarf B stars are highly evolved stars which pulsate non-radially in several modes with different frequencies. ... Over 60,000 images were obtained, which when played in sequence show the star's oscillations in red, green and ultraviolet light. ... Figure 3: ULTRACAM light curve for PG0014+067, from 2004 August 20 to 2004 August 25 (top to bottom). ...

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Winer Observatory P.O. Box 797, Sonoita, Arizona 85637-0797, USA . ... Asteroid . ... Site . ... The evening of October 26, 2011, Mark Trueblood, Robert Crawford, and Larry Lebofsky used the Kitt Peak 2.1-m telescope to observe Near Earth Asteroid (NEA) 2008 QT3. ... single still jpeg frame . ... The National Optical Astronomy Observatory (NOAO) issued a press release concerning Morgan's work on Monday, November 21, 2011 and posted it on the home page of their web site . ... 2013 Winer Observatory. ...

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... Single-crystalline eutectic oxide fibres are needed to reinforce metal, intermetallic and ceramic matrices to obtain high temperature composites. ... The method of internal crystallization was developed in Laboratory of Reinforced Systems of Solid State Physics Institute initially to produce oxide-matrix/molybdenum-matrix composites, which were considered mainly as model ones. ... Figure 1 . ... The oxide/molybdenum block is then moved to a cold zone of the furnace to crystallize the fibres. ...

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... 2013 May 14 . Galaxy Collisions: Simulation vs Observations . Images Credit: NASA , ESA ; Visualization: Frank Summers ( STScI ); Simulation: Chris Mihos ( CWRU ) Lars Hernquist ( Harvard ). Explanation: What happens when two galaxies collide? Although it may take over a billion years, such titanic clashes are quite common. ... Pictured above is a computer simulation of two large spiral galaxies colliding , interspersed with real still images taken by the Hubble Space Telescope . ...

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• GLI - GiST layered insertion algorithm

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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