... Science User Portal . ... ESO, the European Southern Observatory . ... Travel and Contacts . Travel to ESO Headquarters . ... Travel to Guesthouse . ... Survey Telescopes . ... This video fades back and forth between views of the stellar nursery Monoceros R2 in visible and infrared light. The visible-light view was created from digitised photographs through red and blue filters forming part of the Digitized Sky Survey 2 (DSS) and the new infrared view comes from the VISTA telescope at Paranal. ...

... Carlo Baffa This email address is being protected from spambots. You need JavaScript enabled to view it. , tel (+39) 055 2752 298 . Valdemaro Biliotti, This email address is being protected from spambots. ... This email address is being protected from spambots. ... Gilbetro Falcini, This email address is being protected from spambots. ... Debora Ferruzzi, This email address is being protected from spambots. ... Elisabetta Giani, This email address is being protected from spambots. ...

STScI . WFIRST . ... What is STScI . ... Missions . ... Hubble Heritage Project . Future Missions and . ... Missions Office . ... Library . ... Hubble Fellowships . ... This page provides links to WFIRST brochures and handouts created by STScI, or describing work done at STScI. GSFC maintains a library of images and multimedia a library of presentations and visuals , and a WFIRST Fact Sheet . WFIRST STScI Support . ... Pushing Astronomy's Bounds: Hubble, Webb, and WFIRST Copyright | ...

3D NIR IFU spectrograph from MPE. CIRPASS on Gemini. COHSI on UKIRT. ... SINFONI NIR IFU spectrograph for the VLT (and here ). SPIFFI on the VLT. ... LUCIFER at Heidelberg. GNIRS on Gemini(and IFU ). ... NIRSPEC on Keck and at UCLA . ... Omega-Prime from MPIA, Heidelberg. ... Gemini instrumentation. ... UKIRT instrumentation ( Future Instruments ). ... NTT Deep Field ( SUSI optical images , SOFI infrared images ). ... Instrumentation Links * Gemini Project Links * Other IR Instruments ...

Next: Spectroscopic Data Up: Calculation of Extinction Previous: Calculation of Extinction . Near--infrared observations were made on 5--6 February 1996 at CTIO using the CIRIM imager. ... In the infrared, the sky background is high relative to the dynamic range of the detector. ... As the first step in the reduction, all frames had a linearity correction applied (Elston 1994). ... In some cases, the dithering procedure caused stars to overlap with other stars on the final frame. ...

... material . ... n,k [fig] . ... cryst. ... Cooke (1976) Astrophys. ... cryst. polyoxymethylene . n,k [fig, appr] . ... Astron. ... Ariz. cryst. ... transm. [fig] . ... 1984) Astron. Astrophys. 133, 77. organic refractory . ... abs. [fig] . ... d'Hendecourt, Allamandola (1986) Astron. ... Ashok et al. (1991) in Palik E. (ed) Handbook of Optical Constants of Solids, II. ... Astrophys. 317, 929. cryst. ... For mixtures of CH 4 , CH 3 OH and other solid organics see the material group Ices . ...

Astronomy Picture of the Day . ... 28.08.1997 . ... Explanation: The Trifid nebula (M20) is a bright star forming region in Sagittarius , 5000 light years from Earth. In visible light , the interstellar gas cloud is crossed by dark, obscuring dust lanes which roughly divide the glowing emission nebula into three major parts. ... August . ... August 1997 . ... NASA Web Site Statements, Warnings, and Disclaimers . ... Publications with keywords: infrared . Publications with words: infrared . ...

... Up: Data Analysis Applications . Previous: Mixing IRAF and Starlink Applications - FIGARO under IRAF . ... An infrared-array reduction and analysis package which is written in the IRAF environment has been developed to handle the huge amount of data obtained at the Teide Observatory using the 1.5 m Carlos S?nchez Telescope with the new infrared Camera/Instituto de Astrof?sica de Canarias(IRCAM/IAC). ... One of the advantages of this package is that it can easily handle the large amount of data. ...

The Cosmic InfraRed Background (CIRB) is the radiation from stars in many faint galaxies. ... The near-infrared (wavelengths near 2-3 microns) and optical (wavelengths near 500 nm) part of this extragalactic background light is just starlight redshifted into the infrared. But some starlight is absorbed by dust and re-emitted in the far-infrared (wavelengths near 100 microns). ... The CMB is by far the largest of these radiation fields, with a total intensity of 996 nW/m 2 /sr. ... Part 2 | ...

