From the 1 of 1.8k papers with an AI index.
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- University of Science and Technology of ChinaCN557 papers
- Joint Institute for Nuclear ResearchRU490 papers
- Johannes Gutenberg University MainzDE480 papers
- Brookhaven National LaboratoryUS460 papers
- University of ManchesterGB437 papers
- Michigan State UniversityUS431 papers
- Uppsala UniversitySE424 papers
- University of WashingtonUS408 papers
- Centre National de la Recherche ScientifiqueFR385 papers
- Charles UniversityCZ378 papers
- Fermi National Accelerator LaboratoryUS378 papers
- University of MichiganUS377 papers
45 papers · 1 filter
The HST large programme on NGC 6752 -- IV. The White Dwarf Sequence
L. R. Bedin, M. Salaris, J. Anderson +13
We present our final study of the white dwarf cooling sequence (WD CS) in the globular cluster NGC 6752. The investigation is the main goal of a dedicated Hubble Space Telescope la…
X-ray Sources in the SSA22 Chandra Field
Brandon T. Radzom, Anthony J. Taylor, Amy J. Barger +1
The Hawaii Survey Field SSA22 is the fourth deepest Chandra X-ray field. To allow for the fullest exploration of this field, we present new optical spectroscopy from Keck/DEIMOS an…
Improved measurement of the strong-phase difference in quantum-correlated decays
BESIII Collaboration, M. Ablikim, M. N. Achasov +568
The decay is studied in a sample of quantum-correlated pairs, based on a data set corresponding to an integrated luminosity of 2.93\,fb collected at…
The Development of the NNBAR Experiment
F. Backman, J. Barrow, Y. Beßler +40
The NNBAR experiment for the European Spallation Source will search for free neutrons converting to antineutrons with a sensitivity improvement of three orders of magnitude compare…
The role of rotation on the formation of second generation stars in globular clusters
Elena Lacchin, Francesco Calura, Enrico Vesperini +1
By means of 3D hydrodynamic simulations, we explore the effects of rotation in the formation of second-generation (SG) stars in globular clusters (GC). Our simulations follow the S…
SFR estimations from z=0 to z=0.9 -- A comparison of SFR calibrators for star-forming galaxies
M. Figueira, A. Pollo, K. Małek +7
Using VIPERS, we estimated a set of SFR based on photometric and spectroscopic data. We used, as estimators, photometric bands from ultraviolet to mid-infrared, and spectral lines.…