EB
E. Bernhard
astro-ph.GAastro-ph.IMastro-ph.SR
On Valency
published · living versionsW_qye9bppt·v1 · currentpublished
Constraining the properties of AGN host galaxies with Spectral Energy Distribution modeling
with L. Ciesla, V. Charmandaris, A. Georgakakis, P. D. Mitchell +6
1 version
Preprints & journals
15 papers in the corpus · 2014–2025Exploration of groups and outliers in Gaia RVS stellar spectra with metric learning2508.00071v2 · Yarden Eilat Bloch, Dovi Poznanski, Nick L. J. Cox et al.2025 · 0 citationsarXiv
Deep Herschel observations of the 2Jy sample: assessing the non-thermal and AGN contributions to the far-IR continuum2211.13031v1 · D. Dicken, C. N. Tadhunter, N. P. H. Nesvadba et al.2022 · 4 citationsarXiv
Quantifying the cool ISM in radio AGNs: evidence for late-time re-triggering by galaxy mergers and interactions2202.08276v1 · E. Bernhard, C. N. Tadhunter, J. C. S. Pierce et al.2022 · 13 citationsarXiv
Taking snapshots of the jet-ISM interplay: The case of PKS0023-262109.13516v1 · Raffaella Morganti, Tom Oosterloo, Clive Tadhunter et al.2021 · 39 citationsA&A 656, A55 (2021)
The post-Herschel view of intrinsic AGN emission: constructing templates for galaxy and AGN emission at IR wavelengths2102.05663v1 · E. Bernhard, C. Tadhunter, J. R. Mullaney et al.2021 · 21 citationsarXiv
The evolving AGN duty cycle in galaxies since z$\sim$3 as encoded in the X-ray luminosity function2002.08965v1 · I. Delvecchio, E. Daddi, J. Aird et al.2020 · 28 citationsarXiv
A binning-free method reveals a continuous relationship between galaxies' AGN power and offset from main sequence2001.11573v2 · L. P. Grimmett, J. R. Mullaney, E. P. Bernhard et al.2020 · 19 citationsarXiv
A contribution of star-forming clumps and accreting satellites to the mass assembly of z ~ 2 galaxies1907.12136v1 · A. Zanella, E. Le Floc'h, C. M. Harrison et al.2019 · 76 citationsarXiv
Revealing the differences in the SMBH accretion rate distributions of starburst and non-starburst galaxies1904.08406v1 · L.P. Grimmett, J.R.Mullaney, S. Jin et al.2019 · 8 citationsarXiv
Inferring a difference in the star-forming properties of lower versus higher X-ray luminosity AGNs1811.05980v1 · E. Bernhard, L.P. Grimmett, J.R. Mullaney et al.2018 · 39 citationsarXiv
Evidence for a mass-dependent AGN Eddington ratio distribution via the flat relationship between SFR and AGN luminosity1801.07717v2 · E. Bernhard, J.R. Mullaney, J. Aird et al.2018 · 17 citationsarXiv
An enhanced fraction of starbursting galaxies among high Eddington ratio AGNs1604.06455v1 · E. Bernhard, J. R. Mullaney, E. Daddi et al.2016 · 40 citationsarXiv
ALMA and Herschel reveal that X-ray selected AGN and main-sequence galaxies have different star formation rate distributions1506.05459v2 · J. R. Mullaney, D. M. Alexander, J. Aird et al.2015 · 124 citationsarXiv
Constraining the properties of AGN host galaxies with Spectral Energy Distribution modeling1501.03672v2 · L. Ciesla, V. Charmandaris, A. Georgakakis et al.2015 · 253 citationsA&A 576, A10 (2015)on Valency
Modeling the connection between ultraviolet and infrared galaxy populations across cosmic times1405.1425v1 · E. Bernhard, M. B'ethermin, M. Sargent et al.2014 · 31 citationsarXiv
Career total: 25 works. 15 are in this corpus.
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