THE CHANGING EVENT SURVEY: TRANSIENTS, SPACE DEBRIS & NEOs

IF 1.1 4区 物理与天体物理 Q3 ASTRONOMY & ASTROPHYSICS Revista Mexicana de Astronomia y Astrofisica Pub Date : 2021-09-01 DOI:10.22201/ia.14052059p.2021.53.34
T. Sun, C. Zhang, Y. Ping, X. Wu
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Abstract

Motivated by the promising era of time-domain and multi-messenger astronomy, CHanging Event Survey (CHES) is designed to join the ongoing campaign with a powerful wide-field optical telescope array. CHES project aims to monitor the transient universe, including gamma-ray bursts, fast radio bursts, the electromagnetic counterpart of gravitational waves events (kilonova), supernova, variable stars, near-earth objects, and space debris. The array consists of 12 individual wide field refractors with aperture 280 mm, covering 600 square degrees in total. In the same project, two 800 mm prime focus telescopes can be triggered for follow-up observation. Furthermore, CHES can effectively monitor 300 square deg in a dual band simultaneously, which enable the array to do candidate identification and follow-up for the triggers from LIGO/Virgo collaboration, Fermi, Swift, GECam and SVOM satellites.
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变化事件调查:瞬变,空间碎片和近地天体
受时域和多信使天文学前景广阔的时代的激励,变化事件调查(CHES)被设计成与一个强大的宽视场光学望远镜阵列一起加入正在进行的运动。CHES项目旨在监测瞬态宇宙,包括伽马射线暴、快速射电暴、电磁引力波事件(千新星)、超新星、变星、近地天体和空间碎片。该阵列由12个单独的宽视场折射器组成,孔径为280毫米,总面积为600平方度。在同一个项目中,可以触发两台800毫米定焦望远镜进行后续观测。此外,CHES可以同时有效地监测300平方度的双波段,这使得阵列能够对LIGO/Virgo合作、Fermi、Swift、GECam和SVOM卫星的触发点进行候选识别和跟踪。
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来源期刊
Revista Mexicana de Astronomia y Astrofisica
Revista Mexicana de Astronomia y Astrofisica 地学天文-天文与天体物理
CiteScore
1.30
自引率
10.00%
发文量
14
审稿时长
>12 weeks
期刊介绍: The Revista Mexicana de Astronomía y Astrofísica, founded in 1974, publishes original research papers in all branches of astronomy, astrophysics and closely related fields. Two numbers per year are issued and are distributed free of charge to all institutions engaged in the fields covered by the RMxAA.
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