Metals in the IGM approaching the re-ionization epoch: results from X-shooter at the VLT

被引:83
作者
D'Odorico, V. [1 ]
Cupani, G. [1 ]
Cristiani, S. [1 ,2 ]
Maiolino, R. [3 ,4 ,5 ]
Molaro, P. [1 ]
Nonino, M. [1 ]
Centurion, M. [1 ]
Cimatti, A. [6 ]
Alighieri, S. di Serego [7 ]
Fiore, F. [3 ]
Fontana, A. [3 ]
Gallerani, S. [8 ]
Giallongo, E. [3 ]
Mannucci, F. [7 ]
Marconi, A. [9 ]
Pentericci, L. [3 ]
Viel, M. [1 ,2 ]
Vladilo, G. [1 ]
机构
[1] INAF OATS, I-34143 Trieste, Italy
[2] INFN Natl Inst Nucl Phys, I-34127 Trieste, Italy
[3] INAF OAR, I-00040 Monte Porzio Catone, Italy
[4] Univ Cambridge, Cavendish Lab, Cambridge CB3 0HE, England
[5] Kavli Inst Cosmol, Cambridge CB3 0HA, England
[6] Univ Bologna, Dipartimento Astron, I-40127 Bologna, Italy
[7] INAF OAArcetri, I-50125 Florence, Italy
[8] Scuola Normale Super Pisa, I-56126 Pisa, Italy
[9] Univ Florence, Dipartimento Fis & Astron, I-50019 Florence, Italy
关键词
galaxies: abundances; intergalactic medium; quasars: absorption lines; cosmology: observations; STAR-FORMING GALAXIES; INTERGALACTIC C-IV; DIGITAL SKY SURVEY; BLACK-HOLE MASSES; LY-ALPHA FOREST; SIMILAR-TO; 6; IONIZING-RADIATION; ABSORPTION-LINES; INFRARED-SPECTRA; LYMAN FOREST;
D O I
10.1093/mnras/stt1365
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present the results of observations taken with the X-shooter spectrograph devoted to the study of quasars at z similar to 6. This paper focuses on the properties of metals at high redshift traced, in particular, by the C IV doublet absorption systems. Six objects were observed with resolutions similar or equal to 27 and 34 km s(-1) in the visual, and 37.5 and 53.5 kms(-1) in the near-infrared. We detected 102 C IV lines in the range: 4.35 < z < 6.2 of which 27 are above z similar to 5. Thanks to the characteristics of resolution and spectral coverage of X-shooter, we could also detect 25 Si IV doublets associated with the C IV at z greater than or similar to 5. The column density distribution function of the C IV line sample is observed to evolve in redshift for z greater than or similar to 5.3, with respect to the normalization defined by low-redshift (1.5 < z < 4) C IV lines. This behaviour is reflected in the redshift evolution of the C IV cosmic mass density, Omega(C IV), of lines with column density in the range 13.4 < log N(C IV) < 15, which is consistent with a drop of a factor of similar to 2 for z greater than or similar to 5.3. Considering only the stronger C IV lines (13.8 < log N(C IV) < 15), Omega(C IV) gently rises by a factor of similar to 10 between z similar or equal to 6.2 and z similar or equal to 1.5 with a possible flattening towards z similar to 0. The increase is well fitted by a power law: Omega(C IV) = (2 +/- 1) x 10(-8)[(1 + z)/4](-3.1 +/- 0.1). An insight into the properties of the C IV absorbers and their evolution with redshift is obtained by comparing the observed column densities of associated C IV, Si IV and C II absorptions with the output of a set of CLOUDY photoionization models. As already claimed by cosmological simulations, we find that C IV is a good tracer of the metallicity in the low-density intergalactic medium (IGM) gas at z similar to 5-6 while at z similar to 3 it arises in gas with overdensity delta similar to 100.
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收藏
页码:1198 / 1232
页数:35
相关论文
共 61 条
  • [1] The connection between galaxies and intergalactic absorption lines at redshift 2≲z≲3
    Adelberger, KL
    Shapley, AE
    Steidel, CC
    Pettini, M
    Erb, DK
    Reddy, NA
    [J]. ASTROPHYSICAL JOURNAL, 2005, 629 (02) : 636 - 653
  • [2] Spectral shape of the UV ionizing background and HeII absorption at redshifts 1.8&lt;z&lt;2.9
    Agafonova, I. I.
    Levshakov, S. A.
    Reimers, D.
    Fechner, C.
    Tytler, D.
    Simcoe, R. A.
    Songaila, A.
    [J]. ASTRONOMY & ASTROPHYSICS, 2007, 461 (03) : 893 - 909
  • [3] Ballester P., 2000, MESSENGER, V101, P31
  • [4] Discovery of excess OI absorption toward the z=6.42 QSO SDSS J1148+5251
    Becker, GD
    Sargent, WLW
    Rauch, M
    Simcoe, RA
    [J]. ASTROPHYSICAL JOURNAL, 2006, 640 (01) : 69 - 80
  • [5] IRON AND α-ELEMENT PRODUCTION IN THE FIRST ONE BILLION YEARS AFTER THE BIG BANG
    Becker, George D.
    Sargent, Wallace L. W.
    Rauch, Michael
    Carswell, Robert F.
    [J]. ASTROPHYSICAL JOURNAL, 2012, 744 (02)
  • [6] HIGH-REDSHIFT METALS. II. PROBING REIONIZATION GALAXIES WITH LOW-IONIZATION ABSORPTION LINES AT REDSHIFT SIX
    Becker, George D.
    Sargent, Wallace L. W.
    Rauch, Michael
    Calverley, Alexander P.
    [J]. ASTROPHYSICAL JOURNAL, 2011, 735 (02)
  • [7] HIGH-REDSHIFT METALS. I. THE DECLINE OF C IV AT z &gt; 5.3
    Becker, George D.
    Rauch, Michael
    Sargent, Wallace L. W.
    [J]. ASTROPHYSICAL JOURNAL, 2009, 698 (02) : 1010 - 1019
  • [8] The contribution of galaxies to the UV ionising background and the evolution of the Lyman forest
    Bianchi, S
    Cristiani, S
    Kim, TS
    [J]. ASTRONOMY & ASTROPHYSICS, 2001, 376 (01) : 1 - 9
  • [9] Boksenberg A., 2003, PREPRINT
  • [10] The impact of spatial fluctuations in the ultraviolet background on intergalactic carbon and silicon
    Bolton, James S.
    Viel, Matteo
    [J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2011, 414 (01) : 241 - 252