Counting papers with at most 25 authors, so collaboration author lists do not stand in for the people here.
- Centre National de la Recherche ScientifiqueFR1.3k papers
- Vrije Universiteit BrusselBE1.1k papers
- Université Libre de BruxellesBE1k papers
- University of Maryland, College ParkUS1k papers
- RWTH Aachen UniversityDE957 papers
- The Ohio State UniversityUS957 papers
- Commissariat à l'Énergie Atomique et aux Énergies AlternativesFR951 papers
- University of Wisconsin–MadisonUS935 papers
- University of CanterburyNZ926 papers
- Massachusetts Institute of TechnologyUS922 papers
- California Institute of TechnologyUS909 papers
- University of KansasUS899 papers
29 papers · 2 filters
Candidate high-z proto-clusters among the Planck compact sources, as revealed by Herschel-SPIRE
J. Greenslade, D. L. Clements, T. Cheng +19
By determining the nature of all the Planck compact sources within 808.4 deg^2 of large Herschel surveys, we have identified 27 candidate proto-clusters of dusty star forming galax…
Data release of UV to submm broadband fluxes for simulated galaxies from the EAGLE project
Peter Camps, Ana Trčka, James Trayford +6
We present dust-attenuated and dust emission fluxes for sufficiently resolved galaxies in the EAGLE suite of cosmological hydrodynamical simulations, calculated with the SKIRT radi…
The Herschel-ATLAS Data Release 2, Paper I. Submillimeter and Far-infrared Images of the South and North Galactic Poles: The Largest Herschel Survey of the Extragalactic Sky
Matthew W. L. Smith, Edo Ibar, Steve J. Maddox +11
We present the largest submillimeter images that have been made of the extragalactic sky. The Herschel Astrophysical Terahertz Large Area Survey (H-ATLAS) is a survey of 660 deg$^2…
GAMA/H-ATLAS: The Local Dust Mass Function and Cosmic Density as a Function of Galaxy Type - A Benchmark for Models of Galaxy Evolution
R. A. Beeston, A. H. Wright, S. Maddox +22
We present the dust mass function (DMF) of 15,750 galaxies with redshift , drawn from the overlapping area of the GAMA and {\it H-}ATLAS surveys. The DMF is derived using t…
NGC 5626: a massive fast rotator with a twist
S. Viaene, M. Sarzi, M. Baes +1
We present a kinematic analysis of the dust-lane elliptical NGC 5626 based on MUSE observations. These data allow to robustly classify this galaxy as a fast rotator and to infer a…
The New Galaxy Evolution Paradigm Revealed by the Herschel Surveys
Stephen Eales, Dan Smith, Nathan Bourne +22
The Herschel Space Observatory has revealed a very different galaxyscape from that shown by optical surveys which presents a challenge for galaxy-evolution models. The Herschel sur…
Unbiased large spectroscopic surveys of galaxies selected by SPICA using dust bands
H. Kaneda, D. Ishihara, S. Oyabu +27
The mid-infrared (IR) range contains many spectral features associated with large molecules and dust grains such as polycyclic aromatic hydrocarbons (PAHs) and silicates. These are…
Tracing the evolution of dust obscured star-formation and accretion back to the reionisation epoch with SPICA
C. Gruppioni, L. Ciesla, E. Hatziminaoglou +35
Our current knowledge of star formation and accretion luminosity at high-redshift (z>3-4), as well as the possible connections between them, relies mostly on observations in the re…
Galaxy evolution studies with the SPace IR telescope for Cosmology and Astrophysics (SPICA): the power of IR spectroscopy
L. Spinoglio, A. Alonso-Herrero, L. Armus +65
IR spectroscopy in the range 12-230 micron with the SPace IR telescope for Cosmology and Astrophysics (SPICA) will reveal the physical processes that govern the formation and evolu…
SPICA and the Chemical Evolution of Galaxies: The Rise of Metals and Dust
J. A. Fernández-Ontiveros, L. Armus, M. Baes +33
The physical processes driving the chemical evolution of galaxies in the last cannot be understood without directly probing the dust-obscured phase of star-for…
The Herschel Bright Sources (HerBS): Sample definition and SCUBA-2 observations
Tom J. L. C. Bakx, S. A. Eales, M. Negrello +20
We present the Herschel Bright Sources (HerBS) sample, a sample of bright, high-redshift Herschel sources detected in the 616.4 square degree H-ATLAS survey. The HerBS sample conta…
