This is a new popup window - close it when you are done . Submitted by Paul Cicchetti on 10/27/2013 16:56:16 . ... Used St-8300 CCD camera with filter wheel for LRGB image. ... Stacked in CCDStack and further processed in Photoshop CS5. Final image was cropped from original. New (Oct 27, 2013): Further processed the original image with new technique. ... Copyright (c) Amateur Telescope Makers of Boston, Inc. ...

This page is devoted to information on Supernova 1999gh in NGC 2986 . Basic information on this SN, including the last reported brightness, on this Supernova can be found on the Bright supernova page. Information on the original web pages for many of these images can be found on the Supernova links web page. ... AUDE has a 1999gh page in French [ Translate ] . ... Arno van Werven image . ... vsnet-alert 3782 ] SN 1999gh in NGC 2986 . ... vsnet-alert 3799 ] Re: SN 1999gh in NGC 2986 . ...

... To save time, I will only provide ephemerides in 2000 coordinates. ... Note: most the orbital elements used to create these ephemerides were obtained from the International Astronomical Union Circulars (IAUCs), Minor Planet Circulars (MPCs) or the ICQ Comet Handbook. ... The following 1-day ephemeris (March 1, 1997 - October 1, 1997) is from Donald Yeomans of JPL and is based on Reference Orbit #55 (March 4, 1997). 2000 coordinates (March - September, 1997) [3/4/97] . ... Epoch: 1997 Feb. 1.0 . ...

... Many observatories around the world will follow these events, with the purpose of obtaining accurate measurements of the angular diameter of this red giant, from the recording of the lightcurve during the disappearance (or reappearance) behind the limb of the Moon. ... 6 November 1998: both disappearance and reappearance recorded under very good conditions at the TIRGO observatory by A. Richichi . ... A preliminary analysis confirms the findings of the previous event observed in February (see below)...

Sternberg Astronomical Institute, Moscow University, . Moscow, Russia . Supernovae make us brighter .. Search russian astronomical resources . Mirror of International Supernovae Network ( Original site ) . Catalogue of Supernovae Stars . HTTP access to SAI Catalogue of Supernovae Stars . SAI SN Light Curves Online . ... Sternberg Astronomical Institute ( in Russian ) . ... Astronet - Russian Astronomical Network . ... Russian Foundation for Basic Research . ...

The spherical aberration affecting the HST primary mirror (Burrows et al. 1992) can seriously alter the core brightness profile of elliptical galaxies. ... In this paper we test the performance of deconvolution in recovering the original surface brightness profile in the case of elliptical galaxies observed with the HST Planetary Camera (PC). ...

... omdetect (omdetect-5.14.2) [?? Meta Index / Home Page / Algorithm Omdetect will find sources on an image using both a peak-finding and connected-pixel algorithm. The former will mainly detect ``point'' sources and the latter ``extended'' sources. The peak-finding algorithm is used first to try to locate all point sources, in order of decreasing brightness. This algorithm mainly overcomes problems with modular-8 patterns around bright sources and scattered light features. ...

... Ciel Espace, le magazine qui vous guide toujours plus loin . ... les plus belles images de l'Univers d–їcrypt–їes pour vous . ... des pages consacr–їes –Љ la publication de vos photos Mais c'est aussi une vraie communaut–ї avec laquelle partager votre passion et nourrir votre curiosit–ї. ... Les plan–Rtes, les –їtoiles, les n–їbuleuses, les galaxies, jusqu'aux grandes structures de l'Univers : les astronomes font tout pour les voir en relief. ... 09/11/2015 - Penser l'Univers aujourd'hui . ...

Astronotes Armagh Planetarium's Stellar Blog! ... Stars . ... Posted on January 30, 2012 | 1 Comment If you look towards the west just after sunset this February you will see a very bright star in the darkening sky. ... Continue Reading.. ... 1 Comment After last yearтАЩs success, BBC2тАЩs Stargazing Live returned to our screens this month for another three nights of astronomy wonders.€а Holding the reins again were the charismatic Professor Brian Cox [ ] . ... Posted on December 5, 2011 | ...

In this gallery are many images of Low Surface Brightness Galaxies which have recently been discovered and analyzed. ... The central surface brightness of this galaxy is 24.28 . Malin 2 This galaxy is another huge disk galaxy with a scale length of 15 kpc and a redshift of 15000 km/a. The high surface brightness knot in one of its spiral arms actually has the same color, luminosity and H-alpha equivalent width as the entire Large Magellanic Cloud . ... Truly it is a Low Surface Brightness Galaxy. ...

http://hea-www.harvard.edu/AstroStat/slog/2008/kepler-inference/ Weaving together Astronomy+Statistics+Computer Science+Engineering+Intrumentation, far beyond the growing borders Fri, 01 Jun 2012 18:47:52 +0000 hourly 1 http://wordpress.org/?v=3.4 http://hea-www.harvard.edu/AstroStat/slog/2008/kepler-inference/comment-page-1/#comment-200 vlk Fri, 18 Apr 2008 03:55:28 +0000 http://hea-www.harvard.edu/AstroStat/slog/?p=270#comment-200 Good point, Aneta. ... Good point, Aneta. ...

