... 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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... About ATNF overview . ... Australia Telescope Steering Committee . ... Murchison Radio-astronomy Observatory . ... Parkes radio telescope . ... Australia Telescope 20GHz Survey . ... Bright prospects: Comparing the H Survey with large-scale radio continuum emission . ... Prospects for comparisons between the AAO/UKST H \ survey and large-scale radio continuum emission are considered, with particular reference to the recently completed Parkes 2.4-GHz survey of the southern Galactic Plane. ...

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• LMC HII Region Luminosities versus Observed Ionizing Stars
• Problems with the details of the treaty
• Australia Telescope National Facility

... the time of observation . ... Observing the Changing Position of the Sun To Establish Cardinal Directions . ... Observations of the Sun's apparent movement across the sky and its pattern of rising and setting in the east and west horizon helped to establish the cardinal directions. ... The final stage of the Sun's return was marked by the observation that the Sun had reached its highest altitude when the full width of your mitted hand could fill the gap between the Sun and the horizon. ...

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• ASP: Star Science in the Autumn Sky
• ASP: Up, Up, and Away
• ASP: A Taste of Real Astronomy ? The ESA/ESO Astronomy Exercises

... HST Overview . ... First on-orbit absolute photometric calibrations for NICMOS were obtained during SMOV. The results of these limited calibrations were used to establish in July 1997 preliminary corrections to the predicted photometry based on ground-based vacuum measurements. ... To quantify the accuracy in the absolute photometry, the observed/predicted countrate ratios for NIC1 , NIC2 and NIC3 filters have been computed with SYNPHOT after photometric corrections for each camera were applied. ...

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• compare_table.pro
• Convolving data models with PSF models
• Projects and Papers

... Data is taken from Hilton (2011): Active M3-M5, 332 hours on 4 stars observing 157 flares; Active M6-M8, 59 hours on 4 stars observing 39 flares; Less Active M3тАУM5, 147 hrs on 8 stars observing 28 flares; Inactive M0-M2, 256 hours on 16 stars observing 9 flares; Inactive M3-M5, 153 hours on 6 stars observing 3 flares; Active M0-M1, data from Moffett (1974), Doyle Mathiouidakis (1990) and Dal Evren (2011), 156 hours on 2 stars observing 63 flares. ...

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• Observations with the Faulkes Telescopes
• Solar Eclipse Observed Armagh Observatory
• Gary, Callum and Peter: `Stars' of the Future

Winer Observatory P.O. Box 797, Sonoita, Arizona 85637-0797, USA . ... 2/3-m Telescope . ... Site . ... Commanding . ... In a typical robotic observing scenario, each afternoon, a telescope control computer obtains a set of objects to observe from its home institution from a command or script file. ... The file is then transferred to the telescope control computer at the Winer Observatory in Sonoita. ... The Iowa control computer then begins processing the telrun.sls file. ... 2013 Winer Observatory. ...

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• Winer Observatory
• Winer Observatory Operations
• Winer Observatory - Our Science

... For each observed position the table contains designation of object as in file of observations, the time of observation, the number and name/ preliminary designation of minor planet supposedly identical with observed object, the values of O – C (observed position minus computed one) in right ascension and declination expressed in arcsec, the difference O – C between observed magnitude and computed one, the code of observatory in the Observatory list (see Observatories section). ...

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RADIOASTROPHYSICAL DEPARTMENT • INSTITUTE OF SOLAR-TERRESTRIAL PHYSICS RAS SB . Data processing and software 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 Publication of SSRT - Data processing and software . ...

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... Radio astronomers at Arecibo Observatory observe a wide variety of phenomena in the Milky Way and in other galaxies. ... Some REU projects are carried out on pre-existing data, and others rely on obtaining new data. ... Deriving a new shape model from existing radar images has been a popular student project in past years, and there are data sets that could be used for this. We are collecting thermal infrared emission data for many of the near-Earth asteroids that are also observed with radar. ...

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• Astronomy at Arecibo Observatory
• National Astronomy and Ionosphere Center (Arecibo Observatory)
• The CIMA Homepage

... The nebular spectra of SNeIa can be used to determine the mass, density, and distribution of the SN ejecta, and the distance and reddening to the SN. Synthetic spectra can very rapidly be computed in NLTE and compared to the observed ones. Given the relatively large number of parameters, it is convenient to explore the parameter space in an automated form. The nebular spectrum synthesis code can be run in parallel on a workstation cluster. ...

