| Q58913312 | A transient search using combined human and machine classifications |
| Q58909017 | AGN Host Galaxies atz ~ 0.4-1.3: Bulge-dominated and Lacking Merger-AGN Connection |
| Q58908903 | Active galactic nucleus host galaxy morphologies in COSMOS |
| Q56005255 | An over-massive black hole in a typical star-forming galaxy, 2 billion years after the Big Bang |
| Q56687040 | Assessing data quality in citizen science |
| Q84348065 | Assessing data quality in citizen science (preprint) |
| Q58908589 | Bolometric luminosities and Eddington ratios of X-ray selected active galactic nuclei in theXMM-COSMOS survey |
| Q102154161 | Camera settings and biome influence the accuracy of citizen science approaches to camera trap image classification |
| Q57310932 | Chandra observations of galaxy zoo mergers: frequency of binary active nuclei in massive mergers |
| Q58913342 | Defining and Measuring Success in Online Citizen Science: A Case Study of Zooniverse Projects |
| Q58786585 | Do moderate-luminosity active galactic nuclei suppress star formation? |
| Q58913297 | Doing Good Online: The Changing Relationships Between Motivations, Activity, and Retention Among Online Volunteers |
| Q58245920 | Erratum: Misalignment between cold gas and stellar components in early-type galaxies |
| Q73183939 | Everyone counts? Design considerations in online citizen science |
| Q58908042 | Evidence for Merger-driven Growth in Luminous, High-z, Obscured AGNs in the CANDELS/COSMOS Field |
| Q58786378 | Evidence for three accreting black holes in a galaxy at z ~ 1.35: a snapshot of recently formed black hole seeds? |
| Q68344320 | Evolution of structural parameters of galaxies in the GOODS-south field |
| Q55979406 | Exposing the Science in Citizen Science: Fitness to Purpose and Intentional Design |
| Q58913326 | Faint COSMOS AGNs at z~3.3. I. Black hole properties and constraints on early black hole growth |
| Q114375759 | Galaxy And Mass Assembly: Galaxy Zoo spiral arms and star formation rates |
| Q56882483 | Galaxy Zoo 2: detailed morphological classifications for 304 122 galaxies from the Sloan Digital Sky Survey |
| Q114363216 | Galaxy Zoo Builder: Four-component Photometric Decomposition of Spiral Galaxies Guided by Citizen Science |
| Q108871463 | Galaxy Zoo DECaLS: Detailed visual morphology measurements from volunteers and Deep Learning for 314,000 galaxies |
| Q57310926 | Galaxy Zoo and ALFALFA: atomic gas and the regulation of star formation in barred disc galaxies |
| Q58229824 | Galaxy Zoo and sparcfire: constraints on spiral arm formation mechanisms from spiral arm number and pitch angles |
| Q114375776 | Galaxy Zoo: 3D – crowdsourced bar, spiral, and foreground star masks for MaNGA target galaxies |
| Q58831058 | Galaxy Zoo: Are bars responsible for the feeding of active galactic nuclei at 0.2 < z < 1.0? |
| Q56269200 | Galaxy Zoo: CANDELS barred discs and bar fractions |
| Q114363213 | Galaxy Zoo: Clump Scout: Surveying the Local Universe for Giant Star-forming Clumps |
| Q57797026 | Galaxy Zoo: Major Galaxy Mergers Are Not a Significant Quenching Pathway |
| Q58229807 | Galaxy Zoo: Morphological Classification of Galaxy Images from the Illustris Simulation |
| Q57310901 | Galaxy Zoo: an independent look at the evolution of the bar fraction over the last eight billion years from HST-COSMOS★ |
| Q57310928 | Galaxy Zoo: bulgeless galaxies with growing black holes |
| Q58229917 | Galaxy Zoo: comparing the demographics of spiral arm number and a new method for correcting redshift bias |
| Q58229799 | Galaxy Zoo: constraining the origin of spiral arms |
| Q58245916 | Galaxy Zoo: evidence for diverse star formation histories through the green valley |
| Q58220718 | Galaxy Zoo: evidence for rapid, recent quenching within a population of AGN host galaxies |
| Q58229863 | Galaxy Zoo: finding offset discs and bars in SDSS galaxies★ |