... Цвет: синий . ... Брюки спортивные adidas Originals. ... Линейка: Originals . Категория на маркете: Одежда, обувь и аксессуары/Обувь/Обувь для мальчиков/Ботинки . Тип товара на Маркете: Ботинки детские . ... Тип товара: Ботинки . ... Тип двигателя Серводвигатель . Тип подачи материала протяжный . ... Максимально тонкий материал 0.8 мм . ... Ширина материала 1326 мм . ... Материал рамы: сталь . ... Тип переднего ободного тормоза: клещевой . ... Форма ковра: прямоугольник . ...

Next: BASIC PROPERTIES Up: R CORONAE BOREALIS STARS Previous: INTRODUCTION . RCB stars are named after a star just visible to the naked eye in the constellation of Corona Borealis. RCrB was discovered by Edward Pigott (1797), an English amateur astronomer, who had been observing a star in the `Northern Crown' for over a decade. ... Since 1795, other RCB stars have been discovered and their properties have been carefully observed. ...

. Comment on J1130-1449 . There are two dominant components in our image. Comparison with the 15 GHz image of Kellermann et al. (1998) reveals that the western component is brighter at the higher frequency, indicating that the brighter (eastern) component in our image may have a steep spectrum. VLBApls home page . Last modified: 16 Oct 2000

mom0 mom1 mom2 w50 w20 -------------------------------------------------------------------------------- ADD 216 07:31:39 -69:02:28 new -tidal_clo 0.114 11.7 1489.5 40.8 69.3 261.8 HIP 522 12:27:37 +01:34:14 HGcloud 0.491 29.7 1286.6 16.7 60.4 87.2 ZSS 102 16:18:46 -55:37:33 new -J1616-55e 0.124 3.7 399.5 7.0 30.5 43.3 HIP 827 17:11:57 -64:41:19 new -(VK- cloud 0.187 5.3 454.8 7.0 30.8 52.2 EXA 39 17:22:00 -59:45:00 new -(BK- ...

... Chandra | ESO | ... Field selection . ... Color composite image of the Chandra Deep Field South of 940 ks (pixel size = 0.984 arcsec, smoothed with a s =1 arcsec Gaussian). ... The Chandra Deep Field South (CDF-S) is one of the deepest observations obtained with the X-ray Chandra satellite, which stared at the same path of the sky for 11 days. ... ESO press release on March 13 , 2001 . ... APOD : The Chandra Deep Field South has been the Astronomical Picture of the Day on March 28, 2001 . ...

SAI, graduates year 1982. ... Note: when just a 7-digit phone number is shown, it refers to a phone located in Moscow (international access 007-495). "+" in front of a number means that you must dial an international access code first (or just press "+" on your mobile phone keypad). ... 939-1672(work); . ... Ataev Sasha . 1-(703)-536-8881(home) (USA); . ... Bychkov Sergey . ... 1-(410)-740-8205(home), +1-(301)-286-2150(work) (USA); . ... 1-(412)-767-0332(home), +1-(412)-608-9339(mobile) (USA); . ...

saturn_g_02_95d.fits Date of observation is 2006-11-16T17:47:56 Mt. ... rings is Titan: VI Saturn II III IV V VI Titan II Enceladus IV Dione V Rhea III Tethys Header listing for HDU #1: SIMPLE = T / file does conform to FITS standard BITPIX = 16 / number of bits per data pixel NAXIS = 2 / number of data axes NAXIS1 = 3072 / length of data axis 1 NAXIS2 = 2048 / length of data axis 2 EXTEND = T / FITS dataset may contain extensions COMMENT FITS (Flexible 376.. ...

... A Nearby Supernova in M51 . ... Credit: R Jay GaBany ( Cosmotography.com ) Explanation: One of the nearest supernovas of recent years was discovered late last month in the bright nearby galaxy M51 . ... The supernova has been identified as a Type II but has an unusual brightness history, creating speculation that is similar in nature to the brightest supernova of modern times: 1987A . The progenitor star has been identified as a bright blue star. ... Publications with keywords: supernova - M51 . ...

Загрузить программу (~10 MB). ... Программа izmccd предназначена для высокоточной астрометрической обработки числовых изображений небесных объектов. Программа позволяет получать как измеренные, так и экваториальные координаты малых планет, комет, спутников больших планет, визуально-двойных звезд и других объектов, а также идентифицировать уже известные малые планеты и найти на числовых изображениях движущиеся объекты. ... Программа является бесплатной. ... Автоматическая обработка, один объект. ...