Wide field astronomy at Dome C: Two IR surveys complementary to SNAP

被引：3
|
作者：
Burgarella, D. [1 ]
Ferrari, M. [1 ]
Fusco, T. [1 ]
Langlois, M. [1 ]
Lemaitre, G. [1 ]
Le Roux, B. [1 ]
Moretto, G. [1 ]
Nicole, M. [1 ]
机构：
[1] LAM, OAMP, F-13376 Marseille 12, France
来源：
1st ARENA Conference on Large Astronomical Infrastructures at CONCORDIA, Prospects and Constraints for Antarctic Optical/IR Astronomy | 2007年 / 25卷
关键词：
D O I：
10.1051/eas:2007086
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
Surveys provide a wealth of data to the astronomical community that are used well after their completion. In this paper, we propose a project that would take the maximum benefit of Dome C in Antarctica by performing two surveys, in the wavelength range from 1-5 mu m, complementary to SNAP space surveys. The first one over 1000 sq. deg. (1 KdF) for 4 years and the second one over 15 sq. deg (SNAP-IR) for the next 4 years at the same time as SNAP 0.35-1.7 mu m survey. By using a Ground-Layer Adaptive Optics system, we would be able to recover, at the ice level and over at least half a degree in radius, the similar to 300 mas angular resolution available above the 30-m high turbulent layer. Such a survey, combining a high angular resolution with high sensitivities in the NIR and MIR, should also play the role of a pre-survey for JWST and ALMA.
引用
收藏
页码：147 / 154
页数：8
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