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High-Redshift Galaxies

Published online by Cambridge University Press:  23 September 2016

Amy Barger
Amy Barger*
Affiliation:
Department of Astronomy, University of Wisconsin-Madison, 475 N. Charter St., Madison, WI 53706 Department of Physics and Astronomy, University of Hawaii, 2505 Correa Road, Honolulu, HI 96822 Institute for Astronomy, University of Hawaii, 2680 Woodlawn Drive, Honolulu, HI 96822

Abstract

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Mapping the history of star formation requires combining observations at many wavelengths. The most dramatic episodes of star formation occurred in high-redshift (z > 1) galaxies obscured by dust. These galaxies can be seen at submillimeter wavelengths. While these episodes clearly constitute much of the star formation in the universe, we still do not know the redshift distribution. Although progess has been made in determining the nature of the brightest members of the submillimeter population, these galaxies comprise only a tiny fraction of the submillimeter extragalactic background light. Optical star formation, by contrast, is well mapped but hard to interpret because of the problems of extinction. At recent times there is still substantial star formation, but it primarily takes place in small galaxies. This cosmic downsizing is paralleled by similar evolution in the properties of AGNs.

Type
Session VI: The Distant Universe
Information
Symposium - International Astronomical Union , Volume 216: Maps of the Cosmos , 2005 , pp. 309 - 324
Copyright
Copyright © Astronomical Society of the Pacific 2005 

