Results from the Wide-field Infrared Survey Explorer (WISE) Future Uses Session at the WISE at 5 Meeting

• Published in: arXiv.org 2015-05
• Main Authors: Faherty, Jacqueline K, Alatalo, K, Anderson, L D, Assef, Roberto J, Daniella C Bardalez Gagliuffi, Barry, Megan, Benford, Dominic J, Bilicki, Maciej, Burningham, Ben, Christian, Damian J, Cushing, Michael C, Eisenhardt, Peter R, Elvisx, Martin, Fajardo-Acosta, S B, Finkbeiner, Douglas P, Fischer, William J, rest, William J, Fowler, John, Gardner, Jonathan P, Gelino, Christopher R, Gorjian, V, Grillmair, Carl J, Gromadzki, Mariusz, Hall, Kendall P, Ivezi'c, Zeljko, Izumi, Natsuko, J Davy Kirkpatrick, Kovács, András, Lang, Dustin, Leisawitz, David, Liu, Fengchuan, Mainzer, A, Malek, Katarzyna, Marton, Gábor, Masci, Frank J, McLean, Ian S, Meisner, Aaron, Nikutta, Robert, Padgett, Deborah L, Patel, Rahul, Rebull, L M, Rich, J A, Ringwald, Frederick A, Rose, Marvin, Schneider, Adam C, Stassun, Keivan G, Stern, Daniel, Chao-Wei, Tsai, Wang, Feige, Weston, Madalyn E, Edward, L, Wright, Wu, Jingwen, Yang, Jinyi
• Format: Article
• Language: English
• Subjects: Bifurcations; Machine learning; Parallax; Photometry; Wide-field Infrared Survey Explorer
• ISSN: 2331-8422

During the "WISE at 5: Legacy and Prospects" conference in Pasadena, CA -- which ran from February 10 - 12, 2015 -- attendees were invited to engage in an interactive session exploring the future uses of the Wide-field Infrared Survey Explorer (WISE) data. The 65 participants -- many of whom are extensive users of the data -- brainstormed the top questions still to be answered by the mission, as well as the complementary current and future datasets and additional processing of WISE/NEOWISE data that would aid in addressing these most important scientific questions. The results were mainly bifurcated between topics related to extragalactic studies (e.g. AGN, QSOs) and substellar mass objects. In summary, participants found that complementing WISE/NEOWISE data with cross-correlated multiwavelength surveys (e.g. SDSS, Pan-STARRS, LSST, Gaia, Euclid, etc.) would be highly beneficial for all future mission goals. Moreover, developing or implementing machine-learning tools to comb through and understand cross-correlated data was often mentioned for future uses. Finally, attendees agreed that additional processing of the data such as co-adding WISE and NEOWISE and extracting a multi-epoch photometric database and parallax and proper motion catalog would greatly improve the scientific results of the most important projects identified. In that respect, a project such as MaxWISE which would execute the most important additional processing and extraction as well as make the data and catalogs easily accessible via a public portal was deemed extremely important.