AKARI near- to mid-infrared imaging and spectroscopic observations of the small magellanic cloud. I bright point source list

Yoshifusa Ita; Takashi Onaka; Toshihiko Tanabé; Noriyuki Matsunaga; Mikako Matsuura; Issei Yamamura; Yoshikazu Nakada; Hideyuki Izumiura; Toshiya Ueta; Hiroyuki Mito; Hinako Fukushi; Daisuke Kato

doi:10.1093/pasj/62.2.273

AKARI near- to mid-infrared imaging and spectroscopic observations of the small magellanic cloud. I bright point source list

Yoshifusa Ita, Takashi Onaka, Toshihiko Tanabé, Noriyuki Matsunaga, Mikako Matsuura, Issei Yamamura, Yoshikazu Nakada, Hideyuki Izumiura, Toshiya Ueta, Hiroyuki Mito, Hinako Fukushi, Daisuke Kato

SCI - Astronomy

Research output: Contribution to journal › Article › peer-review

19 Citations (Scopus)

Abstract

We carried out near- to mid-infrared imaging and spectroscopic observations of patchy areas in the Small Magellanic Cloud using the Infrared Camera aboard AKARI. Two lOOarcmin² areas were imaged in 3.2, 4.1, 7, 11, 15, and 24 μm, and also spectroscopically observed in the wavelength range continuously from 2.5 to 13.4μm. The spectral resolving power, λ/△λ, values were about 20, 50, and 50 at 3.5, 6.6, and 10.6 μm, respectively. Other than the two 100 arcmin² areas, some patchy areas were imaged and/or spectroscopically observed as well. In this paper, we overview the observations and present a list of near- to mid-infrared photometric results, which lists ̃ 12000 near-infrared and ̃ 1800 mid-infrared bright point sources detected in the observed areas. The 10 σ limits are 16.50, 16.12, 13.28, 11.26, 9.62, and 8.76 in Vega magnitudes at 3.2, 4.1, 7, 11, 15, and 24 μm bands, respectively.

Original language	English
Pages (from-to)	273-286
Number of pages	14
Journal	Publication of the Astronomical Society of Japan
Volume	62
Issue number	2
DOIs	https://doi.org/10.1093/pasj/62.2.273
Publication status	Published - 2010 Apr 25

Keywords

Galaxies: magellanic clouds
Infrared: stars
Stars: Agb and post-AGB

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Ita, Y., Onaka, T., Tanabé, T., Matsunaga, N., Matsuura, M., Yamamura, I., Nakada, Y., Izumiura, H., Ueta, T., Mito, H., Fukushi, H., & Kato, D. (2010). AKARI near- to mid-infrared imaging and spectroscopic observations of the small magellanic cloud. I bright point source list. Publication of the Astronomical Society of Japan, 62(2), 273-286. https://doi.org/10.1093/pasj/62.2.273

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abstract = "We carried out near- to mid-infrared imaging and spectroscopic observations of patchy areas in the Small Magellanic Cloud using the Infrared Camera aboard AKARI. Two lOOarcmin2 areas were imaged in 3.2, 4.1, 7, 11, 15, and 24 μm, and also spectroscopically observed in the wavelength range continuously from 2.5 to 13.4μm. The spectral resolving power, λ/△λ, values were about 20, 50, and 50 at 3.5, 6.6, and 10.6 μm, respectively. Other than the two 100 arcmin2 areas, some patchy areas were imaged and/or spectroscopically observed as well. In this paper, we overview the observations and present a list of near- to mid-infrared photometric results, which lists{\~ } 12000 near-infrared and{\~ } 1800 mid-infrared bright point sources detected in the observed areas. The 10 σ limits are 16.50, 16.12, 13.28, 11.26, 9.62, and 8.76 in Vega magnitudes at 3.2, 4.1, 7, 11, 15, and 24 μm bands, respectively.",

keywords = "Galaxies: magellanic clouds, Infrared: stars, Stars: Agb and post-AGB",

author = "Yoshifusa Ita and Takashi Onaka and Toshihiko Tanab{\'e} and Noriyuki Matsunaga and Mikako Matsuura and Issei Yamamura and Yoshikazu Nakada and Hideyuki Izumiura and Toshiya Ueta and Hiroyuki Mito and Hinako Fukushi and Daisuke Kato",

