151 research outputs found
WISEA J083011.95+283716.0: A Missing Link Planetary-mass Object
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
WISEA J083011.95+283716.0: A Missing Link Planetary-Mass Object
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
detection in multi-epoch \textit{AllWISE} and unWISE images. We have
characterized this object with Spitzer Space Telescope and \textit{Hubble Space
Telescope} follow-up imaging. With mid-infrared detections in
\textit{Spitzer}'s \emph{ch1} and \emph{ch2} bands and flux upper limits in
Hubble Space Telescope and filters, we find that this object is
both very faint and has extremely red colors ( mag,
mag), consistent with a T K source, as
estimated from the known Y dwarf population. A preliminary parallax provides a
distance of pc, leading to a slightly warmer temperature
of K. The extreme faintness and red Hubble Space Telescope and
Spitzer Space Telescope colors of this object suggest it may be a link between
the broader Y dwarf population and the coldest known brown dwarf WISE
J08550714, and 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.Comment: 13 pages, 6 figures, 5 table
Spitzer Follow-up of Extremely Cold Brown Dwarfs Discovered by the Backyard Worlds: Planet 9 Citizen Science Project
We present Spitzer follow-up imaging of 95 candidate extremely cold brown dwarfs discovered by the Backyard Worlds: Planet 9 citizen science project, which uses visually perceived motion in multiepoch Wide-field Infrared Survey Explorer (WISE) images to identify previously unrecognized substellar neighbors to the Sun. We measure Spitzer [3.6]–[4.5] color to phototype our brown dwarf candidates, with an emphasis on pinpointing the coldest and closest Y dwarfs within our sample. The combination of WISE and Spitzer astrometry provides quantitative confirmation of the transverse motion of 75 of our discoveries. Nine of our motion-confirmed objects have best-fit linear motions larger than 1'' yr⁻¹; our fastest-moving discovery is WISEA J155349.96+693355.2 (μ ≈ 2.”15 yr⁻¹), a possible T-type subdwarf. We also report a newly discovered wide-separation (~400 au) T8 comoving companion to the white dwarf LSPM J0055+5948 (the fourth such system to be found), plus a candidate late T companion to the white dwarf LSR J0002+6357 at 5 5 projected separation (~8700 au if associated). Among our motion-confirmed targets, five have Spitzer colors most consistent with spectral type Y. Four of these five have exceptionally red Spitzer colors suggesting types of Y1 or later, adding considerably to the small sample of known objects in this especially valuable low-temperature regime. Our Y dwarf candidates begin bridging the gap between the bulk of the Y dwarf population and the coldest known brown dwarf
Spitzer Follow-up of Extremely Cold Brown Dwarfs Discovered by the Backyard Worlds: Planet 9 Citizen Science Project
We present Spitzer follow-up imaging of 95 candidate extremely cold brown
dwarfs discovered by the Backyard Worlds: Planet 9 citizen science project,
which uses visually perceived motion in multi-epoch WISE images to identify
previously unrecognized substellar neighbors to the Sun. We measure Spitzer
[3.6]-[4.5] color to phototype our brown dwarf candidates, with an emphasis on
pinpointing the coldest and closest Y dwarfs within our sample. The combination
of WISE and Spitzer astrometry provides quantitative confirmation of the
transverse motion of 75 of our discoveries. Nine of our motion-confirmed
objects have best-fit linear motions larger than 1"/yr; our fastest-moving
discovery is WISEA J155349.96+693355.2 (total motion ~2.15"/yr), a possible T
type subdwarf. We also report a newly discovered wide-separation (~400 AU) T8
comoving companion to the white dwarf LSPM J0055+5948 (the fourth such system
to be found), plus a candidate late T companion to the white dwarf LSR
J0002+6357 at 5.5' projected separation (~8,700 AU if associated). Among our
motion-confirmed targets, five have Spitzer colors most consistent with
spectral type Y. Four of these five have exceptionally red Spitzer colors
suggesting types of Y1 or later, adding considerably to the small sample of
known objects in this especially valuable low-temperature regime. Our Y dwarf
candidates begin bridging the gap between the bulk of the Y dwarf population
and the coldest known brown dwarf.Comment: accepted for publication in The Astrophysical Journa
E_multistrigaria_70.fastq
Individual fastq file from the genotyping by sequencing dataset
E_nr_catana_146.fastq
Individual fastq file from the genotyping by sequencing dataset
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