... SERENDIP IV, the latest SERENDIP instrument, consists of 40 spectrum analyzer boards working in parallel to look at 168 million narrow (0.6Hz) channels every 1.7 seconds. ... We installed SERENDIP IV at the Arecibo Observatory on June 11, 1997, and have been since receiving raw data from the observatory at the rate of one megabyte every four minutes. ... The SERENDIP I instrument consisted of a 100-channel spectrum analyzer which was located at UC Berkeley's Hat Creek Observatory. ...

... Telescopes . ... Method "Spectroscopy with the Main Stellar Spectrograph (MSS) of the BTA" . ... The MSS of the 6-m BTA telescope is a long-slit spectrograph, stationary installed in the rack of the Nasmyth-2 focus (Vasiliev et al. ... Design, engineering and manufacturing of the spectrograph were carried out in parallel with the creation of the BTA telescope. ... Panchuk V.E., SAO Preprint ? ... BTA telescope. ... The main stellar spectrograph, Leningrad: LOMO (1974) (in Russian). ...

... INTERCOSMOS 19 . ... Personnel . Get the data . ... webmaster@izmiran.ru . Team . The ionospheric station ION-1 and the sounder IS-338 installed onboard the Intercosmos-19 were designed and manufactured by talented scientists and engineers of elder generation of IZMIRAN: M.D.Fligel, L.P.Goncharov, Yu.V.Kushnerevsky, and G.V.Vasiliev under supervision of Academician V.V.Migulin. ... Participants in this work were S.P.Gaidash, A.T.Karpachev, and S.A.Pulinets, young researchers at that time. ...

Main News Phones Research area Brief history Institute Structure Experimental Base Observational data English/Russian . research on the site(Google) . ... 7(4112)390400 . Fax: . 7(4112)390450 . ... Station for Receiving of Satellite Information . ... Phone: +7(4112) 390-480 . Fax: +7(4112) 390-450 . Web: (on Russian) . ... Station installed at the Institute. ... The SCANOR station receives data from NOAA satellites in HKPT channels. Переход к сообщению об ошибке и поиску . ...

Winer Observatory P.O. Box 797, Sonoita, Arizona 85637-0797, USA . Home . ... Science . ... Mike Schwartz of Tenagra Observatories installed the equipment shown at left in October, 1998 at Position No. 4 of our Sonoita Facility. ... There were no discoveries between October and the end of 1998, but in early January, 1999 Mike discovered his first supernova remotely (he had discovered seven before at his home in Oregon), and shortly thereafter, discovered yet another. ... 2013 Winer Observatory. ...

... The Science Operation Department is composed of Astronomers, Telescope Instruments Operators(TIOs) and Data Handling Administrators(DHAs). ... Astronomers have proposed several methods to quantitatively measure the amount of turbulence above the telescope, which the most common ones is Differential Image Motion Monitor (DIMM). In optical testing, the Hartmann test is the common method to test the quality of optical components. ... Hartmann mask consists of 48 lenses. ...

[Installer] Title="" Package="3dinput.msi" Version=1.10 Msi9x=instmsi.exe MsiNT=instmsiw.exe Silent=TRUE

ARMAGH PLANETARIUM IN THE 1990s Dawn of the Digistar era This decade saw the arrival of our first digital projector, an Evans & Sutherland Digistar 1. This was a revolutionary new approach to planetarium display equipment. ... This was the first Digistar projector to be installed in the UK. ... In 1994 a new section was added to our building, doubling its size. ... A walk through the stars Our Astropark opened in 1994. ... Armagh's Astropark allows visitors to walk through the Cosmos ...

. The Cygnus commercial resupply craft is installed by the Canadarm2 to the Harmony node. NASA TV

яЁѓ . Les nouveaux panneaux solaires de la Station spatiale d†йploy†йs aujourdтАЩhui . L'un des astronautes de Discovery, lors de la premi†иre sortie dans l'espace pour installer les panneaux solaires. Cr†йdit : Nasa

A Large Programme 171.A-3045 (PI: Cesarsky) has been approved in period 71 to carry out a spectroscopic survey in the CDF-S with VIMOS, now installed on UT3. ... MOS (LR_Blue/MR grisms) . ... The VIMOS coverage of the GOODS field (right). ... With an average integration time of 4h per mask and 30% overheads, this makes a total of 125h. The VIMOS spectroscopic campaign is designed to complement the FORS2 spectroscopic program. ... OII],Hbeta,[OIII],(Halpha),CaII H . ... OII],CaII H CIV,AlIII . ...

