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Published June 1, 2020 | Accepted Version + Published
Journal Article Open

WISEA J083011.95+283716.0: A Missing Link Planetary-mass Object

Abstract

We present the discovery of WISEA J083011.95+283716.0, the first Y-dwarf candidate identified through the "Backyard Worlds: Planet 9" citizen science project. We identified this object as a red, fast-moving source with a faint W2 detection in multiepoch AllWISE and unWISE images. We have characterized this object with Spitzer and Hubble Space Telescope's (HST) follow-up imaging. With mid-infrared detections in Spitzer's ch1 and ch2 bands and flux upper limits in HST F105W and F125W filters, we find that this object is both very faint and has extremely red colors (ch1 − ch2 = 3.25 ± 0.23 mag, F125W − ch2 ≥ 9.36 mag), consistent with a T_(eff) ~ 300 K source, as estimated from the known Y-dwarf population. A preliminary parallax provides a distance of 11.1_(-1.5)^(+2.0) pc, leading to a slightly warmer temperature of ~350 K. The extreme faintness and red HST and Spitzer colors of this object suggest that it may be a link between the broader Y-dwarf population and the coldest known brown dwarf WISE J0855−0714, and may highlight our limited knowledge of the true spread of Y-dwarf colors. We also present four additional "Backyard Worlds: Planet 9" late-T brown dwarf discoveries within 30 pc.

Additional Information

© 2020. The American Astronomical Society. Received 2020 February 4; revised 2020 April 23; accepted 2020 April 25; published 2020 June 5. We thank the anonymous referee for their helpful and insightful suggestions that have greatly improved the clarity of this paper. The "Backyard Worlds: Planet 9" team would like to thank the many Zooniverse volunteers who have participated in this project, from providing feedback during the beta review stage to classifying flipbooks to contributing to the discussions on TALK. We would also like to thank the Zooniverse web development team for their work creating and maintaining the Zooniverse platform and the Project Builder tools. This research was supported by NASA ADAP grant NNH17AE75I. This publication makes use of data products from the Wide-field Infrared Survey Explorer, which is a joint project of the University of California, Los Angeles, and the Jet Propulsion Laboratory/California Institute of Technology, funded by the National Aeronautics and Space Administration. This research has made use of the NASA/IPAC Infrared Science Archive, which is funded by the National Aeronautics and Space Administration and operated by the California Institute of Technology. This research has made use of the VizieR catalog access tool, CDS, Strasbourg, France (DOI:10.26093/cds/vizier). The original description of the VizieR service was published in 2000, A&A 143, 23. This research made use of APLpy, an open-source plotting package for Python (Robitaille & Bressert 2012). Facilities: HST (WFC3) - , Spitzer (IRAC) - , IRSA - , WISE. - Software: APLpy (Robitaille & Bressert 2012), astrodrizzle (Gonzaga et al. 2012), astropy (Astropy Collaboration et al. 2013), MOPEX/APEX (Makovoz & Marleau 2005), Pandas (McKinney 2013), photutils (Bradley et al. 2019), SAOviewerDS9 (Joye & Mandel 2003), WiseView (Caselden et al. 2018).

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Published - Bardalez_Gagliuffi_2020_ApJ_895_145.pdf

Accepted Version - 2004.12829.pdf

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Additional details

Created:
August 22, 2023
Modified:
October 20, 2023