Hectochelle: a multi-object echelle spectrograph for the converted MMT

被引：56

作者：

Szentgyorgyi, A ^{[1
]}

Cheimets, P ^{[1
]}

Eng, R ^{[1
]}

Fabricant, D ^{[1
]}

Geary, J ^{[1
]}

Hartmann, L ^{[1
]}

Pieri, M ^{[1
]}

Roll, J ^{[1
]}

机构：

[1] Harvard Smithsonian Ctr Astrophys, Cambridge, MA 02138 USA

来源：

OPTICAL ASTRONOMICAL INSTRUMENTATION, PTS 1 AND 2 | 1998年 / 3355卷

关键词：

echelle spectrograph; high resolution spectroscopy;

D O I：

10.1117/12.316766

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The Hectochelle will be a fiber-fed, multi-object spectrograph for the post-conversion MMT which will take 255 simultaneous spectra at a resolution of 32,000-40,000. The absolute efficiency, including optical fiber losses, is predicted to be 6%-10%, depending on the position of a line within a diffractive order. In one hour, features with 60 m Angstrom should be resolved in m(R) = 18 stars with a signal to noise of 10.

引用

页码：242 / 252

页数：3