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        VVV-WIT-04: an extragalactic variable source caught by the VVV Survey

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        1909.07516v1.pdf (PDF, 1Mb)
        Author
        Saito, Roberto K.
        Minniti, Dante
        Ivanov, Valentin D.
        Masetti, Nicola
        Navarro, Maria Gabriela
        Fernandes, Roberto Cid
        Ruschel-Dutra, Daniel
        Smith, Leigh C.
        Lucas, Philip W.
        Gonzalez-Fernandez, Carlos
        Ramos, Rodrigo Contreras
        Attention
        2299/21745
        Abstract
        We report the discovery of VVV-WIT-04, a near-infrared (near-IR) variable source towards the Galactic disc located ∼0.2 arcsec apart from the position of the radio source PMN J1515−5559. The object was found serendipitously in the near-IR data of the ESO public survey VISTA Variables in the Vía Láctea (VVV). Our analysis is based on variability, multicolour, and proper motion data from VVV and VVV eXtended surveys, complemented with archive data at longer wavelengths. We suggest that VVV-WIT-04 has an extragalactic origin as the near-IR counterpart of PMN J1515−5559. The K s-band light curve of VVV-WIT-04 is highly variable and consistent with that of an optically violent variable quasar. The variability in the near-IR can be interpreted as the redshifted optical variability. Residuals to the proper motion vary with the magnitude suggesting contamination by a blended source. Alternative scenarios, including a transient event such as a nova or supernova, or even a binary microlensing event, are not in agreement with the available data.
        Publication date
        2019-09-20
        Published in
        Monthly Notices of the Royal Astronomical Society
        Published version
        https://doi.org/10.1093/mnras/stz2631
        Other links
        http://hdl.handle.net/2299/21745
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