Open Access

Table A.1.

Names of galaxy samples used in this study

Sample name No. of Section Description Other notes
galaxies
Known RPS candidates 212 Sect. 3.2 A compilation of known ram pressure stripping candidates that overlap with Galaxy Zoo 2 data Sources given in Table 1. A subset of 100 of these are used in Sect. 4
Known strong RPS candidates 58 Sect. 3.3 Known RPS candidates that only have optical features and a high RPS strength Includes known RPS sample galaxies classified in Sect. 2.2 for this study
Known Radio RPS candidates 134 Sect. 3.4 Known RPS candidates that have radio features Includes galaxies that have optical features
Known radio only RPS candidates 75 Sect. 3.4 Known RPS candidates that only have radio features No optical features reported in other studies or from classification in Sect. 2.2
Field comparison sample 1696 Sect. 3.1 A sample of galaxies that are magnitude and redshift matched to the known RPS sample that are away from clusters Cut to match strong and radio-identified RPS samples where appropriate
Cluster comparison sample 1696 Sect. 3.1 A sample of galaxies that are magnitude and redshift matched to the known RPS sample that are around cluster cores Cut to match strong and radio-identified RPS samples where appropriate
GZ-selected sample 319 Sect. 4.1 GZ2 classified disk galaxies that have properties consistent with the known RPS sample in clusters
Non-GZ control sample 319 Sect. 4.2 A sample of disk galaxies around cluster cores that are magnitude and redshift matched to the GZ-selected sample, but do not have unwinding and odd morphologies consistent with the GZ selected sample.
GZ-field sample 319 Sect. 4.3 GZ2 classified disk galaxies that have properties consistent with the known RPS sample, but are not in clusters.
Expert classified RPS candidates 101 Sect. 4.5 A combined subsample of the GZ-selected sample and the non-GZ control sample that have been classified by experts as being ram pressure stripped Table of candidates is available online

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