1. The First Brown Dwarf Discovered by the Backyard Worlds: Planet 9 Citizen Science Project
- Author
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Marc J. Kuchner, Rosa Castro, Laura Trouille, Khasan Mokaev, Steven M. Silverberg, Adam C. Schneider, Jacqueline K. Faherty, Jonathan Gagné, Joseph C. Filippazzo, Aaron Meisner, Bob Fletcher, and Tamara Stajic
- Subjects
Physics ,Earth and Planetary Astrophysics (astro-ph.EP) ,Solar System ,Proper motion ,010504 meteorology & atmospheric sciences ,Brown dwarf ,Astronomy ,FOS: Physical sciences ,Astronomy and Astrophysics ,01 natural sciences ,Astrophysics - Solar and Stellar Astrophysics ,13. Climate action ,Space and Planetary Science ,Planet ,0103 physical sciences ,Magnitude (astronomy) ,Citizen science ,Substellar object ,010303 astronomy & astrophysics ,Solar and Stellar Astrophysics (astro-ph.SR) ,Astrophysics - Earth and Planetary Astrophysics ,0105 earth and related environmental sciences - Abstract
The Wide-field Infrared Survey Explorer (WISE) is a powerful tool for finding nearby brown dwarfs and searching for new planets in the outer solar system, especially with the incorporation of NEOWISE and NEOWISE-Reactivation data. So far, searches for brown dwarfs in WISE data have yet to take advantage of the full depth of the WISE images. To efficiently search this unexplored space via visual inspection, we have launched a new citizen science project, called "Backyard Worlds: Planet 9," which asks volunteers to examine short animations composed of difference images constructed from time-resolved WISE coadds. We report the discovery of the first new substellar object found by this project, WISEA J110125.95+540052.8, a T5.5 brown dwarf located approximately 34 pc from the Sun with a total proper motion of $\sim$0.7 as yr$^{-1}$. WISEA J110125.95+540052.8 has a WISE $W2$ magnitude of $W2=15.37 \pm 0.09$, this discovery demonstrates the ability of citizen scientists to identify moving objects via visual inspection that are 0.9 magnitudes fainter than the $W2$ single-exposure sensitivity, a threshold that has limited prior motion-based brown dwarf searches with WISE., Comment: 9 pages, 4 figures, 1 table. Accepted for publication in the Astrophysical Journal Letters
- Published
- 2017
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