Correction of the atmospheric transmission in infrared spectroscopy

被引：89

作者：

Maiolino, R ^{[1
]}

Rieke, GH ^{[1
]}

Rieke, MJ ^{[1
]}

机构：

[1] UNIV ARIZONA,STEWARD OBSERV,TUCSON,AZ 85721

来源：

ASTRONOMICAL JOURNAL | 1996年 / 111卷 / 01期

关键词：

D O I：

10.1086/117804

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

High-resolution and sensitive near-infrared spectroscopy is often limited by the ability to correct the atmospheric transmission. The simple division of the object spectrum by the spectrum of a nearby star turns out to be unsatisfactory because of the stellar features in the latter. We show how to measure the atmospheric transmission with a nearby early GV or late FV star, and to correct for the stellar features by means of the (atmospheric-transmission-corrected) solar spectrum. (C) 1995 American Astronomical Society.

引用

页码：537 / 540

页数：4