7.1k citations
- California Institute of TechnologyUS692 papers
- Centre National de la Recherche ScientifiqueFR183 papers
- Jet Propulsion LaboratoryUS175 papers
- Space Telescope Science InstituteUS153 papers
- Goddard Space Flight CenterUS122 papers
- University of ArizonaUS111 papers
- Center for Astrophysics Harvard & SmithsonianUS106 papers
- University of California, BerkeleyUS102 papers
- Max Planck Institute for AstronomyDE98 papers
- European Southern ObservatoryCL94 papers
- Université Bourgogne Franche-ComtéFR79 papers
- University of California, Los AngelesUS76 papers
27 papers · 2 filters
An alternate approach to measure specific star formation rates at 2<z<7
Iary Davidzon, Olivier Ilbert, Andreas L. Faisst +2
We trace the specific star formation rate (sSFR) of massive star-forming galaxies () from to 7. Our method is substantially different…
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 Outer Halo of the Milky Way as Probed by RR Lyr Variables from the Palomar Transient Facility
Judith Cohen, Branimir Sesar, Sophianna Bahnolzer +5
RR Lyr stars are ideal massless tracers that can be used to study the total mass and dark matter content of the outer halo of the Milky Way. This is because they are easy to find i…