Name: Census of the Galaxy: Challenges for Photometry and Spectrometry with Gaia: Proceedings of the Workshop Held in Vilnius, Lithuania 2-6 July 2001 (en Inglés)
SKU: 58579499
Price: 1691.50 MXN
Availability: InStock
Author: Vansevicius, Vladas ; Kucinskas, Arunas ; Sudzius, Jokubas
ISBN: 9789401039116

portada Census of the Galaxy: Challenges for Photometry and Spectrometry with Gaia: Proceedings of the Workshop Held in Vilnius, Lithuania 2-6 July 2001 (en Inglés)

Census of the Galaxy: Challenges for Photometry and Spectrometry with Gaia: Proceedings of the Workshop Held in Vilnius, Lithuania 2-6 July 2001 (en Inglés)

Formato

Libro Físico

Editorial

Springer

Autor

Vansevicius, Vladas ; Kucinskas, Arunas ; Sudzius, Jokubas

Idioma

Inglés

N° páginas

194

Encuadernación

Tapa Blanda

Dimensiones

23.4x15.6x1.1 cm

Peso

0.30 kg.

ISBN13

9789401039116

Categorías

Astronomía, espacio y tiempo
Gravedad
Análisis espectral, espectroquímica, espectrometría de masas

Census of the Galaxy: Challenges for Photometry and Spectrometry with Gaia: Proceedings of the Workshop Held in Vilnius, Lithuania 2-6 July 2001 (en Inglés)

Vansevicius, Vladas ; Kucinskas, Arunas ; Sudzius, Jokubas (Autor) · Springer · Tapa Blanda

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Reseña del libro "Census of the Galaxy: Challenges for Photometry and Spectrometry with Gaia: Proceedings of the Workshop Held in Vilnius, Lithuania 2-6 July 2001 (en Inglés)"

Astrometry from space was performed for the first time and with great success by the ESA Hipparcos satellite (1989-93). This mission was designed as an as- trometry mission, but the use of a photon counting detector made it possible to produce very important photometric results: the most accurate astronomical pho- tometry ever by the main Hipparcos mission in a very broad band of 120000 stars, and the two-colour Tycho-2 photometry of 2.5 million stars. The cornerstone ESA mission GAIA was approved in October 2000 for launch not later than 2012. This mission will use CCDs in time-delayed integration mode instead of the photo-cathode detectors used in Hipparcos. Due to the higher quantum efficiency of the CCDs, simultaneous integration of many stars, and larger tele- scope apertures GAIA will utilize the star light a million times more efficiently than Hipparcos, resulting in astrometry and multi-colour photometry for one billion stars. GAIA photometry is crucial for the scientific utilization of the astrometric results, and the photometric data have a high scientific content in themselves.