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Seeking Completeness for high-z ULIRGs: from SCUBA to Herschel

Published online by Cambridge University Press:  05 December 2011

Caitlin M. Casey
Caitlin M. Casey*
Affiliation:
Institute for Astronomy, University of Hawai'i, 2680 Woodlawn Dr, Honolulu, HI 96822, USA email: cmcasey@ifa.hawaii.edu
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Abstract

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Selection effects in the submillimeter/far-infrared inhibit detailed analysis of extreme starbursts in the early Universe. Submillimeter Galaxy (SMG) detection and characterization biases against warm temperature SEDs Tdust ~50 K, against the highest redshift ULIRGs z > 3, and has so far been limited to a small sample of ~100 sources that have reliably identified optical or radio counterparts and spectroscopic redshifts. Recent observations by Herschel ⋅ ⋅ ⋅ ⋅ and ⋅ ⋅ ⋅⋅ ⋅ in the ~70–500 μm wavelength range provide a more complete census of high-z ULIRG activity than previous SMG surveys. However, source confusion and lack of spectroscopic identification of reliable counterparts limit the analysis of extreme ULIRGs to the most basic calculations, frought with a priori assumptions (e.g. Tdust/(1+z) degeneracy, far-IR/radio relation, confusion boosting factors, etc). Herein I address the biases on conclusions of SMG work and I demonstrate the need for thorough, spectroscopic follow-up of high-z ULIRGs in order to infer their physical conditions.

Keywords

galaxies–starburstgalaxies–infrared
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 6 , Symposium S277: Tracing the Ancestry of Galaxies (on the land of our ancestors) , December 2010 , pp. 142 - 145
Copyright
Copyright © International Astronomical Union 2011

References

Barger, A. J., Cowie, L. L., & Richards, E. A., 2000, AJ, 119, 2092CrossRefGoogle Scholar
Barger, A. J., Cowie, L. L., Sanders, D. B., Fulton, E., Taniguchi, Y., Sato, Y., Kawara, K., & Okuda, H., 1998, Nature, 394, 248CrossRefGoogle Scholar
Barger, A. J., Cowie, L. L., Smail, I., Ivison, R. J., Blain, A. W., & Kneib, J., 1999, AJ, 117, 2656CrossRefGoogle Scholar
Blain, A. W., Chapman, S. C., Smail, I., & Ivison, R., 2004, ApJ, 611, 725CrossRefGoogle Scholar
Bouwens, R. J., Illingworth, G. D., Franx, M., Chary, R., Meurer, G. R., Conselice, C. J., Ford, H., Giavalisco, M., & vanAAAADokkum, P., 2009, ApJ, 705, 936CrossRefGoogle Scholar
Bradford, C. M., Aguirre, J. E., Aikin, R., Bock, J. J., Earle, L., Glenn, J., Inami, H., Maloney, P. R., Matsuhara, H., Naylor, B. J., Nguyen, H. T., & Zmuidzinas, J., 2009, ApJ, 705, 112CrossRefGoogle Scholar
Casey, C. M., et al. , 2009, MNRAS, 399, 121CrossRefGoogle Scholar
Chapman, S. C., Blain, A. W., Smail, I., & Ivison, R. J., 2005, ApJ, 622, 772CrossRefGoogle Scholar
Chapman, S. C., Smail, I., Blain, A. W., & Ivison, R. J., 2004, ApJ, 614, 671CrossRefGoogle Scholar
Cowie, L. L., Barger, A. J., & Kneib, J.Google Scholar
Dwek, E., Arendt, R. G., Hauser, M. G., Fixsen, D., Kelsall, T., Leisawitz, D., Pei, Y. C., Wright, E. L., Mather, J. C., Moseley, S. H., Odegard, N., Shafer, R., Silverberg, R. F., & Weiland, J. L., 1998, ApJ, 508, 106CrossRefGoogle Scholar
Engel, H., et al. , 2010, ApJ, 724, 233CrossRefGoogle Scholar
Hughes, D. H., Serjeant, S., Dunlop, J., Rowan-Robinson, M., Blain, A., Mann, R. G., Ivison, R., Peacock, J., Efstathiou, A., Gear, W., Oliver, S., Lawrence, A., Longair, M., Goldschmidt, P., & Jenness, T., 1998, Nature, 394, 241CrossRefGoogle Scholar
Kennicutt, R. C. Jr., 1998, ApJ, 498, 541CrossRefGoogle Scholar
Pope, A., Scott, D., Dickinson, M., Chary, R., Morrison, G., Borys, C., Sajina, A., Alexander, D. M., Daddi, E., Frayer, D., MacDonald, E., & Stern, D., 2006, MNRAS, 370, 1185CrossRefGoogle Scholar
Sanders, D. B., Soifer, B. T., Elias, J. H., Madore, B. F., Matthews, K., Neugebauer, G., & Scoville, N. Z., 1988, ApJ, 325, 74CrossRefGoogle Scholar
Sanders, D. B., Soifer, B. T., Elias, J. H., Neugebauer, G., & Matthews, K., 1988, ApJL, 328, L35CrossRefGoogle Scholar
Smail, I., Ivison, R. J., Blain, A. W., & Kneib, J., 2002, MNRAS, 331, 495CrossRefGoogle Scholar
Wang, W., Cowie, L. L., Barger, A. J., & Williams, J. P., 2011, ApJL, 726, L18+CrossRefGoogle Scholar