# coding=utf-8
"""
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"""

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        "abstract":"There is evidence of an overdensity of strong intervening MgII absorption line systems distributed along the lines of sight toward gamma-ray burst (GRB) afterglows relative to quasar sight-lines. If this excess is real, one should also expect an overdensity of field galaxies around GRB sight-lines, as strong MgII tends to trace these sources. In this work, we test this expectation by calculating the two point angular correlation function of galaxies within 120'' (~470 h<SUP>-1</SUP><SUB>71</SUB> Kpc at ⟨ z ⟩ ~ 0.4) of GRB afterglows. We compare the gamma-ray burst optical and near-infrared detector (GROND) GRB afterglow sample - one of the largest and most homogeneous samples of GRB fields - with galaxies and active galactic nuclei found in the COSMOS-30 photometric catalog. We find no significant signal of anomalous clustering of galaxies at an estimated median redshift of z ~ 0.3 around GRB sight-lines, down to K<SUB>AB</SUB> 〈 19.3. This result is contrary to the expectations from the MgII excess derived from GRB afterglow spectroscopy, although many confirmed galaxy counterparts to MgII absorbers may be too faint to detect in our sample - especially those at z 〉 1. We note that the addition of higher sensitivity Spitzer/IRAC or HST/WFC3 data for even a subset of our sample would increase this survey's depth by several orders of magnitude, simultaneously increasing statistics and enabling the investigation of a much larger redshift space.Table 1 is available in electronic form at <A href=\"http://www.aanda.org\">http://www.aanda.org</A>",
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        "ack":"We thank the anonymous referee for his or her helpful comments. We thank Sotoria Fotopoulou for insightful discussion regarding photometric calibration techniques, and David Gruber for his projection plotting routine. S.K., D.A.K., and A.R. acknowledge support by DFG grant Kl 766/16-1. S.S. acknowledges support through project M.FE.A.Ext 00003 of the MPG, and P.S. acknowledges support by DFG grant SA 2001/1-1. T.K. acknowledges support by the European Commission under the Marie Curie Intra-European Fellowship Programme. The Dark Cosmology Centre is funded by the Danish National Research Foundation.",
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        "abstract":"Prochter and coworkers recently found that the number density of strong intervening 0.5〈z〈2 Mg II absorbers detected in gamma-ray burst (GRB) afterglow spectra is nearly 4 times larger than those in QSO spectra. We have conducted a similar study using C IV absorbers. Our C IV sample, consisting of a total of 19 systems, is drawn from three high-resolution and high to moderate signal-to-noise ratio VLT UVES spectra of three long-duration GRB afterglows, covering the redshift interval 1.6〈z〈3.1. The column density distribution and number density of this sample do not show any statistical difference from the same quantities measured in QSO spectra. We discuss several possibilities for the discrepancy between C IV and Mg II absorbers and conclude that a higher dust extinction in the Mg II QSO samples studied up to now would give the most straightforward solution. However, this effect is only important for the strong Mg II absorbers. Regardless of the reasons for this discrepancy, this result confirms once more that GRBs can be used to detect a side of the universe that was unknown before, not necessarily connected with GRBs themselves, providing an alternative and fundamental investigative tool of the cosmic evolution of the universe.Based on observations collected at the European Southern Observatory, Chile; proposals 75.A-0385, 75.A-0603, and 77.D-0661.",
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        "ack":"The authors thank Alec Boksenberg, Alex Kann, Cristiano Porciani, and Tony Songaila for interesting comments. The authors especially thank Sara Ellison for sharing her insights concerning dust extinction and offering suggestions for follow‐up work. V. S. acknowledges the generosity of the Winslow Womack grant awarded by Guilford College for undergraduate research and the kind hospitality of the Max Planck Institute for Extraterrestrial Physics, at which a large part of this work was performed.",
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        "title":["Intervening Metal Systems in GRB and QSO Sight Lines: The Mg II and C IV Question"],
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        "pubdate":"2009-07-00",
        "first_author":"Sudilovsky, Vladimir",
