... Tonight's Sky . ... The Magazine . ... Star Atlas . ... An artificial comet holds secrets to Earths life . ... Astronomy for Kids . ... Observing springtime deep-sky objects with a large telescope . ... The planet has extreme temperature swings and perhaps active lava flows. ... A digital supplement to Astronomy magazine. ... Join TravelQuest International with Astronomy and Discover magazines on one of three great tour options surrounding this celestial spectacle . ... Astronomy Magazine . ...

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• CSIRO, Sydney, Australia | Astronomy.com
• International Center for Radio Astronomy Research, Perth, Western Australia |
• Caastro, Australia | Astronomy.com

... Home Astro-Imaging OLYMPUS DIGITAL CAMERA . ... Lecture Series 2014-2015 . ... Clear Sky Chart . ... This Month's Sky - 2015 . ... Beyond New York City . ... Observing Resources for Amateur Astronomers - Part 1: Beginning Observers . ... A History of the First Forty Years of the Amateur Astronomers Association . ... Published February 15, 2015 at dimensions 2048 1536 in OLYMPUS DIGITAL CAMERA . ... 2016 Amateur Astronomers Association of New York Designed by Press Customizr Powered by . ...

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• Astronomy Workshop: Observing Variable Stars from the City ? February 15, 2015
• Astro-Imaging ? Page 12 ? Amateur Astronomers Association of New York
• Observing ? Amateur Astronomers Association of New York

... Has Jupiter been hit, or does it have a new storm? From Anthony Wesley, Australia: " Yes, believe it or not, it seems that Jupiter has been hit by something and there is a jet black impact mark near its south pole. ... The last one I remember was the Shoemaker-Levy impacts in 1994." Link to the Irish Astronomy blog . ... Sunday, 19 July 2009 22:52 . International Year of Astronomy, Ireland National Node . ...

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• Observing Jupiter | International Year of Astronomy in Ireland | Astronomy 2009
• Observing with a 100-metre telescope - Wed 21 October, Belfast | International
• Observing times | International Year of Astronomy in Ireland | Astronomy 2009

... Current APO Weather . ... Search Site . ... Information for New Users . ... Technical Staff pages . Night Logs and Mailing Lists (maintained by APO) . ... Technical Documents and Database Search . ... Observer's Documentation and Procedures . ... Problem Reporting and APO Technical Documents Database Search . ... APO Drawing/Document Management Procedures . ... APO Technical Documents Database Search . Home Astrophysical Research Consortium . ... Mail Lists (maintained by APO) . ...

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• ARC 3.5m | Closure Conditions
• APO Telescope Documentation
• Information for Observers

... Moore Observatory is a research and advanced teaching facility of the University of Louisville. ... The 24-inch Ritchie Chretien (RC24) telescope is a research instrument used by faculty and graduate students involved in studies of exoplanets, optical properties of the atmosphere, and the development of imaging and spectroscopic technology. ... Kent (CDK20S) are collaboratively operated by the University of Louisville and the University of Southern Queensland for both research and education. ...

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• Night Sky Images
• University of Louisville Observatory at Mt. Kent in Queensland Australia
• Remote Access to Mt. Kent Observatory in Queensland Australia

... 1999 . I полугодие . 2000 . ... 2001 . ... 2002 . ... 2003 . ... 2015 . ... Последнее обновление: 28/12/2015 ...

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• HD965
• Measurement of the dark halo shape in polar ring galaxies

... The choice of the spectrograph design (Fig.2) is determined by the quantity R, the overall dimensions of the PF cage and the restrictions on the rigidity of the structure of the device. ... As the camera's objective a fast 4-lens aplanat is used having a focal distance F cam =140 mm and a relative aperture of 1:1.8, the resolution at the centre is no less than 80 gr/mm, that over the field at a distance of 3 mm from the edge along the frame ( ) diagonal is 35 gr/mm. ...

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Astronotes Armagh Planetarium's Stellar Blog! ... Armagh Planetarium . ... Space Flight . ... Posted on August 7, 2012 | No Comments The summer months have been particularly uneventful, or more so the events have been hard to spot in the bright summer nights but the month of August has some amazing [ ] . Continue Reading.. ... 2 Comments ItтАЩs the beautiful clear morning of 6 June 2012 here in Armagh and the Sun is rising into a cerulean blue sky.But look closer, and you can see a tiny [ ] . ...

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• observing | Astronotes - Part 9
• observing | Astronotes
• observing | Astronotes - Part 5

... NICS will be the only infrared instrument for the first light of the TNG; as a consequence, we decided to incorporate a sufficient degree of operation flexibility by providing the instrument with six different observing modes, three aimed at imaging and three at spectroscopy: . ... It will be possible to use the narrow band filters as order sorters; this will allow to perform high resolution long-slit spectroscopy in the wavelength ranges covered by the available narrow band filters. ...

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• Autocorrelatore Digitale a Larga Banda
• IBIS: SolarNet Access
• Index of /~gcauzzi/SOLARNET/SN.2013.1.06/21Aug2013/observing_logs

... Fitting the observed dependence includes calculations of the polarization cross-sections averaged over particles orientation and size distribution, their normalization and the comparison of obtained dependencies with Serkowski's curve representing observational data for a chosen star. ... Variations of the polarization factors with wavelength are shown in Fig. 16 for homogeneous spheroidal particles with PF orientation. ... The distinction between prolate and oblate spheroids is also clearly seen. ...

