Counting papers with at most 25 authors, so collaboration author lists do not stand in for the people here.
- Commissariat à l'Énergie Atomique et aux Énergies AlternativesFR14k papers
- Centre National de la Recherche ScientifiqueFR9.8k papers
- Université Paris-SaclayFR5.1k papers
- Institut de Recherche sur les Lois Fondamentales de l'UniversFR5k papers
- Institut National de Physique Nucléaire et de Physique des ParticulesFR3.8k papers
- Astrophysique, Instrumentation et ModélisationFR3.3k papers
- Université Paris CitéFR3.3k papers
- Istituto Nazionale di Fisica Nucleare, Sezione di Roma IIT2.4k papers
- European Organization for Nuclear ResearchCH2.4k papers
- The Ohio State UniversityUS2.3k papers
- Istituto Nazionale di Fisica Nucleare, Sezione di BolognaIT2.3k papers
- Istituto Nazionale di Fisica Nucleare, Sezione di GenovaIT2.2k papers
105 papers · 2 filters
CLASH: Extreme Emission Line Galaxies and Their Implication on Selection of High-Redshift Galaxies
Xingxing Huang, Wei Zheng, Junxian Wang +23
We utilize the CLASH (Cluster Lensing And Supernova survey with Hubble) observations of 25 clusters to search for extreme emission-line galaxies (EELGs). The selections are carried…
The reversal of the SF-density relation in a massive, X-ray selected galaxy cluster at z=1.58: results from Herschel
Joana S. Santos, . Bruno Altieri, Ivan Valtchanov +8
Dusty, star-forming galaxies have a critical role in the formation and evolution of massive galaxies in the Universe. Using deep far-infrared imaging in the range 100-500um obtaine…
Spatially resolved physical conditions of molecular gas and potential star formation tracers in M83, revealed by the Herschel SPIRE FTS
Ronin Wu, Suzanne Madden, Frédéric Galliano +19
Since the launch of the Herschel Space Observatory, our understanding about the photo-dissociation regions (PDR) has taken a step forward. In the bandwidth of the Fourier Transform…
COLDz: Karl G. Jansky Very Large Array discovery of a gas-rich galaxy in COSMOS
L. Lentati, J. Wagg, C. L. Carilli +15
The broad spectral bandwidth at mm and cm-wavelengths provided by the recent upgrades to the Karl G. Jansky Very Large Array (VLA) has made it possible to conduct unbiased searches…
Black hole growth and AGN feedback under clumpy accretion
Colin DeGraf, Avishai Dekel, Jared Gabor +1
High-resolution simulations of supermassive black holes in isolated galaxies have suggested the importance of short (~10 Myr) episodes of rapid accretion caused by interactions bet…
A Detailed Study of Feedback from a Massive Star
Sam Geen, Joakim Rosdahl, Jeremy Blaizot +2
We present numerical simulations of a 15 solar mass star in a suite of idealised environments in order to quantify the amount of energy transmitted to the interstellar medium (ISM)…
The Herschel Virgo Cluster Survey. XVIII. Star-forming dwarf galaxies in a cluster environment
M. Grossi, L. K. Hunt, S. C. Madden +22
To assess the effects of the cluster environment on the different components of the interstellar medium, we analyse the FIR-submm properties of a sample of star-forming dwarf (SFD)…
Mutual influence of supernovae and molecular clouds
Olivier Iffrig, Patrick Hennebelle
Context. Molecular clouds are known to be turbulent and strongly affected by stellar feedback. Moreover, stellar feedback is believed to drive turbulence at large scales in galaxie…
The inefficiency of satellite accretion in forming extended star clusters
Paolo Bianchini, Florent Renaud, Mark Gieles +1
The distinction between globular clusters and dwarf galaxies has been progressively blurred by the recent discoveries of several extended star clusters, with size (20-30 pc) and lu…
The ages, metallicities and element abundance ratios of massive quenched galaxies at z~1.6
M. Onodera, C. M. Carollo, A. Renzini +8
We investigate the stellar population properties of a sample of 24 massive quenched galaxies at identified in the COSMOS field with our Subaru/MOIRCS ne…
Planck intermediate results. XXXIII. Signature of the magnetic field geometry of interstellar filaments in dust polarization maps
Planck Collaboration, P. A. R. Ade, N. Aghanim +187
Planck observations at 353GHz provide the first fully-sampled maps of the polarized dust emission towards interstellar filaments and their backgrounds. The polarization data provid…
