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Shocked POststarburst Galaxy Survey. IV. Outflows in Shocked Poststarburst Galaxies Are Not Responsible for Quenching
Published 2025-01-01Subjects: “…Galaxy evolution…”
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Properties of the Photometric Components of Lenticular Galaxies
Published 2012-01-01“…A unique opportunity for understanding the origin of S0 galaxies will shortly be forthcoming. This is due to the morphological classifications of large galaxy samples that have recently been published. …”
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Analysis of ∼106 Spiral Galaxies from Four Telescopes Shows Large-Scale Patterns of Asymmetry in Galaxy Spin Directions
Published 2022-01-01“…The profiles also agree when using automatic or manual annotation of the galaxies, showing very similar large-scale patterns. …”
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Dark Matter Halos of Luminous Active Galactic Nuclei from Galaxy–Galaxy Lensing with the HSC Subaru Strategic Program
Published 2024-01-01Subjects: “…Active galaxies…”
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Evidence for AGN Feedback in Galaxy Clusters and Groups
Published 2012-01-01“…Understanding the physics of the hot gas and its interplay with the relativistic plasma ejected by the AGN is key for understanding the growth and evolution of galaxies and their central black holes, the history of star formation, and the formation of large-scale structures. …”
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Star Formation in the Lopsided Galaxy Arp 291
Published 2025-01-01Subjects: “…Late-type galaxies…”
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On the Use of Galaxy Catalogs in Gravitational-wave Parameter Estimation
Published 2025-01-01“…For GW170817, we recover the true host galaxy as the most probable galaxy after a straightforward mass reweighting, with significantly decreased localization area and volume. …”
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A Characterization of the Diffuse Galactic Emissions in the Anticenter of the Galaxy
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The First Galaxies and the Likely Discovery of Their Fossils in the Local Group
Published 2010-01-01“…The lower bound for the mass of a galaxy is unknown, as are the typical luminosity of the smallest galaxies and their numbers. …”
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Cluster Candidates with Massive Quiescent Galaxies at z ∼ 2
Published 2025-01-01Subjects: “…Galaxy clusters…”
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UNCOVER: The Rest-ultraviolet to Near-infrared Multiwavelength Structures and Dust Distributions of Submillimeter-detected Galaxies in A2744
Published 2025-01-01Subjects: “…Galaxy formation…”
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Overview of the Near-IR S0 Galaxy Survey (NIRS0S)
Published 2011-01-01“…An overview of the results of the near-IR S0 galaxy survey (NIRS0S) is presented. NIRS0S is a magnitude- (mB⩽12.5 mag) and inclination- (<65∘) limited sample of ̃200 nearby galaxies, mainly S0s, but includes also Sa and E galaxies. …”
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Dwarf Galaxies in Voids: Dark Matter Halos and Gas Cooling
Published 2010-01-01“…Galaxy surveys have shown that luminous galaxies are mainly distributed in large filaments and galaxy clusters. …”
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Improving the Determination of Supernova Cosmological Redshifts by Using Galaxy Groups
Published 2025-01-01Subjects: Get full text
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High Energy Neutrino Emission from Astrophysical Jets in the Galaxy
Published 2015-01-01“…We address simulated neutrino emission originated from astrophysical jets of compact objects within the Galaxy. These neutrinos are of high energies (Eν of the order up to a few TeV) and for their observation specialized instruments are in operation, both on Earth and in orbit. …”
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The Study of Nebular Emission on Nearby Spiral Galaxies in the IFU Era
Published 2013-01-01“…Here I review some highlights of our current studies employing this technique: (1) the case study of NGC 628, the largest galaxy ever sampled with an IFU; (2) a statistical approach to the abundance gradients of spiral galaxies, which indicates a universal radial gradient for oxygen abundance; and (3) the discovery of a new scaling relation of HII regions in spiral galaxies, the local mass-metallicity relation of star-forming galaxies. …”
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Introducing the Condor Array Telescope. V. Deep Broad- and Narrowband Imaging Observations of the M81 Group
Published 2025-01-01Subjects: “…Galaxies…”
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The Quest for a Stable Disk
Published 2025-01-01Subjects: “…Galaxy dynamics…”
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PhotoD with LSST: Stellar Photometric Distances Out to the Edge of the Galaxy
Published 2025-01-01“…We validate our pipeline, named PhotoD (in analogy with photo- z , photometric redshifts of galaxies) using both simulated catalogs and SDSS, DECam, and Gaia photometry. …”
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