SIRUS: a near infrared simultaneous three-band camera

By T. Nagayama, C. Nagashima, Y. Nakajima, T. Nagata, S. Sato, H. Nakaya, T. Yamamuro, K. Sugitani, Motohide Tamura. SPIE Astronomical Telescopes + Instrumentation, 2003

207 citations recorded by the source corpus.

Subfields: Aerospace Engineering, Electrical and Electronic Engineering

View Paper: https://www.semanticscholar.org/paper/51a5724c72cb611c565215bf34e5831e8eeb8dc3

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In Aerospace Engineering

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Citations in the corpus

• Vvv dr1: the first data release of the milky way bulge and southern plane from the near-infrared eso public survey vista variables in the via lactea (2011, background): “The tests were performed using theapermag3 aperture fluxes, that are used in the CASU catalogues as well as in the VSA database as the default values to represent the flux for all as well as one of the most crowded regions near the Galactic Centre (tile b314).”
• J-GEM observations of an electromagnetic counterpart to the neutron star merger GW170817 (2017, background): “…Mt. John Observatory in New Zealand; 1.5 m Kanata/HONIR (Akitaya et al. 2014) at the Higashi-Hiroshima Astronomical Observatory in Japan; 1.4 m IRSF/SIRIUS (Nagayama et al. 2003) at the South African Astronomical Observatory; and 50 cm MITSuME (Kotani et al. 2005) at the Akeno Observatory in Japan.”
• Interstellar Extinction Law in the J, H, and Ks Bands toward the Galactic Center (2006, methodology): “Our observations were obtained in 2002 March−July, and 2003 April−August using the near-infrared camera SIRIUS (Simultaneous Infrared Imager for Unbiased Survey; Nagashima et al. 1999; Nagayama et al. 2003) on the IRSF (Infrared Survey Facility) telescope.”
• INTERSTELLAR EXTINCTION LAW TOWARD THE GALACTIC CENTER III: J, H, KS BANDS IN THE 2MASS AND THE MKO SYSTEMS, AND 3.6, 4.5, 5.8, 8.0 μm IN THE SPITZER/IRAC SYSTEM (2009, methodology): “◦0 (Figure 1), was observed from 2002 to 2004 using the NIR camera SIRIUS (Simultaneous Infrared Imager for Unbiased Survey; Nagashima et al. 1999; Nagayama et al. 2003) on the 1.4 m telescope IRSF (Infrared Survey Facility).”