Publication: Pathways to quiescence: SHARDS view on the star formation histories of massive quiescent galaxies at 1.0 < z < 1.5
Loading...
Official URL
Full text at PDC
Publication Date
2016-04-21
Authors
Domínguez Sánchez, Helena
Esquej Alonso, María del Pilar
Eliche Moral, María del Carmen
Advisors (or tutors)
Editors
Journal Title
Journal ISSN
Volume Title
Publisher
Wiley
Citations
Exportar
Abstract
We present star formation histories (SFHs) for a sample of 104 massive (stellar mass M > 10^10 M_⊙) quiescent galaxies (MQGs) at z = 1.0–1.5 from the analysis of spectrophotometric data from the Survey for High-z Absorption Red and Dead Sources (SHARDS) and HST/WFC3 G102 and G141 surveys of the GOODS-North field, jointly with broad-band observations from ultraviolet (UV) to far-infrared (far-IR). The sample is constructed on the basis of rest-frame UVJ colours and specific star formation rates (sSFRs = SFR/Mass). The spectral energy distributions (SEDs) of each galaxy are compared to models assuming a delayed exponentially declining SFH. A Monte Carlo algorithm characterizes the degeneracies, which we are able to break taking advantage of the SHARDS data resolution, by measuring indices such as MgUV and D4000. The population of MQGs shows a duality in their properties. The sample is dominated (85 per cent) by galaxies with young mass-weighted ages, t_M t_M < 2 Gyr, short star formation time-scales, 〈τ〉 ∼ 60–200 Myr, and masses log(M/M_⊙) ∼ 10.5. There is an older population (15 per cent) with t_M t_M = 2–4 Gyr, longer star formation time-scales, 〈τ〉∼ 400 Myr, and larger masses, log(M/M_⊙) ∼ 10.7. The SFHs of our MQGs are consistent with the slope and the location of the main sequence of star-forming galaxies at z > 1.0, when our galaxies were 0.5–1.0 Gyr old. According to these SFHs, all the MQGs experienced a luminous infrared galaxy phase that lasts for ∼500 Myr, and half of them an ultraluminous infrared galaxy phase for ∼100 Myr. We find that the MQG population is almost assembled at z ∼ 1, and continues evolving passively with few additions to the population.
Description
Artículo firmado por 15 autores. © 2016 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society.
The authors would like to thank the anonymous referee for the careful reading and useful suggestions which helped to improve the manuscript. We acknowledge support from the Spanish Programa Nacional de Astronomiía y Astrofísica under grants AYA2012-31277. NCL acknowledges financial support from AYA2013-46724-P. AAH and AHC acknowledge support from the Spanish Programa Nacional de Astronomía y Astrofísica under grant AYA2012-31447, which is partly funded by the Fondo Europeo de Desarrollo Regional programme. The work of AC is supported by the STARFORM Sinergia Project funded by the Swiss National Science Foundation. SC acknowledges support from the ERC via an Advanced Grant under grant agreement no. 321323-NEOGAL. DC thanks AYA2012-32295. GB acknowledges support for this work from the National Autonomous University of Mexico (UNAM), through grant PAPIIT IG100115. HDS thanks Giovanni Zamorani for useful discussion. This work has made use of the Rainbow Cosmological Surveys Database, which is operated by the Universidad Complutense de Madrid (UCM) partnered with the University of California Observatories at Santa Cruz (UCO/Lick, UCSC). Based on observations made with the GTC installed at the Spanish Observatorio del Roque de los Muchachos of the Instituto de Astrofísica de Canarias, in the island of La Palma. We thank all the GTC Staff for their support and enthusiasm with the SHARDS project.
