... The Real Reality Show: Would aliens be anything like us? ... The Real Reality Show: All about the Drake Equation . ... The Real Reality Show . ... Why is one of the three filters in the Hubble palette ionized sulfur? Is Sulfur really that prevalent in the universe? ... RELATED TOPICS: SULFUR . Sulfur is not terribly abundant in the universe. ... Get instant access to subscriber content on Astronomy.com! ... If you are already registered on Astronomy.com, please log in below. ...

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• Hubble observes galaxies' evolution in slow motion | Astronomy.com
• Hubble observes a dwarf galaxy with a bright nebula | Astronomy.com
• Baby galaxy isn't so young | Astronomy.com

... astro-ph . ... We present the goals and preliminary results of an unbiased, near-infrared, narrow-band imaging survey of the First Galactic Quadrant (10deg<l<65deg ; -1.3deg<b<+1.3deg). ... We publish 16 Doppler imaging temperature maps for the years 1994-2002 of the active RS CVn star II Peg. ... Through Doppler imaging we want to study the spot evolution of the star and in particular compare this with previous results showing a cyclic spot behaviour and persistent active longitudes. ...

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In autumn 1994, two groups of astronomers announced that they had discovered Cepheid variable stars in a distant cluster of galaxies. ... As the term suggests, variable stars change in brightness over time. ... Variable stars are an ideal way to get high-school students doing real science, with real data, from the real sky. ... a sky chart to find the stars . ... Students can use the nearby stars to estimate the magnitude of Delta. ... Locate the star Delta in Cepheus and estimate its brightness . ...

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• ASP: A Taste of Real Astronomy ? The ESA/ESO Astronomy Exercises
• ASP: Light Pollution
• ASP: Eclipse Watching: Making a Solar Filter

A computer controlled low light photometer for nightglow observations. Hardware units of portable photometer for low light measurements, especially night glow emission is described. ... Interface card contain three channels of 24 bit counter, 4 channels of 12 bit ADC and the buffer bus for the controlled motors of the altazimuthal fork mounting and filters wheel, the position encoders. ... Where N( ) is output signal photometer generated input light flux F( l ) . ... PMT # . 599 . ...

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• EVOLUTION OF SHELLS (SPIRAL JETS)

Chapter 11. Specifying OpenGL Environment Variable Settings . ... Several antialiasing methods are available and you can select between them by setting the __GL_FSAA_MODE environment variable appropriately. ... To see the available values for __GL_FSAA_MODE along with their descriptions, run: nvidia-settings --query=fsaa --verbose . The __GL_FSAA_MODE environment variable uses the same integer values that are used to configure FSAA through nvidia-settings and the NV-CONTROL X extension. ...

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• The Pleiades
• Technical Data for the Arecibo Airglow and Optical Instrumentation
• Thesis Figures

... Общероссийская неделя "Астрономия на тротуаре" - 15-17 апреля . ... Новости астрономии и космонавтики (Модераторы: Karen , recarrion , LeMay ) ? А кто это так бумкнул?" (с) . ... 20.06.2006 [09:40:21] ? http://lenta.ru/news/2006/06/19/supersupernovae/ . ... No. c546 (15 June 2006) . VARIABLE OBJECT IN BOOTES . ... The new variable has . ... magnitudes for the new variable: 2006 Jan. 29 (and two earlier images, . ... Selected F775W magnitudes for the new variable: 2006 Jan. ...

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• arxiv:0705.4195 VSOP: The Variable Star One-shot Project - Научная панорама

PhD Thesis (PDF) . ... The evolution of stars and gas in galaxies. Observing the atomic neutral hydrogen (HI) 21 cm emission and radio continuum emission of galaxies. ... The goal of research is to quantify the neutral atomic hydrogen (HI) gas content galaxies as they evolve with time. ... Neutral atomic hydrogen gas produces a radio signal that can be used to directly measure the amount of gas present. ... USyd Summer Research Scholarship Report (PDF) . ... Research Topic Write Up (PDF) . ...

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• Dopita Papers
• GSAOI Bulk Motions Science Page
• Emma Kirby - Science

... There are preliminary series of photometric and radio spectral observations of the above-mentioned stars, archival data on the light curves of the stars, results of the search for OH and H 2 O maser emission in IRAS point sources that possess the IR parameters similar to Miras. ... The aim is a detailed study of the maser emission variability. ... In 1996-1997, astronomical observations of Mira Ceti-type stars (miras) were carried out in three spectral ranges: optical, infrared, and radio. ...

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• Rudnitskij Georgij M. Home Page
• Dm. Bizyaev's Publications

... Fractional flux density variations of between 5 and 100 per cent (typically 15-25 per cent) have been detected on a range of time-scales from 1 to 12 years. ... The 151-MHz flux densities have been indirectly scaled to the 6C flux scale. ... Amongst the 72 sources for which the chance of being a true variable is greater than 0.8, typical maximum flux density variations of 15-25 per cent are seen; eight objects show variations greater than 50 per cent, with one source varying by more than 100 per...

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• Variable radio sources
• "Structure" publications in 1996 year
• Individual data

... Summary: PmWiki group header. ... Summary:Variables used for uploads/attachments:) . ... This array contains forbidden strings for an uploaded file (case insensitive). ... This variable sets additional unix permissions applied to newly uploaded files, and should be 0 (recommended as of 2013). ... This variable sets unix permissions unconditionally applied to newly uploaded files, for example 0604 . ... Sets the prefix for uploaded files to allow attachments to be organized other than by groups. ...

