Opticam: a triple-camera optical system designed to explore the fastest timescales in astronomy
ABSTRACT We report the development of a high-time resolution, 3-colour, simultaneous optical imaging system for the 2.1 m telescope in the San Pedro Mártir Observatory, México. OPTICAM will be equipped with three 2,048×2,048 pixel Andor Zyla 4.2-Plus sCMOS cameras and a set of SDSS filters allowing optical coverage in the 320-1,100 nm range. OPTICAM will nominally allow sub-second exposures. Given its instrumental design, a wide range of fast-variability astrophysical sources can be targeted with OPTICAM including X-ray binaries, pulsating white dwarfs, accreting compact objects, eclipsing binaries and exoplanets. OPTICAM observations will be proprietary for only six months and will then be made publicly available to the astronomical community.
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Universidad Nacional Autónoma de México, Instituto de Astronomía
2019
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oai:scielo:S0185-110120190002003632020-11-23Opticam: a triple-camera optical system designed to explore the fastest timescales in astronomyCastro,A.Altamirano,D.Michel,R.Gandhi,P.Hernández Santisteban,J. V.Echevarría,J.Tejada,C.Knigge,C.Sierra,G.Colorado,E.Hernández-Landa,J.Whiter,D.Middleton,M.García,B.Guisa,G.Castro Segura,N. telescopes ABSTRACT We report the development of a high-time resolution, 3-colour, simultaneous optical imaging system for the 2.1 m telescope in the San Pedro Mártir Observatory, México. OPTICAM will be equipped with three 2,048×2,048 pixel Andor Zyla 4.2-Plus sCMOS cameras and a set of SDSS filters allowing optical coverage in the 320-1,100 nm range. OPTICAM will nominally allow sub-second exposures. Given its instrumental design, a wide range of fast-variability astrophysical sources can be targeted with OPTICAM including X-ray binaries, pulsating white dwarfs, accreting compact objects, eclipsing binaries and exoplanets. OPTICAM observations will be proprietary for only six months and will then be made publicly available to the astronomical community.info:eu-repo/semantics/openAccessUniversidad Nacional Autónoma de México, Instituto de AstronomíaRevista mexicana de astronomía y astrofísica v.55 n.2 20192019-01-01info:eu-repo/semantics/articletext/htmlhttp://www.scielo.org.mx/scielo.php?script=sci_arttext&pid=S0185-11012019000200363en10.22201/ia.01851101p.2019.55.02.20 |
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Castro,A. Altamirano,D. Michel,R. Gandhi,P. Hernández Santisteban,J. V. Echevarría,J. Tejada,C. Knigge,C. Sierra,G. Colorado,E. Hernández-Landa,J. Whiter,D. Middleton,M. García,B. Guisa,G. Castro Segura,N. |
spellingShingle |
Castro,A. Altamirano,D. Michel,R. Gandhi,P. Hernández Santisteban,J. V. Echevarría,J. Tejada,C. Knigge,C. Sierra,G. Colorado,E. Hernández-Landa,J. Whiter,D. Middleton,M. García,B. Guisa,G. Castro Segura,N. Opticam: a triple-camera optical system designed to explore the fastest timescales in astronomy |
author_facet |
Castro,A. Altamirano,D. Michel,R. Gandhi,P. Hernández Santisteban,J. V. Echevarría,J. Tejada,C. Knigge,C. Sierra,G. Colorado,E. Hernández-Landa,J. Whiter,D. Middleton,M. García,B. Guisa,G. Castro Segura,N. |
author_sort |
Castro,A. |
title |
Opticam: a triple-camera optical system designed to explore the fastest timescales in astronomy |
title_short |
Opticam: a triple-camera optical system designed to explore the fastest timescales in astronomy |
title_full |
Opticam: a triple-camera optical system designed to explore the fastest timescales in astronomy |
title_fullStr |
Opticam: a triple-camera optical system designed to explore the fastest timescales in astronomy |
title_full_unstemmed |
Opticam: a triple-camera optical system designed to explore the fastest timescales in astronomy |
title_sort |
opticam: a triple-camera optical system designed to explore the fastest timescales in astronomy |
description |
ABSTRACT We report the development of a high-time resolution, 3-colour, simultaneous optical imaging system for the 2.1 m telescope in the San Pedro Mártir Observatory, México. OPTICAM will be equipped with three 2,048×2,048 pixel Andor Zyla 4.2-Plus sCMOS cameras and a set of SDSS filters allowing optical coverage in the 320-1,100 nm range. OPTICAM will nominally allow sub-second exposures. Given its instrumental design, a wide range of fast-variability astrophysical sources can be targeted with OPTICAM including X-ray binaries, pulsating white dwarfs, accreting compact objects, eclipsing binaries and exoplanets. OPTICAM observations will be proprietary for only six months and will then be made publicly available to the astronomical community. |
publisher |
Universidad Nacional Autónoma de México, Instituto de Astronomía |
publishDate |
2019 |
url |
http://www.scielo.org.mx/scielo.php?script=sci_arttext&pid=S0185-11012019000200363 |
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