... 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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Winer Observatory P.O. Box 797, Sonoita, Arizona 85637-0797, USA . ... Irvin M. Winer . ... Site Map . ... Hint : Find and stay on Arizona State Route 83, which bounds our property). Use the interactive map below or use our GPS position N31 39' 56.08" W110 36' 06.42" (or 31.665578N, 110.601783W). ... From Tucson, take I-10 east about 20 miles to Exit 281, which is marked "State Route 83 Sonoita/Patagonia". ... Go three miles, staying on the paved road of State Route 83. ... 2013 Winer Observatory. ...

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• Mark 1 Consciousness
• Winer Observatory History
• Mark 3 Consciousness

Электронная библиотека астронома-любителя. ... архив RSN . ... Ru.Space.News: . Апрель 1998 . ... Дата: 22 апреля 1998 (1998-04-22) От: Alexander Bondugin Тема: NASA Astronomers Find Planet Construction Zone Around Nearby Star Привет всем! ... Дата: 22 апреля 1998 (1998-04-22) От: Alexander Bondugin Тема: NASA Hosts Web Chats For "Take Our Daughters To Work Day" Привет всем! ... Дата: 22 апреля 1998 (1998-04-22) От: Alexander Bondugin Тема: SJI's Sky and Space Update - April 15, 1998 Привет всем! ...

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• Электронная библиотека астронома-любителя. RU.SPACE.NEWS - архив за 12 мая...
• Электронная библиотека астронома-любителя. RU.SPACE.NEWS - архив за 23 июля
• Электронная библиотека астронома-любителя. RU.SPACE.NEWS - архив за 10 марта

Abstract -- Calculations are performed for the linear polarization of starlight due to extinction by aligned dust grains when the starlight traverses a medium with irregular magnetic fields. This medium is intended to represent the optically thick components of interstellar clouds which are observed to make little, if any, contribution to the polarization of starlight. ...

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... For the past years I have been working on the problem of synthesis of light curves of close binary systems, consisting of a normal star and a compact object (point object with fixed X-ray luminosity). ... Possible existence of a bright spot on the disk's lateral surface is taken into account. ... The last of then will be published in Gordon and Breach Publishers ( Cherepashchuk A.M., Katysheva N.A., Khruzina T.S., Shugarov S.Yu. ... Cherepashchuk A.M., Katysheva N.A., Khruzina T.S., Shugarov S.Yu. ...

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• Linux on CLEVO 8750

Maxim Tarasenko , a leading Russian space history scholar and a member of Space Policy?s editorial board, who contributed greatly to the elucidation of the Russian space programme in the journal and elsewhere, died in 1999. In order to commemorate his pioneering work in space policy, Elsevier Science has decided to hold an annual competition, open to all law school students and graduate students of space policy, to find the best essay. ...

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... un oculaire Orion DeepView 35mm (2") . un oeilleton de collimation (le Takahashi offert plus bas Гїtant plus prГїcis) . ... un ventilateur pouvant Г?tre fixГї Г la base du tube pour faciliter la mise en tempГїrature du mirroir primaire . les outils necessaire pour le montage/demontage et le rГїglage (tournevis, clГїs Allen etc.) . et bien entendu la commande et les cГ?blages pourle GoTo, le porte oculaire, adaptateur 2", le manuel Orion etc. ... Oculaire de collimation Takahashi (1.25") . ...

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• http://www.cieletespace.fr/node/11535?thickbox=1&width=700

... Limit of star magnitude. If you want to obtain best results, you should use reference stars not more dimly than limiting star magnitude of your telescope. Limiting star magnitude depends on time of an exposition also.) This value should be set as " maximum of star magnitude " in a dialog box " Extraction from catalogue". To find darkest stars in the frame, make the following: . ... Two star magnitudes (m1, m2 in two photometric systems) will be outputted in the window "Information". ...

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... Astro Space Centre , Lebedev Physical Institute RAS, Moscow. ... Cosmonaut Training Centre, Star City, Moscow Region. ... Coordinational Scientific Information Center of Russian Space Forces. ... Institute for Chemistry and Physics RAS, Moscow. ... Institute for Geo-Electromagnetic Research RAS, Moscow Region, Troitsk. ... Institute for Physics and Power Engineering RAS, Kaluga Region, Obninsk. ... Copyright RSSI 1993-1997, Space Research Institute RAS Network Information Centre ...

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• RSSI Sites Administration
• RSSI Homepage

. To the main page . Astrology . The following articles are translated from Russian. If you find any grammatical errors, please send me a note . Astrology is an excellent means for brainwashing (interview with scientist) [new] . Russia under the sign of jackass [new] .

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• Skepticism

... Using the photometric data for about 1400 disk-population red giants, we investigate the metallicity variations in function of the spectral class (colour and of the luminosity. ... The metal-dificient giant population of the galactic disk os fund to lack stars which could be older than the open cluster NGC 188, i.e. 7x10 9 years. ... По фотометрическим данным, примерно для 1400 красных гигантов диска Галактики исследованы вариации металличности в зависимости от спектра (цвета) и светимости. ...

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... GRB060712 ( GCN5303 ) The first R image was at 2006-07-12 21:10:32 UT, 72 s after notice time and 212 s after the GRB time. ... HETE Alert 4006 ( GCN 4549 ) - MASTER promt optical limit time . ... GCN 4173 | ... GRB050410 ( GCN 3221 5 h after Swift GRB trigger time . ... GRB05017 ( GCN 2954 19m at between 2h and 4h after Swift GRB trigger time (first Swift GRB with X-ray promt observation) . GRB05017 ( GCN 2953 17m at 2h after Swift GRB trigger time (first Swift GRB with X-ray promt observation) . ...

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• MASTER GLOBAL ROBOTIC TELESCOPES NET

. Comment on J1239-1023 . No image is shown by Dallacasa et al. (1998) as they did not find the VLBI structure at 2.3 and 8.4 GHz prominent, just dominated by a compact region barely resolved in position angle about -45 . In our case the source is well resolved, with a jet pointing to the W-NW direction, in agreement with what is seen in the images at 2.3 and 8.4 GHz from the VLBA Calibrators database. VLBApls home page . Last modified: 16 Oct 2000

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... From the chain visibility point of view, it is very recommended to look at the Javascript movies , especially if the frame rate can be not regulated in your MPEG player. ... The non-CH-associated large-scale chains visible on the SOHO/EIT images at three wavelengths of 171, 195 and 284 as well as on the MLSO/HAO He I 10830 spectroheliogram of December 16, 1997. ... The SOHO/EIT movies at 171 and 195 show the chain dynamics on June 1-3, 1998. ... Javascript movie (230 KB), SOHO/EIT, 171 . ...

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