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• Circular polarization: change of sign
• Database of interstellar extinction and polarization curves

... Up: Telescope and Instrument Control Systems . ... The software is based on a client/server architecture and provides remote access for controlling, monitoring and troubleshooting the array. ... The server software is developed in C++ and runs on a UNIX host machine. ... This computer demonstration consists of remote observing with the Caltech Millimeter Array located at Owens Valley in California to show the feasibility and features of this software package. ... Figure 2: Array Status window. ...

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• Electronic Submission of HST Phase I Observing Proposals
• Data Structure and Software of the UCAC-S Project
• The NOAO Web-based Observing Proposal System

... A Partial Eclipse Over Manila Bay . ... An eclipse! ... In particular the above image, taken from the Mall of Asia seawall, caught a partially eclipsed Sun setting over Manila Bay in the Philippines. ... GALEX: The Andromeda Galaxy . ... A mere 2.5 million light-years away, the Andromeda Galaxy really is just next door as large galaxy's go. ... In fact, while the spiky foreground stars are hundreds of light-years distant, the Hydra Cluster galaxies are over 100 million light-years away. ...

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RADIOASTROPHYSICAL DEPARTMENT • INSTITUTE OF SOLAR-TERRESTRIAL PHYSICS RAS SB . Research results on fast active processes General information Main characteristics of the Radio telescope Observing programs General view of the antenna array Main research areas Principle of generation of radio images Radio telescope's beam Receiving systems Main characteristics of the base receiving-recording complex Calibrations Data archive and databases ... Distribution of the recorded spikes in duration . ...

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Space Radio Telescope . The space radio telescope antenna consists of a deployable parabolic reflector (10-m diameter) which is made of 27 carbon fiber petals and central solid portion (3 m in diameter). The radio telescope has focus to diameter ratio F/D=0.43 and overall RMS surface accuracy 0.7 mm. ... A concentric feed arrangement at prime focus will provide the possibility of observing at two frequencies or two circular polarizations simultaneously. ... Observing frequency (MHz) . ...

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• RSOG Pre-Observation Products
• RadioAstron meetings

... International Astronomical Union . Russian Foundation for Basic Research . Abastumani Astrophysical Observatory . Australian Astronomical Observatory . ... Byurakan Astrophysical Observatory . Hartebeesthoek Radio Astronomy Observatory . ... National Radio Astronomy Observatory . Nobeyama Radio Observatory . ... Pushchino Radio Astronomy Observatory . ... AGU journals . ... Astronomy and Astrophysics Springer . ... Astronomy Letters (ПАЖ) . ... Astrophysical Journal Letters . ...

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• G. Rudnitskij's Links

... Sun as a Source of Perturbation of Near-Earth Medium and Solar System Bodies. ... Tidal Influence of the Sun on the Earth. ... Structure of Solar Atmosphere. ... Observing Manifestations of Solar Activity. ... Forecasting of Solar Activity. ... Influence of Solar Activity on the Structure and Dynamics of Terrestrial Atmosphere. ... Problem of Mechanism of Solar-Troposphere Connections. ... Phenomenons in Auroral Zones of the Earth as a Result of the Sun Influence on the Terrestrial Atmosphere. ...

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• Physics of Heliosphere
• SPECTRUM ANALYZER OF MAGNETIC PHENOMENA SAMW
• SET OF MAGNETIC AND ELECTRIC FIELD DETECTORS EXO-EM

... Chandra Survey . ... Fields Observed . ... X-ray Database . ... Bulge Windows Survey . Bulge Latitude Survey . ... The ChaMPlane survey is being conducted at the Harvard-Smithsonian Center for Astrophysics. Date Instrument Fields ---------- ---------------- ------------------------------------- 2004-06 Magellan + PANIC Galactic Center 10'x10', JHKBg 2005-07 CTIO4m + ISPI Wang Fields, GC, JHK 2006-07 CTIO4m + ISPI Bulge-Latitude Strip South, GC, JHKBg 2006-08 Magellan + PANIC GC, K,J,Bg . ...

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• V. Kashyap and J. Drake Figure 1a - Interactive Figure Using the Ov Applet

... This applet generates an observing list based on an observer's location and time. ... To use this program, enter in your location, and the local times at which you wish to begin and end observing. The date you enter should correspond to the calendar day at the time at which you begin observing. For example, if you wish to observe from 9:37 PM October 23, 2007 until 3:21 AM October 24, 2007, you would enter 21:37 for the starting time, 03:21 for the finish time, and 10/23/2007 for the date. ...

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... Under certain conditions, like those in the nucleus of a QSO, all atoms can be made to emit light at particular wavelengths. ... If that source is approaching the observer, the wave is squashed up onto itself making the wavelength shorter. ... This is redshift. ... You can see how the section of the QSO spectrum which we observe changes with redshift. ... We then see how far we had to slide the observed spectrum along the scale to make it match and that is the objects redshift. ... The 2QZ team . ...

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NMW survey overview . Access image archive . ... The New Milky Way survey aims to detect bright (V<13.5) optical transients near the Galactic plane using an automated wide-field (8x6 deg.) system capable of surveying the whole Milky Way area visible from the observing site in one night. ... All images obtained during the transient search survey are available online (please use the image archive access form ). ... Images per field: . ... Images per night: . ... Milky Way imaging time: . ...

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