There are still many open questions on galaxy formation and evolution, such as e.g. the predominance of hierarchical or monolithic processes in the galaxy formation or the temporal evolution of disk metallicity gradients. ... Chemical abundances of stellar populations of different ages are essential to constrain the past history of nearby galaxies, both in terms of their past metal contents and of SFHs. ...

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• Displaying Errors with the JavaScript Console
• The Hubble Deep Field
• dbmmanage - Manage user authentication files in DBM format - Apache HTTP Server

Astronomy Picture of the Day . Jupiter's Auroras . ... 18.10.1996 . ... HST , NASA Explanation: Auroras are especially large on Jupiter. In pictures released yesterday, the Hubble Space Telescope imaged these unusual light displays in more detail than ever before. ... The resulting auroral displays may be thousands of times brighter than any auroral display on Earth , and involve unusual spots. ... U. Based on Astronomy Picture Of the Day . Publications with keywords: Jupiter . ...

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• Journal "Peremennye Zvezdy"
• Astronet > Sky Map, professional edition
• XWare > APOD

... Bit Fields . Bit Fields: Practical Example . ... NOTE: The combination of pointers and bit-level operators makes C useful for many low level applications and can almost replace assembly code. ... To illustrate many points of bitwise operators let us write a function, Bitcount , that counts bits set to 1 in an 8 bit number ( unsigned char ) passed as an argument to the function. int bitcount(unsigned char x) { int count; for (count=0; x != 0; x>>=1); if ( x & 01) count++; return count; } . ...

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• Principles of organization
• File Locking
• Running UNIX Commands from C

The 2dF QSO Redshift Survey (2QZ) . ... Before jumping into all the finer details of teh survey, a brief non-astronomer's guide to redshift surveys is available. ... The primary scientific aims of the QSO survey are: (1) to obtain the primordial fluctuation power spectrum out to COBE scales, (2) to determine the rate of QSO clustering evolution in the non-linear and linear regimes and hence obtain new limits on the value of and the bias parameter, (3) to apply a powerful geometric method to measure . ...

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... Spectral regions highlighted by green bars have been used to detemine the тЯиB z тЯй value from H Balmer lines, and the magenta bars highlight the spectral regions used to estimate the magnetic field from metal lines. ... The FORS1 instrument of the ESO Very Large Telescope was used to obtain low resolution circular polarized spectra of nearly a thousand of different stars, with the aim of measuring their mean longitudinal magnetic fields. ...

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• Online materials for the coronal holes brightening events paper
• M.D. Smith, Research Astronomer

... xntpd is an operating system daemon which sets and maintains the system time-of-day in synchronism with Internet standard time servers. xntpd is a complete implementation of the Network Time Protocol (NTP) version 3, as defined by RFC-1305, but also retains compatibility with version 1 and 2 servers as defined by RFC- 1059 and RFC-1119, respectively. xntpd does all computations in 64-bit fixed point arithmetic and requires no floating point support. ... Specify the name and path of the log file. ...

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• Psql support
• Monitoring Options
• APOD: September 15, 1998 - The NTT SUSI Deep Field

... Detailed information about each program can be found in the separate manual pages. blockmean L2 (x,y,z) data filter/decimator blockmedian L1 (x,y,z) data filter/decimator blockmode Mode (x,y,z) data filter/decimator filter1d Filter 1-D data sets (time series) fitcircle Finds the best-fitting great circle for a set of points gmtconvert Convert between ASCII and binary 1-D ... Wessel, P., and W. H. F. Smith, 1991, Free Software Helps Map and Display Data, EOS Trans., ...

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• The Environment of the Rotator
• Константин Александрович Постнов
• Seminars

Next: STScI NICMOS Software Up: NICMOS Data Calibration and Previous: Some Experiments with the . ... Programs Available . ... Display . ... E. Stobie, D. Lytle, I. Barg, and A. Ferro NICMOS Project, University of Arizona, Tucson, AZ 85721, E-mail: bstobie@as.arizona.edu . The NICMOS Software Group at the University of Arizona has built a number of software tools for processing NICMOS data. ... NICMOS, PSF subtraction, image registration, image deconvolution, polarimetry data reduction . ...

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• STScI NICMOS Software
• ST-ECF Grism Spectrum Software for NICMOS Grism Data
• NICMOS Data Calibration and Analysis

OptInt PmWiki : MROI Fast Tip Tilt / Tech Meet 12 . ... Open Design Issues . Choose ISS interface flavour: "C" (threads/processes)/"C-no-threads" (event loop) . ... GraphicalInterface and LocalDataCollector grouped into single process . ... ISS Data Collector probably not suitable as LocalDataCollector (e.g. issues with retrieval of recorded data), and unlikely to be ready in time . ... Printable View of http://www.mrao.cam.ac.uk/projects/OAS/pmwiki/pmwiki.php/MROIFastTipTilt/TechMeet12) ...

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• NVSS Postage Stamp Server Documentation Help for NVSS Postage Stamp Server
• DUST: Dust::MMPUV Class Reference
• VLSS Postage Stamp Server Documentation Help for VLSS Postage Stamp Server

filecommander (2.50-alpha2) lenny; urgency=low * Alpha 2 - Add support for XZ compressed files. Fix detection of same source & destination volumes when moving files from File Find's search results. ... Stop function key bar being left blank after executing an external command, especially an archiver command to update an edited file in an archive. Fix infinite loop when Delete All Read-Only is selected and a read-only file can't be deleted. ... Fix sorting of unicode file names in the panels. ...

