AGN photoionization of gas in companion galaxies as a probe of AGN radiation in time and direction

Monthly Notices of the Royal Astronomical Society 483:4 (2019) 4847-4865

Authors:

WC Keel, VN Bennert, A Pancoast, CE Harris, A Nierenberg, SD Chojnowski, AV Moiseev, DV Oparin, CJ Lintott, K Schawinski, G Mitchell, C Cornen

Abstract:

© 2018 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society. We consider active galactic nucleus (AGN) photoionization of gas in companion galaxies (cross-ionization) as a way to sample the intensity of AGN radiation in both direction and time, independent of the gas properties of the AGN host galaxies. From an initial set of 212 AGN+companion systems, identified with the help of Galaxy Zoo participants, we obtained long-slit optical spectra of 32 pairs that were a priori likely to show cross-ionization based on projected separation or angular extent of the companion. From emission-line ratios, 10 of these systems are candidates for cross-ionization, roughly the fraction expected if most AGNs have ionization cones with 70° opening angles. Among these, Was 49 remains the strongest nearby candidate. NGC 5278/9 and UGC 6081 are dual-AGN systems with tidal debris, complicating identification of cross-ionization. The two weak AGNs in the NGC 5278/9 system ionize gas filaments to a projected radius 14 kpc from each galaxy. In UGC 6081, an irregular high-ionization emission region encompasses both AGNs, extending more than 15 kpc from each. The observed AGN companion galaxies with and without signs of external AGN photoionization have similar distributions in estimated incident AGN flux, suggesting that geometry of escaping radiation or long-term variability controls this facet of the AGN environment. This parallels conclusions for luminous QSOs based on the proximity effect among Lyman α absorbers. In some galaxies, mismatch between spectroscopic classifications in the common BPT diagram and the intensity of weaker He ii and [Ne v] emission lines highlights the limits of common classifications in low-metallicity environments.

Identification of low surface brightness tidal features in galaxies using convolutional neural networks

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 483:3 (2019) 2968-2982

Authors:

Mike Walmsley, Annette MN Ferguson, Robert G Mann, Chris J Lintott

Machine Learning for the Zwicky Transient Facility

PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC 131:997 (2019) ARTN 038002

Authors:

Ashish Mahabal, Umaa Rebbapragada, Richard Walters, Frank J Masci, Nadejda Blagorodnova, Jan van Roestel, Quan-Zhi Ye, Rahul Biswas, Kevin Burdge, Chan-Kao Chang, Dmitry A Duev, V Zach Golkhou, Adam A Miller, Jakob Nordin, Charlotte Ward, Scott Adams, Eric C Bellm, Doug Branton, Brian Bue, Chris Cannella, Andrew Connolly, Richard Dekany, Ulrich Feindt, Tiara Hung, Lucy Fortson, Sara Frederick, C Fremling, Suvi Gezari, Matthew Graham, Steven Groom, Mansi M Kasliwal, Shrinivas Kulkarni, Thomas Kupfer, Hsing Wen Lin, Chris Lintott, Ragnhild Lunnan, John Parejko, Thomas A Prince, Reed Riddle, Ben Rusholme, Nicholas Saunders, Nima Sedaghat, David L Shupe, Leo P Singer, Maayane T Soumagnac, Paula Szkody, Yutaro Tachibana, Kushal Tirumala, Sjoert van Velzen, Darryl Wright

Citizen science frontiers: Efficiency, engagement, and serendipitous discovery with human-machine systems.

Proceedings of the National Academy of Sciences of the United States of America 116:6 (2019) 1902-1909

Authors:

Laura Trouille, Chris J Lintott, Lucy F Fortson

Abstract:

Citizen science has proved to be a unique and effective tool in helping science and society cope with the ever-growing data rates and volumes that characterize the modern research landscape. It also serves a critical role in engaging the public with research in a direct, authentic fashion and by doing so promotes a better understanding of the processes of science. To take full advantage of the onslaught of data being experienced across the disciplines, it is essential that citizen science platforms leverage the complementary strengths of humans and machines. This Perspectives piece explores the issues encountered in designing human-machine systems optimized for both efficiency and volunteer engagement, while striving to safeguard and encourage opportunities for serendipitous discovery. We discuss case studies from Zooniverse, a large online citizen science platform, and show that combining human and machine classifications can efficiently produce results superior to those of either one alone and how smart task allocation can lead to further efficiencies in the system. While these examples make clear the promise of human-machine integration within an online citizen science system, we then explore in detail how system design choices can inadvertently lower volunteer engagement, create exclusionary practices, and reduce opportunity for serendipitous discovery. Throughout we investigate the tensions that arise when designing a human-machine system serving the dual goals of carrying out research in the most efficient manner possible while empowering a broad community to authentically engage in this research.

K2-288Bb: A Small Temperate Planet in a Low-mass Binary System Discovered by Citizen Scientists

ASTRONOMICAL JOURNAL 157:2 (2019) ARTN 40

Authors:

Adina D Feinstein, Joshua E Schlieder, John H Livingston, David R Ciardi, Andrew W Howard, Lauren Arnold, Geert Barentsen, Makennah Bristow, Jessie L Christiansen, Ian JM Crossfield, Courtney D Dressing, Erica J Gonzales, Molly Kosiarek, Chris J Lintott, Grant Miller, Farisa Y Morales, Erik A Petigura, Beverly Thackeray, Joanne Ault, Elisabeth Baeten, Alexander F Jonkeren, James Langley, Houssen Moshinaly, Kirk Pearson, Christopher Tanner, Joanna Treasure