{ "id": "1812.08479", "version": "v1", "published": "2018-12-20T10:58:56.000Z", "updated": "2018-12-20T10:58:56.000Z", "title": "The angular momentum of disc galaxies at z=1", "authors": [ "A. Marasco", "F. Fraternali", "L. Posti", "M. Ijtsma", "E. M. Di Teodoro", "T. Oosterloo" ], "comment": "11 pages, 4 figures, 1 table. Accepted by A&A", "categories": [ "astro-ph.GA" ], "abstract": "We investigate the relation between stellar mass and specific stellar angular momentum, or `Fall relation', for a sample of 17 isolated, regularly rotating disc galaxies at z=1. All galaxies have a) rotation curves determined from Halpha emission-line data; b) HST imaging in optical and infrared filters; c) robust determinations of their stellar masses. We use HST images in f814w and f160w filters, roughly corresponding to rest-frames B and I bands, to extract surface brightness profiles for our systems. We robustly bracket the specific angular momentum by assuming that rotation curves beyond the outermost Halpha rotation point stay either flat or follow a Keplerian fall-off. By comparing our measurements with those determined for disc galaxies in the local Universe, we find no evolution in the Fall relation in the redshift range 0