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doi = "10.1093/pasj/62.2.273",

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Ita, Y, Onaka, T, Tanabé, T, Matsunaga, N, Matsuura, M, Yamamura, I, Nakada, Y, Izumiura, H, Ueta, T, Mito, H, Fukushi, H & Kato, D 2010, 'AKARI near- to mid-infrared imaging and spectroscopic observations of the small magellanic cloud. I bright point source list', Publication of the Astronomical Society of Japan, vol. 62, no. 2, pp. 273-286. https://doi.org/10.1093/pasj/62.2.273

TY - JOUR

T1 - AKARI near- to mid-infrared imaging and spectroscopic observations of the small magellanic cloud. I bright point source list

AU - Ita, Yoshifusa

AU - Onaka, Takashi

AU - Tanabé, Toshihiko

AU - Matsunaga, Noriyuki

AU - Matsuura, Mikako

AU - Yamamura, Issei

AU - Nakada, Yoshikazu

AU - Izumiura, Hideyuki

AU - Ueta, Toshiya

AU - Mito, Hiroyuki

AU - Fukushi, Hinako

AU - Kato, Daisuke

PY - 2010/4/25

Y1 - 2010/4/25

N2 - We carried out near- to mid-infrared imaging and spectroscopic observations of patchy areas in the Small Magellanic Cloud using the Infrared Camera aboard AKARI. Two lOOarcmin2 areas were imaged in 3.2, 4.1, 7, 11, 15, and 24 μm, and also spectroscopically observed in the wavelength range continuously from 2.5 to 13.4μm. The spectral resolving power, λ/△λ, values were about 20, 50, and 50 at 3.5, 6.6, and 10.6 μm, respectively. Other than the two 100 arcmin2 areas, some patchy areas were imaged and/or spectroscopically observed as well. In this paper, we overview the observations and present a list of near- to mid-infrared photometric results, which lists ̃ 12000 near-infrared and ̃ 1800 mid-infrared bright point sources detected in the observed areas. The 10 σ limits are 16.50, 16.12, 13.28, 11.26, 9.62, and 8.76 in Vega magnitudes at 3.2, 4.1, 7, 11, 15, and 24 μm bands, respectively.

AB - We carried out near- to mid-infrared imaging and spectroscopic observations of patchy areas in the Small Magellanic Cloud using the Infrared Camera aboard AKARI. Two lOOarcmin2 areas were imaged in 3.2, 4.1, 7, 11, 15, and 24 μm, and also spectroscopically observed in the wavelength range continuously from 2.5 to 13.4μm. The spectral resolving power, λ/△λ, values were about 20, 50, and 50 at 3.5, 6.6, and 10.6 μm, respectively. Other than the two 100 arcmin2 areas, some patchy areas were imaged and/or spectroscopically observed as well. In this paper, we overview the observations and present a list of near- to mid-infrared photometric results, which lists ̃ 12000 near-infrared and ̃ 1800 mid-infrared bright point sources detected in the observed areas. The 10 σ limits are 16.50, 16.12, 13.28, 11.26, 9.62, and 8.76 in Vega magnitudes at 3.2, 4.1, 7, 11, 15, and 24 μm bands, respectively.

KW - Galaxies: magellanic clouds

KW - Infrared: stars

KW - Stars: Agb and post-AGB

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DO - 10.1093/pasj/62.2.273

M3 - Article

AN - SCOPUS:77953338638

SN - 0004-6264

VL - 62

SP - 273

EP - 286

JO - Publication of the Astronomical Society of Japan

JF - Publication of the Astronomical Society of Japan

IS - 2

ER -

AKARI near- to mid-infrared imaging and spectroscopic observations of the small magellanic cloud. I bright point source list

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Keywords

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