Karen L Masters
Galaxy Zoo: 3D - Crowdsourced bar, spiral, and foreground star masks for MaNGA target galaxies
Masters, Karen L; Krawczyk, Coleman; Shamsi, Shoaib; Todd, Alexander; Finnegan, Daniel; Bershady, Matthew; Bundy, Kevin; Cherinka, Brian; Fraser-Mckelvie, Amelia; Krishnarao, Dhanesh; Kruk, Sandor; Lane, Richard R; Law, David; Lintott, Chris; Merrifield, Michael; Simmons, Brooke; Weijmans, Anne Marie; Yan, Renbin
Authors
Coleman Krawczyk
Shoaib Shamsi
Alexander Todd
Daniel Finnegan
Matthew Bershady
Kevin Bundy
Brian Cherinka
Amelia Fraser-Mckelvie
Dhanesh Krishnarao
Sandor Kruk
Richard R Lane
David Law
Chris Lintott
Michael Merrifield
Brooke Simmons
Anne Marie Weijmans
Renbin Yan
Abstract
The challenge of consistent identification of internal structure in galaxies - in particular disc galaxy components like spiral arms, bars, and bulges - has hindered our ability to study the physical impact of such structure across large samples. In this paper we present Galaxy Zoo: 3D (GZ:3D) a crowdsourcing project built on the Zooniverse platform that we used to create spatial pixel (spaxel) maps that identify galaxy centres, foreground stars, galactic bars, and spiral arms for 29 831 galaxies that were potential targets of the MaNGA survey (Mapping Nearby Galaxies at Apache Point Observatory, part of the fourth phase of the Sloan Digital Sky Surveys or SDSS-IV), including nearly all of the 10 010 galaxies ultimately observed. Our crowdsourced visual identification of asymmetric internal structures provides valuable insight on the evolutionary role of non-axisymmetric processes that is otherwise lost when MaNGA data cubes are azimuthally averaged. We present the publicly available GZ:3D catalogue alongside validation tests and example use cases. These data may in the future provide a useful training set for automated identification of spiral arm features. As an illustration, we use the spiral masks in a sample of 825 galaxies to measure the enhancement of star formation spatially linked to spiral arms, which we measure to be a factor of three over the background disc, and how this enhancement increases with radius.
Citation
Masters, K. L., Krawczyk, C., Shamsi, S., Todd, A., Finnegan, D., Bershady, M., …Yan, R. (2021). Galaxy Zoo: 3D - Crowdsourced bar, spiral, and foreground star masks for MaNGA target galaxies. Monthly Notices of the Royal Astronomical Society, 507(3), 3923-3935. https://doi.org/10.1093/mnras/stab2282
Journal Article Type | Article |
---|---|
Acceptance Date | Aug 3, 2021 |
Online Publication Date | Aug 10, 2021 |
Publication Date | Nov 1, 2021 |
Deposit Date | Sep 14, 2021 |
Publicly Available Date | Sep 14, 2021 |
Journal | Monthly Notices of the Royal Astronomical Society |
Print ISSN | 0035-8711 |
Electronic ISSN | 1365-2966 |
Publisher | Oxford University Press (OUP) |
Peer Reviewed | Peer Reviewed |
Volume | 507 |
Issue | 3 |
Pages | 3923-3935 |
DOI | https://doi.org/10.1093/mnras/stab2282 |
Keywords | Space and Planetary Science; Astronomy and Astrophysics |
Public URL | https://nottingham-repository.worktribe.com/output/6239095 |
Publisher URL | https://academic.oup.com/mnras/article/507/3/3923/6347355 |
Additional Information | This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society ©: 2021 The Author(s), Published by Oxford University Press on behalf of Royal Astronomical Society. All rights reserved. |
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