| Q57310903 | Galaxy Zoo: morphological classifications for 120 000 galaxies in HST legacy imaging |
| Q84348064 | Galaxy Zoo: probabilistic morphology through Bayesian CNNs and active learning |
| Q57310904 | Galaxy Zoo: quantitative visual morphological classifications for 48 000 galaxies from CANDELS |
| Q58229810 | Galaxy Zoo: secular evolution of barred galaxies from structural decomposition of multiband images |
| Q58220734 | Galaxy Zoo: the dependence of the star formation–stellar mass relation on spiral disc morphology |
| Q58913338 | Galaxy Zoo: the effect of bar-driven fuelling on the presence of an active galactic nucleus in disc galaxies |
| Q58229866 | Galaxy Zoo: the interplay of quenching mechanisms in the group environment |
| Q114375785 | Galaxy zoo builder: Morphological dependence of spiral galaxy pitch angle |
| Q114375781 | Galaxy zoo: stronger bars facilitate quenching in star-forming galaxies |
| Q114819579 | Gems of the Galaxy Zoos—A Wide-ranging Hubble Space Telescope Gap-filler Program* |
| Q58913301 | Getting Connected: An Empirical Investigation of the Relationship Between Social Capital and Philanthropy Among Online Volunteers |
| Q58786449 | HST WFC3/IR observations of active galactic nucleus host galaxies at z ~ 2: supermassive black holes grow in disk galaxies |
| Q58786318 | Heavily obscured quasar host galaxies at are discs, not major mergers★ |
| Q68346040 | Host galaxy morphologies in the GOODS-south HST ACS images |
| Q58229796 | Integrating human and machine intelligence in galaxy morphology classification tasks |
| Q114363215 | Investigating Clumpy Galaxies in the Sloan Digital Sky Survey Stripe 82 Using the Galaxy Zoo |
| Q58786309 | Major galaxy mergers only trigger the most luminous active galactic nuclei |
| Q58913334 | Major mergers host the most-luminous red quasars at z ~ 2: a Hubble Space Telescope WFC3/IR study |
| Q58913309 | Major merging history in CANDELS. I. Evolution of the incidence of massive galaxy–galaxy pairs from z = 3 to z ∼ 0 |
| Q58220736 | Misalignment between cold gas and stellar components in early-type galaxies |
| Q58913350 | Moderate-luminosity growing black holes from 1.25 < z < 2.7: varied accretion in disk-dominated hosts |
| Q58913322 | Morphology and the color-mass diagram as clues to galaxy evolution at z~1 |
| Q58245938 | Morphology in the era of large surveys |
| Q58786439 | Obscured GOODS active galactic nuclei and their host galaxies at z < 1.25: the slow black hole growth phase |
| Q68641621 | Optical properties of all the X-ray sources within the GOODS HST/ACS survey of the Chandra deep field south |
| Q58795250 | Playing with science |
| Q110634700 | Quantifying the poor purity and completeness of morphological samples selected by galaxy colour |
| Q58913316 | Radio Galaxy Zoo: A Search for Hybrid Morphology Radio Galaxies |
| Q24577176 | Radio Galaxy Zoo: host galaxies and radio morphologies derived from visual inspection |
| Q62615653 | SNITCH: seeking a simple, informative star formation history inference tool |
| Q58913329 | Science learning via participation in online citizen science |
| Q110630495 | Secularly powered outflows from AGNs: the dominance of non-merger driven supermassive black hole growth |
| Q58229945 | Stellar populations of barred quiescent galaxies |
| Q56019894 | Supermassive black holes in disc-dominated galaxies outgrow their bulges and co-evolve with their host galaxies |
| Q58913356 | The Accuracy of Morphological Decomposition of Active Galactic Nucleus Host Galaxies |
| Q56603826 | The First Post-Kepler Brightness Dips of KIC 8462852 |
| Q49185175 | The K2-138 System: A Near-resonant Chain of Five Sub-Neptune Planets Discovered by Citizen Scientists |
| Q58913345 | The Multiwavelength AGN Population and the X-ray Background |
| Q56882494 | The green valley is a red herring: Galaxy Zoo reveals two evolutionary pathways towards quenching of star formation in early- and late-type galaxies★ |