10.9k citations
- Johannes Gutenberg University MainzDE216 papers
- Joint Institute for Nuclear ResearchRU216 papers
- Uppsala UniversitySE215 papers
- Indiana University BloomingtonUS212 papers
- Shandong UniversityCN212 papers
- University of Science and Technology of ChinaCN210 papers
- Nanjing UniversityCN207 papers
- Budker Institute of Nuclear PhysicsRU206 papers
- Istituto Nazionale di Fisica Nucleare, Laboratori Nazionali di FrascatiIT199 papers
- Justus-Liebig-Universität GießenDE197 papers
- Institute of High Energy PhysicsCN194 papers
- Siberian Branch of the Russian Academy of SciencesRU191 papers
5 papers · 1 filter
One-neutron transfer reaction in the O + Ti collision at 275 MeV
O. Sgouros, M. Cutuli, F. Cappuzzello +29
The present article reports new data on the Ti(O,O)Ti reaction at 275 MeV incident energy as part of the systematic research pursued within the NUMEN pr…
Multi-Modal Multi-Task (3MT) Road Segmentation
Erkan Milli, Özgür Erkent, Asım Egemen Yılmaz
Multi-modal systems have the capacity of producing more reliable results than systems with a single modality in road detection due to perceiving different aspects of the scene. We…
Surface structure of 45 Hercules: An otherwise unremarkable Ap star with a surprisingly weak magnetic field
O. Kochukhov, H. Gürsoytrak Mutlay, A. M. Amarsi +3
The origin of magnetic fields and their role in chemical spot formation on magnetic Ap stars is currently not understood. Here we contribute to solving this problem with a detailed…
A Search for Chemical Anomalies of Seven A-types Stars
Yahya Nasolo, Şeyma Çalışkan
We present a chemical abundance analysis of seven A-type stars with no detailed chemical abundance measurements in the literature. High-resolution spectra of the targets HD 2924, H…
Transit timing variation analysis of the low-mass brown dwarf KELT-1 b
Ö. Baştürk, J. Southworth, S. Yalçınkaya +8
We investigate whether there is a variation in the orbital period of the short-period brown dwarf-mass KELT-1\,b, which is one of the best candidates to observe orbital decay. We o…