WFPC2 . Images: version1 , version2 . Catalogs: Version 1 HDF-S , HDF-N ;Version 2 HDF-S . STIS . ... NICMOS . Images: Camera 3 , V2 of psf-convolved STIS 50CCD on NICMOS . ... Images: WFPC2 FF , STIS FF ; Version2: WFPC2 FF , STIS FF , NICMOS FF . Catalogs: Version2 WFPC2 FF , STIS FF , NICMOS FF . ... Check the instrument specific technical pages for a description of the data products and the implemented data reduction steps: STIS , WFPC2 , NICMOS , Flanking Fields . ...

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• GOODS: The Great Observatories Origins Deep Survey
• Spitzer Observations of NGC 2547: The Disk Population at 25 Million Years
• Spitzer Observations of a 24 ЮМm Shadow: Bok Globule CB 190

... A radio galaxy is a galaxy that emits an unusually big amount of energy at radio wavelengths. ... Inside of each galaxy with an active nucleus (radio galaxies are among them) there must be a system of a "central machine" responsible for the colossal amount of the emitted energy from radio to gamma ranges. ... Sometimes a radio source in an active galaxy may flare again if the needed conditions appear (a new portion of matter would fall into the furnace of the "central machine"). ...

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• Observations Support Laboratory BTA
• Electronic version of Russian Bulletin
• Observations Support BTA

... Many scientific institutions maintain bibliographies of articles published by their scientists and monitor references made to these publications; these figures are often used to evaluate the effectiveness of the institution. ... a) Identification of papers that are based, at least partly, on new data Publications based on observations can be subdivided into two groups: those presenting new, previously unreported data, and those that make use of already published data. ... Published by . ...

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• ESO - Guaranteed Time Observations
• ESO - Period 95 Phase 2 Deadline for VIMOS Observations
• ESO - Release of VISTA Deep Extragalactic Observations Survey Data in the

... Update . MOS response files for all modes have been updated . ... Response files for both MOS and pn have been updated . ... Information about the canned PN EPIC response files updated . ... EPIC canned response files no longer needed with SAS 5.3.0 . ... EPIC background files updated . ... Clarification about the updated PN responses . ... A further update to the EPIC PN responses is available . ... Updated responses for MOS and PN . ... Technical note on SAS vs ad hoc responses updated . ...

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• Selection of observations of empty RGS files
• Observation/ Slew Record

Next: IPCS observations and data Up: Spectral survey of Case Previous: The sample description . The observations were carried out with the 6m telescope of the Special Astrophysical Observatory of Russian Academy of Sciences (SAO RAS) in the period from December 1992 to October 1996. ... 1986 ]). Since January 1996 we used for registration Tektronix CCD 1024 1024 provided by Astrophysical Institute Potsdam (AIP, Germany) in the frame of mutual cooperation between AIP and SAO RAS. ...

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• "Structure" publications in 2002 year
• To main page
• Reducing the observations

... We have developed an integrated system that performs astronomical observations in Near Infrared bands operating two-dimensional instruments at the Italian National Infrared Facility's ARNICA and LONGSP . ... The user interface is organized as widget-based X11 client. ... 1993; Di Giacomo et al. 1993). ... Moreover, if the interprocess communication interface includes support for networking, the software immediately becomes network distributed software. ... DESQview/X User Guide 1993, Quarterdeck . ...

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• Modern CCD Observations of Moving Celestial Objects: Algorithms and Software
• On-The-Fly Re-Calibration of HST Observations
• Observation Planning and Scheduling

... IAA VLBI Analysis Center . ... First IAA SLR EOP submission to IERS Annual Report . ... Beginning of operational processing of SLR observations . ... We use several program packages for analysis mostly developed at the IAA: GROSS for processing of the SLR observations and analysis of EOP and coordinates time series, OCCAM/GROSS for computation of EOP, station coordinates, and troposphere parameters time series from the VLBI observations, GRAPE for processing of GPS observations. ...

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• (Untitled)
• LAAI_2012,observation
• Keywords_58

... Observations have received at the telescope AT-64 of the Crimean Astrophysical Observatory . GRB . ... RA(2000): 11h 45m 10.54s . DEC(2000): 17o 24' 34.44" . ... Filter: none . ... Date, time (UT) . Exposure . ... 2000.07.29 18:21:52 . 30 sec . ... RA(2000): 19h 58m 19.61s . DEC(2000): 23o 32' 35.15" . ... 120 sec . ... DEC(2000): 6o 20' 47.07" . ... 240 sec . ... DEC(2000): 51o 46' 34.93" . ... DEC(2000): -13o 04' 30" . ... DEC(2000): +55o 18' 25.0" . ... 2000-11-09T16:03:19 . ...

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• IKI partnership for optical observation of Gamma-Ray Bursts
• Two points (INTERBALL-1 and MAGION-4) observations of magnetopause motion
• OFO IKI / TV System for Navigation and Observation

... Bright star to be occulted by asteroid, 20/21 July. ... The star is magnitude 6m.4, and will be occulted by 773 Irmintraud, magnitude 13.8, so the drop in combined brightness will be 7.4 magnitudes - in effect the star will totally disappear for up to 10 seconds or so! ... The following details were sent to me by Tolis Christo at Armagh Observatory, who will co-ordinate any observations "Hi Terry, I don't know whether you've made any plans for the Irmintraud occultation on the night of the 20th July...