        "abstract":"There is nearly a factor of 4 difference in the number density of intervening Mg II absorbers as determined from gamma-ray burst (GRB) and quasar lines of sight. We use a Monte Carlo simulation to test if a dust extinction bias can account for this discrepancy. We apply an empirically determined relationship between the dust column density and Mg II rest equivalent width to simulated quasar sight lines and model the underlying number of quasars that must be present to explain the published magnitude distribution of Sloan Digital Sky Survey quasars. We find that an input Mg II number density dn/dz of 0.273 ± 0.002 over the range 0.4 〈= z 〈= 2.0 and with Mg II equivalent width W <SUB>0</SUB> 〉= 1.0 Å accurately reproduces observed distributions. From this value, we conclude that a dust obstruction bias cannot be the sole cause of the observed discrepancy between GRB and quasar sight lines: this bias is likely to reduce the discrepancy only by ~10%.",
        "citation":["2009AJ....138.1690P",
          "2009ApJ...706.1309T",
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          "2011arXiv1102.4228G",
          "2011MNRAS.414..209W",
          "2011MNRAS.416.1871B",
          "2012A&A...546A..67L",
          "2013A&A...552A.143S",
          "2013ApJ...766...23R",
          "2013ApJ...768....3E"],
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        "year":"2009",
        "property":["OPENACCESS",
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        "id":"1753715",
        "recid":1753715,
        "bibcode":"2009ApJ...699...56S",
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          "2009ApJ...697..345C"],
        "aff":["Physics Department, Guilford College, 5800 Friendly Avenue, Greensboro, NC 27410, USA; Max-Planck-Institut für extraterrestrische Physik, Garching bei München, Germany",
          "Physics Department, Guilford College, 5800 Friendly Avenue, Greensboro, NC 27410, USA",
          "Max-Planck-Institut für extraterrestrische Physik, Garching bei München, Germany"],
        "keyword_schema":["Astronomy",
          "Astronomy",
          "Astronomy",
          "Astronomy",
          "arXiv",
          "arXiv"],
        "issue":"1",
        "pub_raw":"The Astrophysical Journal, Volume 699, Issue 1, pp. 56-59 (2009).",
        "pub":"The Astrophysical Journal",
        "volume":"699",
        "author_norm":["Sudilovsky, V",
          "Smith, D",
          "Savaglio, S"],
        "date":"2009-07-01T00:00:00Z",
        "doi":["10.1088/0004-637X/699/1/56"],
        "keyword":["dust",
          "extinction",
          "quasars: general",
          "surveys",
          "Astrophysics - Cosmology and Nongalactic Astrophysics",
          "Astrophysics - High Energy Astrophysical Phenomena"],
        "database":["astronomy"],
        "ack":"The authors acknowledge support from the Winslow Womack Research grant. The authors thank Brice Ménard, Hsiao-Wen Chen, and the referee for useful comments. V.S. acknowledges the support of the Guilford College Physics Department and the Max Planck Society. Funding for the SDSS and SDSS-II has been provided by the Alfred P. Sloan Foundation, the Participating Institutions, the National Science Foundation, the U.S. Department of Energy, the National Aeronautics and Space Administration, the Japanese Monbukagakusho, the Max Planck Society, and the Higher Education Funding Council for England. The SDSS Web site is http://www.sdss.org/. The SDSS is managed by the Astrophysical Research Consortium for the Participating Institutions. The Participating Institutions are the American Museum of Natural History, Astrophysical Institute Potsdam, University of Basel, University of Cambridge, Case Western Reserve University, University of Chicago, Drexel University, Fermilab, the Institute for Advanced Study, the Japan Participation Group, Johns Hopkins University, the Joint Institute for Nuclear Astrophysics, the Kavli Institute for Particle Astrophysics and Cosmology, the Korean Scientist Group, the Chinese Academy of Sciences (LAMOST), Los Alamos National Laboratory, the Max-Planck-Institute for Astronomy (MPIA), the Max-Planck-Institute for Astrophysics (MPA), New Mexico State University, Ohio State University, University of Pittsburgh, University of Portsmouth, Princeton University, the United States Naval Observatory, and the University of Washington.",
        "keyword_facet":["dust",
          "ism dust extinction",
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        "author":["Sudilovsky, Vladimir",
          "Smith, Donald",
          "Savaglio, Sandra"],
        "citation_count":12,
        "email":["-",
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        "cite_read_boost":0.31,
        "orcid_pub":["-",
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        "title":["Dusty Mg II Absorbers: Implications for the Gamma-ray Burst/Quasar Incidence Discrepancy"],
        "page":["56"],
        "_version_":1505343681984462848,
        "indexstamp":"2015-06-29T19:53:26.54Z"}]
  }}
'''

