Michael Brown

Publications

• Galaxy And Mass Assembly (GAMA): z ~ 0 galaxy luminosity function down to L ~ 106 L⊙ via clustering based redshift inference
• Deep ASKAP EMU Survey of the GAMA23 field: properties of radio sources
• The XXL Survey
• The causes of the red sequence, the blue cloud, the green valley, and the green mountain
• Multiple mechanisms quench passive spiral galaxies
• The XXL Survey
• Connecting MeerKAT Radio Continuum Properties to GAMA Optical Emission-line and WISE Mid-infrared Activity
• The XXL Survey
• Galaxy And Mass Assembly (GAMA)
• A search for missing radio sources at z ≳ 4 using Lyman dropouts
• Self-supervised clustering on image-subtracted data with deep-embedded self-organizing map
• Deep Extragalactic VIsible Legacy Survey (DEVILS): identification of AGN through SED fitting and the evolution of the bolometric AGN luminosity function
• Deep investigation of neutral gas origins (DINGO): H i stacking experiments with early science data
• Erratum: “Calibrating Star Formation in WISE Using Total Infrared Luminosity” (2017, ApJ, 850, 68)
• Relationships between Hi Gas Mass, Stellar Mass, and the Star Formation Rate of HICAT+WISE (H i-WISE) Galaxies
• The Ultraviolet–Infrared Color–Magnitude Relation of Star-forming Galaxies
• Calibrating the James Webb Space Telescope Filters as Star Formation Rate Indicators
• The XXL Survey
• The XXL Survey
• The XXL Survey
• Galaxy and Mass Assembly (GAMA): The environmental dependence of the galaxy main sequence
• Photometric redshifts for the Kilo-Degree Survey
• H i galaxies with little star formation: an abundance of LIERs
• Evolution of the Stellar Mass Function and Infrared Luminosity Function of Galaxies since z = 1.2
• The 1.4-GHz cosmic star formation history at z < 1.3
• Galaxy And Mass Assembly (GAMA)
• Deep Extragalactic VIsible Legacy Survey (DEVILS)
• Galaxy And Mass Assembly (GAMA)
• Galaxy and Mass Assembly (GAMA)
• Group quenching and galactic conformity at low redshift
• Photometric redshifts for the next generation of deep radio continuum surveys - I. template fitting
• Galaxy And Mass Assembly
• The Nearby “Changing Look” Seyfert NGC 1346
• Luminous red galaxies in the Kilo-Degree Survey: selection with broad-band photometry and weak lensing measurements
• Star-forming, rotating spheroidal galaxies in the GAMA and SAMI surveys
• The spectral energy distributions of active galactic nuclei
• Effect of galaxy mergers on star-formation rates
• Galaxy And Mass Assembly (GAMA): properties and evolution of red spiral galaxies
• The WISE Extended Source Catalog (WXSC). I. The 100 Largest Galaxies
• Galaxy And Mass Assembly (GAMA): Defining passive galaxy samples and searching for the UV upturn
• Tully–Fisher Distances for Southern Galaxies with HIPASS and WISE
• The spectral energy distributions of active galactic nuclei
• Galaxy and mass assembly: luminosity and stellar mass functions in GAMA groups
• The Chandra Deep Wide-field Survey: A New Chandra Legacy Survey in the Boötes Field. I. X-Ray Point Source Catalog, Number Counts, and Multiwavelength Counterparts
• Galaxy and Mass Assembly: A Comparison between Galaxy–Galaxy Lens Searches in KiDS/GAMA
• Measuring the total infrared light from galaxy clusters at z = 0.5–1.6: connecting stellar populations to dusty star formation
• Galaxy and Mass Assembly (GAMA): A WISE Study of the Activity of Emission-line Systems in G23
