Mass assembly in quiescent and star-forming galaxies since z ≃ 4 from UltraVISTA

O. Ilbert; H. J. McCracken; O. Le Fevre; P. Capak; J. Dunlop; A. Karim; M. A. Renzini; K. Caputi; S. Boissier; S. Arnouts; H. Aussel; J. Comparat; Q. Guo; P. Hudelot; J. Kartaltepe; J. P. Kneib; J. K. Krogager; E. Le Floc'h; S. Lilly; Y. Mellier; B. Milvang-Jensen; T. Moutard; M. Onodera; J. Richard; M. Salvato; D. B. Sanders; N. Scoville; J. Silverman; Y. Taniguchi; L. Tasca; R. Thomas; S. Toft; L. Tresse; D. Vergani; M. Wolk; A. Zirm

doi:10.1051/0004-6361/201321100

Mass assembly in quiescent and star-forming galaxies since z ≃ 4 from UltraVISTA

O. Ilbert, H. J. McCracken, O. Le Fevre, P. Capak, J. Dunlop, A. Karim, M. A. Renzini, K. Caputi, S. Boissier, S. Arnouts, H. Aussel, J. Comparat, Q. Guo, P. Hudelot, J. Kartaltepe, J. P. Kneib, J. K. Krogager, E. Le Floc'h, S. Lilly, Y. MellierB. Milvang-Jensen, T. Moutard, M. Onodera, J. Richard, M. Salvato, D. B. Sanders, N. Scoville, J. Silverman, Y. Taniguchi, L. Tasca, R. Thomas, S. Toft, L. Tresse, D. Vergani, M. Wolk, A. Zirm

School of Physics and Astronomy

Research output: Contribution to journal › Article › peer-review

Abstract / Description of output

We estimate the galaxy stellar mass function and stellar mass density for star-forming and quiescent galaxies with 0.210^10.7Msun. For the mass function of the quiescent galaxies, we do not find any significant evolution of the high-mass end at z1.5 consistent with the expected uncertainties. We also develop a new method to infer the specific SFR from the mass function of star-forming galaxies. We find that the sSFR of 10^10Msun galaxies increases continuously in the redshift range 1

Original language	English
Article number	A55
Number of pages	19
Journal	Astronomy & Astrophysics
Volume	556
DOIs	https://doi.org/10.1051/0004-6361/201321100
Publication status	Published - 1 Jan 2013

Keywords / Materials (for Non-textual outputs)

Astrophysics - Cosmology and Extragalactic Astrophysics

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10.1051/0004-6361/201321100

http://adsabs.harvard.edu/abs/2013arXiv1301.3157I

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Ilbert, O., McCracken, H. J., Le Fevre, O., Capak, P., Dunlop, J., Karim, A., Renzini, M. A., Caputi, K., Boissier, S., Arnouts, S., Aussel, H., Comparat, J., Guo, Q., Hudelot, P., Kartaltepe, J., Kneib, J. P., Krogager, J. K., Le Floc'h, E., Lilly, S., ... Zirm, A. (2013). Mass assembly in quiescent and star-forming galaxies since z ≃ 4 from UltraVISTA. Astronomy & Astrophysics, 556, Article A55. https://doi.org/10.1051/0004-6361/201321100

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title = "Mass assembly in quiescent and star-forming galaxies since z ≃ 4 from UltraVISTA",

abstract = "We estimate the galaxy stellar mass function and stellar mass density for star-forming and quiescent galaxies with 0.210^10.7Msun. For the mass function of the quiescent galaxies, we do not find any significant evolution of the high-mass end at z1.5 consistent with the expected uncertainties. We also develop a new method to infer the specific SFR from the mass function of star-forming galaxies. We find that the sSFR of 10^10Msun galaxies increases continuously in the redshift range 1",

keywords = "Astrophysics - Cosmology and Extragalactic Astrophysics",

author = "O. Ilbert and McCracken, {H. J.} and {Le Fevre}, O. and P. Capak and J. Dunlop and A. Karim and Renzini, {M. A.} and K. Caputi and S. Boissier and S. Arnouts and H. Aussel and J. Comparat and Q. Guo and P. Hudelot and J. Kartaltepe and Kneib, {J. P.} and Krogager, {J. K.} and {Le Floc'h}, E. and S. Lilly and Y. Mellier and B. Milvang-Jensen and T. Moutard and M. Onodera and J. Richard and M. Salvato and Sanders, {D. B.} and N. Scoville and J. Silverman and Y. Taniguchi and L. Tasca and R. Thomas and S. Toft and L. Tresse and D. Vergani and M. Wolk and A. Zirm",

