... Armagh Observatory, College Hill, Armagh BT61 9DG, +44 (0)28 3752 2928 . ... Risks Comparable to NEOs . ... The Increasing Rate of Discovery of Asteroids . ... Comet and Asteroid Collision Probabilities . ... Extreme albedo comets and the impact hazard (PDF Format) . ... Asteroid Impact Animations . ... Workshop on Scientific Requirements for Mitigation of Hazardous Comets and Asteroids - 2002 . ... The Spaceguard Survey Report, 1992 (PDF) . Tsunami from Asteroid/Comet Impacts . ...

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M1 image More About M1 Nice Color Picture . ... M16 image More About M16 HST image . ... M31 image More About M31 Nice Color Picture . ... M42 image ; M43 image More About M42/43 Nice Color CCD Picture . M51 image More About M51 Color Image of M51 M51 Supernova . M57 image More About M57 Nice Color CCD Picture Very Deep M57 Image . ... M81 image More About M81 M81 Supernova Ultraviolet Image of M81 More about Ultraviolet Imaging . M82 image More About M82 M82 False Color M82 True Color . ...

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... Main santific objetives: . ... Main characteristics . ... Cooperation . ... IMAP-6 magnetometer Main santific objetives: In the beginning of the chapter . ... chemistry of rocks; . ... Scientific payload: In the beginning of the chapter . ... Main characteristics: In the beginning of the chapter . ... mass of penetrator . ... Cooperation In the beginning of the chapter . ... CHARACTERISTICS OF SCIENTIFIC INSTRUMENTS: In the beginning of the chapter . ... time of measurements - 0,3 hour; . ... mass ....

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... An OBJECT column gives the name of the object observed (usually a star name). ... In critical cases, it is common practice to measure sky on two or more positions around a target object, and these positions must be identified. ... A general treatment of this problem requires a column called OBJECT, bearing the usual name of the object (as in the star tables); a column labelled STARSKY, to distinguish between star+sky, star alone, or sky alone; and additional columns to identify the sky position. ...

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• Temperature and humidity data

... Near Infrared Camera and Multi-Object Spectrometer Instrument Handbook for Cycle 17 > Chapter 8: Detector Readout Modes > 8.6 Trade-offs Between MULTIACCUM and ACCUM . 8.6 Trade-offs Between MULTIACCUM and ACCUM . There are a variety of advantages to the MULTIACCUM mode. First, the ability present in a MULTIACCUM exposure to filter out CR hits which occur during the exposure is lost in the ACCUM mode. ...

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... The category of records is controlled by the 'category' parameter. 4 Parameters This section documents the parameters recognized by this task (if any). Parameter Mand Type Default Constraints category yes String process Category of information to be retrieved objects yes StringList List of fully quali ed object names on which to run dsinfo xmmsas 20070708 1801-7.1.0 XMM-Newton Science Analysis System Page: 2 5 Errors This section documents warnings and errors generated by this task (if any). ...

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• http://xmm.vilspa.esa.es/sas/5.4.1/doc/dsinfo.ps.gz
• http://xmm.vilspa.esa.es/sas/6.1.0/doc/dsinfo.ps.gz

... The recently discovered quasar labeled APM 08279+5255 has set a new record as being the brightest continuously emitting object yet known. APM 08279+5255 's great distance, though, makes it only appear as bright as magnitude 15.2, an object which can be seen with a moderate sized telescope. ... One possible explanation of APM 08279+5255's record luminosity is that it is partly a mirage: its light is highly magnified by an intervening galaxy that acts as a gravitational lens . ...

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• Астронет > APM 08279+5255: The Brightest Object Yet Known
• Астронет > Микролинзирование
• Behind CL1358+62: A New Farthest Object

TUI supports the following offsets: . Object Arc offset by a given amount on the sky (i.e. along the arc of a great circle). ... Arc offsets are useful for moving a different portion of your object or a different nearby object onto the boresight . ... Object Arc XY this is identical to an Object offset except that it has been rotated to align along the instrument x-y axes. ... This is just like the Calibration XY offset, except that it is typically cleared when you slew to a new object. ...

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• TwistedActor.Actor Standard Commands

... Definition at line 95 of file TableExprId.h . ... Definition at line 139 of file TableExprId.h . ... Definition at line 145 of file TableExprId.h . ... Definition at line 151 of file TableExprId.h . ... Definition at line 192 of file TableExprId.h . ... Definition at line 187 of file TableExprId.h . ... Definition at line 182 of file TableExprId.h . ... Definition at line 167 of file TableExprId.h . ... Definition at line 162 of file TableExprId.h . ... Definition at line 157 of file TableExprId.h ....

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• casacore: casa::RecordFieldPtr< T > Class Template Reference
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• casacore: casa::ScalarRecordColumnDesc Class Reference

... S.P. KOROLEV ROCKET AND SPACE CORPORATION ENERGIA . ... OAO RSC "Energia" . ... Rocket Systems . ... ISS Russian Segment . ... Automatic Space Systems . ... Guidance, navigation and control system sensors measuring the Station angular velocities; . ... Telemetry information concerning measurements of nominal sensors of the ISS RS power supply system and guidance, navigation and control system, received from the Station. ... AUTOMATIC SPACE SYSTEMS . ... 2015 JSC "S.P. Korolev RSC "Energia" . ...

