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
• GOODS Supporting Observations

... 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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• New data on the cpmplex field structure of chemically peculiar stars
• Observations Support Laboratory BTA
• Ratan-600 observation schedule

... Optical, X-ray, -ray, UV . ... Crab, B0540-69, Geminga, B1509-58, Vela . Optical - Crab, B0540-69, Geminga, Vela . ... X-ray - 27 pulsars (13 pulsed), 7 msps (3 pulsed) . X-ray - 3 thermal surface cooling emission . X-rays pulsed, unpulsed or from bow shock . Outer gap emission . ...

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• Observations from Australasia using the Gravitational Microlensing Technique
• Loading data into Miriad: ATLOD
• ATNF Daily Astronomy Picture

... 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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... As the 430 MHz line-feed radar beam is approximately 300 m in diameter in the meteor zone, the sodium lidar beam will need to be expanded to approximately that diameter and the receive telescope suitably aligned and field-of-view adjusted. The lidar would be operated synchronously with the radar at the same IPP and raw data from each pulse would be retained for post-processing. ... The lidar IPP must be synchronized with the 1 msec radar IPP with data readout every IPP over the meteor zone. ...

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• http://www.naic.edu/vscience/schedule/tpfiles/FriedmantagT2248tp.pdf
• hydrocarbon lakes on Titan
• NAIC Arecibo Observatory Lidar Publications Page

... kupry@sai.msu.ru also kupry@asu.cas.cz . ... Solar expeditions. Astronomical Institute Czech Republic Examples IDL procedures Evpatoria Space Image Evpatoria Winter 2012 European Solar Physics Meeting Digital Images Album IDL Lib Karlovy Vary, 2008 List of publications Masha MAX MILLENNIUM PROGRAM My family (new) HSFA-2, 2005 Ondrejov (brezen 2005 ) Ondrejov webcam Photo Ondrejov observatory Praha SatTV Seznam SOHO Solar eclipse 31 July 1981 Software IDL programmes ...

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• Natural Satellites Service. Observations
• IMCCE-SAI: Natural Satellites Data Center. Observations
• IMCCE-SAI: NSDC. Observations. Galileans

Nowadays at the Department the experimental and theoretical investigations, including astronomical and ionospheric observations, active experiments with space vehicles are taking place. ... Solar Corona physics and erruptive phenomenae. ... Stellar astronomy. ... The Department has organized and put into practice more then 50 expeditions for observation of Solar ecllipces, aurorae polaris, comets, meteor streams, controlled space experiments, and also for investigations of geophysical characteristics. ...

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• CAMERA ELECTRONICS FOR THE CCD FOURIER SPECTROMETER
• Mykola I. Dzubenko
• Lunar physical observations. Explanations for Computer Ephemeris.

... The J, H and K bands are characterized by a bright background, such a background is mainly due to the emission of atmospheric lines and of thermal radiation. ... If the source cover a large fraction of the slit, spectra off-source must be observed to adequately sample the sky background. ... The on chip integration time (time spent in each position of the slit) must not exceed 40 seconds in J and H bands and 60 seconds in K band. ... We suggest a sequence of 10 for each elementary integration time. ...

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• Hubble Observations Shed New Light on Jupiter Collision
• Arcetri Solar Physics Group: High Resolution Studies
• Hubble Finds Oxygen Atmosphere On Jupiter's Moon Europa

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

... BTA and RATAN-600 are largest optical and radio telescopes in Russia. ... Antenna of RATAN radio telescope consist of 576-m circle of 895 elements (2 x 11.5 m), which could use as four independent sectors (225 elements) of that reflector (named: North, South, West and East). Four different feed-cabines (N1,2,3,5) with secondary mirrors could simulteniously collect radio emission from these four sectors and be used in programs of Continuum , Spectral and Solar observations. ...

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• Publications of Klochkova Valentina
• On the problem of high spectral resolution observations of faint objects
• Optimization of spectroscopic observations

... The comet 169P was first observed by the Near-Earth Asteroid Tracking system. In order to observe this comet we had to figure out if it was possible to view it from Faulkes Telescope South, a 2m reflecting telescope which is used for research as well as for use by school students around the world over the internet. ... Since 169P is such a bright object, we were able to use a red filter on some of our observations to provide a clearer image. ...

