The Hα-based star formation rate density of the universe at z=0.84
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2008
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American Astronomical Society
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Adelman-McCarthy, J. K., et al. 2006, ApJS, 162, 38
Alexander, D. M., et al. 2003, AJ, 126, 539
Alonso Herrero, A., et al. 2006, ApJ, 640, 167
Arnouts, S., et al. 2005, ApJ, 619, L43
Baugh, C. M. 2006, Rep. Prog. Phys., 69, 3101
Bell, E. F. 2003, ApJ, 586, 794
Bertin, E., & Arnouts, S. 1996, A&AS, 117, 393
Brinchmann, J., Charlot, S., White, S. D. M., Tremonti, C., Kauffmann, G., Heckman, T., & Brinkmann, J. 2004, MNRAS, 351, 1151
Buat, V., et al. 2005, ApJ, 619, L51
Calzetti, D., Armus, L., Bohlin, R. C., Kinney, A. L., Koornneef, J., & StorchiBergmann, T. 2000, ApJ, 533, 682
Calzetti, D., et al. 2005, ApJ, 633, 871
Capak, P., et al. 2004, AJ, 127, 180
Charlot, S., & Longhetti, M. 2001, MNRAS, 323, 887
Chary, R., & Elbaz, D. 2001, ApJ, 556, 562
Coil, A. L., Newman, J. A., Kaiser, N., Davis, M., Ma, C.-P., Kocevski, D. D., & Koo, D. C. 2004, ApJ, 617, 765
Cowie, L. L., Barger, A. J., Hu, E. M., Capak, P., & Songaila, A. 2004, AJ, 127, 3137
Daddi, E., Cimatti, A., Renzini, A., Fontana, A., Mignoli, M., Pozzetti, L., Tozzi, P., & Zamorani, G. 2004, ApJ, 617, 746
Davis, M., et al. 2007, ApJ, 660, L1
Doherty, M., Bunker, A., Sharp, R., Dalton, G., Parry, I., & Lewis, I. 2006, MNRAS, 370, 331
Eisenhardt, P. R., et al. 2004, ApJS, 154, 48
Erb, D. K., Steidel, C. C., Shapley, A. E., Pettini, M., Reddy, N. A., & Adelberger, K. L. 2006, ApJ, 647, 128
Faber, S. M., et al. 2003, Proc. SPIE, 4841, 1657
Ferguson, H. C., Dickinson, M., & Williams, R. 2000, ARA&A, 38, 667
Gallego, J., Zamorano, J., Aragón Salamanca, A., & Rego, M. 1995, ApJ, 455, L1
Gallego, J., Zamorano, J., Rego, M., & Vitores, A. G. 1997, ApJ, 475, 502
Gil de Paz, A., et al. 2007, ApJS, 173, 185
Glazebrook, K., Blake, C., Economou, F., Lilly, S., & Colless, M. 1999, MNRAS, 306, 843
Glazebrook, K., Tober, J., Thomson, S., Bland-Hawthorn, J., & Abraham, R. 2004, AJ, 128, 2652
Hanish, D. J., et al. 2006, ApJ, 649, 150
Hopkins, A. M. 2004, ApJ, 615, 209
Hopkins, A. M., & Beacom, J. F. 2006, ApJ, 651, 142
Hopkins, A. M., Connolly, A. J., & Szalay, A. S. 2000, AJ, 120, 2843
Jones, D. H., & Bland-Hawthorn, J. 2001, ApJ, 550, 593
Kennicutt, R. C., Jr. 1998, ARA&A, 36, 189
Kong, X., Charlot, S., Brinchmann, J., & Fall, S. M. 2004, MNRAS, 349, 769
Lahav, O., & Liddle, A. R. 2006, preprint (astro-ph/0601168)
Ly, C., et al. 2007, ApJ, 657, 738
Meurer, G. R., Heckman, T. M., Leitherer, C., Kinney, A., Robert, C., & Garnett, D. R. 1995, AJ, 110, 2665
Moorwood, A. F. M., van der Werf, P. P., Cuby, J. G., & Oliva, E. 2000, A&A, 362, 9
Moustakas, J., Kennicutt, R. C., Jr., & Tremonti, C. A. 2006, ApJ, 642, 775
Nakamura, O., Fukugita, M., Brinkmann, J., & Schneider, D. P. 2004, AJ, 127, 2511
Pascual, S. 2005, PASP, 117, 120
Pascual, S., Gallego, J., Aragón Salamanca, A., & Zamorano, J. 2001, A&A, 379, 798
Pascual, S., Gallego, J., & Zamorano, J. 2007, PASP, 119, 30
Peng, C. Y., Ho, L. C., Impey, C. D., & Rix, H.-W. 2002, AJ, 124, 266
Pérez González, P. G., Gallego, J., Zamorano, J., & Gil de Paz, A. 2001, A&A, 365, 370
