FMOS near-IR spectroscopy of Herschel-selected galaxies: star formation rates, metallicity and dust attenuation at z ∼ 1
Article first published online: 8 OCT 2012
© 2012 The Authors Monthly Notices of the Royal Astronomical Society © 2012 RAS
Monthly Notices of the Royal Astronomical Society
Volume 426, Issue 3, pages 1782–1792, 1 November 2012
How to Cite
Roseboom, I. G., Bunker, A., Sumiyoshi, M., Wang, L., Dalton, G., Akiyama, M., Bock, J., Bonfield, D., Buat, V., Casey, C., Chapin, E., Clements, D. L., Conley, A., Curtis-Lake, E., Cooray, A., Dunlop, J. S., Farrah, D., Ham, S. J., Ibar, E., Iwamuro, F., Kimura, M., Lewis, I., Macaulay, E., Magdis, G., Maihara, T., Marsden, G., Mauch, T., Moritani, Y., Ohta, K., Oliver, S. J., Page, M. J., Schulz, B., Scott, D., Symeonidis, M., Takato, N., Tamura, N., Totani, T., Yabe, K. and Zemcov, M. (2012), FMOS near-IR spectroscopy of Herschel-selected galaxies: star formation rates, metallicity and dust attenuation at z ∼ 1. Monthly Notices of the Royal Astronomical Society, 426: 1782–1792. doi: 10.1111/j.1365-2966.2012.21777.x
- Issue published online: 8 OCT 2012
- Article first published online: 8 OCT 2012
- Manuscript Accepted: 23 JUL 2012
- Manuscript Received: 23 JUL 2012
- Science and Technology Facilities Council. Grant Numbers: ST/F002858/1, ST/I000976/1
- European Research Council
- Alfred P. Sloan Foundation
- National Science Foundation
- US Department of Energy
- National Aeronautics and Space Administration
- Japanese Monbukagakusho
- Max Planck Society
- Higher Education Funding Council for England
- Japanese Monbukagakusho
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