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
{"title":"First light simultaneous triple-channel optical observations of the OPTICAM system at the OAN-SPM","authors":"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","doi":"10.1016/j.newast.2024.102262","DOIUrl":null,"url":null,"abstract":"<div><p>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 (<span><math><mrow><msup><mrow><mi>u</mi></mrow><mrow><mo>′</mo></mrow></msup><msup><mrow><mi>g</mi></mrow><mrow><mo>′</mo></mrow></msup><msup><mrow><mi>r</mi></mrow><mrow><mo>′</mo></mrow></msup><msup><mrow><mi>i</mi></mrow><mrow><mo>′</mo></mrow></msup><msup><mrow><mi>z</mi></mrow><mrow><mo>′</mo></mrow></msup></mrow></math></span>), 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.</p></div>","PeriodicalId":54727,"journal":{"name":"New Astronomy","volume":"112 ","pages":"Article 102262"},"PeriodicalIF":1.9000,"publicationDate":"2024-06-25","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"New Astronomy","FirstCategoryId":"101","ListUrlMain":"https://www.sciencedirect.com/science/article/pii/S1384107624000769","RegionNum":4,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q2","JCRName":"ASTRONOMY & ASTROPHYSICS","Score":null,"Total":0}
引用次数: 0
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 (), 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.
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.