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• Dispersion Removal
• The SM Tutorial - How do I define variables, and how can I use them?
• Definitions of Of stars, WR stars, and LBVs

... We have compiled the Catalogue of extragalactic supernovae using the GCVS card catalogue. ... Doubtful (?), or rejected (-) SN 8 A1 --- RemFlag [*] The '*' indicates a remark in sn_rem.dat 10- 19 A10 --- Gal Parent galaxy designation 21- 22 I2 h RAh Right Ascension 1950 of Parent galaxy 23- 24 I2 min RAm Right Ascension 1950 (minutes) 25- 28 F4.1 s RAs Right Ascension 1950 (seconds) 29 A1 --- DE- Declination 1950 (sign) 30- 31 I2 deg DEd Declination 1950 of Parent ...

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• http://www.sai.msu.su/gcvs/gcvs/GCVS5/ReadMe.txt
• http://www.sai.msu.su/gcvs/gcvs/v/readme
• General Catalogue of Variable Stars: Vols I-III (the new electronic version).

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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Lab . Main page News People . ASA . Master . Master net Homepage . ... Lomonosov Moscow State University Sternberg Astronomical Institute . ... MASTER . ... Lomonosov (ShOK) . ... About Space Monitoring Laboratory, scientific directions, instruments, contacts . People, who work in lab . Latest news and news archive . ... GRB 100131A: MASTER-Amur alert observations 76 sec after Notice time.The limit of the main telescope images is aboute 15 mag (unfiltered). ... All news ...

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... Parameter . ... Type . ... data set . ... The name of the observation-wide attitude time series data set created by atthkgen . ... name of existing D -type column in attset . The name of the column in the attitude data set containing the time tags - passed to tabgtigen in parameter timecolumn . ... A selection switch which determines the type of selection expression that the attitude time series is filtered with. cone and pyramid select the fixed cone- and pyramid filters (see above) respectively. ...

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• Generation from In-Orbit Data
• XMM-Newton OM Response Files Page

... Dept. for Physics of Stars&Galaxies . ... Using a database view Sloan Digital Sky Survey (SDSS), containing almost a million spectra created 15,000 sample galaxies with active star formation, which is used for various studies and physical state of evolution of galaxies. ... Star clusters of the Galaxy . The project MWSC (Milky Way Star Clusters) directory using 2MASS, which includes nearly 500 million vision to the limit Ks = 15.3, analyzed more than 4,000 cluster-like objects in the galaxy. ...

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• Dept. for Physics of Stars&Galaxies

Next: Large Scale Clustering in the Universe - A Package of Codes . ... The discovery of a correlation between the light curve shape and intrinsic brightness has made Type Ia supernovae exceptionally accurate distance indicators out to cosmologically interesting redshifts. ... But supernovae are relatively rare events. ... Type Ia supernovae make excellent distance indicators, so these events at high redshift can be used to map out the history of the expanding Universe. ...

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• A Method for Visualizing Time Variability in X-Ray Images
• ADASS 2002 Conference Proceedings
• ADASS 2003 Conference Proceedings

... The study of the Large-scale structure of the Universe and measurements of the Dark Energy equation of state; The exploration of the growth and cosmological evolution of supermassive Black holes in the Universe. ... In course of the all sky survey SRG will discover about 100 000 galaxy clusters and 3 million AGNs. Galaxy clusters are the largest gravitationally bounded objects in the Universe and are best explored through the study of X-ray emission from the hot intergalactic gas. ... 2016 IKI RAN ...

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• Second Spectrum-RG/eROSITA Conference
• GRANAT Home Page
• The best images from RTT150

... The clustering of galaxies is usually described in terms of two-point correlation functions (r) and (). ... 2007): Evolution of the galaxy structure Morphological evolution Evolution of the galaxy structure Morphological evolution Abraham van den Bergh (2001): Evolution of the galaxy structure Radial surface brightness of spiral galaxies Evolution of the galaxy structure Radial surface brightness of spiral galaxies Evolution of the galaxy ...

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• http://www.astro.spbu.ru/staff/resh/Lectures/lec6.pdf
• http://www.astro.spbu.ru/staff/ilin2/INTAS2/PAP/P6_5.pdf
• http://www.astro.spbu.ru/staff/afk/Papers/2006/delOriE.pdf

The project of the informational system creation on the problem of evolution of radio galaxies, as a part of the "Big Trio" project aimed on studing of distant radio galaxies, is designed. This system allows a user to operate with simulated curves of spectral energy distributions (SED) to estimate ages and redshifts by photometry data. Authors use SEDs of several models for different types of galaxies. ... The HTTP and e-mail access is organized to this system. ...

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• astro-ph authors/title/abstract search for 'galaxy cluster' (skipped 200) all
• Description of SED models
• Radio galaxies

THE 75th NAME-LIST OF VARIABLE STARS. ... The 75th Name-List consists of two tables. ... the literature, taken from positional catalogues, including USNO A1.0/A2.0 and GSC, or determined by the authors); the range of variability (sometimes the column Min gives, in parentheses, the amplitude of light variation; the symbol ( means that the star , in minimum light, becomes fainter, than the magnitude indicated); and the system of magnitudes used ( P are photographic ...

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• http://www.sai.msu.su/gcvs/gcvs/nl74/readme
• Moscow Astronomical Plate Archives: Contents, Digitization, Current and