Pérez González, P. G., Zamorano, J., Gallego, J., Aragón Salamanca, A., & Gil de Paz, A. 2003, ApJ, 591, 827
Pérez González, P. G., et al. 2005, ApJ, 630, 82
———. 2006, ApJ, 648, 987
———. 2008, ApJ, 675, 234
Pettini, M., Shapley, A. E., Steidel, C. C., Cuby, J.-G., Dickinson, M., Moorwood, A. F. M., Adelberger, K. L., & Giavalisco, M. 2001, ApJ, 554, 981
Reddy, N. A., Steidel, C. C., Erb, D. K., Shapley, A. E., & Pettini, M. 2006, ApJ, 653, 1004
Reddy, N. A., Steidel, C. C., Pettini, M., Adelberger, K. L., Shapley, A. E., Erb, D. K., & Dickinson, M. 2008, ApJS, 175, 48
Rowan-Robinson, M., et al. 2005, AJ, 129, 1183
Schechter, P. 1976, ApJ, 203, 297
Schiminovich, D., et al. 2005, ApJ, 619, L47
Schmidt, M. 1968, ApJ, 151, 393
Shioya, Y., et al. 2008, ApJS, 175, 128
Sullivan, M., Treyer, M. A., Ellis, R. S., Bridges, T. J., Milliard, B., & Donas, J. 2000, MNRAS, 312, 442
Takahashi, M. I., et al. 2007, ApJS, 172, 456
Tresse, L., & Maddox, S. J. 1998, ApJ, 495, 691
Tresse, L., Maddox, S. J., Le Fèvre, O., & Cuby, J.-G. 2002, MNRAS, 337, 369
Tresse, L., et al. 2007, A&A, 472, 403
Vitores, A. G., Zamorano, J., Rego, M., Gallego, J., & Alonso, O. 1996, A&AS, 120, 385
Willis, J. P., & Courbin, F. 2005, MNRAS, 357, 1348
Wirth, G. D., et al. 2004, AJ, 127, 3121
Yan, L., McCarthy, P. J., Freudling, W., Teplitz, H. I., Malumuth, E. M., Weymann, R. J., & Malkan, M. A. 1999, ApJ, 519, L47
Yan, R., Newman, J. A., Faber, S. M., Konidaris, N., Koo, D., & Davis, M. 2006, ApJ, 648, 281
Zamorano, J., Gallego, J., Rego, M., Vitores, A. G., & Alonso, O. 1996, ApJS, 105, 343
Zamorano, J., Rego, M., Gallego, J. G., Vitores, A. G., González Riestra, R., & Rodríguez Caderot, G. 1994, ApJS, 95, 387
Abstract
We present the results of an Hα near-infrared narrowband survey searching for star-forming galaxies at redshift z = 0.84. This work is an extension of our previous narrowband studies in the optical at lower redshifts. After removal of stars and redshift interlopers (using spectroscopic and photometric redshifts), we build a complete sample of 165 Hα emitters in the extended Groth strip and GOODS-N fields with L(Hα) > 10^41 ergs s^−1. We compute the Hα luminosity function at z = 0.84 after corrections for [N_π] flux contamination, extinction, systematic errors, and incompleteness. Our sources present an average dust extinction of A(H α) = 1.5 mag. Adopting Hα as a surrogate for the instantaneous SFR, we measure an extinction-corrected SFR density of 0.17^+0.03_−0.03 M_☉ yr^−1 Mpc^−3. Combining this result to our prior measurements at z = 0.02, 0.24, and 0.40, we derive an Hα-based evolution of the SFR density proportional to (1 + z)^β with β = 3.8 ± 0.5. This evolution is consistent with that derived by other authors using different SFR tracers.
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© 2008. The American Astronomical Society. We thank Nicolás Cardiel and Armando Gil de Paz for advice and useful comments. V. V. acknowledges the receipt of a Formación de Personal Investigador Fellowship from the Spanish Ministerio de Educación y Ciencia. This work was supported in part by the Spanish Plan Nacional de Astronomía y Astrofísica under grants AYA2003-01676 and AYA2006-02358. This work was supported in part by a generous grant of the New del Amo Foundation Program.