856 citations
- J. Fynbo3 profiles14 · h 60
- A. Jensen13 · h 30
- E. Garrido3 profiles13 · h 19
- D. Fedorov11 · h 29
- B. Thomsen3 profiles10 · h 24
- H. Kjeldsen3 profiles9 · h 77
- J. Hjorth3 profiles9 · h 80
- M. Weidinger2 profiles9 · h 13
- P. Møller3 profiles9 · h 41
- H. Fynbo2 profiles8 · h 24
- J. Gorosabel2 profiles8 · h 67
- S. Hannestad8 · h 61
- University of CopenhagenDK18 papers
- Consejo Superior de Investigaciones CientíficasES15 papers
- European Southern ObservatoryCL13 papers
- Instituto de Estructura de la MateriaES13 papers
- Centre National de la Recherche ScientifiqueFR12 papers
- Lundbeck FoundationDK11 papers
- Instituto de Astrofísica de AndalucíaES8 papers
- The University of SydneyAU8 papers
- Max Planck Institute for PhysicsDE5 papers
- Space Telescope Science InstituteUS5 papers
- Universidad Autónoma de MadridES5 papers
- Universitat de ValènciaES5 papers
22 papers · 2 filters
The carbon-rich type Ic SN 2007gr: the photospheric phase
S. Valenti, N. Elias-Rosa, S. Taubenberger +20
The first two months of spectroscopic and photometric monitoring of the nearby type Ic SN 2007gr are presented. The very early discovery (less than 5 days after the explosion) and…
Ultra-high energy Neutrinos from Centaurus A and the Auger hot spot
Alessandro Cuoco, Steen Hannestad
The Pierre Auger collaboration has reported a correlation between Ultra-High Energy Cosmic Rays (UHECR) and nearby Active Galactic Nuclei (AGNs) within 75 Mpc. Two of these events…
Stroemgren metallicity calibration: the m1, b-y relation
A. Calamida, G. Bono, P. B. Stetson +15
We performed a new calibration of the Stroemgren metallicity index m1 based on the b-y color of cluster red giant stars. The current Metallicity-Index-Color relation is not linear…
Inter-comparison of the g-, f- and p-modes calculated using different oscillation codes for a given stellar model
A. Moya, J. Christensen-Dalsgaard, S. Charpinet +9
In order to make astroseismology a powerful tool to explore stellar interiors, different numerical codes should give the same oscillation frequencies for the same input physics. Th…
Oscillations in Procyon A: First results from a multi-site campaign
S. Hekker, T. Arentoft, H. Kjeldsen +45
Procyon A is a bright F5IV star in a binary system. Although the distance, mass and angular diameter of this star are all known with high precision, the exact evolutionary state is…
Disentangling neutrino-nucleon cross section and high energy neutrino flux with a km^3 neutrino telescope
E. Borriello, A. Cuoco, G. Mangano +4
The energy--zenith angular event distribution in a neutrino telescope provides a unique tool to determine at the same time the neutrino-nucleon cross section at extreme kinematical…