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De re metallica: the cosmic chemical evolution of galaxies
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February 2019 |
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Giant Lyα nebulae in the high redshift (z⩾2) Universe
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February 2007 |
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Cold streams in early massive hot haloes as the main mode of galaxy formation
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January 2009 |
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A cosmic web filament revealed in Lyman-α emission around a luminous high-redshift quasar
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Array programming with NumPy
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September 2020 |
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Kinematically quiet haloes around z 2.5 radio galaxies. Keck spectroscopy
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Astropy: A community Python package for astronomy
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The VIMOS VLT Deep Survey final data release: a spectroscopic sample of 35 016 galaxies and AGN out to z ~ 6.7 selected with 17.5 ≤ i AB ≤ 24.75
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October 2013 |
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Planck 2018 results: VI. Cosmological parameters
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September 2020 |
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Three Lyman- α -emitting filaments converging to a massive galaxy group at z = 2.91: discussing the case for cold gas infall
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May 2021 |
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A search for dust and molecular gas in enormous Ly α nebulae at z ≈ 2
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December 2020 |
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A MUltiwavelength Study of ELAN Environments (AMUSE 2 ): Ubiquitous dusty star-forming galaxies associated with enormous Ly α nebulae on megaparsec scales
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February 2022 |
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Secondary standard stars for absolute spectrophotometry
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The FIRST Survey: Faint Images of the Radio Sky at Twenty Centimeters
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Spatially Resolved High-Ionization Nebulae in a High-Redshift Radio Galaxy: Evidence for Shock Ionization and Photoionization
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Spectroscopic Target Selection in the Sloan Digital Sky Survey: The Main Galaxy Sample
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The Sloan Digital Sky Survey Quasar Survey: Quasar Luminosity Function from Data Release 3
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Black Hole Masses and Eddington Ratios at 0.3 < z < 4
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Exploring the Optical Transient Sky with the Palomar Transient Factory
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The Palomar Transient Factory: System Overview, Performance, and First Results
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Publications of the Astronomical Society of the Pacific, Vol. 121, Issue 886
https://doi.org/10.1086/648598
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December 2009 |
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Photometric Response Functions of the Sloan Digital sky Survey Imager
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March 2010 |
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The Wide-Field Infrared Survey Explorer (Wise): Mission Description and Initial On-Orbit Performance
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Spectral Classification and Redshift Measurement for the Sdss-Iii Baryon Oscillation Spectroscopic Survey
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The Multi-Object, Fiber-Fed Spectrographs for the Sloan Digital sky Survey and the Baryon Oscillation Spectroscopic Survey
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Lyα COOLING EMISSION FROM GALAXY FORMATION
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The Prism Multi-Object Survey (Primus). i. Survey Overview and Characteristics
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A SUCCESSFUL BROADBAND SURVEY FOR GIANT Lyα NEBULAE. I. SURVEY DESIGN AND CANDIDATE SELECTION
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A SUCCESSFUL BROADBAND SURVEY FOR GIANT Lyα NEBULAE. II. SPECTROSCOPIC CONFIRMATION
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The Prism Multi-Object Survey (Primus). ii. data Reduction and Redshift Fitting
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SPATIALLY RESOLVED GAS KINEMATICS WITHIN A Lyα NEBULA: EVIDENCE FOR LARGE-SCALE ROTATION
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January 2015 |
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DEEP HE ii AND C iv SPECTROSCOPY OF A GIANT LY α NEBULA: DENSE COMPACT GAS CLUMPS IN THE CIRCUMGALACTIC MEDIUM OF A z ∼ 2 QUASAR
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August 2015 |
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3D-HST: A WIDE-FIELD GRISM SPECTROSCOPIC SURVEY WITH THE HUBBLE SPACE TELESCOPE
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The Sdss-Iv Extended Baryon Oscillation Spectroscopic Survey: Quasar Target Selection
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December 2015 |
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FILAMENTARY LARGE-SCALE STRUCTURE TRACED BY SIX Lyα BLOBS AT z = 2.3
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The maximum accretion rate of hot gas in dark matter haloes
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January 2020 |
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Revealing the impact of quasar luminosity on giant Ly α nebulae
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October 2020 |