UCM subjects
Unesco subjects
Keywords
Citation
Balogh M. L., Morris S. L., Yee H. K. C., Carlberg R. G., Ellingson E., 1999, ApJ, 527, 54
Barro G., et al., 2011, ApJS, 193, 13
Barro G., Faber S. M., Pérez González P. G. e. a., 2014, ApJ, 791, 52
Barro G., et al., 2015, preprint, (arXiv:1503.07164)
Bedregal A. G., et al., 2013, ApJ, 778, 126
Bell E. F., et al., 2005, ApJ, 625, 23
Belli S., Newman A. B., Ellis R. S., 2014, ApJ, 783, 117
Belli S., Newman A. B., Ellis R. S., 2015, ApJ, 799, 206
Bendo G. J., et al., 2012, MNRAS, 419, 1833
Bluck A. F. L., Conselice C. J., Bouwens R. J., Daddi E., Dickinson M., Papovich C., Yan H., 2009, MNRAS, 394, L51
Brammer G. B., van Dokkum P. G., Coppi P., 2008, ApJ, 686, 1503
Bruzual A. G., 1983, ApJ, 273, 105
Bruzual G., Charlot S., 2003, MNRAS, 344, 1000
Buitrago F., Trujillo I., Conselice C. J., Bouwens R. J., Dickinson M., Yan H., 2008, ApJ, 687, L61
Bundy K., Treu T., Ellis R. S., 2007, ApJ, 665, L5
Calzetti D., Armus L., Bohlin R. C., Kinney A. L., Koornneef J., Storchi-Bergmann T., 2000, ApJ, 533, 682
Chary R., Elbaz D., 2001, ApJ, 556, 562
Choi J., Conroy C., Moustakas J., Graves G. J., Holden B. P., Brodwin M., Brown M. J. I., van Dokkum P. G., 2014, ApJ, 792, 95
Cimatti A., et al., 2004, Nature, 430, 184
Cimatti A., Daddi E., Renzini A., 2006, A&A, 453, L29
Cimatti A., et al., 2008, A&A, 482, 21
Cowie L. L., Songaila A., Hu E. M., Cohen J. G., 1996, AJ, 112, 839
Daddi E., et al., 2005, ApJ, 626, 680
Dale D. A., Helou G., 2002, ApJ, 576, 159
Davidzon I., et al., 2013, A&A, 558, A23
Domínguez Sánchez H., Pozzi F., Gruppioni C. e. a., 2011, MNRAS, 417, 900
Elbaz D., et al., 2007, A&A, 468, 33
Elbaz D., Dickinson M., Hwang H. S., Díaz Santos T., Magdis G. e. a., 2011, A&A, 533, A119
Eliche Moral M. C., et al., 2010, A&A, 519, A55
Elsner F., Feulner G., Hopp U., 2008, A&A, 477, 503
Ferreras I., et al., 2012, AJ, 144, 47
Ferreras I., et al., 2014, MNRAS, 444, 906
Fontana A., et al., 2009, A&A, 501, 15
Fumagalli M., et al., 2014, ApJ, 796, 35
Gorgas J., Cardiel N., Pedraz S., González J. J., 1999, A&AS, 139, 29
Grazian A., et al., 2015, A&A, 575, A96
Grogin N. A., et al., 2011, ApJS, 197, 35
Hernán Caballero A., et al., 2013, MNRAS, 434, 2136
Hopkins P. F., Hernquist L., Cox T. J., Kereš D., 2008, ApJS, 175, 356
Ilbert O., et al., 2010, ApJ, 709, 644
Ilbert O., McCracken H. J., Le Fèvre O. e. a., 2013, A&A, 556, A55
Kauffmann G., et al., 2003, MNRAS, 341, 33
Kennicutt Jr. R. C., 1998, ApJ, 498, 541
Koekemoer A. M., et al., 2011, ApJS, 197, 36
Kong X., Charlot S., Brinchmann J., Fall S. M., 2004, MNRAS, 349, 769
Kriek M., van Dokkum P. G., Labbé I., Franx M., Illingworth G. D., Marchesini D., Quadri R. F., 2009, ApJ, 700, 221
Kriek M., van Dokkum P. G., Whitaker K. E., Labbé I., Franx M., Brammer G. B., 2011, ApJ, 743, 168
Krogager J.-K., et al., 2013, MNRAS, 433, 3091
Kroupa P., 2001, MNRAS, 322, 231
Madau P., Ferguson H. C., Dickinson M. E., Giavalisco M., Steidel C. C., Fruchter A., 1996, MNRAS, 283, 1388
Magnelli B., et al., 2013, A&A, 553, A132