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• Small-Scale Dynamic Events in the Solar Atmosphere
• Armagh Observatory
• First CCD Observations of Asteroids from Armagh

Page move

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• Observations
• IPCS observations and data reduction
• SAO 6m observations

... Julian Date Flux Densities (mJy) Julian Date Flux Densities (mJy) 2440000:0 A1 A2 B C 2440000:0 A1 A2 B C 8930.9968 153.8 134.6 59.8 22.6 9021.6846 154.0 137.0 59.0 22.9 8939.7717 163.7 146.0 66.1 22.9 9024.6766 151.4 134.6 58.4 22.1 8940.8936 153.2 135.8 59.2 22.6 9030.5334 156.7 139.1 59.0 22.4 8944.7380 161.7 142.2 63.7 23.1 9032.6650 151.8 136.5 57.7 22.6 8951.8637 148.4 131.3 58.3 21.7 9036.7067 155.1 137.1 58.8 ...

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... 28.11.2001 . ... Credit: Greg Bacon ( STScI /AVL) Explanation: By directly detecting the atmosphere of a planet outside our Solar System , humanity has taken another small step toward finding extraterrestrial life . ... November 2001 . ... 2001 2002 . ... NASA Web Site Statements, Warnings, and Disclaimers . NASA Official: Jay Norris. ... Publications with keywords: extrasolar planet . Publications with words: extrasolar planet . ... Atmospheres Detected on Two Extrasolar Planets . ...

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• Atmospheres Detected on Two Extrasolar Planets
• Астронет > Atmospheres Detected on Two Extrasolar Planets
• Астронет > Extra Solar Planetary Atmosphere Detected

Next: SAS processing Up: Maintenance procedures Previous: Maintenance procedures Contents . Suitable observations should be longer than about 20 ksec, cover all the considered time period, and have different background levels, in particular the highest ones, so the sample should include observations taken at the beginning and end of the science window. It is helpful to consider objects for which no RGS spectrum is expected or to look at the RGS monitor pages. ... Michael Smith 2011-09-20 ...

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• Observation/ Slew Record
• XMM-Newton Planned and Performed Observations
• Combination of the selected observations to make the templates and build CCFs

... 2007 February 27 . Atmospheres Detected for Two Extrasolar Planets . ... Explanation: Do extrasolar planets have water? In an attempt to find out, the orbiting Spitzer Space Telescope made detailed observations of the atmospheres of two planets that orbit stars other than our Sun. ... Although no water vapor was detected this time, the techniques of measuring exoplanet atmospheres are quite promising, and the search for distant water and other biomarkers is just beginning. ... About APOD | ...

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• Titan
• APOD: 2013 May 14 - Galaxy Collisions: Simulation vs Observations
• APOD: 2014 June 23 - Four Lasers over Mauna Kea

... 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
• Publications of Laboratory for atmosphere optics

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 From Coyle 07/19/03 - an Astronomy Net Observation_reports
• Observation Report On Mars And ... - an Astronomy Net Observation_reports Forum

... Public . Science . ... Science Users Information > Observing with ESO Telescopes > Policies and Procedures > Guaranteed Time Observations . ... Guaranteed Time Observations . Public Surveys . Publications with ESO Data . ... Large Programmes . ... Public Surveys Programmes . ... Phase 1 Proposals . ... ESO Data . ... In the case of GTO surveys or focused projects taking a large fraction of the GTO time, i.e. Large GTO Programmes, the whole observing plan may be made public at once. ...

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• ESO - Period 95 Phase 2 Deadline for VIMOS Observations
• ESO - Release of VISTA Deep Extragalactic Observations Survey Data in the
• ESO - Spiral Structure in the Milky Way: Confronting observations and theory

... Up: Data Analysis and Processing Techniques . ... Also, a method for quality control of CCD observations is suggested. ... Everyone who observes a celestial object using a CCD detects moving celestial objects as a ``by product''. ... We hope that our investigations may be useful for near-Earth space control and also for searches of the moving celestial objects through analysis of old and new CCD frames obtained at any amateur or professional astronomical observatory. ...

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• Distributed Software for Observations in the Near Infrared
• On-The-Fly Re-Calibration of HST Observations
• Observation Planning and Scheduling