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Disk Detective: Discovery of New Circumstellar Disk Candidates through Citizen Science

Kuchner, Marc J. and Silverberg, Steven M. and Bans, Alissa S. and Bhattacharjee, Shambo and Kenyon, Scott J. and Debes, John H. and Currie, Thayne and García, Luciano and Jung, Dawoon and Lintott, Chris and McElwain, Michael and Padgett, Deborah L. and Rebull, Luisa M. and Wisniewski, John P. and Nesvold, Erika and Schawinski, Kevin and Thaller, Michelle L. and Grady, Carol A. and Biggs, Joseph and Bosch, Milton and C̆ernohous, Tadeás̆ and Durantini Luca, Hugo A. and Hyogo, Michiharu and Wah, Lily Lau Wan and Piipuu, Art and Piñeiro, Fernanda (2016) Disk Detective: Discovery of New Circumstellar Disk Candidates through Citizen Science. Astrophysical Journal, 830 (2). Art. No. 84. ISSN 0004-637X. https://resolver.caltech.edu/CaltechAUTHORS:20161014-101530106

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Abstract

The Disk Detective citizen science project aims to find new stars with 22 μm excess emission from circumstellar dust using data from NASA's Wide-field Infrared Survey Explorer (WISE) mission. Initial cuts on the AllWISE catalog provide an input catalog of 277,686 sources. Volunteers then view images of each source online in 10 different bands to identify false positives (galaxies, interstellar matter, image artifacts, etc.). Sources that survive this online vetting are followed up with spectroscopy on the FLWO Tillinghast telescope. This approach should allow us to unleash the full potential of WISE for finding new debris disks and protoplanetary disks. We announce a first list of 37 new disk candidates discovered by the project, and we describe our vetting and follow-up process. One of these systems appears to contain the first debris disk discovered around a star with a white dwarf companion: HD 74389. We also report four newly discovered classical Be stars (HD 6612, HD 7406, HD 164137, and HD 218546) and a new detection of 22 μm excess around the previously known debris disk host star HD 22128.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.3847/0004-637X/830/2/84DOIArticle
http://iopscience.iop.org/article/10.3847/0004-637X/830/2/84PublisherArticle
https://arxiv.org/abs/1607.05713arXivDiscussion Paper
ORCID:
AuthorORCID
Kuchner, Marc J.0000-0002-2387-5489
Silverberg, Steven M.0000-0002-3741-4181
Bans, Alissa S.0000-0003-0426-7987
Kenyon, Scott J.0000-0003-0214-609X
Debes, John H.0000-0002-1783-8817
Currie, Thayne0000-0002-7405-3119
Lintott, Chris0000-0001-5578-359X
McElwain, Michael0000-0003-0241-8956
Padgett, Deborah L.0000-0001-5334-5107
Rebull, Luisa M.0000-0001-6381-515X
Wisniewski, John P.0000-0001-9209-1808
Schawinski, Kevin0000-0001-5464-0888
Bosch, Milton0000-0002-9766-2400
Durantini Luca, Hugo A.0000-0002-4143-2550
Hyogo, Michiharu0000-0001-8343-0820
Additional Information:© 2016. The American Astronomical Society. Received 2016 March 21; revised 2016 July 1; accepted 2016 July 14; published 2016 October 14. We acknowledge support from grant 14-ADAP14-0161 from the NASA Astrophysics Data Analysis Program. M.K. acknowledges funding from the NASA Astrobiology Program via the Goddard Center for Astrobiology and support from NASA's Science Innovation Fund. Development of the Disk Detectives site was supported by a grant from the Alfred P. Sloan foundation, and the Zooniverse platform is supported by a Google Global Impact award. WISE is a joint project of the University of California, Los Angeles, and the Jet Propulsion Laboratory (JPL)/California Institute of Technology (Caltech), funded by NASA. 2MASS is a joint project of the University of Massachusetts and the Infrared Processing and Analysis Center (IPAC) at Caltech, funded by NASA and the NSF. This paper uses data products produced by the OIR Telescope Data Center, supported by the Smithsonian Astrophysical Observatory. The DSS was produced at the Space Telescope Science Institute under U.S. Government grant NAG W-2166. The images of these surveys are based on photographic data obtained using the Oschin Schmidt Telescope on Palomar Mountain and the UK Schmidt Telescope. The plates were processed into the present compressed digital form with the permission of these institutions. This work has made use of the BeSS database, operated at LESIA, Observatoire de Meudon, France: http://basebe.obspm.fr. Funding for the SDSS