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| DOI | 10.1093/MNRAS/STAA2395 | ||||
| Año | 2020 | ||||
| Tipo | artículo de investigación |
Citas Totales
Autores Afiliación Chile
Instituciones Chile
% Participación
Internacional
Autores
Afiliación Extranjera
Instituciones
Extranjeras
Identification of anomalous light curves within time-domain surveys is often challenging. In addition, with the growing number of wide-field surveys and the volume of data produced exceeding astronomers' ability for manual evaluation, outlier and anomaly detection is becoming vital for transient science. We present an unsupervised method for transient discovery using a clustering technique and the ASTRONOMALY package. As proof of concept, we evaluate 85 553 min-cadenced light curves collected over two similar to 1.5 h periods as part of the Deeper, Wider, Faster program, using two different telescope dithering strategies. By combining the clustering technique HDBSCAN with the isolation forest anomaly detection algorithm via the visual interface of ASTRONOMALY, we are able to rapidly isolate anomalous sources for further analysis. We successfully recover the known variable sources, across a range of catalogues from within the fields, and find a further seven uncatalogued variables and two stellar flare events, including a rarely observed ultrafast flare (similar to 5min) from a likely M-dwarf.
| Ord. | Autor | Género | Institución - País |
|---|---|---|---|
| 1 | Webb, Sara | Mujer |
Swinburne Univ Technol - Australia
ARC Ctr Excellence Gravitat Wave Discovery OzGrav - Australia Swinburne University of Technology - Australia ARC Centre of Excellence for Gravitational Wave Discovery - Australia |
| 2 | Lochner, Michelle | Mujer |
Univ Western Cape - República de Sudáfrica
African Inst Math Sci - República de Sudáfrica South African Radio Astron Observ - República de Sudáfrica University of the Western Cape - República de Sudáfrica African Institute of Mathematical Sciences - República de Sudáfrica Observatory - República de Sudáfrica African Institute for Mathematical Sciences - República de Sudáfrica South African Radio Astronomical Observatory - República de Sudáfrica |
| 3 | Muthukrishna, D. | Hombre |
UNIV CAMBRIDGE - Reino Unido
Institute of Astronomy - Reino Unido |
| 4 | Cooke, Jeff | Hombre |
Swinburne Univ Technol - Australia
ARC Ctr Excellence Gravitat Wave Discovery OzGrav - Australia Swinburne University of Technology - Australia ARC Centre of Excellence for Gravitational Wave Discovery - Australia |
| 5 | Flynn, Chris | Hombre |
Swinburne Univ Technol - Australia
ARC Ctr Excellence Gravitat Wave Discovery OzGrav - Australia Swinburne University of Technology - Australia ARC Centre of Excellence for Gravitational Wave Discovery - Australia |
| 6 | Mahabal, A. A. | Hombre |
CALTECH - Estados Unidos
California Institute of Technology - Estados Unidos California Institute of Technology Division of Engineering and Applied Science - Estados Unidos |
| 7 | Goode, Simon | Hombre |
Swinburne Univ Technol - Australia
ARC Ctr Excellence Gravitat Wave Discovery OzGrav - Australia Swinburne University of Technology - Australia ARC Centre of Excellence for Gravitational Wave Discovery - Australia |
| 8 | Andreoni, I. | Hombre |
CALTECH - Estados Unidos
California Institute of Technology - Estados Unidos California Institute of Technology Division of Engineering and Applied Science - Estados Unidos |
| 9 | Pritchard, Tyler | Hombre |
NYU - Estados Unidos
The Center for Cosmology and Particle Physics - Estados Unidos |
| 10 | ABBOTT, TIMOTHY | Hombre |
Observatorio Interamericano del Cerro Tololo - Chile
Cerro Tololo Inter American Observatory - Chile |
| Fuente |
|---|
| National Science Foundation |
| Fundação Carlos Chagas Filho de Amparo à Pesquisa do Estado do Rio de Janeiro |
| Conselho Nacional de Desenvolvimento Científico e Tecnológico |
| Deutsche Forschungsgemeinschaft |
| Financiadora de Estudos e Projetos |
| U.S. Department of Energy |
| U.S. National Science Foundation |
| Ohio State University |
| National Research Foundation (NRF) |
| Center for Cosmology and AstroParticle Physics at the Ohio State University |
| University of Portsmouth |
| University of Chicago |
| Science and Technology Facilities Council of the United Kingdom |
| University of Michigan |
| Ministry of Science and Education of Spain |
| Higher Education Funding Council for England |
| National Center for Supercomputing Applications at the University of Illinois at Urbana-Champaign |
| Kavli Institute of Cosmological Physics at the University of Chicago |
| Mitchell Institute for Fundamental Physics and Astronomy at Texas AM University |
| Ministerio da Ciencia, Tecnologia e Inovacao |
| Argonne National Laboratory |
| University College London |
| University of Edinburgh |
| Eidgenossische Technische Hochschule (ETH) Zurich |
| Institut de Ciencies de l'Espai (IEEC/CSIC) |
| Ludwig-Maximilians Universitat Munchen |
| National Optical Astronomy Observatory |
| University of Nottingham |
| SLAC National Accelerator Laboratory |
| University of Sussex |
| Texas AM University |
| University of California at Santa Cruz |
| Stanford University |
| DES-Brazil Consortium |
| University of Illinois at Urbana Champaign |
| Simons Foundation |
| University of Cambridge, Centro de Investigaciones Energeticas, Medioambientales y Tecnologicas-Madrid |
| Collaborating Institutions in the Dark Energy Survey |
| Kavli Foundation |
| UC Santa Cruz |
| Institut de Fisica d'Altes Energies, Lawrence Berkeley National Laboratory |
| OzDES Membership Consortium the University of Pennsylvania |
| GROWTH (Global Relay of Observatories Watching Transients Happen) - National Science Foundation under PIRE |
| Fermi NationalAccelerator Laboratory |
| Agradecimiento |
|---|
| r Based on observations at Cerro Tololo Inter-American Observatory, National Optical Astronomy Observatory which is operated by the Association of Universities for Research in Astronomy (AURA) under a cooperative agreement with the National Science Foundation. |
| Based on observations at Cerro Tololo Inter-American Observatory, National Optical Astronomy Observatory which is operated by the Association of Universities for Research in Astronomy (AURA) under a cooperative agreement with the National Science Foundation. |