AROMA (AGU Robotic Optical Monitor for Astrophysical Objects)

We are developing and operating the automatic telescope Aoyama Gakuin University Robotic Optical Monitor for Astrophysical objects (AROMA) in the Sagamihara Campus of Aoyama Gakuin University. AROMA is composed of two observational equipments, AROMA-N and AROMA-W. AROMA-N is a 30-cm aperture telesco...

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Main Authors: Ichiro Takahashi, Kosuke Tsunashima, Takayuki Shiraki, Toru Kojima, Atsumasa Yoshida, Yujin E. Nakagawa
Format: Article
Language:English
Published: Hindawi Limited 2010-01-01
Series:Advances in Astronomy
Online Access:http://dx.doi.org/10.1155/2010/214604
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spelling doaj-599acff03d8544c1bb3cd8fdc5da9dbc2020-11-24T23:20:42ZengHindawi LimitedAdvances in Astronomy1687-79691687-79772010-01-01201010.1155/2010/214604214604AROMA (AGU Robotic Optical Monitor for Astrophysical Objects)Ichiro Takahashi0Kosuke Tsunashima1Takayuki Shiraki2Toru Kojima3Atsumasa Yoshida4Yujin E. Nakagawa5Department of Physics and Mathematics, Aoyama Gakuin University, 5-10-1 Fuchinobe, Sagamihara, Kanagawa 229-8558, JapanDepartment of Physics and Mathematics, Aoyama Gakuin University, 5-10-1 Fuchinobe, Sagamihara, Kanagawa 229-8558, JapanDepartment of Physics and Mathematics, Aoyama Gakuin University, 5-10-1 Fuchinobe, Sagamihara, Kanagawa 229-8558, JapanDepartment of Physics and Mathematics, Aoyama Gakuin University, 5-10-1 Fuchinobe, Sagamihara, Kanagawa 229-8558, JapanDepartment of Physics and Mathematics, Aoyama Gakuin University, 5-10-1 Fuchinobe, Sagamihara, Kanagawa 229-8558, JapanInstitute of Physical and Chemical Research, 2-1 Hirosawa, Wako, Sait ama 351-0198, JapanWe are developing and operating the automatic telescope Aoyama Gakuin University Robotic Optical Monitor for Astrophysical objects (AROMA) in the Sagamihara Campus of Aoyama Gakuin University. AROMA is composed of two observational equipments, AROMA-N and AROMA-W. AROMA-N is a 30-cm aperture telescope system for rapid follow-up observations of the optical afterglow of gamma-ray bursts. Automatic analysis pipeline for AROMA-N has been developed and is working. The other observational equipment AROMA-W is a wide-field observation system using multiple digital single-lens reflex cameras. It covers a large FOV of about 35∘×25∘. AROMAW provides photometric data in four bands with a limiting V magnitude of about 12-13 mag. Software to analyze massive image data automatically is being developed. We plan to monitor the luminosities of all the stars in the FOV of AROMA-W, detect optical transients, and trigger a follow-up observation with AROMA-N. We report on the development status and observational results of AROMA.http://dx.doi.org/10.1155/2010/214604
collection DOAJ
language English
format Article
sources DOAJ
author Ichiro Takahashi
Kosuke Tsunashima
Takayuki Shiraki
Toru Kojima
Atsumasa Yoshida
Yujin E. Nakagawa
spellingShingle Ichiro Takahashi
Kosuke Tsunashima
Takayuki Shiraki
Toru Kojima
Atsumasa Yoshida
Yujin E. Nakagawa
AROMA (AGU Robotic Optical Monitor for Astrophysical Objects)
Advances in Astronomy
author_facet Ichiro Takahashi
Kosuke Tsunashima
Takayuki Shiraki
Toru Kojima
Atsumasa Yoshida
Yujin E. Nakagawa
author_sort Ichiro Takahashi
title AROMA (AGU Robotic Optical Monitor for Astrophysical Objects)
title_short AROMA (AGU Robotic Optical Monitor for Astrophysical Objects)
title_full AROMA (AGU Robotic Optical Monitor for Astrophysical Objects)
title_fullStr AROMA (AGU Robotic Optical Monitor for Astrophysical Objects)
title_full_unstemmed AROMA (AGU Robotic Optical Monitor for Astrophysical Objects)
title_sort aroma (agu robotic optical monitor for astrophysical objects)
publisher Hindawi Limited
series Advances in Astronomy
issn 1687-7969
1687-7977
publishDate 2010-01-01
description We are developing and operating the automatic telescope Aoyama Gakuin University Robotic Optical Monitor for Astrophysical objects (AROMA) in the Sagamihara Campus of Aoyama Gakuin University. AROMA is composed of two observational equipments, AROMA-N and AROMA-W. AROMA-N is a 30-cm aperture telescope system for rapid follow-up observations of the optical afterglow of gamma-ray bursts. Automatic analysis pipeline for AROMA-N has been developed and is working. The other observational equipment AROMA-W is a wide-field observation system using multiple digital single-lens reflex cameras. It covers a large FOV of about 35∘×25∘. AROMAW provides photometric data in four bands with a limiting V magnitude of about 12-13 mag. Software to analyze massive image data automatically is being developed. We plan to monitor the luminosities of all the stars in the FOV of AROMA-W, detect optical transients, and trigger a follow-up observation with AROMA-N. We report on the development status and observational results of AROMA.
url http://dx.doi.org/10.1155/2010/214604
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