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Browsing publications by Dr David Rosario.

Newcastle AuthorsTitleYearFull text
Dr David Rosario
AGN feedback in the Local Universe: Multiphase outflow of the Seyfert galaxy NGC 55062024
Dr David Rosario
Deconvolution of JWST/MIRI Images: Applications to an Active Galactic Nucleus Model and GATOS Observations of NGC 57282024
Houda Haidar
Dr David Rosario
Dr Steph Campbell
Dr Chris Harrison
Dust beyond the torus: Revealing the mid-infrared heart of local Seyfert ESO 428-G14 with JWST/MIRI2024
Dr Steph Campbell
Houda Haidar
Dr David Rosario
GATOS: missing molecular gas in the outflow of NGC 5728 revealed by JWST2024
Dr Chris Harrison
Dr David Rosario
Obscuration beyond the nucleus: infrared quasars can be buried in extreme compact starbursts2024
Sean Dougherty
Dr Chris Harrison
Dr David Rosario
Obscured AGN enhancement in galaxy pairs at cosmic noon: Evidence from a probabilistic treatment of photometric redshifts2024
Dr David Rosario
A radio-jet-driven outflow in the Seyfert 2 galaxy NGC 2110?2023
Dr Vicky Fawcett
Dr David Rosario
Dr Chris Harrison
A striking relationship between dust extinction and radio detection in DESI QSOs: evidence for a dusty blow-out phase in red QSOs2023
Dr Chris Harrison
Dr David Rosario
The AGNIFS survey: spatially resolved observations of hot molecular and ionized outflows in nearby active galaxies2023
Dr David Rosario
A high angular resolution view of the PAH emission in Seyfert galaxies using JWST/MRS data2022
Dr Vicky Fawcett
Dr David Rosario
Fundamental differences in the properties of red and blue quasars: measuring the reddening and accretion properties with X-shooter2022
Dr David Rosario
Host Dark Matter Halos of SDSS Red and Blue Quasars: No Significant Difference in Large-scale Environment2022
Dr David Rosario
Dr Vicky Fawcett
Dr Chris Harrison
Fundamental differences in the radio properties of red and blue quasars: Kiloparsec-scale structures revealed by e-MERLIN2021
Dr Vicky Fawcett
Dr David Rosario
How Are Red and Blue Quasars Different? The Radio Properties2021
Dr Chris Harrison
Dr David Rosario
The impact of ionized outflows from z - 2.5 quasars is not through instantaneous in situ quenching: The evidence from ALMA and VLT/SINFONI2021
Dr Vicky Fawcett
Dr David Rosario
Fundamental differences in the radio properties of red and blue quasars: enhanced compact AGN emission in red quasars2020
Dr Chris Harrison
Dr David Rosario
KASHz: No evidence for ionised outflows instantaneously suppressing star formation in moderate luminosity AGN at z ≈ 1.4-2.62020
Dr Chris Harrison
Dr David Rosario
Do AGN really suppress star formation?2019