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MUSE analysis of gas around galaxies (MAGG) – III. The gas and galaxy environment of z = 3–4.5 quasars
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March 2021 |
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Subaru Hyper Suprime-Cam excavates colossal over- and underdense structures over 360 deg2 out to z = 1
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March 2021 |
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An early phase of environmental effects on galaxy properties unveiled by near-infrared spectroscopy of protocluster galaxies at z > 2
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February 2015 |
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MUSE searches for galaxies near very metal-poor gas clouds at z ∼ 3: new constraints for cold accretion models
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July 2016 |
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Ionization and feedback in Lyα haloes around two radio galaxies at z ∼ 2.5
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November 2016 |
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The cosmic baryon cycle and galaxy mass assembly in the FIRE simulations
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June 2017 |
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Inspiraling halo accretion mapped in Ly α emission around a z ∼ 3 quasar
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September 2017 |
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The uniformity and time-invariance of the intra-cluster metal distribution in galaxy clusters from the IllustrisTNG simulations
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November 2017 |
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The MUSE 3D view of feedback in a high-metallicity radio galaxy at z = 2.9
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November 2017 |
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Galaxy And Mass Assembly: the G02 field, Herschel–ATLAS target selection and data release 3
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November 2017 |
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The detection of intergalactic H α emission from the Slug Nebula at z ∼ 2.3
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July 2018 |
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MAHALO Deep Cluster Survey II. Characterizing massive forming galaxies in the Spiderweb protocluster at z = 2.2
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September 2018 |
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QSO MUSEUM I: a sample of 61 extended Ly α-emission nebulae surrounding z ∼ 3 quasars
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October 2018 |
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Zooming in on accretion – II. Cold circumgalactic gas simulated with a super-Lagrangian refinement scheme
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December 2018 |
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The large- and small-scale properties of the intergalactic gas in the Slug Ly α nebula revealed by MUSE He ii emission observations
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December 2018 |
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Gas accretion and galactic fountain flows in the Auriga cosmological simulations: angular momentum and metal redistribution
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October 2019 |
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Where’s Swimmy?: Mining unique color features buried in galaxies by deep anomaly detection using Subaru Hyper Suprime-Cam data
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November 2021 |
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Third data release of the Hyper Suprime-Cam Subaru Strategic Program
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February 2022 |
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An optically-selected cluster catalog at redshift 0.1 < z < 1.1 from the Hyper Suprime-Cam Subaru Strategic Program S16A data
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June 2017 |
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The bright-star masks for the HSC-SSP survey
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July 2017 |
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Hyper Suprime-Cam: System design and verification of image quality
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September 2017 |
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The Hyper Suprime-Cam SSP Survey: Overview and survey design
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September 2017 |
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Hyper Suprime-Cam: Camera dewar design
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September 2017 |
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The on-site quality-assurance system for Hyper Suprime-Cam: OSQAH†
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September 2017 |
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The Hyper Suprime-Cam software pipeline
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October 2017 |
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Great Optically Luminous Dropout Research Using Subaru HSC (GOLDRUSH). I. UV luminosity functions at z ∼ 4–7 derived with the half-million dropouts on the 100 deg2 sky†
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November 2017 |
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Hyper Suprime-Cam: Filters
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June 2018 |
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Lyα view around a z = 2.84 hyperluminous QSO at a node of the cosmic web†
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Matplotlib: A 2D Graphics Environment
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The cosmological evolution of quasar black hole masses
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How do galaxies get their gas?
