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    Discovery of a z=0.65 post-starburst BAL quasar in the DES supernova fields

    Access Status
    Fulltext not available
    Authors
    Mudd, D.
    Martini, P.
    Tie, S.
    Lidman, C.
    McMahon, R.
    Banerji, M.
    Davis, T.
    Peterson, B.
    Sharp, R.
    Seymour, Nick
    Childress, M.
    Lewis, G.
    Tucker, B.
    Yuan, F.
    Abbot, T.
    Abdalla, F.
    Allam, S.
    Benoit-Levy, A.
    Bertin, E.
    Brooks, D.
    Camero Rosell, A.
    Kind, M.
    Carretero, J.
    da Costa, L.
    Desai, S.
    Diehl, T.
    Eifler, T.
    Finley, D.
    Flaugher, B.
    Glazebrook, K.
    Gruen, D.
    Gruendl, R.
    Gutierrez, G.
    Hinton, S.
    Honscheid, K.
    James, D.
    Kuehn, K.
    Kuropatkin, N.
    Macaulay, E.
    Maia, M.
    Miquel, R.
    Ogando, R.
    Plazas, A.
    Riel, K.
    Sanchez, E.
    Santiago, B.
    Schubnell, M.
    Sevilla-Noarbe, I.
    Smith, R.
    Soares-Santos, M.
    Sobreira, F.
    Suchyta, E.
    Swanson, M.
    Tarle, G.
    Thomas, D.
    Uddin, S.
    Walker, A.
    Zhang, B.
    Date
    2017
    Type
    Journal Article
    
    Metadata
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    Citation
    Mudd, D. and Martini, P. and Tie, S. and Lidman, C. and McMahon, R. and Banerji, M. and Davis, T. et al. 2017. Discovery of a z=0.65 post-starburst BAL quasar in the DES supernova fields. Monthly Notices of the Royal Astronomical Society. 468 (3): pp. 3682-3688.
    Source Title
    Monthly Notices of the Royal Astronomical Society
    DOI
    10.1093/mnras/stx708
    ISSN
    0035-8711
    School
    Department of Physics and Astronomy
    URI
    http://hdl.handle.net/20.500.11937/63152
    Collection
    • Curtin Research Publications
    Abstract

    We present the discovery of a z = 0.65 low-ionization broad absorption line (LoBAL) quasar in a post-starburst galaxy in data from the Dark Energy Survey (DES) and spectroscopy from the Australian Dark Energy Survey (OzDES). LoBAL quasars are a minority of all BALs, and rarer still is that this object also exhibits broad Fe ii (an FeLoBAL) and Balmer absorption. This is the first BAL quasar that has signatures of recently truncated star formation, which we estimate ended about 40 Myr ago. The characteristic signatures of an FeLoBAL require high column densities, which could be explained by the emergence of a young quasar from an early, dust-enshrouded phase, or by clouds compressed by a blast wave. The age of the starburst component is comparable to estimates of the lifetime of quasars, so if we assume the quasar activity is related to the truncation of the star formation, this object is better explained by the blast wave scenario.

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