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541
Investigating the Unification of LOFAR-detected powerful AGN in the Boötes Field
Published 2017“…We identify 60 radio sources with powers P > 10<sup>25.5</sup> W Hz<sup>−1,</sup> at 150 MHz using cross-matched multiwavelength information from the AGN and Galaxy Evolution Survey, which provides spectroscopic redshifts and photometric identification of 16 quasars and 44 radio galaxies. …”
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542
The XXL Survey: XLII. Detection and characterisation of the galaxy population of distant galaxy clusters in the XXL-N/VIDEO field: A tale of variety
Published 2020“…Distant galaxy clusters provide an effective laboratory in which to study galaxy evolution in dense environments and at early cosmic times. …”
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543
Identifying merging galaxies in MaNGA using H-α and Hi observations
Published 2022“…Reliable methods that could recognise and distinguish galactic mergers are important for better understanding of galaxy evolution. This paper explores the feasibility of using observations on Hα and HI as a method to identify mergers. …”
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544
The Missing Symbiotic Stars: A Joint Analysis with Gaia, GALEX, and XMM-Newton Data
Published 2024-01-01“…In this work, we present an investigation on SySts candidates consisting of asymptotic giant branch stars (AGBs) by cross-correlating the Gaia DR3, the Galaxy Evolution Explorer All-Sky Imaging Survey, and the 4XMM DR13 catalogs. …”
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545
Empirical Temperature- and Extinction-dependent Extinction Coefficients for the GALEX, Pan-STARRS 1, Gaia, SDSS, 2MASS, and WISE Passbands
Published 2022-01-01“…We have obtained accurate dust reddening from the far-ultraviolet to the mid-infrared for up to 5 million stars by the star-pair algorithm based on LAMOST stellar parameters along with Galaxy Evolution Explorer, Pan-STARRS 1, Gaia, Sloan Digital Sky Survey, Two Micron All Sky Survey, and Wide-field Infrared Survey Explorer photometric data. …”
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546
The missing satellite problem in 3D
Published 2017“…This result highlights the continued need for improvement in understanding the fundamental physics that governs satellite galaxy evolution.…”
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547
Galaxy Merger Candidates in High-redshift Cluster Environments
Published 2017“…Key words: galaxies: clusters: general – galaxies: evolution – galaxies: high-redshift – galaxies: interactions…”
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548
Automated distant galaxy merger classifications from Space Telescope images using the Illustris simulation
Published 2021“…By blending large surveys and large simulations, such machine learning techniques offer a promising opportunity to teach us the strengths and weaknesses of inferences about galaxy evolution.…”
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549
Automated distant galaxy merger classifications from Space Telescope images using the Illustris simulation
Published 2022“…By blending large surveys and large simulations, such machine learning techniques offer a promising opportunity to teach us the strengths and weaknesses of inferences about galaxy evolution.…”
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550
The jet/wind outflow in Centaurus A: a local laboratory for AGN feedback
Published 2021“…Thus, our observational overview of Centaurus A reveals a number of features proposed to be associated with active galactic nucleus feedback mechanisms, often cited as likely to have significant effects in galaxy evolution models. As one of the closest galaxies to us, Centaurus A therefore provides a unique laboratory to examine feedback mechanisms in detail.…”
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551
A journey from the outskirts to the cores of groups I: Color- and mass-segregation in 20K-zCOSMOS groups
Published 2012“…In poorer groups the environmental effects are caught in action superimposed to secular galaxy evolution. Their member galaxies display increasing blue fractions when moving from the group center to more external regions, presumably reflecting the recent accretion history of these groups.…”
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552
The environments of radio-loud AGN from the LOFAR Two-Metre Sky Survey (LoTSS)
Published 2019“…<p>An understanding of the relationship between radio-loud active galaxies and their large-scale environments is essential for realistic modelling of radio-galaxy evolution and environmental impact, for understanding AGN triggering and life cycles, and for calibrating galaxy feedback in cosmological models. …”
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553
The evolution of gas-phase metallicity and resolved abundances in star-forming galaxies at z ≈ 0.6 – 1.8
Published 2020“…The metallicity gradient of a galaxy is independent of its rest-frame optical morphology, whilst correlating with its stellar mass and specific star-formation rate, in agreement with an inside-out model of galaxy evolution, as well as its rotation dominance. We quantify the evolution of metallicity gradients, comparing the distribution of ΔZ/ΔR in our sample with numerical simulations and observations at z ≈ 0 – 3. …”
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554
The SAURON project - XVIII. The integrated UV-line-strength relations of early-type galaxies
Published 2011“…Using far-ultraviolet (FUV) and near-ultraviolet (NUV) photometry from guest investigator programmes on the Galaxy Evolution Explorer (GALEX) satellite, optical photometry from the MDM Observatory and optical integral-field spectroscopy from SAURON, we explore the UV-line-strength relations of the 48 nearby early-type galaxies in the SAURON sample. …”
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555
The cosmos2015 catalog: exploring the 1
Published 2016“…Including new images from the UltraVISTA-DR2 survey, Y-band images from Subaru/Hyper-Suprime-Cam, and infrared data from the Spitzer Large Area Survey with the Hyper-Suprime-Cam Spitzer legacy program, this near-infrared-selected catalog is highly optimized for the study of galaxy evolution and environments in the early universe. …”
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556
MIGHTEE: total intensity radio continuum imaging and the COSMOS/XMM-LSS Early Science fields
Published 2021“…MIGHTEE is a galaxy evolution survey using siltaneous radio continuum, spectropolarimetry, and spectral line observations from the South African MeerKAT telescope. …”
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557
WISDOM project – XVIII. Molecular gas distributions and kinematics of three megamaser galaxies
Published 2023“…The co-evolution of galaxies and supermassive black holes (SMBHs) underpins our understanding of galaxy evolution, but different methods to measure SMBH masses have only infrequently been cross-checked. …”
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558
Dry Mergers in GEMS: The Dynamical Evolution of Massive Early-Type Galaxies
Published 2005“…We have used the 28'x 28' HST image mosaic from the GEMS (Galaxy Evolution from Morphology and SEDs) survey in conjunction with the COMBO-17 photometric redshift survey to constrain the incidence of major mergers between spheroid-dominated galaxies with little cold gas (dry mergers) since z = 0.7. …”
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559
Far-infrared line spectra of active galaxies from the Herschel/PACS spectrometer: The complete database
Published 2016“…The diagnostic power of mid- to far-infrared spectroscopy shown here for local galaxies will be of crucial importance to study galaxy evolution during the dust-obscured phase at the peak of the star formation and black hole accretion activity (1 < z < 4). …”
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560
LOFAR discovery of a 700-kpc remnant radio galaxy at low redshift
Published 2015“…Remnant radio galaxies represent the final dying phase of radio galaxy evolution in which the jets are no longer active. …”
Journal article