SAINT: a Wide-Field Multichannel Optical Telescope Project

被引：0

作者：

Beskin, G. ^{[1
,3
]}

Biryukov, A. ^{[4
]}

Bondar, S. ^{[1
,2
]}

Ivanov, E. ^{[2
]}

Karpov, S. ^{[3
]}

Katkova, E. ^{[2
]}

Orekhova, N. ^{[2
]}

Perkov, A. ^{[2
]}

Plokhotnichenko, V. ^{[1
]}

Sasyuk, V. ^{[2
]}

机构：

[1] Russian Acad Sci, Special Astrophys Observ, Nizhnii Arkhyz, Russia

[2] Res & Prod Corp Precis Syst & Instruments, Nizhnii Arkhyz, Russia

[3] Kazan Volga Reg Fed Univ, Kazan, Russia

[4] Moscow MV Lomonosov State Univ, Moscow, Russia

来源：

STARS: FROM COLLAPSE TO COLLAPSE | 2017年 / 510卷

基金：

俄罗斯科学基金会;

关键词：

2-TELESCOPE COMPLEX; TRANSIENTS; SEARCH;

D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Here we present the project of a Small Aperture Imaging Network Telescope (SAINT), which consists of 500 small telescopes - channels - with 1 sq.deg. fields of view each. The telescope operates either in wide-field monitoring mode, covering 500 square degrees of the sky simultaneously with 0.1 s temporal resolution and detection limit of about 22-23 mag in 1000 s, or in follow-up regime, upon detection of a transient. In the latter case, all the channels immediately repoint towards the transient for its detailed (multicolor, polarimetric, spectroscopic) investigation. In this regime, SAINT is equivalent to 8-m telescope and may be used to solve most of standard astro-physical problems.

引用

页码：530 / 534

页数：5

共 25 条

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