CARTAS DE LOCALIZACI N PARA GALAXIAS WR ENANAS . Objetos para las noches del 26 al 29 de abril de 2006 en 2.6m NOT . ... Tol 9 10 34 38.7 -28 35 00 14.4 3190 0.010641 R, Ha deep 24 36 SI . ESO443-61 To30 13 05 46.7 -28 25 20 15.5 2299 0.007669 U,B,V,R 12 36 SI ATCA . ... Mkn 33 10 32 31.9 +54 24 03 13.5 1430 0.004769 Deep R - - SI . ... SBS 1054+365 10 57 47.0 +36 15 26 16.0 603 0.002010 R - - Verti . ... Tol 35 13 27 06.5 -27 57 23 14.4 2023 0.006748 - - - SI . ... Tol 9 . ... SBS 1054+365 . ...

... Espaц±ol (Chile) . ... ESO, Observatorio Europeo Austral . ... Arquitectura en ESO . ... Galaxias . ... Formatos de imagen . ... Pedidos al por mayor . ... MUSE . ... 50 years of ESO in Chile . ... Esta imagen estцЎ basada en datos de la galaxia anular polar NGC 4650A, obtenidos poco despuц©s de la primera luz del instrumento, que se hizo a principios de 2014. Esta imagen a color fue creada uniendo los datos 3D de MUSE en tres secciones que fueron coloreadas de azul, verde y rojo. ... NGC 4650A . ...

Mapa del Sitio . ... En una noche oscura ellas forman una banda brillante a lo largo del cielo -"La V?a L?ctea" para los antiguos observadores Griegos, y para nosotros, nuestra galaxia. ... Los astr?nomos desde hace tiempo han sospechado que era un agujero negro muy masivo, y que cada galaxia tiene dicha masa central, creada muy temprano en la historia del universo. ... La intensa gravedad del agujero negro impide que cualquier luz escape de ?l, y es por lo tanto, invisible. ("negro" de hecho!) ...

Los c lculos orbitales adem s revelaron que el cometa deber a pasar mucho m s cerca del Sol. ... Debido a que un cometa brilla m s en cuanto se aproxima al Sol, Hale-Bopp solamente podr a hacerse m s visible. Podr a ser uno de los cometas m s brillantes del siglo, si no es que del ltimo milenio. ... Al incitar a los profanos en astronom a a mirar a los cielos un rato, Hale-Bopp puede hacer que las personas se sientan un poquito m s cercanas al universo del cual todos somos parte. ...

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ARNICA (ARcetri Near Infrared CAmera) is the imaging camera for the near infrared bands between 1.0 and 2.5 m that Arcetri Observatory has designed and built as a general facility for the Tirgo telescope. The scale is 1 arcsec per pixel, with sky coverage of more than 4 arcmin times 4 arcmin on the NICMOS 3 (256 X 256 pixels, 40 m side( detector array. ... Arnica progress report : performance and technical results obtained in the last years at Tirgo , Not , and Vatt . ... Arnica and Longsp data: . ...

... Nuevos БЂњrecordsБЂ™ se establecieron en enero cuando telescopios en tierra se unieron al satц©lite БЂњRadioAstronБЂќ, formando un radio telescopio de 220,000 km de diцЎmetro, aproximadamente 20 veces mayor que la Tierra.. RadioAstron, un telescopio orbital Ruso de 10 metros de diцЎmetro , se uniцЕ a observatorios en tierra para estudiar objetos 50 veces mцЎs pequeц±os de lo que es posible con el Telescopio Espacial Hubble. ... Para mцЎs informaciцЕn favor de comunicarse con los autores, . ...

... This file twosigma.dat 79 46186 The 2-sigma catalog -------------------------------------------------------------------------------- See also: VII/152: Einstein Medium Sensitivity Survey Catalog Byte-by-byte Description of file: twosigma.dat -------------------------------------------------------------------------------- ... Format Units Label Explanations -------------------------------------------------------------------------------- 1- 2 I2 h RAh RA ( 1950 ) of the ...

. True Color Image Gallery: Galactic SNR | Magellanic Cloud SNR . Images show regions used to extract spectra . Regions with red strikes are excluded . Background was subtracted from a region around or close to the SNR. Back to G006.4-00.1 Index . Chandra Supernova Remnant Catalog . Main Page | Galactic SNR | Magellanic Cloud SNR . True Color Image Gallery: Galactic SNR | Magellanic Cloud SNR .

... The mutual angular distances between pairs of satellites are given in arcminutes. ... This file table3.dat 128 319 Ephemerides of the apparent encounters for 2005 table4.dat 92 320 Ephemerides of the apparent encounters for 2006 table5.dat 92 322 Ephemerides of the apparent encounters for 2007 table6.dat 98 323 Ephemerides of the apparent encounters for 2008 table7.dat 86 329 Ephemerides of the apparent encounters for 2009 table8.dat 98 266 Ephemerides of the ...