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• http://crydee.sai.msu.ru/ftproot/pub/comp/software/silk/fcl/filecommander_2.50-alpha3_amd64.changelog
• Adding Variables to CONFIG.SYS
• ApSA courses

... 2014: . Suppression of cooling by strong magnetic fields in white dwarf stars . ... 69, 439, 2014. Evidence of supercritical accretion in SS433 . ... We discovered a flat portion (white noise) in the power spectrum of SS433 due to an abrupt increase of the disk thickness in the supercritical region. ... Both the hard X-ray radiation and the visual light are seen reflected from the walls of the funnel that forms in the wind of the supercritical disk of SS433. ... Archive . ...

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• Galaxy sector, archive 2012
• HD965
• topic_en

... SADT CASE- Bpwin (AllFusion Process Modeler) Erwin (AllFusion Erwin Data Modeler) Computer Associates, , . ... SADT IDEF0, CASE- BPWin. 34.003-90 ". " (automated system, ) ­ , , . ... 8 Tools/Reports/Model Report. ... ERwin , « » : · Column Reports ­ ; · Attribute Reports ­ ; · Entity Reports ­ , ; · Domain Reports ­ ; · Table Reports ­ ; · Subject Area Reports ­ ; · Model Validation Reports ­ ; 33 · Stored Procedure Reports ­ ; · Relationship Reports ­ ; · View Reports ­ ; · ERWin Volume Reports ­ ...

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• SSAU will develop international cooperation in the field of additive
• Breakthrough in the field of information
• Leading experts in the field of engine dynamics and vibroacoustics will gather

Operating Instructions Starlock PEC Utility Tool For use with Meade Starlock Equipped Telescopes Only PEC Utility The PEC Utility Tool allows you greater control over the Periodic Error Correction functions of your Starlock equipped telescope. ... Sharpening: The sharpening function makes the error corrections determined by Starlock be applied more aggressively while chasing small variations in the tracking. ... Sharpening, on the other hand, tends to increase the magnitude of the corrections applied. ...

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• Meade 16" Super Giant LX Field Tripod
• Meade Giant Field Tripod
• Meade Standard Field Tripod

It is possible to piece together the processes that have shaped the observed characteristics of a galaxy by studying its stars in detail. The Large Magellanic Cloud (LMC) is an excellent candidate for this type of study because of its favourable viewing angle and ongoing star formation. I present the results of high-resolution VLT/FLAMES observations of ~80 red giant stars around star cluster NGC 1846, located in the disc of the LMC. ...

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• http://www.mso.anu.edu.au/seminars/abstracts/20150326-1100.html
• COALA - Computational Astrophysics Laboratory
• Raquel Salmeron - Research Interests and Experience

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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... It is found that the correlation coefficients between these two parameters calculated separately inside and outside the sunspot formation zone ±30 have cyclic variation and occur in anti-phase. This suggests different mechanisms of formation of the corona in the fields of small, medium, and large scales. ... The relationship between the coronal green line brightness (CGLB) and the magnetic field strength (MFS) has been investigated by constructing the corresponding synoptic maps for the 1977-2001. ...

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• http://www.izmiran.rssi.ru/~obridko/papers/2009ASPC_405_205C.pdf
• http://www.izmiran.rssi.ru/~obridko/papers/2007ASPC_368_245I
• http://www.izmiran.rssi.ru/~obridko/papers/2004IAUS_223_69B.pdf

SET OF MAGNETIC AND ELECTRIC FIELD DETECTORS EXO-EM . ... 3 components measurements of both magnetic and electric fields; . ... wide frequency range (0 - 10000) Hz; . ... ECHO-EM is intended for measurement of a complete vector and three components of both electric and magnetic fields, and transfers the received data to the block of the processing of the information and also in telemetry. ... digital 0.1-20 Hz; . ... frequency band (0.01- 10000) Hz; . ... digital (500 - 1000) Hz; . ...

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• Wave Processes in Inhomogeneous Plasma
• Satellite Data Processing
• Researches of Astronomy and Space Physics Department

M obile A stronomical Sy stem of TE lescope- R obots MASTER-II Kislovodsk Lomonosov Moscow State University, Sternberg Astronomical Institute , Moscow Union "Optic" , Kislovodsk Solar Station Latitude = 43 o љ44'.767љN; Longitude = 42 o љ31'.417љE; Altitude = 2067љm MASTERљIIљ(8љsquareљdegress) + MASTERљVWF(VeryљWideљFieldљCameras (FOV=800 square degrees, Timeљresolutionљupљtoљ150љms, with unfiltered m_lim=14m on 5 sec. exposure, and ~10.5m with 0.15 sec) . ... 11h 38m 38.0s , -09d 59m 59s) . ...

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... Exposure Time Calculator (ETC) . Survey processing . ... VISTA is a 4-m class wide field survey telescope for the southern hemisphere, equipped with a near infrared camera (1.65 degree diameter field of view at VISTA's nominal pixel size) containing 67 million pixels of mean size 0.34 arcsec and available broad band filters at Z,Y,J,H,K s and a narrow band filter at 1.18 micron. A wide field visible camera, if constructed, could also be used on VISTA. ... Tile . ... ESO VISTA Public Surveys . ...

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. Newly reprocessed archival data from STEREO-A/SECCHI show details of the first Earth-directed coronal mass ejection of the STEREO mission, from inception December 12, 2008, to Earth impact December 15, 2008. New processing enables following the details of the CME with the wide-field heliospheric imager cameras out to impact with the Earth 93 million miles (150 million km) from the Sun. Courtesy SwRI/NASA

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• Pluto's complex terrain on display | Astronomy.com
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• NASA's Ames Research Center in Moffett Field, California | Astronomy.com