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- S. Nishida3 profiles241 · h 54
- S. Stanič2 profiles237 · h 70
- M. Bračko2 profiles235 · h 73
- G. Varner2 profiles233 · h 84
- S. Uno2 profiles227 · h 74
- K. Senyo2 profiles223 · h 72
- Y. Sakai2 profiles221 · h 79
- T. Sumiyoshi2 profiles217 · h 76
- M. Starič2 profiles216 · h 66
- H. Miyata2 profiles214 · h 75
- G. Pakhlova2 profiles210 · h 64
- D. Liventsev2 profiles209 · h 71
- Jožef Stefan InstituteSI348 papers
- Institute of Nuclear Physics, Polish Academy of SciencesPL315 papers
- University of LjubljanaSI293 papers
- University of Hawaii SystemUS291 papers
- Nagoya UniversityJP283 papers
- The University of TokyoJP276 papers
- Institute for High Energy PhysicsES274 papers
- University of Hawaiʻi at MānoaUS267 papers
- École Polytechnique Fédérale de LausanneCH253 papers
- University of MariborSI253 papers
- Karlsruhe Institute of TechnologyDE252 papers
- Sungkyunkwan UniversityKR252 papers
25 papers · 1 filter
Euclid Quick Data Release (Q1) Euclid spectroscopy of quasars. 2. Physical properties from spectral fitting
Euclid Collaboration, J. Calhau, G. Calderone +312
A substantial volume of spectroscopic data has become available with the Euclid Data Release (Q1), which represents a unique opportunity to study quasars (QSOs) in the Euclid Deep…
Euclid. A two-point correlation approach to diagnosing star-related systematics in the Euclid spectroscopic survey
Euclid Collaboration, I. Risso, B. R. Granett +298
The Euclid spectroscopic survey will measure galaxy clustering with unprecedented precision, requiring stringent control of observational and instrumental systematics. Star-related…
Euclid preparation. The shape of halo profiles in CDM and non-standard cosmologies
Euclid Collaboration, L. Pizzuti, G. Y. Ferron +304
We study the shape of three-dimensional and projected dark-matter halo profiles extracted from cosmological -body simulations in CDM and non-standard cosmologies, using the \…
Physically motivated AGN emissivity profiles and their effects on quasar microlensing signatures. 1. Multi-epoch accretion disc size inference
Scott Hagen, Carina Fian
Quasar microlensing is uniquely sensitive to the size-scale of the accretion flow, offering one of the few direct probes of the accretion structure on micro-arcsecond scales. Howev…
Euclid Quick Data Release (Q1): The geometry of dark matter halos from extragalactic streams
Euclid Collaboration, N. Starkman, J. Nibauer +295
Wide-field surveys like Euclid mark a new era of extragalactic stellar stream studies. With a large number of streams, it is now possible to constrain the dark matter halos of gala…
Detection of persistent helium absorption in the 91bg-like type Ia Supernova 2022an
Ping Chen, Avishay Gal-Yam, Subo Dong +14
We present optical and near-infrared observations of the fast-declining Type Ia supernova (SN Ia) 2022an. The photometric and spectroscopic properties identify it as a standard 91b…