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- European Southern ObservatoryCL534 papers
- Centre National de la Recherche ScientifiqueFR446 papers
- National Radio Astronomy ObservatoryUS369 papers
- National Astronomical Observatory of JapanJP337 papers
- Center for Astrophysics Harvard & SmithsonianUS293 papers
- California Institute of TechnologyUS247 papers
- Leiden UniversityNL229 papers
- Institute of Astronomy and Astrophysics, Academia SinicaTW225 papers
- University of CambridgeGB210 papers
- Max Planck Institute for Radio AstronomyDE208 papers
- Institut de Planétologie et d'Astrophysique de GrenobleFR206 papers
- Commissariat à l'Énergie Atomique et aux Énergies AlternativesFR196 papers
31 papers · 2 filters
Star Formation and AGN activity in Galaxies classified using the 1.6 μm Bump and PAH features at
Hitoshi Hanami, Tsuyoshi Ishigaki, Naofumi Fujishiro +17
We have studied the star-formation and AGN activity of massive galaxies in the redshift range , which are detected in a deep survey field using the AKARI InfraRed (IR) ast…
The Herschel Reference Survey: Dust in Early-Type Galaxies and Across the Hubble Sequence
M. W. L. Smith, H. L. Gomez, S. A. Eales +24
We present Herschel observations of 62 Early-Type Galaxies (ETGs), including 39 galaxies morphologically classified as S0+S0a and 23 galaxies classified as ellipticals using SPIRE…
Star formation laws in Luminous Infrared Galaxies. New observational constraints on models
S. Garcia-Burillo, A. Usero, A. Alonso-Herrero +5
The observational study of star formation relations in galaxies is central to unraveling the physical processes at work on local and global scales. We wish to expand the sample of…
How Do Star-Forming Galaxies at Z>3 Assemble Their Masses?
Kyoung-Soo Lee, Henry C. Ferguson, Tommy Wiklind +8
We investigate how star-forming galaxies typically assemble their masses at high redshift. Using the deep multi-wavelength coverage of the GOODS dataset, we measure stellar mass of…
GOODS-Herschel and CANDELS: The Morphologies of Ultraluminous Infrared Galaxies at z~2
Jeyhan S. Kartaltepe, Mark Dickinson, David M. Alexander +40
Using deep 100-160 micron observations in GOODS-S from the GOODS-H survey, combined with HST/WFC3 NIR imaging from CANDELS, we present the first morphological analysis of a complet…
A lambda = 1.3 mm and 2 mm molecular line survey towards M82
Rebeca Aladro, Sergio Martín, Jesús Martín-Pintado +4
We study the chemical complexity towards the central parts of the starburst galaxy M82, and investigate the role of certain molecules as tracers of the physical processes in the ga…