تقرير
FMOS near-IR spectroscopy of Herschel selected galaxies: star formation rates, metallicity and dust attenuation at z~1
| العنوان: | FMOS near-IR spectroscopy of Herschel selected galaxies: star formation rates, metallicity and dust attenuation at z~1 |
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| المؤلفون: | 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, Douglas, Symeonidis, M., Takato, N., Tamura, N., Totani, T., Yabe, K., Zemcov, M. |
| سنة النشر: | 2012 |
| المجموعة: | Astrophysics |
| مصطلحات موضوعية: | Astrophysics - Cosmology and Nongalactic Astrophysics |
| الوصف: | We investigate the properties (e.g. star formation rate, dust attentuation, stellar mass and metallicity) of a sample of infrared luminous galaxies at z \sim 1 via near-IR spectroscopy with Subaru-FMOS. Our sample consists of Herschel SPIRE and Spitzer MIPS selected sources in the COSMOS field with photometric redshifts in the range 0.7 < z-phot < 1.8, which have been targeted in 2 pointings (0.5 sq. deg.) with FMOS. We find a modest success rate for emission line detections, with candidate H{\alpha} emission lines detected for 57 of 168 SPIRE sources (34 per cent). By stacking the near-IR spectra we directly measure the mean Balmer decrement for the H{\alpha} and H{\beta} lines, finding a value of Comment: 13 pages, 7 figures, MNRAS accepted |
| نوع الوثيقة: | Working Paper |
| DOI: | 10.1111/j.1365-2966.2012.21777.x |
| URL الوصول: | http://arxiv.org/abs/1207.5564 |
| رقم الأكسشن: | edsarx.1207.5564 |
| قاعدة البيانات: | arXiv |
| DOI: | 10.1111/j.1365-2966.2012.21777.x |
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