Search Results - "Floch, E Le"
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1
The Evolution of Galaxy Mergers and Morphology at z < 1.2 in the Extended Groth Strip
Published in The Astrophysical journal (01-01-2008)“…We present the quantitative rest-frame B morphological evolution and galaxy merger fraction at 0.2 < z < 1.2 as observed by the All-Wavelength Extended Groth…”
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2
Optimizing gravitational waves follow-up using galaxies stellar mass
Published in Monthly notices of the Royal Astronomical Society (01-03-2020)“…ABSTRACT We present a new strategy to optimize the electromagnetic follow-up of gravitational wave triggers. This method is based on the widely used galaxy…”
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3
An extremely young massive clump forming by gravitational collapse in a primordial galaxy
Published in Nature (London) (07-05-2015)“…An extremely young star-forming region caught at gravitational collapse in a distant galaxy is shedding new light on the processes driving galaxy growth in the…”
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4
A multiwavelength consensus on the main sequence of star-forming galaxies at z ∼ 2
Published in Monthly notices of the Royal Astronomical Society (01-09-2014)“…We compare various star formation rate (SFR) indicators for star-forming galaxies at 1.4 < z < 2.5 in the COSMOS field. The main focus is on the SFRs from the…”
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5
Non-linearity and environmental dependence of the star-forming galaxies main sequence
Published in Monthly notices of the Royal Astronomical Society (21-01-2016)“…Using data from four deep fields (COSMOS, AEGIS, ECDFS, and CDFN), we study the correlation between the position of galaxies in the star formation rate (SFR)…”
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6
The evolution of star formation activity in galaxy groups
Published in Monthly notices of the Royal Astronomical Society (11-12-2014)“…We study the evolution of the total star formation (SF) activity, total stellar mass (ΣM *) and halo occupation distribution (HOD) in massive haloes by using…”
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7
GOODS- HERSCHEL : STAR FORMATION, DUST ATTENUATION, AND THE FIR–RADIO CORRELATION ON THE MAIN SEQUENCE OF STAR-FORMING GALAXIES UP TO z ≃ 4
Published in The Astrophysical journal (10-07-2015)“…We use deep panchromatic data sets in the GOODS-N field, from GALEX to the deepest Herschel far-infrared (FIR) and VLA radio continuum imaging, to explore the…”
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8
Early- and late-stage mergers among main sequence and starburst galaxies at 0.2 ≤ z ≤ 2
Published in Monthly notices of the Royal Astronomical Society (01-06-2019)“…Abstract We investigate the fraction of close pairs and morphologically identified mergers on and above the star-forming main sequence (MS) at 0.2 ≤ z ≤2.0…”
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9
A contribution of star-forming clumps and accreting satellites to the mass assembly of z ∼ 2 galaxies
Published in Monthly notices of the Royal Astronomical Society (21-10-2019)“…ABSTRACT We investigate the contribution of clumps and satellites to the galaxy mass assembly. We analysed spatially resolved HubbleSpace Telescope…”
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10
The incidence of obscuration in active galactic nuclei
Published in Monthly notices of the Royal Astronomical Society (01-02-2014)“…We study the incidence of nuclear obscuration on a complete sample of 1310 active galactic nuclei (AGN) selected on the basis of their rest-frame 2-10 keV…”
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11
A Comprehensive Study on the Relation between the Metal Enrichment of Ionized and Atomic Gas in Star-forming Galaxies
Published in The Astrophysical journal (01-07-2023)“…Abstract We study the relation between the metallicities of ionized and atomic gas in star-forming galaxies at z = 0–3 using the Evolution and Assembly of…”
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12
Accreting supermassive black holes in the COSMOS field and the connection to their host galaxies
Published in Monthly notices of the Royal Astronomical Society (21-12-2012)“…ABSTRACT Using the wide multiband photometry available in the Cosmic Evolution Survey (COSMOS) field, we explore the host galaxy properties of a large sample…”
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13
A Superluminous Supernova in High Surface Density Molecular Gas within the Bar of a Metal-rich Galaxy
Published in The Astrophysical journal (01-09-2019)“…We report the Atacama Large Millimeter/submillimeter Array observations of the metal-rich host galaxy of superluminous supernova (SLSN) PTF10tpz, a barred…”
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14
A PHYSICAL APPROACH TO THE IDENTIFICATION OF HIGH-Z MERGERS: MORPHOLOGICAL CLASSIFICATION IN THE STELLAR MASS DOMAIN
Published in The Astrophysical journal (01-06-2015)“…ABSTRACT At z 1, the distinction between merging and "normal" star-forming galaxies based on single band morphology is often hampered by the presence of large…”
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15
The Infrared Luminosity Function of Galaxies at Redshifts z = 1 and z ~ 2 in the GOODS Fields
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16
Local Starburst Conditions and Formation of GRB 980425/SN 1998bw within a Collisional Ring
Published in The Astrophysical journal (01-08-2020)“…We present the first spatially resolved study of molecular gas in the vicinity of a gamma-ray burst (GRB), using CO(2−1) emission-line observations with the…”
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Unusual Gas Structure in an Otherwise Normal Spiral Galaxy Hosting GRB 171205A/SN 2017iuk
Published in The Astronomical journal (01-08-2022)“…Abstract We study the structure of atomic hydrogen (H i ) in the host galaxy of GRB 171205A/SN 2017iuk at z = 0.037 through H i 21 cm emission line…”
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18
The Interstellar Medium in the Environment of the Supernova-less Long-duration GRB 111005A
Published in The Astrophysical journal. Supplement series (01-04-2022)“…Abstract Long (>2 s) gamma-ray bursts (GRBs) are associated with explosions of massive stars, although in three instances, supernovae (SNe) have not been…”
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19
Photometric Redshift and Classification for the XMM-COSMOS Sources
Published in The Astrophysical journal (2009)“…We present photometric redshifts and spectral energy distribution (SED) classifications for a sample of 1542 optically identified sources detected with XMM in…”
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20
Star Formation in AEGIS Field Galaxies since z = 1.1: The Dominance of Gradually Declining Star Formation, and the Main Sequence of Star-forming Galaxies
Published in The Astrophysical journal (01-05-2007)“…We analyze star formation (SF) as a function of stellar mass (M sub(*)) and redshift z in the All-Wavelength Extended Groth Strip International Survey. For…”
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