Hostname: page-component-7479d7b7d-jwnkl Total loading time: 0 Render date: 2024-07-11T22:28:46.882Z Has data issue: false hasContentIssue false
  • English
  • Français

Modelling the emission of passive galaxy candidates at z∼3

Published online by Cambridge University Press:  10 June 2020

C. D’Eugenio ,
E. Daddi ,
R. Gobat ,
V. Strazzullo  and
S. Jin
C. D’Eugenio
Affiliation:
CEA, IRFU, DAp, AIM, Université Paris-Saclay, Université Paris Diderot, Sorbonne Paris Cité, CNRS, F-91191 Gif-sur-Yvette, France email: chiara.deugenio@cea.fr
E. Daddi
Affiliation:
CEA, IRFU, DAp, AIM, Université Paris-Saclay, Université Paris Diderot, Sorbonne Paris Cité, CNRS, F-91191 Gif-sur-Yvette, France email: chiara.deugenio@cea.fr
R. Gobat
Affiliation:
Instituto de Física, Pontificia Universidad Católica de Valparaíso, Casilla 4059, Valparaíso, Chile
V. Strazzullo
Affiliation:
Faculty of Physics, Ludwig-Maximilians-Universität, Scheinerstr. 1, 81679 Munich, Germany
S. Jin
Affiliation:
Instituto de Astrofiśica de Canarias (IAC), E-38205 La Laguna, Tenerife, Spain Universidad de La Laguna, Dpto. Astrofiśica, E-38206 La Laguna, Tenerife, Spain
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

Early-type galaxies (ETGs) are of crucial importance to trace back the galaxy mass assembly across cosmic time, yet their formation and quenching remain remarkably elusive. The discoveries of massive, dead galaxies at ever-growing redshifts provided compelling evidence to push their formation up to redshift > 4–5 when the Universe was barely 1 Gyr old. In this talk I will present our results on the ages of a new sample of ETGs at z ∼ 3, built by exploiting HST WFC3/G141 rest-frame optical/near-UV grism spectroscopy to study the nature of 10 passive galaxy candidates at 2.5 < z < 3.5 in COSMOS.

This work is part of a PhD project aimed at quantifying the parent space density of distant genuine passive galaxies. I will also discuss the importance of multi-wavelength data in clarifying the degree of contamination by dusty star-forming galaxies affecting the color selection.

Keywords

Galaxies: evolutionGalaxies: elliptical and lenticularcDGalaxies: high-redshift
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 15 , Symposium S341: Challenges in Panchromatic Modelling with Next Generation Facilities , November 2019 , pp. 44 - 49
Copyright
© International Astronomical Union 2020

