Published October 15, 2010 | Version v1
Journal article

ANIR: Infrared-Optical Simultaneous Imager for miniTAO 1 m Telescope at an Altitude of 5640 m

Description

Early follow-up observations of gamma-ray bursts (GRBs) in wide wavelength range, especially from the optical to the near infrared (NIR) bands, are crucial for search of high-redshift GRBs by detecting their Lyman limit break. For this purpose, we have developed a NIR/optical simultaneous imager called ANIR (Atacama Near InfraRed camera) for the University of Tokyo Atacama 1.0 m telescope. Installed at the summit of Co. Chajnantor (5640 m altitude) in northern Chile, this telescope is the world's highest optical/NIR observatory. ANIR saw the first light in June 2009, and several observing runs have been carried out for performance verification as well as scientific observations. During the run, we have successfully detected an optical/NIR afterglow of GRB091018. Thanks to the excellent seeing (median ∼0''.8), 5σ limiting magnitudes reach 23.3, 20.6, and 20.8 mag(AB) in the B, J and Ks bands, respectively, with 600 sec exposure.

Additional details

Identifiers

Publishing Information

Journal Title
AIP Conference Proceedings
Journal Volume
1279
Journal Issue
1
Journal Page Range
p. 397-399
ISSN
0094-243X
CODEN
APCPCS

Conference

Title
Conference on deciphering the ancient universe with gamma-ray bursts
Dates
19-23 Apr 2010
Place
Kyoto (Japan)

INIS

Country of Publication
United States
Country of Input or Organization
International Atomic Energy Agency (IAEA)
INIS RN
42035200
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY; S46: INSTRUMENTATION RELATED TO NUCLEAR SCIENCE AND TECHNOLOGY;
Resource subtype / Literary indicator
Conference
Descriptors DEI
AFTERGLOW; ASTROPHYSICS; CAMERAS; COSMIC GAMMA BURSTS; GAMMA ASTRONOMY; GAMMA DETECTION; PERFORMANCE; RED SHIFT; TELESCOPE COUNTERS; VISIBLE SPECTRA
Descriptors DEC
ASTRONOMY; COSMIC RADIATION; DETECTION; IONIZING RADIATIONS; PHYSICS; PRIMARY COSMIC RADIATION; RADIATION DETECTION; RADIATIONS; SPECTRA

Optional Information

Notes
(c) 2010 American Institute of Physics