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Unbiased large spectroscopic surveys of galaxies selected by SPICA using dust bands

H Kaneda, D Ishihara, S Oyabu, M Yamagishi, T Wada, L Armus, Maarten Baes (UGent) , V Charmandaris, B Czerny, A Efstathiou, et al.
(2017) PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF AUSTRALIA. 34.
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Abstract
The mid-infrared range contains many spectral features associated with large molecules and dust grains such as polycyclic aromatic hydrocarbons and silicates. These are usually very strong compared to fine-structure gas lines, and thus valuable in studying the spectral properties of faint distant galaxies. In this paper, we evaluate the capability of low-resolution mid-infrared spectroscopic surveys of galaxies that could be performed by SPICA. The surveys are designed to address the question how star formation and black hole accretion activities evolved over cosmic time through spectral diagnostics of the physical conditions of the interstellar/circumnuclear media in galaxies. On the basis of results obtained with Herschel far-infrared photometric surveys of distant galaxies and Spitzer and AKARI near-to mid-infrared spectroscopic observations of nearby galaxies, we estimate the numbers of the galaxies at redshift z > 0.5, which are expected to be detected in the polycyclic aromatic hydrocarbon features or dust continuum by a wide (10 deg(2) ) or deep (1 deg(2) ) blind survey. both for a given observation time of 600 h. As by-products of the wide blind survey, we also expect to detect debris disks, through the mid-infrared excess above the photospheric emission of nearby main-sequence stars, and we estimate their number. We demonstrate that the SPICA mid-infrared surveys will efficiently provide us with unprecedentedly large spectral samples, which can be studied further in the far-infrared with SPICA.
Keywords
galaxies: active, galaxies: evolution, galaxies: star formation, infrared: galaxies, infrared: ISM, methods: observational, ULTRALUMINOUS INFRARED GALAXIES, ACTIVE GALACTIC NUCLEI, POLYCYCLIC AROMATIC-HYDROCARBONS, STAR-FORMING GALAXIES, MU-M SPECTROSCOPY, MIDINFRARED SPECTROSCOPY, SUBMILLIMETER GALAXIES, INTERSTELLAR-MEDIUM, PAH EMISSION, LUMINOUS GALAXIES

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MLA
Kaneda, H., et al. “Unbiased Large Spectroscopic Surveys of Galaxies Selected by SPICA Using Dust Bands.” PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF AUSTRALIA, vol. 34, 2017, doi:10.1017/pasa.2017.56.
APA
Kaneda, H., Ishihara, D., Oyabu, S., Yamagishi, M., Wada, T., Armus, L., … Wang, L. (2017). Unbiased large spectroscopic surveys of galaxies selected by SPICA using dust bands. PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF AUSTRALIA, 34. https://doi.org/10.1017/pasa.2017.56
Chicago author-date
Kaneda, H, D Ishihara, S Oyabu, M Yamagishi, T Wada, L Armus, Maarten Baes, et al. 2017. “Unbiased Large Spectroscopic Surveys of Galaxies Selected by SPICA Using Dust Bands.” PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF AUSTRALIA 34. https://doi.org/10.1017/pasa.2017.56.
Chicago author-date (all authors)
Kaneda, H, D Ishihara, S Oyabu, M Yamagishi, T Wada, L Armus, Maarten Baes, V Charmandaris, B Czerny, A Efstathiou, JA Fernández-Ontiveros, A Ferrara, E González-Alfonso, M Griffin, C Gruppioni, E Hatziminaoglou, M Imanishi, K Kohno, J Kwon, T Nakagawa, T Onaka, F Pozzi, D Scott, J-DT Smith, L Spinoglio, T Suzuki, F van der Tak, M Vaccari, C Vignali, and L Wang. 2017. “Unbiased Large Spectroscopic Surveys of Galaxies Selected by SPICA Using Dust Bands.” PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF AUSTRALIA 34. doi:10.1017/pasa.2017.56.
Vancouver
1.
Kaneda H, Ishihara D, Oyabu S, Yamagishi M, Wada T, Armus L, et al. Unbiased large spectroscopic surveys of galaxies selected by SPICA using dust bands. PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF AUSTRALIA. 2017;34.
IEEE
[1]
H. Kaneda et al., “Unbiased large spectroscopic surveys of galaxies selected by SPICA using dust bands,” PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF AUSTRALIA, vol. 34, 2017.
@article{8545491,
  abstract     = {{The mid-infrared range contains many spectral features associated with large molecules and dust grains such as polycyclic aromatic hydrocarbons and silicates. These are usually very strong compared to fine-structure gas lines, and thus valuable in studying the spectral properties of faint distant galaxies. In this paper, we evaluate the capability of low-resolution mid-infrared spectroscopic surveys of galaxies that could be performed by SPICA. The surveys are designed to address the question how star formation and black hole accretion activities evolved over cosmic time through spectral diagnostics of the physical conditions of the interstellar/circumnuclear media in galaxies. On the basis of results obtained with Herschel far-infrared photometric surveys of distant galaxies and Spitzer and AKARI near-to mid-infrared spectroscopic observations of nearby galaxies, we estimate the numbers of the galaxies at redshift z > 0.5, which are expected to be detected in the polycyclic aromatic hydrocarbon features or dust continuum by a wide (10 deg(2) ) or deep (1 deg(2) ) blind survey. both for a given observation time of 600 h. As by-products of the wide blind survey, we also expect to detect debris disks, through the mid-infrared excess above the photospheric emission of nearby main-sequence stars, and we estimate their number. We demonstrate that the SPICA mid-infrared surveys will efficiently provide us with unprecedentedly large spectral samples, which can be studied further in the far-infrared with SPICA.}},
  articleno    = {{e059}},
  author       = {{Kaneda, H and Ishihara, D and Oyabu, S and Yamagishi, M and Wada, T and Armus, L and Baes, Maarten and Charmandaris, V and Czerny, B and Efstathiou, A and Fernández-Ontiveros, JA and Ferrara, A and González-Alfonso, E and Griffin, M and Gruppioni, C and Hatziminaoglou, E and Imanishi, M and Kohno, K and Kwon, J and Nakagawa, T and Onaka, T and Pozzi, F and Scott, D and Smith, J-DT and Spinoglio, L and Suzuki, T and van der Tak, F and Vaccari, M and Vignali, C and Wang, L}},
  issn         = {{1323-3580}},
  journal      = {{PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF AUSTRALIA}},
  keywords     = {{galaxies: active,galaxies: evolution,galaxies: star formation,infrared: galaxies,infrared: ISM,methods: observational,ULTRALUMINOUS INFRARED GALAXIES,ACTIVE GALACTIC NUCLEI,POLYCYCLIC AROMATIC-HYDROCARBONS,STAR-FORMING GALAXIES,MU-M SPECTROSCOPY,MIDINFRARED SPECTROSCOPY,SUBMILLIMETER GALAXIES,INTERSTELLAR-MEDIUM,PAH EMISSION,LUMINOUS GALAXIES}},
  language     = {{eng}},
  pages        = {{16}},
  title        = {{Unbiased large spectroscopic surveys of galaxies selected by SPICA using dust bands}},
  url          = {{http://doi.org/10.1017/pasa.2017.56}},
  volume       = {{34}},
  year         = {{2017}},
}
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