The commissioning of the REM-IR camera at La Silla.

被引：32

作者：

Conconi, P ^{[1
]}

Cunniffe, R ^{[1
]}

D'Alessio, F ^{[1
]}

Calzoletti, L ^{[1
]}

Jordan, B ^{[1
]}

Mazzoleni, R ^{[1
]}

Melandri, A ^{[1
]}

Molinari, E ^{[1
]}

Testa, V ^{[1
]}

Vitali, F ^{[1
]}

Zerbi, FM ^{[1
]}

Chincarini, G ^{[1
]}

Covino, S ^{[1
]}

Ghisellini, G ^{[1
]}

Rodono, M ^{[1
]}

Tosti, G ^{[1
]}

Antonelli, LA ^{[1
]}

Cutispoto, G ^{[1
]}

Nicastro, L ^{[1
]}

Palazzi, E ^{[1
]}

机构：

[1] INAF Osservatorio Astron Brera Merate, I-23807 Merate, Italy

来源：

GROUND-BASED INSTRUMENTATION FOR ASTRONOMY, PTS 1-3 | 2004年 / 5492卷

关键词：

near infrared imager; cryo-coolers; array control;

D O I：

10.1117/12.551289

中图分类号：

V [航空、航天];

学科分类号：

08 ; 0825 ;

摘要：

During the early Summer 2003, the REM telescope has been installed at La Silla. together with the near infrared camera REM-IR and the optical spectrograph. ROSS. The REM project is a fully automated instrument to follow-up Gamma Ray Burst, triggered mainly by satellites, such as HETE II, INTEGRAL, AGILE and SWIFT. REM-IR will perform high efficiency imaging of the prompt infrared afterglow of GRB and, together with the optical spectrograph ROSS, will cover simultaneously a wide wavelength range, allowing a better understanding of the intriguing scientific case of GRB. In this paper we present the result of the commissioning phase of the near infrared camera REM-IR, lasted for an extended period of time and currently under the final fine tuning.

引用

页码：1602 / 1612

页数：11