... Home Education Classes AAA Winter Astronomy Class: Measuring Distances in Space тАУ Dec 2015 тАУ Feb 2016 . ... Classes . AAA Fall Astronomy Class: Astronomy Basics тАУ October-November 2015 . AAA Winter Astronomy Class: Measuring Distances in Space тАУ Dec 2015 тАУ Feb 2016 . AAA Spring Astronomy Class: The Physics of Astronomy тАУ February - March 2016 . ... This MonthтАЩs Sky тАУ April 2016 . ... Dec. ... Observing Resources for Amateur Astronomers - Part 1: Beginning Observers . ...

. Name . Last modified . Size . Description . Parent Directory . - . attach_update_23x_to_latest.php . 19-Jan-2013 12:53 . 14K . mod_table_inst.php . 19-Jan-2013 12:53 . 7.0K . schemas/ . 19-Jan-2013 12:53 . - . Apache/2.2.15 (CentOS) Server at rp.iszf.irk.ru Port 80

... Regional planning meeting for the Balkan and Black Sea | ... Proposals for a web site of the Regional Network - Information on regional and global activities - Proceedings of this Meeting - Space Weather Alerts for the public - Form for submitting research and observational proposals - Database of scientific data publicly available - Greece provides solar telescope data - Romania provides data on active regions studied with helioseismis holography - Armenia provides access to...

. I measured my limiting magnitude on this picture at about Mag 18.9. I also did some photometry near for the SN positon, and I found a star liked object at about Mag 17.6. I think this object is 1999br. This image is deconvoluted, but I measured the magnitude pre-deconvulution. Kereszty Zsolt . Hungary, Miskolc . Back to Bright Supernovae . David Bishop Last modified: Thu Apr 15 11:44:03 EDT 1999

... Previous: Background Fluctuation Analysis from the Multiscale Entropy . ... A new measure of information is defined which is based on noise modeling and incorporates resolution scale. Properties of this measure are discussed. ... Additionally it allows for image noise modeling, and subsequent noise removal. ... Hence information- and entropy-based processing technologies will be necessary for the effective design and implementation of large, future generation, image databases. ...

We have designed the laboratory model of static Fourier spectrometer for onboard usage for spectral study of atmosphere and ionosphere. The gain of model is to simulate onboard FS which will not have any moving elements (all its optical elements will be mounted at fused quartz monolithic construction), to compare experimental results with theoretical estimations and to measure MTF of CCD array. ... This fact connected with low frequency response of CCD array due to small format of it. ...

To appear in "Fourth Workshop on Robotic Autonomous Observatories (2015)"RevMexAA(SC) MINI-MEGATORTORA WIDE-FIELD MONITORING SYSTEM WITH SUB-SECOND TEMPORAL RESOLUTION: FIRST YEAR OF OPERATION S. Karpov, 1, 3 G . Be s k i n , 1, 3 A. Biryukov4 S. Bondar,2 E. Ivanov,2 E. Katkova,2 A. Perkov,2 and V. Sasyuk RESUMEN 3 Favor de prop orcionar un resumen en espanol. ... The real-time system data analysis pipeline performs automatic detection of rapid transient events, both near-Earth and extragalactic. ...

... VaST is a software tool for finding variable objects on a series of astronomical images. ... VaST performs object detection and aperture photometry using SExtractor on each image, cross-matches lists of detected stars, performs magnitude calibration with respect to the first (reference) image and constructs a lightcurve for each object. ... VaST FITS image viewer ./pgfv . ... Part I" PZP, vol. ... K. V. Sokolovsky, S. A. Korotkiy; "New Variable Stars Discovered by the NMW Survey" PZP, vol. ...