1.8k citations
- H. Miyata2 profiles41 · h 75
- D. Liventsev2 profiles40 · h 71
- G. Varner2 profiles40 · h 84
- T. Sumiyoshi2 profiles40 · h 76
- Y. Sakai2 profiles40 · h 79
- C. Schwanda2 profiles39 · h 71
- F. Simon2 profiles39 · h 82
- H. Aihara2 profiles39 · h 85
- K. Senyo2 profiles39 · h 72
- E. Won2 profiles38 · h 74
- H. Hayashii2 profiles38 · h 75
- T. Aushev2 profiles38 · h 89
- Technical University of MunichDE190 papers
- Ludwig-Maximilians-Universität MünchenDE108 papers
- Max Planck Institute for Extraterrestrial PhysicsDE103 papers
- Centre National de la Recherche ScientifiqueFR78 papers
- European Southern ObservatoryCL73 papers
- The University of TokyoJP69 papers
- Institute for Theoretical and Experimental PhysicsRU58 papers
- Institute for High Energy PhysicsES56 papers
- University of Hawaii SystemUS56 papers
- Chinese Academy of SciencesCN54 papers
- Institute of Nuclear Physics, Polish Academy of SciencesPL54 papers
- The University of MelbourneAU53 papers
4 papers · 1 filter
Physically motivated X-ray obscurer models
Johannes Buchner, Murray Brightman, Mislav Baloković +3
The nuclear obscurer of Active Galactic Nuclei (AGN) is poorly understood in terms of its origin, geometry and dynamics. We investigate whether physically motivated geometries emer…
Modelling H and its effects on star formation using a joint implementation of GADGET-3 and KROME
Emanuel Sillero, Patricia B. Tissera, Diego G. Lambas +5
We present P-GADGET3-K, an updated version of GADGET3, that incorporates the chemistry package KROME. P-GADGET3-K follows the hydrodynamical and chemical evolution of cosmic struct…
HD344787: a true Polaris analogue?
V. Ripepi, G. Catanzaro, L. Molnár +10
Classical Cepheids (DCEPs) are the most important primary indicators for the extragalactic distance scale, but they are also important objects per se, allowing us to put constraint…
The VANDELS ESO public spectroscopic survey: final Data Release of 2087 spectra and spectroscopic measurements
B. Garilli, R. McLure, L. Pentericci +94
VANDELS is an ESO Public Spectroscopic Survey designed to build a sample of high signal to noise, medium resolution spectra of galaxies at redshift between 1 and 6.5. Here we prese…