A consistent view on star-forming galaxies at high redshift from multi-wavelength observations and SED modeling

被引：0
作者：
Schaerer, Daniel [1 ,2 ]
de Barros, Stephane [3 ]
Boone, Frederic [2 ]
机构：
[1] Univ Geneva, Observ Geneve, 51 Ch Maillettes, CH-1290 Versoix, Switzerland
[2] CNRS, IRAP, 14 Ave E Belin, F-31400 Toulouse, France
[3] INAF Osservatorio Astron Bologna, Via Ranzani 1, I-40127 Bologna, Italy
来源：
GALAXIES AT HIGH REDSHIFT AND THEIR EVOLUTION OVER COSMIC TIME | 2016年 / 11卷 / S319期
关键词：
Galaxies: starburst; Galaxies: high-redshift; EVOLUTION; EPOCH;
D O I：
10.1017/S1743921315010303
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
We stress the importance of consistent SED analysis for distant star-forming galaxies (SFGs). We then summarise recent results from such an analysis concerning their basic physical properties, such as the determination of star formation rate (SFR), stellar mass, specific star SFR, UV attenuation, and how this affects our knowledge of star formation properties at high-z.
引用
收藏
页码：45 / 48
页数：4
相关论文
共 22 条
  • [1] UV-CONTINUUM SLOPES AT z ∼ 4-7 FROM THE HUDF09+ERS+CANDELS OBSERVATIONS: DISCOVERY OF A WELL-DEFINED UV COLOR-MAGNITUDE RELATIONSHIP FOR z ≥ 4 STAR-FORMING GALAXIES
    Bouwens, R. J.
    Illingworth, G. D.
    Oesch, P. A.
    Franx, M.
    Labbe, I.
    Trenti, M.
    van Dokkum, P.
    Carollo, C. M.
    Gonzalez, V.
    Smit, R.
    Magee, D.
    [J]. ASTROPHYSICAL JOURNAL, 2012, 754 (02)
  • [2] Herschel PEP/HerMES: the redshift evolution (0 ≤ z ≤ 4) of dust attenuation and of the total (UV plus IR) star formation rate density
    Burgarella, D.
    Buat, V.
    Gruppioni, C.
    Cucciati, O.
    Heinis, S.
    Berta, S.
    Bethermin, M.
    Bock, J.
    Cooray, A.
    Dunlop, J. S.
    Farrah, D.
    Franceschini, A.
    Le Floc'h, E.
    Lutz, D.
    Magnelli, B.
    Nordon, R.
    Oliver, S. J.
    Page, M. J.
    Popesso, P.
    Pozzi, F.
    Riguccini, L.
    Vaccari, M.
    Viero, M.
    [J]. ASTRONOMY & ASTROPHYSICS, 2013, 554
  • [3] Galaxies at redshifts 5 to 6 with systematically low dust content and high [C II] emission
    Capak, P. L.
    Carilli, C.
    Jones, G.
    Casey, C. M.
    Riechers, D.
    Sheth, K.
    Carollo, C. M.
    Ilbert, O.
    Karim, A.
    LeFevre, O.
    Lilly, S.
    Scoville, N.
    Smolcic, V.
    Yan, L.
    [J]. NATURE, 2015, 522 (7557) : 455 - +
  • [4] Constraints on the star-formation rate of z ∼ 3 LBGs with measured metallicity in the CANDELS GOODS-South field
    Castellano, M.
    Sommariva, V.
    Fontana, A.
    Pentericci, L.
    Santini, P.
    Grazian, A.
    Amorin, R.
    Donley, J. L.
    Dunlop, J. S.
    Ferguson, H. C.
    Fiore, F.
    Galametz, A.
    Giallongo, E.
    Guo, Y.
    Huang, K. -H.
    Koekemoer, A.
    Maiolino, R.
    McLure, R. J.
    Paris, D.
    Schaerer, D.
    Troncoso, P.
    Vanzella, E.
    [J]. ASTRONOMY & ASTROPHYSICS, 2014, 566
  • [5] Modeling the Panchromatic Spectral Energy Distributions of Galaxies
    Conroy, Charlie
    [J]. ANNUAL REVIEW OF ASTRONOMY AND ASTROPHYSICS, VOL 51, 2013, 51 : 393 - 455
  • [6] Properties of z ∼ 3-6 Lyman break galaxies II. Impact of nebular emission at high redshift
    de Barros, S.
    Schaerer, D.
    Stark, D. P.
    [J]. ASTRONOMY & ASTROPHYSICS, 2014, 563
  • [7] de Barros S., 2011, SF2A 2011 P ANN M FR, P95
  • [8] DESSAUGESZAVADSKY, 2015, A A, V577, DOI DOI 10.1051/0004-6361/201424661
  • [9] The mass evolution of the first galaxies: stellar mass functions and star formation rates at 4 < z < 7 in the CANDELS GOODS-South field
    Duncan, K.
    Conselice, C. J.
    Mortlock, A.
    Hartley, W. G.
    Guo, Y.
    Ferguson, H. C.
    Dave, R.
    Lu, Y.
    Ownsworth, J.
    Ashby, M. L. N.
    Dekel, A.
    Dickinson, M.
    Faber, S.
    Giavalisco, M.
    Grogin, N.
    Kocevski, D.
    Koekemoer, A.
    Somerville, R. S.
    White, C. E.
    [J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2014, 444 (03) : 2960 - 2984
  • [10] The galaxy stellar mass function at 3.5 ≤ z ≤ 7.5 in the CANDELS/UDS, GOODS-South, and HUDF fields
    Grazian, A.
    Fontana, A.
    Santini, P.
    Dunlop, J. S.
    Ferguson, H. C.
    Castellano, M.
    Amorin, R.
    Ashby, M. L. N.
    Barro, G.
    Behroozi, P.
    Boutsia, K.
    Caputi, K. I.
    Chary, R. R.
    Dekel, A.
    Dickinson, M. E.
    Faber, S. M.
    Fazio, G. G.
    Finkelstein, S. L.
    Galametz, A.
    Giallongo, E.
    Giavalisco, M.
    Grogin, N. A.
    Guo, Y.
    Kocevski, D.
    Koekemoer, A. M.
    Koo, D. C.
    Lee, K. -S.
    Lu, Y.
    Merlin, E.
    Mobasher, B.
    Nonino, M.
    Papovich, C.
    Paris, D.
    Pentericci, L.
    Reddy, N.
    Renzini, A.
    Salmon, B.
    Salvato, M.
    Sommariva, V.
    Song, M.
    Vanzella, E.
    [J]. ASTRONOMY & ASTROPHYSICS, 2015, 575
123