• GAMA/XXL: X-ray point sources in low-luminosity galaxies in the GAMA G02/XXL-N field
• A systematic survey for z< 0.04 CLAGNs
• The LOFAR Two-meter Sky Survey: Deep Fields Data Release 1
• A connection between obscuration and star formation in luminous quasars
• GAMA/WiggleZ: The 1.4 GHz radio luminosity functions of high- and low-excitation radio galaxies and their redshift evolution to z = 0.75
• Galaxy and mass assembly (GAMA): End of survey report and data release 2
• Galaxy And Mass Assembly (GAMA) blended spectra catalogue: Strong galaxy-galaxy lens and occulting galaxy pair candidates
• AN ATLAS OF GALAXY SPECTRAL ENERGY DISTRIBUTIONS FROM THE ULTRAVIOLET TO THE MID-INFRARED
• The rarity of star formation in brightest cluster galaxies as measured by WISE
• Galaxy and Mass Assembly (GAMA): fine filaments of galaxies detected within voids
• Galaxy And Mass Assembly (GAMA): ugrizYJHK Sersic luminosity functions and the cosmic spectral energy distribution by Hubble type
• Galaxy And Mass Assembly (GAMA): galaxy close pairs, mergers and the future fate of stellar mass
• GALAXY AND MASS ASSEMBLY (GAMA): MID-INFRARED PROPERTIES AND EMPIRICAL RELATIONS FROM WISE
• Galaxy And Mass Assembly (GAMA): deconstructing bimodality - I. Red ones and blue ones
• THE INFLUENCE OF RED SPIRAL GALAXIES ON THE SHAPE OF THE LOCAL K -BAND LUMINOSITY FUNCTION
• An accurate new method of calculating absolute magnitudes and K-corrections applied to the sloan filter set
• A UV to mid-IR study of AGN selection
• Galaxy And Mass Assembly (GAMA): The effect of close interactions on star formation in galaxies
• Galaxy and mass assembly (GAMA): Trends in galaxy colours, morphology, and stellar populations with large-scale structure, group, and pair environments
• Galaxy and Mass assembly (GAMA): Maximum-likelihood determination of the luminosity function and its evolution
• A photometrically and spectroscopically confirmed population of passive spiral galaxies
• Galaxy And Mass Assembly (GAMA): Stellar mass growth of spiral galaxies in the cosmic web
• The stellar-to-halo mass relation of GAMA galaxies from 100 deg2 of KiDS weak lensing data
• Galaxy And Mass Assembly (GAMA): The 325 MHz radio luminosity function of AGN and star-forming galaxies
• The masses of satellites in GAMA galaxy groups from 100 square degrees of KiDS weak lensing data
• GAMA/H-ATLAS: Common star formation rate indicators and their dependence on galaxy physical parameters
• GAMA/H-ATLAS: A meta-analysis of SFR indicators - comprehensive measures of the SFR-M* relation and cosmic star formation history at z < 0.4
• Galaxy And Mass Assembly (GAMA): Understanding the wavelength dependence of galaxy structure with bulge-disc decompositions
• Galaxy And Mass Assembly (GAMA): Bivariate functions of Hα star-forming galaxies
• Galaxy and mass assembly (GAMA): Panchromatic data release (far-UV-far-IR) and the low-z energy budget
• Galaxy And Mass Assembly: Accurate panchromatic photometry from optical priors using LAMBDAR
• Galaxy And Mass Assembly (GAMA): Stellar mass functions by Hubble type
• The many assembly histories of massive void galaxies as revealed by integral field spectroscopy
• A NEW STAR FORMATION RATE CALIBRATION from POLYCYCLIC AROMATIC HYDROCARBON EMISSION FEATURES AND APPLICATION TO HIGH-REDSHIFT GALAXIES
• Galaxy And Mass Assembly (GAMA): Growing up in a bad neighbourhood - how do low-mass galaxies become passive?