Accretion-Inhibited Star Formation in the Warm Molecular Disk of the Green-valley Elliptical Galaxy NGC 3226
P. N. Appleton, C. Mundell, T. Bitsakis +7
We present archival Spitzer photometry and spectroscopy, and Herschel photometry, of the peculiar "Green Valley" elliptical galaxy NGC~3226. The galaxy, which contains a low-lumino…
The far-infrared/radio correlation and radio spectral index of galaxies in the SFR-M* plane up to z 2
B. Magnelli, R. J. Ivison, D. Lutz +21
[Abridged] We study the evolution of the radio spectral index and far-infrared/radio correlation (FRC) across the star-formation rate-stellar masse (i.e. SFR-M*) plane up to z 2. W…
The interplay between a galactic bar and a supermassive black hole: nuclear fueling in a sub-parsec resolution galaxy simulation
Eric Emsellem, Florent Renaud, Frédéric Bournaud +3
We study the connection between the large-scale dynamics and the gas fueling toward a central black hole via the analysis of a Milky Way-like simulation at sub-parsec resolution. T…
A parsec-resolution simulation of the Antennae galaxies: Formation of star clusters during the merger
Florent Renaud, Frédéric Bournaud, Pierre-Alain Duc
We present a hydrodynamical simulation of an Antennae-like galaxy merger at parsec resolution, including a multi-component model for stellar feedback and reaching numerical converg…
The Next Generation Virgo Cluster Survey. XV. The photometric redshift estimation for background sources
A. Raichoor, S. Mei, T. Erben +28
The Next Generation Virgo Cluster Survey is an optical imaging survey covering 104 deg^2 centered on the Virgo cluster. Currently, the complete survey area has been observed in the…
Applying galactic archeology to massive galaxies using deep imaging surveys
Pierre-Alain Duc
Various programs aimed at exploring the still largely unknown low surface brightness Universe with deep imaging optical surveys have recently started. They open a new window for st…
The Atlas3D project -- XXIX. The new look of early-type galaxies and surrounding fields disclosed by extremely deep optical images
Pierre-Alain Duc, Jean-Charles Cuillandre, Emin Karabal +24
Galactic archeology based on star counts is instrumental to reconstruct the past mass assembly of Local Group galaxies. The development of new observing techniques and data-reducti…
Are Dusty Galaxies Blue? Insights on UV Attenuation from Dust-Selected Galaxies
C. M. Casey, N. Z. Scoville, D. B. Sanders +12
Galaxies' rest-frame ultraviolet (UV) properties are often used to directly infer the degree to which dust obscuration affects the measurement of star formation rates. While much r…
The mass-metallicity relation of zCOSMOS galaxies at z ~ 0.7, its dependence on SFR, and the existence of massive low-metallicity galaxies
C. Maier, B. L. Ziegler, S. J. Lilly +5
(Abridged) The knowledge of the number and of the physical nature of low-metallicity massive galaxies is crucial for the determination and interpretation of the mass-metallicity re…
The stellar accretion origin of stellar population gradients in massive galaxies at large radii
Michaela Hirschmann, Thorsten Naab, Jeremiah P. Ostriker +5
We investigate the evolution of stellar population gradients from to in massive galaxies at large radii () using ten cosmological zoom simulation…
The Most Luminous Galaxies Discovered by WISE
Chao-Wei Tsai, Peter Eisenhardt, Jingwen Wu +25
We present 20 WISE-selected galaxies with bolometric luminosities L_bol > 10^14 L_sun, including five with infrared luminosities L_IR = L(rest 8-1000 micron) > 10^14 L_sun. These "…
Metal deficiency in cluster star-forming galaxies at z=2
F. Valentino, E. Daddi, V. Strazzullo +8
We investigate the environmental effect on the metal enrichment of star-forming galaxies (SFGs) in the farthest spectroscopically confirmed and X-ray detected cluster, CL~J1449+085…
The Hawk-I UDS and GOODS Survey (HUGS): Survey design and deep K-band number counts
A. Fontana, J. S. Dunlop, D. Paris +40
We present the results of a new, ultra-deep, near-infrared imaging survey executed with the Hawk-I imager at the ESO VLT, of which we make all the data public. This survey, named H…