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Galaxy And Mass Assembly (GAMA): the input catalogue and star-galaxy separation
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Gravity-driven Lyα blobs from cold streams into galaxies: Cold streams as Lyα blobs
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June 2010 |
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Galaxy evolution in cosmological simulations with outflows - II. Metallicities and gas fractions: Galaxy evolution in simulations - II
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The MUSE second-generation VLT instrument
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The Keck Cosmic Web Imager: a capable new integral field spectrograph for the W. M. Keck Observatory
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Quasar quartet embedded in giant nebula reveals rare massive structure in distant universe
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Molecular gas in the halo fuels the growth of a massive cluster galaxy at high redshift
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Gas filaments of the cosmic web located around active galaxies in a protocluster
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SUBARU HIGH- z EXPLORATION OF LOW-LUMINOSITY QUASARS (SHELLQs). I. DISCOVERY OF 15 QUASARS AND BRIGHT GALAXIES AT 5.7 < z < 6.9
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THE STACKED LY α EMISSION PROFILE FROM THE CIRCUM-GALACTIC MEDIUM OF z ∼ 2 QUASARS
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A GIANT LY α NEBULA IN THE CORE OF AN X-RAY CLUSTER AT Z = 1.99: IMPLICATIONS FOR EARLY ENERGY INJECTION
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UBIQUITOUS GIANT Ly α NEBULAE AROUND THE BRIGHTEST QUASARS AT z ∼ 3.5 REVEALED WITH MUSE
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October 2016 |
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THE 3D-HST SURVEY: HUBBLE SPACE TELESCOPE WFC3/G141 GRISM SPECTRA, REDSHIFTS, AND EMISSION LINE MEASUREMENTS FOR ∼100,000 GALAXIES
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Sloan Digital Sky Survey IV: Mapping the Milky Way, Nearby Galaxies, and the Distant Universe
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Discovery of an Enormous Ly α Nebula in a Massive Galaxy Overdensity at z = 2.3
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The DEIMOS 10K Spectroscopic Survey Catalog of the COSMOS Field
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Momentum-driven Winds from Radiatively Efficient Black Hole Accretion and Their Impact on Galaxies
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LSST: From Science Drivers to Reference Design and Anticipated Data Products
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Ly α Halos around z ∼ 6 Quasars
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The Cold Circumgalactic Environment of MAMMOTH-I: Dynamically Cold Gas in the Core of an Enormous Ly α Nebula
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The REQUIEM Survey. I. A Search for Extended Ly α Nebular Emission Around 31 z > 5.7 Quasars
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Metal Enrichment in the Circumgalactic Medium and Ly α Halos around Quasars at z ∼ 3
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Extremely Metal-poor Representatives Explored by the Subaru Survey (EMPRESS). I. A Successful Machine-learning Selection of Metal-poor Galaxies and the Discovery of a Galaxy with M * < 10 6 M ⊙ and 0.016 Z ⊙
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The Origin and Evolution of Lyα Blobs in Cosmological Galaxy Formation Simulations
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A Multiwavelength Study of ELAN Environments (AMUSE 2 ). Detection of a Dusty Star-forming Galaxy within the Enormous Lyα Nebula at z=2.3 Sheds Light on its Origin
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Mapping the Morphology and Kinematics of a Lyα-selected Nebula at z = 3.15 with MUSE
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A Multiwavelength Study of ELAN Environments (AMUSE 2 ). Mass Budget, Satellites Spin Alignment, and Gas Infall in a Massive z ∼ 3 Quasar Host Halo
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The Fifteenth Data Release of the Sloan Digital Sky Surveys: First Release of MaNGA-derived Quantities, Data Visualization Tools, and Stellar Library
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Evolution of the Cool Gas in the Circumgalactic Medium of Massive Halos: A Keck Cosmic Web Imager Survey of Ly α Emission around QSOs at z ≈ 2
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The Sloan Digital Sky Survey Quasar Catalog: Sixteenth Data Release
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Keck/Palomar Cosmic Web Imagers Reveal an Enormous Ly α Nebula in an Extremely Overdense Quasi-stellar Object Pair Field at z = 2.45
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Massive Molecular Outflow and 100 kpc Extended Cold Halo Gas in the Enormous Lyα Nebula of QSO 1228+3128
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Evidence for Cold-stream to Hot-accretion Transition as Traced by Lyα Emission from Groups and Clusters at 2 < z < 3.3
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