• The z < 1.2 optical luminosity function from a sample of ∼410,000 galaxies in Boötes
• Calibration of Ultraviolet, Mid-infrared, and Radio Star Formation Rate Indicators
• WISE × SuperCOSMOS PHOTOMETRIC REDSHIFT CATALOG: 20 MILLION GALAXIES OVER 3 π STERADIANS
• Galaxy and Mass Assembly (GAMA): Exploring the WISE Web in G12
• The X-Ray and Mid-infrared Luminosities in Luminous Type 1 Quasars
• Galaxy And Mass Assembly (GAMA): A “No Smoking” Zone for Giant Elliptical Galaxies?
• Calibrating Star Formation in WISE Using Total Infrared Luminosity
• The Taipan Galaxy Survey: Scientific Goals and Observing Strategy
• Galaxy And Mass Assembly (GAMA)
• Galaxy And Mass Assembly (GAMA)
• Updated 34-band Photometry for the SINGS/KINGFISH Samples of Nearby Galaxies
• Galaxy and mass assembly (GAMA)
• Galaxy and Mass Assembly (GAMA)
• Galaxy and mass assembly (GAMA)
• Near-ultraviolet signatures of environment-driven galaxy quenching in Sloan Digital Sky Survey groups
• Galaxy and Mass Assembly (GAMA)
• Galaxy And Mass Assembly
• Welcome to the Twilight Zone
• TIDAL INTERACTIONS AT THE EDGE OF THE LOCAL GROUP: NEW EVIDENCE FOR TIDAL FEATURES IN THE ANTLIA DWARF GALAXY
• The halo occupation distribution of H i from 21-cm intensity mapping at moderate redshifts
• EMU: Evolutionary map of the universe
• Galaxy And Mass Assembly (GAMA): The 0.013 < z < 0.1 cosmic spectral energy distribution from 0.1 μm to 1 mm
• Infrared spectroscopy of nearby radio active elliptical galaxies
• Galaxy And Mass Assembly (GAMA): Galaxy environments and star formation rate variations
• Herschel detection of dust emission from UV-luminous star-forming galaxies at 3.3 ≲ z ≲ 4.3
• The cluster and field galaxy active galactic nucleus fraction at Z = 1-1.5: Evidence for a reversal of the local anticorrelation between environment and agn fraction
• Galaxy and mass assembly (GAMA): The wavelength-dependent sizes and profiles of galaxies revealed by megamorph
• Galaxy spectra from the UV to the mid-IR
• THE CLUSTERING OF EXTREMELY RED OBJECTS
• Recalibrating the Wide-field Infrared Survey Explorer (WISE) W4 Filter
• GALAXY AND MASS ASSEMBLY (GAMA): WITNESSING THE ASSEMBLY OF THE CLUSTER ABELL 1882
• Galaxy and mass assembly (GAMA): The large-scale structure of galaxies and comparison to mock universes
• Galaxy And Mass Assembly (GAMA): Linking star formation histories and stellar mass growth
• Discussion of Boretti, A., 'Is there any support in the long term tide gauge data to the claims that parts of Sydney will be swamped by rising sea levels?', Coastal Engineering, 64, 161-167, June 2012
• Two-phase galaxy evolution: The cosmic star formation histories of spheroids and discs
• The era of star formation in galaxy clusters
• The clustering of galaxies around radio-loud active galactic nuclei
• Mid-infrared selection of active galactic nuclei with the wide-field infrared survey explorer. II. Properties of wise-selected active galactic nuclei in the NDWFS boötes field
• Galaxy and mass assembly: Evolution of the Hα luminosity function and star formation rate density up to z < 0.35
• Galaxy And Mass Assembly (GAMA): Spectroscopic analysis
• Galaxy and Mass Assembly (GAMA): Ugriz galaxy luminosity functions
• The average physical properties and star formation histories of the UV-brightest star-forming galaxies at z ∼ 3.7
• Galaxy and mass assembly (GAMA): The life and times of L* galaxies
• AGES: The AGN and galaxy evolution survey
• Galaxy And Mass Assembly (GAMA): Stellar mass estimates
• Clustering of obscured and unobscured quasars in the Boötes field: Placing rapidly growing black holes in the cosmic web
• A correlation between star formation rate and average black hole accretion in star-forming galaxies
