activity
20072026
most citedThe Herschel view of the dominant mode of galaxy growth from z=4 to the present day

837 citations · 11.1k across the 165 of their papers we have counts for

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Showing 2018Show all

14 papers · 1 filter

astro-ph.GA2018★ 124 cited

The main sequence of star forming galaxies I. The local relation and its bending

P. Popesso, A. Concas, L. Morselli +11

By using a set of different SFR indicators, including WISE mid-infrared and Halpha emission, we study the slope of the Main Sequence (MS) of local star forming galaxies at stellar…

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★ 67 cited

The Multiple Merger Assembly of a Hyper-luminous Obscured Quasar at redshift 4.6

T. Diaz-Santos, R. J. Assef, A. W. Blain +10

Galaxy mergers and gas accretion from the cosmic web drove the growth of galaxies and their central black holes at early epochs. We report spectroscopic imaging of a multiple merge…

astro-ph.GA2018★ 3 cited

ALMA Observation of NGC5135: The Circumnuclear CO(6-5) and Dust Continuum Emission at 45 Parsec Resolution[]

Tianwen Cao, Nanyao Lu, C. Kevin Xu +10

We present high-resolution (0.17\arcsec 0.14\arcsec) Atacama Large Millimeter/submillimeter Array (ALMA) observations of the CO\,(6-5) line, and 435\um\ dust continuum emi…

astro-ph.GA2018★ 43 cited

MUSE Spectroscopic Identifications of Ultra-Faint Emission Line Galaxies with M -15

Michael V. Maseda, Roland Bacon, Marijn Franx +16

Using an ultra-deep blind survey with the MUSE integral field spectrograph on the ESO Very Large Telescope, we obtain spectroscopic redshifts to a depth never explored before: gala…

astro-ph.GA2018★ 99 cited

The MUSE Hubble Ultra Deep Field Survey XI. Constraining the low-mass end of the stellar mass - star formation rate relation at

Leindert A. Boogaard, Jarle Brinchmann, Nicolas Bouché +16

Star-forming galaxies have been found to follow a relatively tight relation between stellar mass () and star formation rate (SFR), dubbed the `star formation sequence'. A tu…

astro-ph.GA2018★ 23 cited

Properties and redshift evolution of star-forming galaxies with high [OIII]/[OII] ratios with MUSE at 0.28<z<0.85

M. Paalvast, A. Verhamme, L. A. Straka +21

We present a study of the [OIII]5007/[OII]3727 (O32) ratios of star-forming galaxies drawn from MUSE data spanning a redshift range 0.28<z<0.85. Recently discovered Lyman continuum…

astro-ph.GA2018★ 17 cited

AKARI mid-infrared slitless spectroscopic survey of star-forming galaxies at

Y. Ohyama, T. Wada, H. Matsuhara +24

Deep MIR surveys have revealed numerous strongly star-forming galaxies at redshift z~<2. Their MIR fluxes are produced by a combination of continuum and PAH emission features. The…

astro-ph.GA2018★ 26 cited

A census of galaxy constituents in a Coma Progenitor observed at z>3

Ke Shi, Kyoung-Soo Lee, Arjun Dey +15

We present a detailed census of galaxies in and around PC217.96+32.3, a spectroscopically confirmed Coma analog at z=3.78. Diverse galaxy types identified in the field include Lya…

astro-ph.GA2018★ 38 cited

The AKARI 2.5-5 Micron Spectra of Luminous Infrared Galaxies in the Local Universe

H. Inami, L. Armus, H. Matsuhara +10

We present AKARI 2.5-5um spectra of 145 local luminous infrared galaxies in the Great Observatories All-sky LIRG Survey. In all of the spectra, we measure the line fluxes and EQWs…

astro-ph.GA2018★ 45 cited

The MUSE Hubble Ultra Deep Field Survey: XII. MgII emission and absorption in star-forming galaxies

Anna Feltre, Roland Bacon, Laurence Tresse +18

The physical origin of the near-ultraviolet MgII emission remains an under-explored domain, contrary to more typical emission lines detected in the spectra of star-forming galaxies…

astro-ph.GA2018★ 27 cited

Warm Molecular Hydrogen in Nearby, Luminous Infrared Galaxies

Andreea O. Petric, Lee Armus, Nicolas Flagey +19

Mid-infrared molecular hydrogen (H) emission is a powerful cooling agent in galaxy mergers and in radio galaxies; it is a potential key tracer of gas evolution and energy dissi…

astro-ph.GA2018★ 9 cited

Discovery of a Very Large (~20 kpc) Galaxy at z=3.72

Kyoung-Soo Lee, Arjun Dey, Thomas Matheson +12

We report the discovery and spectroscopic confirmation of a very large star-forming Lyman Break galaxy, G6025, at z_spec=3.721+/-0.003. In the rest-frame ~2100A, G6025 subtends ~24…

astro-ph.GA2018★ 51 cited

GOODS-ALMA: 1.1 mm galaxy survey - I. Source catalogue and optically dark galaxies

M. Franco, D. Elbaz, M. Béthermin +36

We present a 69 arcmin ALMA survey at 1.1mm, GOODS-ALMA, matching the deepest HST-WFC3 H-band part of the GOODS-South field. We taper the 0"24 original image with a homogeneous…