and SDSS-II has been provided by the Alfred P. Sloan Foundation, the Participating Institutions, the National Science Foundation, the U.S. Department of Energy, the National Aeronautics and Space Administration, the Japanese Monbukagakusho, the Max Planck Society, and the Higher Education Funding Council for England. The SDSS Web site is http://www.sdss.org/. The SDSS is managed by the Astrophysical Research Consortium for the Participating Institutions. The Participating Institutions are the American Museum of Natural History, Astrophysical Institute Potsdam, University of Basel, University of Cambridge, Case Western Reserve University, University of Chicago, Drexel University, Fermilab, the Institute for Advanced Study, the Japan Participation Group, Johns Hopkins University, the Joint Institute for Nuclear Astrophysics, the Kavli Institute for Particle Astrophysics and Cosmology, the Korean Scientist Group, the Chinese Academy of Sciences (LAMOST), Los Alamos National Laboratory, the Max-Planck-Institute for Astronomy (MPIA), the Max-Planck-Institute for Astrophysics (MPA), New Mexico State University, Ohio State University, University of Pittsburgh, University of Portsmouth, Princeton University, the United States Naval Observatory, and the University of Washington. The data presented in this paper result from the efforts of the Disk Detective volunteers, without whom this work would not have been possible. The following volunteers helped classify the stars listed in this paper: 13lueAngeL, A.Brodersen, abienvenu, AlarmingAlarm, AlbeeLou, alinastart, anowi, anoxie, Arlon, artman40, arvintan, atmosferah, bc2callhome, bellapagano, berlherm, biggsjrex, billweiler, bmw.996, BraehlerM, brainell, breckwilhite, Bromista, cazze74, Chinabob, chloecollins, christania10110, clairwallis, clayzer-ev, Cosmic Jerk, cstickmaker, daisy1000, Deke scott T, dianaz, diplomacy42, djperkins@live.co.uk, DNiergarth, dooces, Ercydive, feder, ferrertiago, fireandice, firewatermoonearth, Fletrik, ftpol, GBav8r, geckzilla, Gez Quiruga, giazira, golfmadman, Grubenm, Haian, hardan, hearzadrsos, HelmutU, i-mac, iponenubs, IrvSet, Ivan_3, j.altman@kpnplanet.n, jacedjohnson, jacobus.valk@polk.de, janiceashdown, JasonJason, jellybelly123, JessicaElizabeth, jgreyes, jmeyers314, JoJeFree, jorge96, josa310, justinsbuzz, kafter, kecsap, keel, KI4FYP, kiarash, kijkuit, Killoch, kmk, lambrosliamis, lehensuge, ljhinton21, Mack777, manemag, marca, marchl, marcin.s, Maria Mar, mattlou117, MDLW, michiharu, miertje, miltonbosch, mlavall2@uwo.ca, Mric116, MylesAtkins, N5bz, namorris, nipper10, nirajsanghvi, norbertf, Noreal, nunolanca, ohio_pugmom, OMHans, onetimegolfer, orionsam1, Pamela Foster, PaulRo, peterw143, Petrusperes, Pini2013, pixelfixx, planetari7, plutoexpress, ptrip2010, QGR, Raymond Hall, RefugeZero, Ridence, RobhJ, Rocketman93, RoLeCa, rt26556@wdmtigers.or, russ jones, ryangeho, ryanstone87, sandrisvi, scottwferg, sheilaandpeter, Shigeru, shocko61, Shroomzz, silviug, Siver, SoloSlayer9, Star hunter 1, starbase3, steve bourne, SUMO_2011, SunJinx, symaski62, TED91, Tigrincs, Timothy Fitzgerald, tom.luthe, Troomander, Trumanator, Tsgt, turtle0920, Victory1, Vinokurov, Vonkohon, voyager1682002, Vulpi, weric1, WizardHowl, Woomaster, WXdestroyer, xantipa, Yiska, Zealex. We also thank Christoph Baranec and Katharina Doll for providing useful comments on this paper.
Group:Infrared Processing and Analysis Center (IPAC)
Funders:
Funding AgencyGrant Number
NASA14-ADAP14-0161
NASA Science Innovation FundUNSPECIFIED
Alfred P. Sloan FoundationUNSPECIFIED
Google Global ImpactUNSPECIFIED
NASA/JPL/CaltechUNSPECIFIED
NASANAG W-2166
Participating InstitutionsUNSPECIFIED
NSFUNSPECIFIED
Department of Energy (DOE)UNSPECIFIED
Japanese MonbukagakushoUNSPECIFIED
Max Planck SocietyUNSPECIFIED
Higher Education Funding Council for EnglandUNSPECIFIED
Subject Keywords:catalogs; infrared: planetary systems; methods: data analysis; protoplanetary disks; stars: emission-line, Be; surveys
Issue or Number:2
Record Number:CaltechAUTHORS:20161014-101530106
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20161014-101530106
Official Citation:Marc J. Kuchner et al 2016 ApJ 830 84
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:71093
Collection:CaltechAUTHORS
Deposited By: George Porter
Deposited On:14 Oct 2016 21:24
Last Modified:01 Nov 2019 18:32

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