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• First CCD Observations of Asteroids from Armagh
• Observations with the Faulkes Telescopes
• ULTRACAM Observations of Subdwarf B Stars

... General information . ... Staff . Research staff . ... Historical highlights . ... For education and public outreach, the Arcetri Astrophysical Observatory opens its doors to the general public by organizing guided visits with observations of the sky. ... The entrance for the daytime and nighttime visits to Arcetri Astrophysical Observatory is from Via Pian de Giullari, 16 In case there is a need to call or to ask for information on accessibility, please contact the number 055/2752280 . ...

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• Procedures for Observations
• Observations of Pre-biotic Complex Organic Molecules in the Pristine Jet-disk
• Program parameters

... Observation codes for VSOP General Observing Time observations have the form . ... The first letter indicates which AO period the observation was proposed in: the letter `v' indicates the first AO period, and the letter `w' indicates the second and third AO periods. The three digits indicate the proposal number. ... For proposals with more than 26 experiments (see next item), 300 is added to the proposal code for the 27th and subsequent experiments. ...

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• Scheduling Mark II Observations
• Mark III Observations
• Archive of VLBI Observations Majordomo List

... Dept. for Astrometry & Space Geodynamics . ... Dept. for Physics of Stars&Galaxies . Dept. for Space Plasma Physics . ... Solar telescopes . ... 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. ... Observations . ... In 2002 regulary observations of comets with using of CCD camera S1C started at Andrushivka Astronomical Observatory, near Zhytomyr. ...

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• Optical systems and devices

... Bad Astronomy . ... Bitesize Astronomy . ... Keep Bad Astronomy close to your heart, and help make me filthy rich. ... Before we get to this week's snack, let me remind you that Leonids meteor shower peaks November 17. ... Theorists take that data and work mathematical models, trying to see if they can get the known laws of physics to mimic reality. ... It was an interesting feeling to actually see that area of sky with my own eyes. ... 2008 Phil Plait. ... Subscribe to the Bad Astronomy Newsletter!...

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Astronomy Discussion Forums . Forums: . ... Discussion Forums . ... Observations Of Mars . Forum List | ... Post Message | ... Using a 15mm plossol and my 2X barlow I can make out the south polar ice cap and some serface detail. ... Login to Post . ... www.astronomy.net . About Astronomy Net | Advertise on 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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• Observation Report 03/15/03 From Coyle Field - an Astronomy Net
• Observation Report On Mars And ... - an Astronomy Net Observation_reports Forum
• Software For Moon Observation - an Astronomy Net Software Forum Message

... Let us first find out which way -- rise in spectral resolution with some loss in the S/N ratio or increase in the S/N ratio with a fixed spectral resolution -- is better for the purpose of reduction of equivalent width determination errors. ... N -- number of counts for 1 ? ... line equivalent width, . ... Thus if the spectral resolution is managed to be increased (i.e. to decrease )without loss in the number of counts falling at 1 ?, the equivalent width measurement error is then proportional to . ...

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• RATAN-600 antenna
• SCORPIO-2 project: publications
• On the problem of high spectral resolution observations of faint objects

Peremennye Zvezdy ( Variable Stars ) 35 , No. ... We present the results of our new observations of QS Draconis, a recently discovered double-mode high-amplitude Scuti variable, HADS(B) type. ... Our CCD observations in the Johnson bands were performed at the Tien Shan Astronomical Observatory of the V.G. Fesenkov Astrophysical Institute, at the altitude of 2750 m above the sea level. ... The finding chart (Fig. 1) identifies the variable star, comparison star, and check star. ... Fig. ...

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• Galaxy Collisions: Simulation vs Observations
• Астронет > Archive of Astronomical and Astrophysical Transactions
• Астронет > Galaxy Collisions: Simulation vs Observations

... Radio emission at around 90 GHz from star-forming galaxies is expected to be strongly dominated by the free-free component due to ionising radiation from massive, short-lived, stars. We present high surface-brightness sensitivity observations at 90 GHz of the nearby star-forming galaxy Messier 66 with resolution of about 9 arcsec (corresponding to a physical scale of about 500 pc) and analyse these observations in combination with archival lower frequency radio and mid-infrared measurements. ...

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• De-convolution of a Gaussian beam from planetary observations Bojan Nikolic web
• Bojan Nikolic -- First WVR and interferometric observations at the OSF
• Summary of Ryle Telescope radio observations of GRB 021004 at 15.2 GHz

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Pulkovo NEO Page . ... NEA Accuracy Estimation . ... The estimation of accuracy of the current CCD observations of asteroids and comets is constantly performed at Pulkovo Observatory. ... The (O-C) values, so called "Observed" minus "Calculated" positions, characterize numerically the observations of any observatory, both professional and amateur, during a short period (one or several close nights). ... So the (O-C) values for these objects nearly entirely define the errors of observations. ...

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• Pulkovo NEO Page: Observations

. The CIMA calibrated pulsar catalog observation mode is an observing mode that only is available via command file observing. You can return to the main CIMA page by clicking here .

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• The CIMA ALFA Observation Monitor Window
• The CIMA Pulsar Catalog Observation Mode
• USING THE AO-CONTROL GUI FOR SPECTRAL LINE OBSERVATIONS