The AstroGuide . ... AstroGuide | ... Other Sites . ... AstroGuide Listing . ... See many more Astronomy Listings by: Category or Alphabet . This site contains plenty of facts and history about Infrared radiation and how it is used in Astronomy. ... Web Site . ... It seems to me that I cannot be the only one to be able to see hidden images when viewing the skies through infrared lenses. ... Unless otherwise specified, web site content Copyright 1994-2016 John Huggins All Rights Reserved . ...

... 2004 April 14 . Massive Star Forming Region DR21 in Infrared . ... Explanation: Deep in the normally hidden recesses of giant molecular cloud DR21, a stellar nursery has been found creating some of the most massive stars yet recorded. The orbiting Spitzer Space Telescope 's Infrared Array Camera opened the window into the cloud last year in mid- infrared light. The cloud is opaque to visible light because of dense interstellar dust . ... About APOD | ...

... ATNF Home . ... About ATNF overview . ... Australia Telescope Steering Committee . ... Murchison Radio-astronomy Observatory . ... Tips on holding a viewing night . ... Infrared Astronomy: in the Heat of the Night . The 1999 Ellery Lecture . ... This paper, which is a brief summary of the 1999 Ellery Lecture, outlines the importance of the infrared, traces some of the key Australian developments in the field, and looks ahead to the challenges facing infrared astronomers in the immediate future. ...

... ST-ECF, ESO, STScI and the NICMOS IDT organized a workshop on near infrared imaging from space and ground was held in Pula on May 26-27, 1998. ... The meeting was held in May 1998, about one year after science observations started with NICMOS, and about half a year before the Infrared Spectrometer and Array Camera (ISAAC) starts to operate on the VLT. Currently, it is expected that NICMOS will operate until the end of 1998. ...

... Bojan Nikolic web pages (r. 329) . Modelling absorption and emission of radiation by interstellar dust . ... The search results are restrict to these pages only . ... Copyright 2005 -- 2016, Bojan Nikolic feedback welcome ...

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Астроплощадка: 53 20 56,505 N 83 46 07,735 E, H абс. = 209 м. + Информационные каналы . ... Анк а дня . ... Закономерная случайность помогла увидеть зарождение массивных звезд . ... С помощью Инфракрасной космической обсерватории (Infrared Space Observatory, ISO), принадлежащей Европейскому космическому агентству, ученые впервые смогли наблюдать рождение огромных звезд, которые светят в 100 тысяч раз ярче Солнца.. Все ключевые слова . Картинка дня . ... Copyright 2002-2014 . ...

Общая Астрономическая Конференция > Практика > Астрономический наблюдательно-информационный портал > Хвостатые гостьи (все о кометах) > C/2016 B1 (NEOWISE) _ CK16B010 _ N0096si object = 25-я Wide-field Infrared Survey Explorer (WISE) / (NEOWISE)! ... Просмотр полной версии : C/2016 B1 (NEOWISE) _ CK16B010 _ N0096si object = 25-я Wide-field Infrared Survey Explorer (WISE) / (NEOWISE)! ... C/2016 B1 (Neowise) / CK16B010 (i=47.5њ, q=4.272 AU, TP=2016 Sept. ... C/2016 B1 (NEOWISE) . T 2016 Sept. ...

K.-H. Hofmann, T. Bl cker, G. Weigelt, and Y. Balega: . ... Annual Scientific Meeting of the Astronomische Gesellschaft at the Joint European and National Meeting JENAM 2001 of the European Astronomical Society and the Astronomische Gesellschaft, Sep 10-15, 2001, Munich, Germany . ... CIT 3 (= WX Psc = IRC +10 011 = IRAS 01037+1219), an oxygen-rich long-period variable evolving along the Asymptotic Giant Branch (AGB), is one of the most extreme infrared AGB objects. ... Back to Group Home Page ...

I-GALFA Infrared Emission . ... The red and yellow emission is in from dust near the Galactic plane; the blank area was not observed. ... The image on this page shows thermal infrared emission from starlight-heated dust particles in the gas I-GALFA will observe. ... I-GALFA will see atomic hydrogen gas with a similar amount of angular detail to that visible here in infrared dust emission, and it is sensitive enough to see every dust filament in the gas. ... I-GALFA Main | ...

INFRARED FOURIER-SPECTROMETER SICH-F . ... Instrument work regimes: 1) Inside. 2) Calibration at inside standard sources 2 - 4 times per a rotation. 3) Calibration at "free space" 2 - 4 times per a rotation. 4) Infrared radiation measuring 10 - 40 min. per a rotation. ... Spectrometer consists of the photodetector block and the block of signal processing and control. ... Diagnostic information and attach data will transfer by state telemetric channels. ... Detector temperature. ...