... Flux density at 1 GHz (/Jy): 28 . ... Radio: Shell, brightest to the S. Optical: Filaments correspond well to the radio shell, brightest in SE. X-ray: Brightest to NW, with point source near centre. Point sources: Central, variable X-ray source, and nearby pulsar. ... Molonglo at 408 MHz (3') and Parkes 64-m at 5 GHz (4'). ADS . ... ASCA observations of compact X-ray source. ... X-ray variability of central source. ... ATCA at 1.4 GHz (50''), including H I absorption to central source. ...

... attfilter (attfilter-1.1) [xmmsas_20050815_1803-6.5.0] . ... attfilter instexpid=PNU003 . Generate attitude GTI table (with default name) from the unscheduled PN exposure 003 in the current ODF from cone-type filtering expression (with default tolerance angle). attfilter instexpid=PNU003 tolangles="0.5*#ARCMIN" . Same as previous example but set the cone half-opening angle to 0.5 arcmin. attfilter instexpid=PNU003 tolangles="0.5*#ARCMIN" gtitable=gti.ds:MYGTI . ...

... 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 . ...

... Armagh Observatory, College Hill, Armagh BT61 9DG, +44 (0)28 3752 2928 . ... The asteroid is only the second known object in a so-called "Martian horseshoe" orbit, going around the Sun on nearly the same orbit as Mars. б Unlike the planet's two known moons, Phobos and Deimos, which orbit Mars much like an artificial satellite orbits the Earth, the unusual asteroid moves in a more complicated "horseshoe" pattern along the orbit of Mars, with the open end of the horseshoe centred near Mars itself. ...

Originally a manually operated photographic telescope, the Uppsala Southern Schmidt (USS, 0.5 metre corrector plate aperture) has been refurbished and modernised. ... This image of omega Centauri shows the central portion of the field. ... Built in 1956 at the Uppsala Observatory workshop in Sweden, the telescope was first located at Mount Stromlo Observatory near Canberra in 1957. ... The Uppsala Southern Station was relocated to Siding Spring Observatory in 1982. ... Siding Spring Survey Main Page . ...

... Note the t wo to reveal individual spectra with emission lines. ... G140H F070LP F100LP G235H F170LP G395H F290LP Continuum ux F (nJy) v G140M F070LP G140M F100LP G235M F170LP G395M F290LP 0 1 2 Line ux (ergux (erg ) cm ) Line s cm s Wavelength ( m) 3 4 5 5x10-19 1 Continuum ux F (nJy) v ) Wavelength ( m) 1 2 3 4 5 5x10-19 200 Line ux (ergux (erg ) cm-2) Line s cm s 1 2 Continuum ux F (nJy) v -2 -1 500 inuum ux F (nJy) v 2000 10 05s 4 Wavelength ( m) ...

... VIMOS GOODS/ADP Imaging Data Release Version 1.0 . ... VIMOS GOODS/ADP Spectroscopy Release: Version 1.0 . ... Final FORS2 GOODS/ADP Spectroscopy Release: Version 3.0 . ... Final ISAAC GOODS/ADP Release: Version 2.0 . ... Imaging and spectroscopic data obtained with ESO telescopes by proprietary programmes in the Chandra Deep Field South will also become public worldwide via the ESO Science Archive before the release of the SIRTF/GOODS data, or after the expiration of the one year proprietary period...

... 2 августа 1958 года (по данным газеты El Pais, в 1991 году ему было 32 года). ... В 1991 году жил и работал в Барселоне (Barcelona). ... Во время проведения в 1991 году второго набора в отряд ЕКА был одним из пяти финалистов национального набора ESA-2 в Испании. ...

... О. Н. Шиврис РАБОТА РАДИОТЕЛЕСКОПА РАТАН-600 С ПЛОСКИМ ОТРАЖАТЕЛЕМ . ... стр 12 Затем рассчитываются эфемериды для заданного азимута источника при помощи программы taglmx. ... При большем числе азимутов следует приготовить несколько входных файлов taglmx (или несколько раз редактировать один) . ... 1)Время прохождения Солнца через диаграмму в данном азимуте t прох . 2)Время прохождения облучателем дуги между двумя последовательными азимутами t обл . ... в данном азимуте. t прох = D солн / v прох . ...

A panoramic view of the CL0939+4713 cluster located 4 billion light-years from Earth. Images were captured with the Subaru Prime Focus Camera (Suprime-Cam), all of which are a composite of a B-band image (blue), a R-band image (green), and a zтАЩ-band image (red). Left 27 arcmin x 27 arcmin field of view. Top-right: Close-up view of the central cluster region, 2.5 arcmin x 2.5 arcmin field of view. ... Subaru Telescope, National Astronomical Observatory of Japan (NAOJ) ...