References

Adelberger, K. L., & Steidel, C. C. 2000, ApJ, 544, 218 CrossRefGoogle Scholar
Alexander, D. M., et al. 2003, AJ, 126, 539 Google Scholar
Almaini, O., et al. 2003, MNRAS, 338, 303 CrossRefGoogle Scholar
Almaini, O., Lawrence, A., & Boyle, B. J. 1999, MNRAS, 305, L59 Google Scholar
Barger, A. J. 2002, Contemporary Physics, 43, 339 Google Scholar
Barger, A. J., Cowie, L. L., Mushotzky, R. F., & Richards, E. A. 2001b, AJ, 121, 662 Google Scholar
Barger, A. J., Cowie, L. L., & Richards, E. A. 2000, AJ, 119, 2092 CrossRefGoogle Scholar
Barger, A. J., Cowie, L. L., & Sanders, D. B. 1999a, ApJ, 518, L5 Google Scholar
Barger, A. J., et al. 1998, Nature, 394, 248 CrossRefGoogle Scholar
Barger, A. J., et al. 1999b, AJ, 117, 2656 CrossRefGoogle Scholar
Barger, A. J., et al. 2001a, ApJ, 560, L23 Google Scholar
Barger, A. J., et al. 2003, AJ, 126, 632 Google Scholar
Bautz, M. W., et al. 2000, ApJ, 543, L119 Google Scholar
Blain, A.W., Kneib, J.-P., Ivison, R.J., & Smail, I. 1999, ApJ, 512, L87 CrossRefGoogle Scholar
Blain, A. W., & Longair, M. S. 1993, MNRAS, 264, 509 Google Scholar
Borys, C., Chapman, S. C., Halpern, M., & Scott, D. 2002, MNRAS, 330, L63 Google Scholar
Campana, S., Moretti, A., Lazzati, D., & Tagliaferri, G. 2001, ApJ, 560, L19 Google Scholar
Carilli, C. L., & Yun, M. S. 1999, ApJ, 513, L13 CrossRefGoogle Scholar
Carilli, C. L., & Yun, M. S. 2000, ApJ, 530, 618 Google Scholar
Chapman, S. C., Blain, A. W., Ivison, R. J., & Smail, I. R. 2003a, Nature, 422, 695 CrossRefGoogle Scholar
Chapman, S. C., et al. 2000, MNRAS, 319, 318 Google Scholar
Chapman, S. C., et al. 2003b, ApJ, 585, 57 CrossRefGoogle Scholar
Chapman, S. C., Scott, D., Borys, C., & Fahlman, G. G. 2002, MNRAS, 330, 92 Google Scholar
Condon, J. J. 1989, ApJ, 338, 13 Google Scholar
Condon, J. J. 1992, ARA&A, 30, 575 Google Scholar
Connolly, A.J., Szalay, A.S., Dickinson, M., SubbaRao, M.U., & Brunner, R.J. 1997, ApJ, 486, L11 Google Scholar
Cowie, L. L., Barger, A. J., Fomalont, E. B., & Capak, P. 2004, ApJ, 603, L69 Google Scholar
Cowie, L. L., Barger, A. J., & Kneib, J.-P. 2002a, AJ, 123, 2197 CrossRefGoogle Scholar
Cowie, L. L., et al. 2002b, ApJ, 566, L5 Google Scholar
Cowie, L. L., Lilly, S. J., Gardner, J., & McLean, I. S. 1988, ApJ, 332, L29 Google Scholar
Cowie, L.L., Songaila, A., & Barger, A.J. 1999, AJ, 118, 603 Google Scholar
Cowie, L. L., Songaila, A., Hu, E. M., & Cohen, J. G. 1996, AJ, 112, 839 Google Scholar
Dunne, L., Clements, D. L., & Eales, S. A. 2000, MNRAS, 319, 813 Google Scholar
Eales, S., et al. 1999, ApJ, 515, 518 CrossRefGoogle Scholar
Eales, S., et al. 2000, AJ, 120, 2244 CrossRefGoogle Scholar
Fabian, A. C., et al. 2000, MNRAS, 315, L8 Google Scholar
Fabian, A. C., & Iwasawa, K. 1999, MNRAS, 303, L34 Google Scholar
Fixsen, D. J., Dwek, E., Mather, J. C., Bennett, C. L., & Shafer, R. A. 1998, ApJ, 508, 123 Google Scholar
Frayer, D. T., et al. 2003, AJ, 126, 73 Google Scholar
Giacconi, R., Gursky, H., Paolini, F. & Rossi, B. 1962, Phys. Rev. Lett, 9, 439 Google Scholar
Gilli, R., et al. 2003, ApJ, 592, 721 Google Scholar
Gispert, R., Lagache, G., & Puget, J. L. 2000, A&A, 360, 1 Google Scholar
Gunn, K. F., & Shanks, T. 1998, Astron. Nach., 319, 66 Google Scholar
Hasinger, G., et al. 1998, A&A, 329, 482 Google Scholar
Hasinger, G., et al. 2001, A&A, 365, L45 Google Scholar
Holland, W. S., et al. 1999, MNRAS, 303, 659 CrossRefGoogle Scholar
Hornschemeier, A. E., et al. 2000, ApJ, 541, 49 Google Scholar
Hughes, D. H., et al. 1998, Nature, 394, 241 Google Scholar
Ivison, R. J., et al. 2002, MNRAS, 337, 1 Google Scholar
Kim, D. -C., Sanders, D. B. 1998, ApJS, 119, 41 CrossRefGoogle Scholar
Lilly, S. J., et al. 1999, ApJ, 518, 641 Google Scholar
Lilly, S. J., Le Fèvre, O., Hammer, F., & Crampton, D. 1996, ApJ, 460, L1 Google Scholar
Machalski, J., & Godlowski, W. 2001, A&A, 370, 923 Google Scholar
Madau, P., et al. 1996, MNRAS, 283, 1388 Google Scholar
Mushotzky, R. F., Cowie, L. L., Barger, A. J., & Arnaud, K. A. 2000, Nature, 404, 459 Google Scholar
Oke, J. B., et al. 1995, PASP, 107, 375 Google Scholar
Peacock, J. A., et al. 2000, MNRAS, 318, 535 Google Scholar
Puget, J. -L., et al. 1996, A&A, 308, L5 Google Scholar
Rengarajan, T. N., & Takeuchi, T. T. 2001, PASJ, 53, 433 CrossRefGoogle Scholar
Richards, E. A. 2000, ApJ, 533, 611 Google Scholar
Rosati, P., et al. 2002, ApJ, 566, 667 CrossRefGoogle Scholar
Sadler, E. M., et al. 2002, MNRAS, 329, 227 Google Scholar
Sanders, D. B., Mazzarella, J. M., Kim, D.-C., Surace, J. A., & Soifer, B. T. 2003, AJ, 126, 1607 Google Scholar
Sanders, D. B., & Mirabel, I. F. 1996, ARA&A, 34, 749 Google Scholar
Schmidt, M., et al. 1998, A&A, 329, 495 Google Scholar
Scott, S. E., et al. 2002, MNRAS, 331, 817 Google Scholar
Smail, I., Ivison, R. J., & Blain, A. W. 1997, ApJ, 490, L5 CrossRefGoogle Scholar
Smail, I., Ivison, R. J., Blain, A. W., & Kneib, J. -P. 1998, ApJ, 507, L21 Google Scholar
Smail, I., Ivison, R. J., Blain, A. W., & Kneib, J. -P. 2002, MNRAS, 331, 495 Google Scholar
Steidel, C. C., Adelberger, L., Giavalisco, M., Dickinson, M., & Pettini, M. 1999, ApJ, 519, 1 CrossRefGoogle Scholar
Steidel, C. C., Giavalisco, M., Pettini, M., Dickinson, M., & Adelberger, K. L. 1996, ApJ, 462, L17 Google Scholar
Takata, T., et al. 2003, PASJ, 55, 789 Google Scholar
Treyer, M. A., Ellis, R. S., Milliard, B., Donas, J., & Bridges, T. J. 1998, MNRAS, 300, 303 Google Scholar
Waskett, T. J., et al. 2003, MNRAS, 341, 1217 Google Scholar
Webb, T. M., et al. 2003a, ApJ, 582, 6 Google Scholar
Webb, T. M., et al. 2003b, ApJ, 587, 41 Google Scholar
Webb, T. M., et al. 2003c, ApJ, 597, 680 Google Scholar
Wehner, E. H., Barger, A. J., & Kneib, J. -P. 2002, ApJ, 577, L83 CrossRefGoogle Scholar
Yang, Y., et al. 2003, ApJ, 585, L85 Google Scholar