year = "2013",

month = jan,

day = "1",

doi = "10.1051/0004-6361/201321100",

language = "English",

volume = "556",

journal = "Astronomy & Astrophysics",

issn = "0004-6361",

publisher = "EDP Sciences",

}

Ilbert, O, McCracken, HJ, Le Fevre, O, Capak, P, Dunlop, J, Karim, A, Renzini, MA, Caputi, K, Boissier, S, Arnouts, S, Aussel, H, Comparat, J, Guo, Q, Hudelot, P, Kartaltepe, J, Kneib, JP, Krogager, JK, Le Floc'h, E, Lilly, S, Mellier, Y, Milvang-Jensen, B, Moutard, T, Onodera, M, Richard, J, Salvato, M, Sanders, DB, Scoville, N, Silverman, J, Taniguchi, Y, Tasca, L, Thomas, R, Toft, S, Tresse, L, Vergani, D, Wolk, M & Zirm, A 2013, 'Mass assembly in quiescent and star-forming galaxies since z ≃ 4 from UltraVISTA', Astronomy & Astrophysics, vol. 556, A55. https://doi.org/10.1051/0004-6361/201321100

TY - JOUR

T1 - Mass assembly in quiescent and star-forming galaxies since z ≃ 4 from UltraVISTA

AU - Ilbert, O.

AU - McCracken, H. J.

AU - Le Fevre, O.

AU - Capak, P.

AU - Dunlop, J.

AU - Karim, A.

AU - Renzini, M. A.

AU - Caputi, K.

AU - Boissier, S.

AU - Arnouts, S.

AU - Aussel, H.

AU - Comparat, J.

AU - Guo, Q.

AU - Hudelot, P.

AU - Kartaltepe, J.

AU - Kneib, J. P.

AU - Krogager, J. K.

AU - Le Floc'h, E.

AU - Lilly, S.

AU - Mellier, Y.

AU - Milvang-Jensen, B.

AU - Moutard, T.

AU - Onodera, M.

AU - Richard, J.

AU - Salvato, M.

AU - Sanders, D. B.

AU - Scoville, N.

AU - Silverman, J.

AU - Taniguchi, Y.

AU - Tasca, L.

AU - Thomas, R.

AU - Toft, S.

AU - Tresse, L.

AU - Vergani, D.

AU - Wolk, M.

AU - Zirm, A.

PY - 2013/1/1

Y1 - 2013/1/1

N2 - We estimate the galaxy stellar mass function and stellar mass density for star-forming and quiescent galaxies with 0.210^10.7Msun. For the mass function of the quiescent galaxies, we do not find any significant evolution of the high-mass end at z1.5 consistent with the expected uncertainties. We also develop a new method to infer the specific SFR from the mass function of star-forming galaxies. We find that the sSFR of 10^10Msun galaxies increases continuously in the redshift range 1

AB - We estimate the galaxy stellar mass function and stellar mass density for star-forming and quiescent galaxies with 0.210^10.7Msun. For the mass function of the quiescent galaxies, we do not find any significant evolution of the high-mass end at z1.5 consistent with the expected uncertainties. We also develop a new method to infer the specific SFR from the mass function of star-forming galaxies. We find that the sSFR of 10^10Msun galaxies increases continuously in the redshift range 1

KW - Astrophysics - Cosmology and Extragalactic Astrophysics

U2 - 10.1051/0004-6361/201321100

DO - 10.1051/0004-6361/201321100

M3 - Article

SN - 0004-6361

VL - 556

JO - Astronomy & Astrophysics

JF - Astronomy & Astrophysics

M1 - A55

ER -

Mass assembly in quiescent and star-forming galaxies since z ≃ 4 from UltraVISTA

Abstract / Description of output

Keywords / Materials (for Non-textual outputs)

Access to Document

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