References

Baldry, I. K., Glazebrook, K., Brinkmann, J., Ivezić, Ž., Lupton, R. H., Nichol, R. C., Szalay, A. S., et al. 2004, ApJ, 600, 681–69410.1086/380092CrossRefGoogle Scholar
Bruzual, G. & Charlot, S. 2003, MNRAS, 344, 100010.1046/j.1365-8711.2003.06897.xCrossRefGoogle Scholar
Behroozi, P. & Silk, J. 2018, MNRAS, 477, 538210.1093/mnras/sty945CrossRefGoogle Scholar
Calzetti, D., Armus, L., Bohlin, R. C., Kinney, A. L., Koornneef, J., Storchi-Bergmann, T., et al. 2000, ApJ, 533, 68210.1086/308692CrossRefGoogle Scholar
Chabrier, G. 2003, PASP, 115, 76310.1086/376392CrossRefGoogle Scholar
Cimatti, A., Daddi, E., Renzini, A., Cassata, P., Vanzella, E., Pozzetti, L., Cristiani, S., Fontana, A., et al. 2004, Nature, 430, 18410.1038/nature02668CrossRefGoogle Scholar
Franx, M., Labbé, I., Rudnick, G., van Dokkum, P. G., Daddi, E., Förster Schreiber, N. M., Moorwood, A., Rix, H.-W., Röttgering, H., et al. 2003, ApJ, 587, L7910.1086/375155CrossRefGoogle Scholar
Daddi, E., Cimatti, A., Renzini, A., Fontana, A., Mignoli, M., Pozzetti, L., Tozzi, P., Zamorani, G., et al. 2004, ApJ, 617, 74610.1086/425569CrossRefGoogle Scholar
Davidzon, I., Ilbert, O., Laigle, C., Coupon, J., McCracken, H. J., Delvecchio, I., Masters, D., Capak, P., et al. 2017, A&A, 605, A70Google Scholar
Davé, R., Thompson, R., Hopkins, P. F., et al. 2016, MNRAS, 462, 326510.1093/mnras/stw1862CrossRefGoogle Scholar
Draine, B. T. & Li, A. 2007, ApJ, 657, 81010.1086/511055CrossRefGoogle Scholar
Galametz, M., Madden, S. C., Galliano, F., Hony, S., Bendo, G. J., Sauvage, M., et al. 2011, A&A 532, A56Google Scholar
Glazebrook, K., Schreiber, C., Labbé, I., Nanayakkara, T., Kacprzak, G. G., Oesch, P. A., Papovich, C., Spitler, et al. 2017, Nature, 544, 7110.1038/nature21680CrossRefGoogle Scholar
Gobat, R., Strazzullo, V., Daddi, E., Onodera, M., Renzini, A., Béthermin, M., Dickinson, M., Carollo, M., Cimatti, A., et al. 2012, ApJ, 759, L4410.1088/2041-8205/759/2/L44CrossRefGoogle Scholar
Gobat, R., Daddi, E., Strazzullo, V., Garilli, B., Mignoli, M., Ma, Z., Jin, S., Maraston, C., Magdis, G., Béthermin, M., Cappellari, M., Carollo, M., Cimatti, A., et al. 2017, A&A, 599, A95.Google Scholar
Gobat, R., Daddi, E., Magdis, G., Bournaud, F., Sargent, M., Martig, M., Jin, S., Finoguenov, A., et al. 2018, Nature Astronomy, 2, 23910.1038/s41550-017-0352-5CrossRefGoogle Scholar
Horne, K. 1986, PASP, 98, 60910.1086/131801CrossRefGoogle Scholar
Kennicutt, R. C. 1998, ARAA, 36, 189.10.1146/annurev.astro.36.1.189CrossRefGoogle Scholar
Kriek, M., van Dokkum, P. G., Franx, M., Quadri, R., Gawiser, E., Herrera, D., Illingworth, G. D., Labbé et al. 2006, ApJ, 649, L7110.1086/508371CrossRefGoogle Scholar
Qin, Y., Mutch, S. J., Duffy, A.R., Geil, P. M., Poole, G. B., Mesinger, A., Wyithe, J. S. B., et al. 2017, MNRAS 471, 434510.1093/mnras/stx1852CrossRefGoogle Scholar
Qin, Y., Mutch, S. J., Poole, G. B., Liu, C., Angel, P. W., Duffy, A. R., Geil, P. M., Mesinger, A., Wyithe, J. S. B., et al. 2017, MNRAS, 472, 200910.1093/mnras/stx1909CrossRefGoogle Scholar
Magdis, G. E., Daddi, E., Elbaz, D., Sargent, M., Dickinson, M., Dannerbauer, H., Aussel, H., Walter, F., et al. 2011, ApJ 740, L1510.1088/2041-8205/740/1/L15CrossRefGoogle Scholar
Magdis, G. E., Daddi, E., Béthermin, M., Sargent, M., Elbaz, D., Pannella, M., Dickinson, M., Dannerbauer, H., et al. 2012, Astrophys. J. 760, 610.1088/0004-637X/760/1/6CrossRefGoogle Scholar
McCracken, H. J., Capak, P., Salvato, M., Aussel, H., Thompson, D., Daddi, E., Sanders, D. B., Kneib, J.-P., et al. 2010, ApJ, 708, 20210.1088/0004-637X/708/1/202CrossRefGoogle Scholar
Muzzin, A., Marchesini, D., Stefanon, M., Franx, M., McCracken, H. J., Milvang-Jensen, B., Dunlop, J. S., Fynbo, J. P. U., et al. 2013, ApJ, 777, 1810.1088/0004-637X/777/1/18CrossRefGoogle Scholar
Newman, A. B., Belli, S., Ellis, R. S., Patel, S. G., et al. 2018, ApJ, 862, 12510.3847/1538-4357/aacd4dCrossRefGoogle Scholar
Renzini, A. & Peng, Y.-jie. 2015, ApJ, 801, L2910.1088/2041-8205/801/2/L29CrossRefGoogle Scholar
Salpeter, E. E. 1955, ApJ, 121, 16110.1086/145971CrossRefGoogle Scholar
Schreiber, C., Glazebrook, K., Nanayakkara, T., Kacprzak, G. G., Labbé, I., Oesch, P., Yuan, T., Tran, K.-V., et al. 2018, ApJ, 618, A85Google Scholar
Scoville, N. 2013, AAMA, 221, 03Google Scholar
Straatman, C. M. S., Labbé, I., Spitler, L. R., Allen, R., Altieri, B., Brammer, G. B., Dickinson, M., van Dokkum, P., et al. 2014, ApJ, 783, L1410.1088/2041-8205/783/1/L14CrossRefGoogle Scholar
Strazzullo, V., Daddi, E., Gobat, R., Garilli, B., Mignoli, M., Valentino, F., Onodera, M., Renzini et al. 2015, A&A, 576, L6Google Scholar
Thomas, D., Maraston, C., Schawinski, K., Sarzi, M., Silk, J., et al. 2010, MNRAS, 404, 1775Google Scholar
Valentino, F., Daddi, E., Silverman, J. D., Puglisi, A., Kashino, D., Renzini, A., Cimatti, A., Pozzetti, L., Rodighiero, G., Pannella, M., Gobat, R., Zamorani, G., et al. 2017, MNRAS, 472, 487810.1093/mnras/stx2305CrossRefGoogle Scholar
Williams, R. J., Quadri, R. F., Franx, M., van Dokkum, P., Labbé, I., et al. 2009, ApJ, 691, 1879–189510.1088/0004-637X/691/2/1879CrossRefGoogle Scholar
Wellons, S., Torrey, P., Ma, C.-P., Rodriguez-Gomez, V., Vogelsberger, M., Kriek, M., van Dokkum, P., Nelson, E., Genel, S., et al. 2015, MNRAS 449, 36110.1093/mnras/stv303CrossRefGoogle Scholar
Yan, R., Newman, J. A., Faber, S.M., Konidaris, N., Koo, D., Davis, M., et al. 2006, ApJ, 648, 28110.1086/505629CrossRefGoogle Scholar