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Turning the Camera Skyward . A reconfigured camera can take wide-field exposures of astronomical objects (constellations, the Milky Way, zodiacal light, moving artificial satellites, meteor showers, variable stars, etc.) to reveal much fainter objects and structures than seen by naked eye. ... This picture reveals objects more than 2.5 times fainter than can be seen by the naked eye, including not only stars but also the Orion nebula (M42), where new stars are being born. ...

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... Why does X-ray astronomy require satellite telescopes? ... That is why scientists use space based satellites to record and observe data from X-ray sources. ... It primarily observes X-ray sources and has a moderate imaging capabilities. ... X-rays (because of their short wavelengths) , as opposed to visual light, can penetrate through otherwise opaque objects e.g. bones X-rays can observe celestial objects that emit shorter wavelengths such as galaxies , quasars, and black holes. ... X-ray image . ...

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• Very Low Mass PMS Objects

... Meade Instruments Corporation . ... How to Calculate Power . How to Calculate Power: The magnification, or power, at which a telescope is operating is a function of the focal length of the telescope's main (objective) lens (or primary mirror) and the focal length of the eyepiece employed. ... Example: The Meade DS-2070AT telescope has an objective lens focal length of 700mm; when this telescope is used with a 25mm eyepiece, a power of 700/25 = 28 power (written as "28x") results. ... about meade | ...

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... Science User Portal . ... ESO, the European Southern Observatory . ... ESO's Governing Bodies . ... Travel and Contacts . Travel to ESO Headquarters . Travel to Vitacura Office . Travel to Guesthouse . Travel to La Silla . ... ESO . ... VLT/Paranal . ... Survey Telescopes . ... Galaxies . ... ESO Science Newsletter . ... VLT Unit Telescopes Names . ... ESO 3.6-metre telescope . ... MPG/ESO 2.2-metre telescope . ... ESO 1-metre Schmidt telescope . ... ESO Science Outreach Network . ...

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• The VLT Records Faint Structures in Colliding Galaxies | ESO Ireland
• The VLT Records Faint Structures in Colliding Galaxies | ESO Australia

ATMoB "Messier Marathon Award " Guidelines Purpose: To promote observing among the membership of the Amateur Telescope Makers of Boston through participation in an all-night Messier Marathon. ... For each Messier object observed, check the space in the "Seen" column on the attached Messier Checklist and note the time and method of observation. ... Challenge Levels: Beginner Intermediate Master Observe and record information on 25 Messier objects in the attached worksheet. ...

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• Amateur Telescope Makers of Boston

... Astrophysics Group . ... Pulsars . ... Stars ? ... The array was designed to detect compact radio sources such as these by virtue of the fact that they would scintillate (twinkle) when observed from the Earth through the interplanetary medium ? ... One of Antony Hewish?s research students, Jocelyn Bell, was set the task of operating the telescope and inspecting the daily charts for the kind deflections in the trace which occurred when a scintillating source passed over the array. ...

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... We have developed a web site using HTML, Php, Python, and MySQL that extracts, processes, and displays data from the Sloan Digital Sky Survey (SDSS) and the Two-Micron All-Sky Survey (2MASS). The goal is to locate brown dwarf candidates in the SDSS database by looking at color cuts; however, this site could also be useful for targeted searches of other databases as well. MySQL databases are created from broad searches of SDSS and 2MASS data. ... 2002). ... 2002, AJ, 123, 3409 . ...

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... August 18, 1998 . APM 08279+5255: The Brightest Object Yet Known . ... Explanation: It shines with the brightness of 100 billion Suns. ... The recently discovered quasar labeled APM 08279+5255 has set a new record as being the brightest continuously emitting object yet known. APM 08279+5255 's great distance, though, makes it only appear as bright as magnitude 15.2, an object which can be seen with a moderate sized telescope. ... About APOD > . ...

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• APOD: July 31, 1997 - Behind CL1358+62: A New Farthest Object
• APOD: 2016 March 7 - Mystery Feature Now Disappears in Titan Lake
• APOD: 2014 October 15 - Mysterious Changing feature on Titan

... Records were made this January when the RadioAstron satellite was joined by ground-based telescopes, forming a radio telescope 220,000 km across тАУ roughly 20 times larger than the Earth. RadioAstron , a Russian orbital telescope of 10 meter diameter, joined with ground-based observatories to resolve objects 50 times smaller than is possible with the Hubble Space Telescope. ... Images: . The RadioAstron spaceantenna observes a celestial radio source simultaneously with ground-based dishes. ...

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• Solar System Studies at AO
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Magnetic field measurements onboard the Interball Tail spacecraft are carried out by the FM-3I instrument which consists of two flux-gate magnetometers covering two different ranges: [-200, +200] nT and [-1000, +1000] nT. Besides scientific goals, the FM-3I experiment data is used to perform the attitude control of the Interball Tail spacecraft. ... August 22, 1995 . ... October 18, 1995 . Top of the page . ... Back to the Interball Home Page . ...

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• INTERBALL/ELECTRON EXPERIMENT
• SPICE System Overview .
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