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• ADASS 2003 Conference Proceedings
• ADASS 2002 Conference Proceedings
• AIRY: Astronomical Image Restoration in interferometrY

... Science . ... Science Users Information Science Software ESO-MIDAS jump to navigation jump to content . ... Science Software . ... ESO-MIDAS . ... ESO-MIDAS uses software standards provided by most computer manufactures, and runs on UNIX or Linux based platforms, as well as on Mac OSX systems. ... RedHat based, e.g. Scientific Linux, CentOS . ... Ubuntu based, e.g. Kubuntu, Ultimate Edition, Linux Mint . ... Debian based, e.g. aptosid . ... based on Linux/X11 emulation software Cygwin_NT-5.1 . ...

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• ESO - The Origin and Fate of the Sun: Evolution of Solar-mass Stars Observed
• ESO - Laser Guide Stars Facility
• ESO - Science Software

... Right: The telescope's octagonal "dome" enclosure. ... MT KENT OBSERVATORY (longitude 1510 51' 19.5 E, latitude 270 S 47' 52.3 , elevation 682 m) Louisville Telescope ( Robotic astronomy research) · 50cm f/6.8 astrograph Celestron C-20 (new product) Supplier : www.celestron.com · 3.5m Sirius fibreglass dome Supplier : siriusobservatories.com · SBIG STL-6303 CCD camera + LRGB filters (UBVRI planned) Supplier : www.sbig.com · Vantage Pro weather station ...

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• http://www.astro.louisville.edu/information/asa2007.pdf
• Student Telescope at Moore Observatory
• Moore Observatory's XmCCD Supporting Software

Peremennye Zvezdy", . ... GSC 4232-02515, NSVS 3147658, NSVS 3174760 . ... 14.2-14.9 (R, NSVS); . ... During observations of a secondary eclipse of GSC 04232-02830 (Goranskij et al., 2005) on August 8, 2007, we identified GSC 4232-02515 as a W UMa eclipsing binary. ... VAST software was used for aperture photometry. ... This method produces a light curve with an arbitrary zero point. ... Light Curve . Light curve of GSC 4232-02515 in NSVS magnitude scale. ... gsc423202515_kadar_nsvs.dat . ...

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• XWare > APOD

... The computer is set up so that the software for whatever camera is running and the switch box set to channel B. This allows the monitor and keyboard upstairs to operate the computer. Now the telescope can be set up. ... In the North west of the dome, there is a motor that turns the dome. The dome opens with a motor that pulls the slit back. ... Each camera had a specific alignment with the telescope. ... The lights on the roof provide a nice target to center in all three telescopes. ...

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• ChaMPlane data_archive_.html
• The AstroStat Slog VO
• The AstroStat Slog PDF

... In order to compare the number of different evolutionary stages obtained and X-ray luminosity of the chosen X-ray sources with the observed galactic values we use the sum of C/O+O/C , where C and O are the calculated and observed values of a given binary type, respectively. If we make comparison for a number of different binary species (for example, we compare the number of CV, number of X-ray pulsars,   total X-ray luminosity of LMXB, etc.), we write this criterion in the form: . ...

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• Evolution of the Double Neutron Star Merging Rate andthe Cosmological Origin of
• Introduction
• Discussion and conclusions

... The Observatory, the cupola of which is 480 cm wide, is equipped with a Ritchey-Cretien 500 mm f/7.5 telescope, a 200 mm f/7.5 guide telescope, and a 250 mm f/13 Baker-Schmidt, a ST4 and a ST6 CCD cameras and four computers. ... Up until now we have archived about 600 images from the first observation, and 100 from the second, thanks to the automatic telescope aiming control program written by Vairo Risoldi. ... A.Nakamura, Japan, took CCD image of NGC5775. ...

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• Light Curve Templete/Observing Form For Visual SNe Observers.
• APOD: November 24, 1998 - Seven Leonids Over Wise Observatory
• Sternberg Astronomical Institute

Astronomy . ... Institutions, Observatories . ... International Astronomical Union . ... 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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. Pulkovo Observatory of Russian Academy of Sciences is situated . near Saint-Petersburg. It was founded in 1839. 196140, Saint-Petersburg, Pulkovskoye chaussee 65/1 . English version . Russian version . This page has been accessed times since May 1, 1999.

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• Pulkovo NEO Page: Ephemeris Support
• Pulkovo NEO Page: Estimation of Accuracy of the Observations

... Дни открытых дверей к юбилею САО РАН (12-14 апреля 2016 г.) . Международная конференция "Dark Ages and White Nights (Spectroscopy of the CMB)" (20-24 июня 2016 г.) . ... Международная конференция MULTI-SPIN GALAXIES - 2016 (26-30 сентября 2016 г.) . Международная астрономическая конференция "Физика звезд: от коллапса до коллапса" (3-7 октября 2016 г.) Архив . ... Подробнее.. ... 10.02.16 . ... БТА в реальном времени . ... Цейсс-1000 в реальном времени . ... Последнее обновление: 22/03/2016 ...

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• Lack of Dwarf Galaxies in the Local Volume Compared to Conventional Cosmology
• Solar eclipse 2015

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