Man A. W. S., Zirm A. W., Toft S., 2014, preprint, (arXiv:1410.3479)
Marchesini D., van Dokkum P. G., Förster Schreiber N. M., Franx M., Labbé I., Wuyts S., 2009, ApJ, 701, 1765
McCracken H. J., et al., 2012, A&A, 544, A156
Mendel J. T., et al., 2015, ApJ, 804, L4
Meurer G. R., Heckman T. M., Calzetti D., 1999, ApJ, 521, 64
Muzzin A., et al., 2013, ApJ, 777, 18
Newman A., 2013, in American Astronomical Society Meeting Abstracts, 221. p. 303.05
Noeske K. G., Weiner B. J., Faber S. M. e. a., 2007, ApJ, 660, L43
Oke J. B., Gunn J. E., 1983, ApJ, 266, 713
Onodera M., et al., 2012, ApJ, 755, 26
Onodera M., et al., 2015, ApJ, 808, 161
Pacifici C., Kassin S. A., Weiner B., Charlot S., Gardner J. P., 2013, ApJ, 762, L15
Papovich C., et al., 2006, ApJ, 640, 92
Pérez González P. G., Gil de Paz A., Zamorano J., Gallego J., Alonso Herrero A., Aragón Salamanca A., 2003, MNRAS, 338, 525
Pérez González P. G., et al., 2005, ApJ, 630, 82
Pérez González P. G., et al., 2008, ApJ, 675, 234
Pérez González P. G., et al., 2010, A&A, 518, L15
Pérez González P. G., Cava A., et al. B., 2013, ApJ, 762, 46
Pozzetti L., et al., 2010, A&A, 523, A13
Prieto M., Eliche Moral M. C., 2015, MNRAS, 451, 1158
Prieto M., et al., 2013, MNRAS, 428, 999
Rawle T. D., et al., 2015, preprint, (arXiv:1508.00586)
Renzini A., 2006, ARA&A, 44, 141
Rieke G. H., Alonso Herrero A., Weiner B. J., Pérez González P. G., Blaylock M., Donley J. L., Marcillac D., 2009, ApJ, 692, 556
Rodighiero G., Cimatti A., Gruppioni C., Popesso P., Andreani P. e. a., 2010, A&A, 518, L25
Rujopakarn W., et al., 2012, ApJ, 755, 168
Rujopakarn W., Rieke G. H., Weiner B. J., Pérez González P., Rex M., Walth G. L., Kartaltepe J. S., 2013, ApJ, 767, 73
Santini P., et al., 2009, A&A, 504, 751
Santini P., et al., 2015, ApJ, 801, 97
Saracco P., et al., 2005, MNRAS, 357, L40
Schiavon R. P., et al., 2006, ApJ, 651, L93
Scoville N., et al., 2007, ApJS, 172, 1
Shankar F., et al., 2015, ApJ, 802, 73
Speagle J. S., Steinhardt C. L., Capak P. L., Silverman J. D., 2014, ApJS, 214, 15
Spergel D. N., et al., 2003, ApJS, 148, 175
Tacconi L. J., et al., 2010, Nature, 463, 781
Takeuchi T. T., Yuan F.-T., Ikeyama A., Murata K. L., Inoue A. K., 2012, ApJ, 755, 144
Thomas D., Greggio L., Bender R., 1999, MNRAS, 302, 537
Thomas D., Maraston C., Bender R., Mendes de Oliveira C., 2005, ApJ, 621, 673
Thomas D., Maraston C., Schawinski K., Sarzi M., Silk J., 2010, MNRAS, 404, 1775
Toft S., Gallazzi A., Zirm A., Wold M., Zibetti S., Grillo C., Man A., 2012, ApJ, 754, 3
Tomczak A. R., et al., 2014, ApJ, 783, 85
Tremonti C. A., et al., 2004, ApJ, 613, 898
Trujillo I., et al., 2006, ApJ, 650, 18
Whitaker K. E., et al., 2011, ApJ, 735, 86
Whitaker K. E., et al., 2013, ApJ, 770, L39
Worthey G., 1998, PASP, 110, 888
Worthey G., Faber S. M., González J. J., 1992, ApJ, 398, 69
Wuyts S., et al., 2011, ApJ, 738, 106
Zolotov A., et al., 2015, MNRAS, 450, 2327
van Dokkum P. G., et al., 2008, ApJ, 677, L5
van Dokkum P. G., et al., 2011, ApJ, 743, L15
van de Sande J., et al., 2013, ApJ, 771, 85