Thermal InfraRed surveys from Antarctica for extragalactic astronomy

International audience The outstanding atmospheric conditions of the Dome C give a unique opportunity to survey deeply large areas of the sky in the thermal infrared reaching interesting sensitivity limits for extragalactic astronomy. Our extragalactic database HyperLeda will benefit from new infrar...

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Bibliographic Details
Main Authors: Vauglin, I., Gavrilovic, Natasa, Prugniel, Philippe
Other Authors: Centre de Recherche Astrophysique de Lyon (CRAL), École normale supérieure de Lyon (ENS de Lyon)-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Astronomical Observatory, Belgrade, Serbia, Zinnecker, H.; Epchtein, N.; Rauer, H.
Format: Conference Object
Language:English
Published: HAL CCSD 2007
Subjects:
[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
Antarc*
Antarctica
Online Access:https://hal.science/hal-03744075
https://doi.org/10.1051/eas:0833043
Description
Summary:International audience The outstanding atmospheric conditions of the Dome C give a unique opportunity to survey deeply large areas of the sky in the thermal infrared reaching interesting sensitivity limits for extragalactic astronomy. Our extragalactic database HyperLeda will benefit from new infrared data, especially for characterizing nuclear and starburst activity of AGNs and ULIRGs.

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