• The star formation histories of z ∼ 2 dust-obscured galaxies and submillimeter-selected galaxies
• The galaxy optical luminosity function from the AGN and galaxy evolution survey
• Galaxy and Mass Assembly (GAMA): Survey diagnostics and core data release
• Galaxy And Mass Assembly (GAMA): In search of Milky Way Magellanic Cloud analogues
• Assembly of the red sequence in infrared-selected galaxy clusters from the irac shallow cluster survey
• The ubiquitous radio continuum emission from the most massive early-type galaxies
• The mid-IR-and X-ray-selected QSO luminosity function
• Hubble space telescope morphologies of z ∼ 2 dust-obscured galaxies. II. Bump sources
• Galaxy and Mass Assembly (GAMA): The red fraction and radial distribution of satellite galaxies
• Galaxy and Mass Assembly (GAMA): Galaxies at the faint end of the Hα luminosity function
• Ultracool field brown dwarf candidates selected at 4.5 μm
• The evolution of the star formation rate of galaxies at 0.0 ≤ z ≤ 1.2
• SDWFS-MT-1: A self-obscured luminous supernova at z ≃ 0.2
• Mid-infrared variability from the spitzer deep wide-field survey
• The clustering and halo masses of star-forming galaxies at z < 1
• The assembly histories of quiescent galaxies since z = 0.7 from absorption line spectroscopy
• Galaxy and mass assembly: The evolution of bias in the radio source population to z ~ 1.5
• The SKA Mid-frequency All-sky continuum survey: Discovering the unexpected and transforming radio-astronomy
• Galaxy and mass assembly (GAMA): The halo mass of galaxy groups from maximum-likelihood weak lensing
• Galaxy and Mass Assembly (GAMA): Refining the local galaxy merger rate using morphological information
• Star formation in luminous quasar host galaxies at z = 1-2
• XBootes: An X-ray survey of the NDWFS Bootes field. II. The X-ray source catalog
• XBootes: An X-ray survey of the NDWFS Bootes field. I. Overview and initial results
• The active galactic nuclei contribution to the mid-infrared emission of luminous infrared galaxies
• Host galaxies, clustering, Eddington ratios, and evolution of radio, X-ray, and infrared-selected AGNs
• Mid-infrared galaxy luminosity functions from the agn and galaxy evolution survey
• Clustering of dust-obscured galaxies at z ∼ 2
• Low-resolution spectral templates for galaxies from 0.2 to 10 μm
• Discovery of a large ∼200 kpc gaseous nebula at z ≈ 2.7 with the Spitzer Space Telescope
• Discovery of hyperluminous infrared galaxies using spitzer and sharc-II
• Evidence for merging or disruption of red galaxies from the evolution of their clustering
• The spitzer deep, wide-field survey
• Slow galaxy growth within rapidly growing dark matter halos
• The evolving luminosity function of red galaxies
• MIPS J142824.0+352619: A hyperluminous starburst galaxy at z = 1.325
• Clustering of the IR background light with spitzer: Contribution from resolved sources
• The cosmic evolution of active galactic nuclei in galaxy clusters
• Radio and infrared selected optically invisible sources in the boötes NDWFS
• The star formation and nuclear accretion histories of normal galaxies in the ages survey
• The slow growth of massive galaxies in rapidly growing dark matter halos
• The origin of the 24 μm excess in red galaxies
• Spitzer 70/160 μm observations of high-redshift ULIRGs and HyLIRGs in the Boötes field
• Radio-loud high-redshift protogalaxy candidates in botes
• Clusters of galaxies in the first half of the universe from the IRAC shallow survey
• Strong polycyclic aromatic hydrocarbon emission from z ≈ 2 ulirgs
• Hubble space telescope morphologies of z ∼ 2 dust obscured galaxies. I. Power-law sources
• Active galactic nuclei and the truncation of star formation in K+A galaxies
• The mid-infrared properties of X-ray sources
