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19912026
Showing 2018 · astro-ph.GAShow all

131 papers · 2 filters

astro-ph.GA2018★ 9 cited

Near-Infrared Survey and Photometric Redshifts in the Extended GOODS-North field

Li-Ting Hsu, Lihwai Lin, Mark Dickinson +22

We present deep and -band images in the extended Great Observatories Origins Deep Survey-North (GOODS-N) field covering an area of 0.22 . The observations were…

astro-ph.GA2018★ 39 cited

Spatial distribution of stellar mass and star formation activity at 0.2<z<1.2 across and along the Main Sequence

Laura Morselli, Paola Popesso, Anna Cibinel +5

High-resolution multi-wavelength photometry is crucial to explore the spatial distribution of star formation in galaxies and understand how these evolve. To this aim, in this paper…

astro-ph.GA2018★ 115 cited

The large and small scale properties of the intergalactic gas in the Slug Ly-alpha nebula revealed by MUSE HeII emission observations

Sebastiano Cantalupo, Gabriele Pezzulli, Simon J. Lilly +11

With a projected size of about 450 kpc at z~2.3, the Slug Ly-alpha nebula is a rare laboratory to study, in emission, the properties of the intergalactic gas in the Cosmic Web. Sin…

astro-ph.GA2018★ 48 cited

[CII] 158 Micron Emission from z~4 HI Absorption-Selected Galaxies

Marcel Neeleman, Nissim Kanekar, J. Xavier Prochaska +2

We report on a search for the [CII] 158 micron emission line from galaxies associated with four high-metallicity damped Ly-alpha absorbers (DLAs) at z ~ 4 using the Atacama Large M…

astro-ph.GA2018★ 49 cited

SDSS-IV MaNGA: local and global chemical abundance patterns in early-type galaxies

Taniya Parikh, Daniel Thomas, Claudia Maraston +6

Chemical enrichment signatures strongly constrain galaxy formation and evolution, and a detailed understanding of abundance patterns provides clues regarding the nucleosynthetic pr…

astro-ph.GA2018★ 59 cited

Chemical Abundance Analysis of Tucana III, the Second -process Enhanced Ultra-Faint Dwarf Galaxy

J. L. Marshall, T. Hansen, J. D. Simon +56

We present a chemical abundance analysis of four additional confirmed member stars of Tucana III, a Milky Way satellite galaxy candidate in the process of being tidally disrupted a…

astro-ph.GA2018★ 19 cited

Candidate Massive Galaxies at in the Dark Energy Survey

Pierandrea Guarnieri, Claudia Maraston, Daniel Thomas +52

Using stellar population models, we predicted that the Dark Energy Survey (DES) - due to its special combination of area (5000 deg. sq.) and depth () - would be in the po…

astro-ph.GA2018★ 142 cited

Formation of ultra-diffuse galaxies in the field and in galaxy groups

Fangzhou Jiang, Avishai Dekel, Jonathan Freundlich +4

We study ultra-diffuse galaxies (UDGs) in zoom in cosmological simulations, seeking the origin of UDGs in the field versus galaxy groups. We find that while field UDGs arise from d…

astro-ph.GA2018★ 34 cited

Keck OSIRIS AO LIRG Analysis: Feedback in the Nuclei of Luminous Infrared Galaxies

Vivian U, Anne M. Medling, Hanae Inami +21

The role of feedback in triggering or quenching star formation and hence driving galaxy evolution can be directly studied with high resolution integral field observations. The mani…

astro-ph.GA2018★ 21 cited

Asymmetric Drift in the Andromeda Galaxy (M31) as a Function of Stellar Age

Amanda C. N. Quirk, Puragra Guhathakurta, Laurent Chemin +5

We analyze the kinematics of Andromeda's disk as a function of stellar age by using photometry from the Panchromatic Hubble Andromeda Treasury (PHAT) survey and spectroscopy from t…

astro-ph.GA2018★ 41 cited

Detecting Radio-AGN signatures in Red geysers

Namrata Roy, Kevin Bundy, Edmond Cheung +19

A new class of quiescent galaxies harboring possible AGN-driven winds has been discovered using spatially resolved optical spectroscopy from the ongoing SDSS-IV MaNGA survey. These…

astro-ph.GA2018★ 3 cited

PS1-13cbe: The Rapid "Turn on" of a Seyfert 1

Reza Katebi, Ryan Chornock, Edo Berger +11

We present a nuclear transient event, PS1-13cbe, that was first discovered in the Pan-STARRS1 survey in 2013. The outburst occurred in the nucleus of the galaxy SDSS J222153.87+003…

astro-ph.GA2018★ 24 cited

Galaxy inclination and the IRX-beta relation: Effects on UV star-formation rate measurements at intermediate to high redshifts

