Items where authors include "Grimmett, LP"
Up a levelArticle
Grimmett, LP orcid.org/0000-0001-6559-4725, Mullaney, JR, Bernhard, EP et al. (5 more authors) (2020) A binning-free method reveals a continuous relationship between galaxies’ AGN power and offset from main sequence. Monthly Notices of the Royal Astronomical Society, 495 (1). pp. 1392-1402. ISSN 0035-8711
Bottrill, AL, Haigh, ME, Hole, MRA et al. (4 more authors) (2020) Exoplanet Detection and Its Dependence on Stochastic Sampling of the Stellar Initial Mass Function. The Astrophysical Journal, 895 (2). 141. ISSN 0004-637X
Delvecchio, I, Daddi, E, Aird, J et al. (10 more authors) (2020) The Evolving AGN Duty Cycle in Galaxies Since z ∼ 3 as Encoded in the X-Ray Luminosity Function. The Astrophysical Journal, 892 (1). 17. ISSN 0004-637X
Delvecchio, I, Daddi, E, Shankar, F et al. (8 more authors) (2019) The Galaxy’s Gas Content Regulated by the Dark Matter Halo Mass Results in a Superlinear M BH–M ⋆ Relation. The Astrophysical Journal Letters, 885 (2). L36. ISSN 2041-8205
Schoettler, C, Parker, RJ, Arnold, B et al. (3 more authors) (2019) Dynamical evolution of star-forming regions: III. Unbound stars and predictions for Gaia. Monthly Notices of the Royal Astronomical Society, 487 (4). pp. 4615-4630. ISSN 0035-8711
Grimmett, LP orcid.org/0000-0001-6559-4725, Mullaney, JR, Jin, S et al. (3 more authors) (2019) Revealing the differences in the SMBH accretion rate distributions of starburst and non-starburst galaxies. Monthly Notices of the Royal Astronomical Society, 487 (3). pp. 4071-4082. ISSN 0035-8711
Bernhard, E, Grimmett, LP orcid.org/0000-0001-6559-4725, Mullaney, JR et al. (3 more authors) (2019) Inferring a difference in the star-forming properties of lower versus higher X-ray luminosity AGNs. Monthly Notices of the Royal Astronomical Society: Letters, 483 (1). L52-L57. ISSN 1745-3933
Bernhard, E, Mullaney, JR, Aird, J et al. (5 more authors) Evidence for a mass-dependent AGN Eddington ratio distribution via the flat relationship between SFR and AGN luminosity.