| human | Q5 |
| P8880 | AstroGen ID | 15486 |
| P6178 | Dimensions author ID | 016275002775.23 |
| P227 | GND ID | 1096340771 |
| P269 | IdRef ID | 192736655 |
| P496 | ORCID iD | 0000-0001-8618-4223 |
| P214 | VIAF ID | 331146094243300331676 |
| P10832 | WorldCat Entities ID | E39PBJcBYVpyvRmWb3RB4vmmVC |
| P69 | educated at | University of Edinburgh | Q160302 |
| Durham University | Q458393 | ||
| P108 | employer | European Southern Observatory | Q151991 |
| Durham University | Q458393 | ||
| Newcastle University | Q837164 | ||
| P734 | family name | Harrison | Q2712864 |
| Harrison | Q2712864 | ||
| Harrison | Q2712864 | ||
| P735 | given name | Chris | Q339346 |
| Chris | Q339346 | ||
| P106 | occupation | astrophysicist | Q752129 |
| P21 | sex or gender | male | Q6581097 |
| Q114823330 | Cosmological simulations predict that AGN preferentially live in gas-rich, star-forming galaxies despite effective feedback |
| Q114823507 | Flat rotation curves of z ∼ 1 star-forming galaxies |
| Q110247480 | Galaxy mergers in eagle do not induce a significant amount of black hole growth yet do increase the rate of luminous AGN |
| Q114823678 | The Evolution of Gas-Phase Metallicity and Resolved Abundances in Star-forming Galaxies at z ≈ 0.6 – 1.8 |
| Q114823550 | The KMOS galaxy evolution survey (KGES): the angular momentum of star-forming galaxies over the last ≈10 Gyr |
| Q59944271 | The growth of typical star-forming galaxies and their supermassive black holes across cosmic time sincez∼ 2 |
| Q114822841 | The resolved chemical abundance properties within the interstellar medium of star-forming galaxies at z≈ 1.5 |
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