First light simultaneous triple-channel optical observations of the OPTICAM system at the OAN-SPM

IF 1.9 4区 物理与天体物理 Q2 ASTRONOMY & ASTROPHYSICS New Astronomy Pub Date : 2024-06-25 DOI:10.1016/j.newast.2024.102262
Angel Castro , Raúl Michel , Noel Castro Segura , Diego Altamirano , Carlos Tejada , Joel Herrera , Enrique Colorado , Gerardo Sierra , Liliana Altamirano-Dévora , Juan Echevarría , Rasjied Sloot , Rudy Wijnands , Iván Zavala , David Rojas , Juan V. Hernández Santisteban , Federico Vincentelli , Javier A. Hernández-Landa , Song Wang , Melissa Fuentes , Poshak Gandhi , Francisco Valenzuela
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Abstract

OPTICAM is a triple-band optical system developed for the 2.1 m telescope of the National Astronomical Observatory in the Sierra de San Pedro Mártir (OAN-SPM). Partial engineering tests were conducted in 2019, with the complete system experiencing its first light in March 2022. The system incorporates two beam splitters, enabling simultaneous observations on three channels. Users can choose three out of the five available filters from the SDSS filter set (ugriz), covering the wavelength range from 320 to 1000 nm. It offers an effective field of view of approximately 4.7, 4.7, and 5.6 arcminutes in each of its arms, respectively. Due to its design and capabilities, OPTICAM is suitable for coordinated observations with other ground-based and space-based observatories. This document presents the final instrument design and the current system status. Some of the optical tests carried out are described. We also present the results of scientific observations conducted during its first light and first year of operations.

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在 OAN-SPM 对 OPTICAM 系统进行首次三通道同步光学观测
OPTICAM 是为圣佩德罗马蒂尔山脉国家天文台(OAN-SPM)的 2.1 米望远镜开发的三波段光学系统。2019 年进行了部分工程测试,整个系统将于 2022 年 3 月首次点亮。该系统包含两个分光镜,可在三个频道上同时进行观测。用户可以从 SDSS 滤光片组()的五个可用滤光片中选择三个,波长范围从 320 纳米到 1000 纳米。它的每个臂的有效视场分别约为 4.7、4.7 和 5.6 弧分。由于其设计和功能,OPTICAM 适合与其他地面和空间观测站进行协调观测。本文件介绍了仪器的最终设计和目前的系统状况。介绍了已进行的一些光学测试。我们还介绍了在其首次点亮和第一年运行期间进行的科学观测的结果。
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来源期刊
New Astronomy
New Astronomy 地学天文-天文与天体物理
CiteScore
4.00
自引率
10.00%
发文量
109
审稿时长
13.6 weeks
期刊介绍: New Astronomy publishes articles in all fields of astronomy and astrophysics, with a particular focus on computational astronomy: mathematical and astronomy techniques and methodology, simulations, modelling and numerical results and computational techniques in instrumentation. New Astronomy includes full length research articles and review articles. The journal covers solar, stellar, galactic and extragalactic astronomy and astrophysics. It reports on original research in all wavelength bands, ranging from radio to gamma-ray.
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