Weichen Wang, Susan A. Kassin, Camilla Pacifici +11

At intermediate and high redshifts, measurements of galaxy star-formation rates are usually based on rest-frame ultraviolet (UV) data. A correction for dust attenuation, A_UV, is n…

astro-ph.GA2018★ 52 cited

Weak Lensing Reveals a Tight Connection Between Dark Matter Halo Mass and the Distribution of Stellar Mass in Massive Galaxies

Song Huang, Alexie Leauthaud, Andrew Hearin +9

Using deep images from the Hyper Suprime-Cam (HSC) survey and taking advantage of its unprecedented weak lensing capabilities, we reveal a remarkably tight connection between the s…

astro-ph.GA2018★ 37 cited

The Red Dead Redemption Survey of Circumgalactic Gas About Massive Galaxies. I. Mass and Metallicity of the Cool Phase

Michelle A. Berg, J. Christopher Howk, Nicolas Lehner +6

We present a search for HI in the circumgalactic medium (CGM) of 21 massive (), luminous red galaxies (LRGs) at . Using UV spectro…

astro-ph.GA2018★ 28 cited

Elemental Abundances in M31: Alpha and Iron Element Abundances from Low-Resolution Resolved Stellar Spectroscopy in the Stellar Halo

Ivanna Escala, Evan N. Kirby, Karoline M. Gilbert +2

Measurements of [Fe/H] and [/Fe] can probe the minor merging history of a galaxy, providing a direct way to test the hierarchical assembly paradigm. While measurements of [/F…

astro-ph.GA2018★ 144 cited

The MAGNUM survey: different gas properties in the outflowing and disk components in nearby active galaxies with MUSE

M. Mingozzi, G. Cresci, G. Venturi +17

We investigated the interstellar medium properties of the disc and outflowing gas in the central regions of nine nearby Seyfert galaxies, all characterised by prominent outflows. T…

astro-ph.GA2018★ 33 cited

The stellar halo of isolated central galaxies in the Hyper Suprime-Cam imaging survey

Wenting Wang, Jiaxin Han, Alessandro Sonnenfeld +14

We study the faint stellar halo of isolated central galaxies, by stacking galaxy images in the HSC survey and accounting for the residual sky background sampled with random points.…

astro-ph.GA2018★ 105 cited

Finding high-redshift strong lenses in DES using convolutional neural networks

C. Jacobs, T. Collett, K. Glazebrook +63

We search Dark Energy Survey (DES) Year 3 imaging data for galaxy-galaxy strong gravitational lenses using convolutional neural networks. We generate 250,000 simulated lenses at re…

astro-ph.GA2018★ 64 cited

Quasar Accretion Disk Sizes from Continuum Reverberation Mapping in the DES Standard Star Fields

Zhefu Yu, Paul Martini, T. M. Davis +72

Measurements of the physical properties of accretion disks in active galactic nuclei are important for better understanding the growth and evolution of supermassive black holes. We…

astro-ph.GA2018★ 1 cited

Spectroscopic Constraints on the Build-up of the Intracluster Light in the Coma Cluster

Meng Gu, Charlie Conroy, David Law +13

The stellar content of the intracluster light (ICL) provides unique insight into the hierarchical assembly process of galaxy clusters.However, the ICL is difficult to study due to…

astro-ph.GA2018★ 20 cited

Hydrodynamic Shielding and the Survival of Cold Streams

John C. Forbes, Douglas N. C. Lin

Cold clouds in hot media are quickly crushed, shredded, and then accelerated as a result of their interaction with the background gas. The persistence of cold clouds moving at subs…

astro-ph.GA2018★ 34 cited

HALO7D II: The Halo Velocity Ellipsoid and Velocity Anisotropy with Distant Main Sequence Stars

Emily C. Cunningham, Alis J. Deason, Robyn E. Sanderson +7

The Halo Assembly in Lambda-CDM: Observations in 7 Dimensions (HALO7D) dataset consists of Keck II/DEIMOS spectroscopy and Hubble Space Telescope-measured proper motions of Milky W…

astro-ph.GA2018★ 13 cited

Complete IRAC mapping of the CFHTLS-DEEP, MUSYC AND NMBS-II FIELDS

Marianna Annunziatella, Danilo Marchesini, Mauro Stefanon +19

The IRAC mapping of the NMBS-II fields program is an imaging survey at 3.6 and 4.5m with the Spitzer Infrared Array Camera (IRAC). The observations cover three Canada-France-Haw…