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
38 papers · 2 filters
Modeling dust emission in the Magellanic Clouds with Spitzer and Herschel
Jeremy Chastenet, Caroline Bot, Karl D. Gordon +4
Dust modeling is crucial to infer dust properties and budget for galaxy studies. However, there are systematic disparities between dust grain models that result in corresponding sy…
Tale of J1328+2752: a misaligned double-double radio galaxy hosted by a binary black-hole?
S. Nandi, M. Jamrozy, R. Roy +4
We present a radio and optical study of the double-double radio galaxy J1328+2752 based on new low-frequency GMRT observations and SDSS data. The radio data were used to investigat…
UV-extended E-MILES stellar population models: young components in massive early-type galaxies
A. Vazdekis, M. Koleva, E. Ricciardelli +2
We present UV-extended E-MILES stellar population synthesis models covering the spectral range 1680-50000A at moderately high resolution. We employ the NGSL space-based stellar lib…
Very Thin Disc Galaxies in The SDSS Catalog of Edge-on Galaxies
D. V. Bizyaev, S. J. Kautsch, N. Ya. Sotnikova +2
We study the properties of galaxies with very thin discs using a sample of 85 objects whose stellar disc radial-to-vertical scale ratio determined from photometric decomposition, e…
VALES: II. The physical conditions of interstellar gas in normal star-forming galaxies up to z=0.2 revealed by ALMA
T. M. Hughes, E. Ibar, V. Villanueva +18
We use new Band-3 CO(1-0) observations taken with the Atacama Large Millimeter/submillimeter Array (ALMA) to study the physical conditions in the interstellar gas of a sample of 27…
The interstellar medium in Andromeda's dwarf spheroidal galaxies: II. Multi-phase gas content and ISM conditions
Ilse De Looze, Maarten Baes, Diane Cormier +11
We make an inventory of the interstellar medium material in three low-metallicity dwarf spheroidal galaxies of the Local Group (NGC147, NGC185 and NGC205). Ancillary HI, CO, Spitze…
The Herschel-ATLAS: a sample of 500μm-selected lensed galaxies over 600 square degrees
M. Negrello, S. Amber, A. Amvrosiadis +43
We present a sample of 80 candidate strongly lensed galaxies with flux density above 100mJy at 500μm extracted from the Herschel Astrophysical Terahertz Large Area Survey (H-ATLAS)…
The Galaxy End Sequence
Stephen Eales, Pieter de Vis, Matthew Smith +4
A common assumption is that galaxies fall in two distinct regions on a plot of specific star-formation rate (SSFR) versus galaxy stellar mass: a star-forming Galaxy Main Sequence (…
Herschel-ATLAS: Revealing dust build-up and decline across gas, dust and stellar mass selected samples: I. Scaling relations
P. De Vis, L. Dunne, S. Maddox +19
We present a study of the dust, stars and atomic gas (HI) in an HI-selected sample of local galaxies (z<0.035) in the Herschel Astrophysical Terahertz Large Area Survey (H-ATLAS) f…
The Herschel Exploitation of Local Galaxy Andromeda (HELGA) VII: A SKIRT radiative transfer model and insights on dust heating
S. Viaene, M. Baes, A. Tamm +17
The radiation of stars heats dust grains in the diffuse interstellar medium and in star-forming regions in galaxies. Modelling this interaction provides information on dust in gala…
DustPedia - A Definitive Study of Cosmic Dust in the Local Universe
J. I. Davies, M. Baes, S. Bianchi +20
The European Space Agency has invested heavily in two cornerstones missions; Herschel and Planck. The legacy data from these missions provides us with an unprecedented opportunity…
The Herschel Virgo Cluster Survey. XX. Dust and gas in the foreground Galactic cirrus
S. Bianchi, C. Giovanardi, M. W. L. Smith +22
We study the correlation between far-infared/submm dust emission and atomic gas column density in order to derive the properties of the high Galactic latitude, low density, Milky W…
