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Titlebook: The Impact of Near-Infrared Sky Surveys on Galactic and Extragalactic Astronomy; Proceedings of the 3 N. Epchtein Conference proceedings 19

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書(shū)目名稱The Impact of Near-Infrared Sky Surveys on Galactic and Extragalactic Astronomy
副標(biāo)題Proceedings of the 3
編輯N. Epchtein
視頻videohttp://file.papertrans.cn/912/911765/911765.mp4
叢書(shū)名稱Astrophysics and Space Science Library
圖書(shū)封面Titlebook: The Impact of Near-Infrared Sky Surveys on Galactic and Extragalactic Astronomy; Proceedings of the 3 N. Epchtein Conference proceedings 19
描述Thirty years after the pioneering enterprise of Neugebauer and collabo- rators, the astronomical sky is surveyed anew in the near infrared range with a gain in sensitivity greater than 4 orders of magnitude. Data have started to come through the "pipelines" routinely and at the turn of the century, the astronomical community will be provided with immense databases that will eventually contain accurate positions and 3- colour (or even 4-colour after merging DENIS and 2MASS data) photometry for hundreds million of stars and millions of galaxies. This fantastic harvest of data will eventually result of the huge effort that has been deployed on both sides of the Antlantic to promote 2 major projects, 2MASS and DENIS. rd The basic aim of this 3 Euroconference (and last in the series), was to put in close contact the scientific teams of 2MASS and DENIS in order to present and discuss the first significant results of the two surveys and to start promoting possible future plans
出版日期Conference proceedings 1998
關(guān)鍵詞Fitting; Likelihood; Statistica; astronomy; galaxy; stars
版次1
doihttps://doi.org/10.1007/978-94-011-5026-2
isbn_softcover978-94-010-6110-0
isbn_ebook978-94-011-5026-2Series ISSN 0067-0057 Series E-ISSN 2214-7985
issn_series 0067-0057
copyrightSpringer Science+Business Media Dordrecht 1998
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0067-0057 ange with a gain in sensitivity greater than 4 orders of magnitude. Data have started to come through the "pipelines" routinely and at the turn of the century, the astronomical community will be provided with immense databases that will eventually contain accurate positions and 3- colour (or even 4-
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Conference proceedings 1998a gain in sensitivity greater than 4 orders of magnitude. Data have started to come through the "pipelines" routinely and at the turn of the century, the astronomical community will be provided with immense databases that will eventually contain accurate positions and 3- colour (or even 4-colour aft
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https://doi.org/10.1007/978-94-011-5026-2Fitting; Likelihood; Statistica; astronomy; galaxy; stars
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978-94-010-6110-0Springer Science+Business Media Dordrecht 1998
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The Impact of Near-Infrared Sky Surveys on Galactic and Extragalactic Astronomy978-94-011-5026-2Series ISSN 0067-0057 Series E-ISSN 2214-7985
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