天网机器人望远镜网络的长期光度测定

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.2021.53.40

S. Zola, V. Kouprianov, D. Reichart, G. Bhatta, D. Caton

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引用次数: 4

摘要

在本文中，我们描述了天网机器人望远镜网络，这是一个跨越四大洲的大约24个小型光学望远镜的网络。对于该网络的潜在用户，我们提供了其操作的详细信息，并提到了可能影响在天网软件控制下进行的观测的某些注意事项。对oj49和3C 279两颗耀变体的长期观测证明了该网络的实际性能。我们展示了它们在2018/19观测季节使用天网望远镜子集获得的光度光曲线。给出了这两个目标的变率分析的初步结果，包括光变化的定量性质和在季节光曲线中发现的可能的准周期振荡(QPOs)的周期。

本文章由计算机程序翻译，如有差异，请以英文原文为准。

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LONG-TERM PHOTOMETRY WITH SKYNET ROBOTIC TELESCOPE NETWORK

In this paper, we describe the Skynet Robotic Telescope Network, a network of about 2 dozen small optical telescopes spanning four continents. For a prospective user of the network, we provide details on its operation and mention certain caveats potentially affecting observations taken under the control of Skynet software. The actual performance of the network is demonstrated by long-term observations of two blazars: OJ 49 and 3C 279. We show their photometric light curves acquired with a subset of Skynet telescopes in the 2018/19 observing seasons. Preliminary results of the analysis of the variability of these two targets are given, including the quantitative properties of light variations and the periods of possible Quasi Periodic Oscillations (QPOs) found in the seasonal light curves.

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来源期刊

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

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.