Discovery of a pseudobulge galaxy launching powerful relativistic jets
J. K. Kotilainen, J. Leon Tavares, A. Olguin-Iglesias +4
Supermassive black holes launching plasma jets at close to speed of light, producing gamma-rays, have ubiquitously been found to be hosted by massive elliptical galaxies. Since ell…
GRB 980425 host: [CII], [OI] and CO lines reveal recent enhancement of star formation due to atomic gas inflow
Michał J. Michałowski, J. M. Castro Ceron, J. L. Wardlow +18
We have recently suggested that gas accretion can be studied using host galaxies of gamma-ray bursts (GRBs). We obtained the first ever far-infrared (FIR) line observations of a GR…
Radiative transfer in disc galaxies V. The accuracy of the KB approximation
Dukhang Lee, Maarten Baes, Kwang-Il Seon +3
We investigate the accuracy of an approximate radiative transfer technique that was first proposed by Kylafis & Bahcall (hereafter the KB approximation) and has been popular in mod…
Asymmetric structure in Sgr A* at 3mm from closure phase measurements with VLBA, GBT and LMT
Christiaan D. Brinkerink, Cornelia Müller, Heino Falcke +19
We present the results of a closure phase analysis of 3 mm very long baseline interferometry (VLBI) measurements performed on Sagittarius A* (Sgr A*). We have analyzed observations…
The Shape of Dark Matter Haloes IV. The Structure of Stellar Discs in Edge-on Galaxies
S. P. C. Peters, G. de Geyter, P. C. van der Kruit +1
We present optical and near-infrared archival observations of eight edge-on galaxies. These observations are used to model the stellar content of each galaxy using the FitSKIRT sof…
The potential role of NGC 205 in generating Andromeda's vast thin co-rotating plane of satellite galaxies
Garry W. Angus, Paul Coppin, Gianfranco Gentile +1
The Andromeda galaxy is observed to have a system of two large dwarf ellipticals and ~13 smaller satellite galaxies that are currently co-rotating in a thin plane, in addition to 2…
Far-infrared and dust properties of present-day galaxies in the EAGLE simulations
Peter Camps, James W. Trayford, Maarten Baes +3
The EAGLE cosmological simulations reproduce the observed galaxy stellar mass function and many galaxy properties. In this work, we study the dust-related properties of present-day…
The Herschel-ATLAS Data Release 1 Paper II: Multi-wavelength counterparts to submillimetre sources
N. Bourne, L. Dunne, S. J. Maddox +27
This paper is the second in a pair of articles presenting data release 1 (DR1) of the Herschel Astrophysical Terahertz Large Area Survey (H-ATLAS), the largest single open-time key…
Galaxies with conspicuous optical warps
Vladimir P. Reshetnikov, Aleksandr V. Mosenkov, Alexei V. Moiseev +2
In this paper, we present results of a photometric and kinematic study for a sample of 13 edge-on spiral galaxies with pronounced integral-shape warps of their stellar discs. The g…
Probing dust-obscured star formation in the most massive Gamma-Ray Burst host galaxies
Jochen Greiner, Michal J. Michalowski, Sylvio Klose +15
Due to their relation to massive stars, long-duration gamma-ray bursts (GRBs) allow pinpointing star formation in galaxies independently of redshift, dust obscuration, or galaxy ma…
The Panchromatic Hubble Andromeda Treasury XV. The BEAST: Bayesian Extinction and Stellar Tool
Karl D. Gordon, Morgan Fouesneau, Heddy Arab +17
We present the Bayesian Extinction And Stellar Tool (BEAST), a probabilistic approach to modeling the dust extinguished photometric spectral energy distribution of an individual st…
Dust Properties in HII Regions in M33
M. Relano, R. Kennicutt, U. Lisenfeld +11
The conversion of the IR emission into star formation rate can be strongly dependent on the physical properties of the dust, which are affected by the environmental conditions wher…