• Redshift distribution of extragalactic 24 μm sources
• Red galaxy growth and the halo occupation distribution
• The weak clustering of gas-rich galaxies
• The local galaxy 8 μm luminosity function
• An IR-selected galaxy cluster at z = 1.41
• A significant population of very luminous dust-obscured galaxies at redshift z ∼ 2
• Mid-infrared selection of brown dwarfs and high-redshift quasars
• Galaxy cluster correlation function to z ∼ 1.5 in the irac shallow cluster survey
• Optical line diagnostics of z ≈ 2 optically faint ultraluminous infrared galaxies in the Spitzer bootes survey
• The 1 < z < 5 infrared luminosity function of type I quasars
• Erratum: The 1 < z < 5 infrared luminosity function of type i quasars (Astrophysical Journal (2006) 638 (88))
• A large population of mid-infrared-selected, obscured active galaxies in the boötes field
• The flamingos extragalactic survey
• The discovery of three new z > 5 quasars in the AGN and Galaxy Evolution Survey
• The Chandra XBoötes survey. III. Optical and near-infrared counterparts
• Spitzer IRS spectra of optically faint infrared sources with weak spectral features
• Photometric redshifts in the IRAC shallow survey
• IRS spectra of two ultraluminous infrared galaxies at z = 1.3
• Tracing the nuclear accretion history of the red galaxy population
• The clustering of extragalactic extremely red objects
• Spitzer observations of optically "invisible" radio and X-ray sources: High-redshift active galactic nuclei
• Spectroscopic redshifts to z > 2 for optically obscured sources discovered with the spitzer space telescope
• Mid-infrared selection of active galaxies
• The motion and size sorting of particles ejected from a protostellar accretion disk.
• X-ray 3 dimensional survey in the NDWFS Bootes field: Large area Chandra shallow X-ray survey -I
• The 172 ks Chandra exposure of the LALA Bootes field: X-ray source catalog
• Infrared array camera (IRAC) shallow survey
• Spectroscopic confirmation of three redshift z ≈ 5.7 Lyα emitters from the Large-Area Lyman Alpha survey
• Red galaxy clustering in the NOAO deep wide-field survey
• Photometry and spectroscopy of GRB 030329 and its associated supernova 2003dh: The first two months
• GRB 011121: A massive star progenitor
• The evolution of radio galaxies at intermediate redshift
• The evolution and star formation of dwarf galaxies in the Fornax Cluster
• The clustering of AGNs and galaxies at intermediate redshift
• The clustering of colour-selected galaxies
• A wide-field CCD survey for Centaurs and Kuiper Belt objects
• A search for distant satellites of Neptune
• A search for bright Kuiper Belt objects
• Occultations by Kuiper belt objects
• Next Generation Wide-Field Multi-Object Spectroscopy
• Infrared spectroscopy of nearby radio active early-type galaxies - II: spectral atlas
• MACHO 311.37557.169: A VY Scl star
• Galaxy And Mass Assembly: The xSAGA Galaxy Complement in Nearby Galaxy Groups
• Galaxy And Mass Assembly: the xSAGA galaxy complement in nearby galaxy groups
• Radio continuum from the most massive early-type galaxies detected with ASKAP RACS
• WISE × SuperCOSMOS PHOTOMETRIC REDSHIFT CATALOG: 20 MILLION GALAXIES OVER 3π STERADIANS
• Evolution of the Stellar Mass Function and Infrared Luminosity Function of Galaxies since z = 1.2
• EMU/GAMA: Radio detected galaxies are more obscured than optically selected galaxies
• EMU/GAMA: A Technique for Detecting Active Galactic Nuclei in Low Mass Systems
• EMU/GAMA: A technique for detecting active galactic nuclei in low mass systems
• EMU/GAMA: Radio-detected galaxies are more obscured than optically selected galaxies
• AGNFITTER-RX: Modeling the radio-to-X-ray spectral energy distributions of AGNs
• The S4G-WISE View of Global Star Formation in the Nearby Universe