Verifying reddening and extinction for Gaia DR1 TGAS main sequence stars
George Gontcharov, Aleksandr Mosenkov
We compare eight sources of reddening and extinction estimates for approximately 60,000 {\it Gaia} DR1 Tycho--Gaia Astrometric Solution (TGAS) main sequence stars younger than 3~Gy…
The Small Magellanic Cloud Investigation of Dust and Gas Evolution (SMIDGE): The Dust Extinction Curve from Red Clump Stars
Petia Yanchulova Merica-Jones, Karin M. Sandstrom, L. Clifton Johnson +6
We use Hubble Space Telescope (HST) observations of red clump stars taken as part of the Small Magellanic Cloud Investigation of Dust and Gas Evolution (SMIDGE) program to measure…
Dissecting the active galactic nucleus in Circinus -- I. Peculiar mid-IR morphology explained by a dusty hollow cone
Marko Stalevski, Daniel Asmus, Konrad R. W. Tristram
Recent high angular resolution observations resolved for the first time the mid-infrared (MIR) structure of nearby active galactic nuclei (AGN). Surprisingly, they revealed that a…
DustPedia: Multiwavelength Photometry and Imagery of 875 Nearby Galaxies in 42 Ultraviolet--Microwave Bands
Christopher J. R. Clark, S. Verstocken, S. Bianchi +16
The DustPedia project is capitalising on the legacy of the Herschel Space Observatory, using cutting-edge modelling techniques to study dust in the 875 DustPedia galaxies - represe…
MUSE stares into the shadows: the high-resolution dust attenuation curve of NGC 5626
S. Viaene, M. Sarzi, M. Baes +2
The newest generation of integral field unit spectrographs brings three-dimensional mapping of nearby galaxies one step closer. While the focus up to this point was mostly on stars…
Measuring the X-shaped structures in edge-on galaxies
S. S. Savchenko, N. Ya. Sotnikova, A. V. Mosenkov +2
We present a detailed photometric study of a sample of 22 edge-on galaxies with clearly visible X-shaped structures. We propose a novel method to derive geometrical parameters of t…
Probing the cold and warm molecular gas in the Whirlpool Galaxy: Herschel SPIRE-FTS Observations of the central region of M51 (NGC 5194)
M. R. P. Schirm, C. D. Wilson, J. Kamenetzky +12
We present Herschel SPIRE-FTS intermediate-sampled mapping observations of the central ~8 kpc (~150") of M51, with a spatial resolution of 40". We detect 4 12CO transitions (J=4-3…
Testing baryon-induced core formation in CDM: A comparison of the DC14 and coreNFW dark matter halo models on galaxy rotation curves
F. Allaert, G. Gentile, M. Baes
Recent cosmological hydrodynamical simulations suggest that baryonic processes, and in particular supernova feedback after bursts of star formation, can alter the structure of dark…
Radial distribution of dust, stars, gas, and star-formation rate in DustPedia face-on galaxies
V. Casasola, L. P. Cassara, S. Bianchi +18
The purpose of this work is the characterization of the radial distribution of dust, stars, gas, and star-formation rate (SFR) in a sub-sample of 18 face-on spiral galaxies extract…
VALES: I. The molecular gas content in star-forming dusty H-ATLAS galaxies up to z=0.35
V. Villanueva, E. Ibar, T. M. Hughes +24
We present an extragalactic survey using observations from the Atacama Large Millimeter/submillimeter Array (ALMA) to characterise galaxy populations up to : the Valparaíso…
Using dust, gas and stellar mass selected samples to probe dust sources and sinks in low metallicity galaxies
P. De Vis, H. L. Gomez, S. P. Schofield +8
We combine samples of nearby galaxies with Herschel photometry selected on their dust, metal, HI, and stellar mass content, and compare these to chemical evolution models in order…
Optical colours and spectral indices of EAGLE galaxies with 3D dust radiative transfer code SKIRT
James W. Trayford, Peter Camps, Tom Theuns +7
We present mock optical images, broad-band and H fluxes, and D4000 spectral indices for 30,145 galaxies from the EAGLE hydrodynamical simulation at redshift , modelling d…
Modelling high resolution ALMA observations of strongly lensed highly star forming galaxies detected by Herschel
S. Dye, C. Furlanetto, L. Dunne +12
We have modelled high resolution ALMA imaging of six strong gravitationally lensed galaxies detected by the Herschel Space Observatory. Our modelling recovers mass properties of th…