The Liverpool Telescope automatic pipeline for real-time GRB afterglow detection

被引：2

作者：

Gomboc, A ^{[1
]}

Monfardini, A

Guidorzi, C

Mundell, CG

Mottram, CJ

Fraser, SN

Smith, RJ

Steele, IA

Carter, D

Bode, MF

Newsam, AM

机构：

[1] Liverpool John Moores Univ, Astrophys Res Inst, Liverpool L3 5UX, Merseyside, England

[2] Univ Ljubljana, Fac Math & Phys, Ljubljana, Slovenia

来源：

NUOVO CIMENTO DELLA SOCIETA ITALIANA DI FISICA C-COLLOQUIA ON PHYSICS | 2005年 / 28卷 / 4-5期

关键词：

D O I：

10.1393/ncc/i2005-10140-3

中图分类号：

学科分类号：

摘要：

The 2-m robotic Liverpool Telescope (LT) is ideally suited to the rapid follow-up of unpredictable and transient events such as GRBs. Our GRB follow-up strategy is designed to identify optical/IR counterparts in real time; it involves the automatic triggering of initial observations, oil receipt of an alert from Gamma Ray Observatories HETE-2, INTEGRAL and Swift, followed by automated data reduction, analysis, OT identification and subsequent observing mode choice. The lack of human intervention in this process requires robustness at all stages of the procedure. Here we describe the telescope, its instrumentation and GRB pipeline.

引用

页码：727 / 730

页数：4

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