LUCIFER1 commissioning at the LBT

被引：18

作者：

Ageorges, N. ^{[2
]}

Seifert, W. ^{[1
]}

Juette, M. ^{[3
]}

Knierim, V ^{[3
]}

Lehmitz, M. ^{[4
]}

Germeroth, A. ^{[1
]}

Buschkamp, P. ^{[2
]}

Polsterer, K. ^{[3
]}

Pasquali, A. ^{[4
]}

Naranjo, V ^{[4
]}

Gemperlein, H. ^{[2
]}

Hill, J. ^{[5
]}

Feiz, C. ^{[1
]}

Hofmann, R. ^{[2
]}

Laun, W. ^{[4
]}

Lederer, R. ^{[2
]}

Lenzen, R. ^{[4
]}

Mall, U. ^{[4
]}

Mandel, H. ^{[1
]}

Mueller, P. ^{[1
]}

Quirrenbach, A. ^{[1
]}

Schaeffner, L. ^{[1
]}

Storz, C. ^{[4
]}

Weiser, P. ^{[6
]}

机构：

[1] Heidelberg Univ, Landessternwarte ZAH, Konigstuhl 12, D-69117 Heidelberg, Germany

[2] Max Planck Inst Extraterr Phys, D-85748 Garching, Germany

[3] Ruhr Univ Bochum, Astron Inst, D-44780 Bochum, Germany

[4] Max Planck Inst Astron, D-69117 Heidelberg, Germany

[5] Univ Arizona, LBT Observ, Tucson, AZ 85721 USA

[6] Fachhochshule Tech & Gestaltung, D-68163 Mannheim, Germany

来源：

GROUND-BASED AND AIRBORNE INSTRUMENTATION FOR ASTRONOMY III | 2010年 / 7735卷

关键词：

NIR; Multi-object spectroscopy; Commissioning; LBT;

D O I：

10.1117/12.857760

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

LUCIFER 1 is the first of two identical camera-spectrograph units installed at the LBT (Large Binocular Telescope) on Mount Graham in Arizona. Its commissioning took place between September 2008 and November 2009 and has immediately been followed by science operations since December 2009. LUCIFER has a 4x4 arcminute field of view. It is equipped with a 2048x2048 pixel HAWAII-2 array, suitable filters (broad-band z, J, H, K & Ks plus 12 medium and narrow band near-infrared filters) and three gratings for spectroscopy for a resolution of up to similar to 15000. LUCIFER has 3 cameras: two specific for seeing limited imaging (the N3.75 camera, with 0.12"/pixel) and spectroscopy (the N1.8 camera, with 0.25"/pixel) and one for diffraction limited observations (the N30 camera). We report here about the completed seeing-limited commissioning, thus using only two of the cameras.

引用

页数：12

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