590 citations
Counting papers with at most 25 authors, so collaboration author lists do not stand in for the people here.
- University of GlasgowGB65 papers
- George Washington UniversityUS64 papers
- Johannes Gutenberg University MainzDE59 papers
- University of BonnDE58 papers
- University of BaselCH56 papers
- Kent State UniversityUS55 papers
- Istituto Nazionale di Fisica Nucleare, Sezione di PaviaIT54 papers
- Institute for Nuclear ResearchRU51 papers
- Ruđer Bošković InstituteHR50 papers
- University of California, Los AngelesUS50 papers
- University of EdinburghGB49 papers
- P.N. Lebedev Physical Institute of the Russian Academy of SciencesRU41 papers
13 papers · 1 filter
A Note on the Parallel Cleaning of Cliques
Alejandro Angeli Ayello, Margaret-Ellen Messinger
We disprove a conjecture proposed in [Gaspers et al., Discrete Applied Mathematics, 2010] and provide a new upper bound for the minimum number of brushes required to continually pa…
Re-examination of the rare decay using holographic light-front QCD
Mohammad Ahmady, Spencer Keller, Michael Thibodeau +1
We calculate the Standard Model (SM) predictions for the differential branching ratio of the rare decays using transition form factors (TFFs) obtaine…
Signatures of the hexaquark in d(,)
M. Bashkanov, D. P. Watts, S. J. D. Kay +74
We report a measurement of the spin polarisation of the recoiling neutron in deuterium photodisintegration, utilising a new large acceptance polarimeter within the Crystal Ball at…
Rotational and pulsational variability in the TESS light curve of HD27463
V. Khalack, C. Lovekin, D. M. Bowman +8
The new photometric data on pulsating Ap star HD~27463 obtained recently with the Transiting Exoplanet Survey Satellite (\textit{TESS}) are analysed to search for variability. Our…
The first view of Scuti and Doradus stars with the TESS mission
V. Antoci, M. S. Cunha, D. M. Bowman +63
We present the first asteroseismic results for Scuti and Doradus stars observed in Sectors 1 and 2 of the TESS mission. We utilise the 2-min cadence TESS data for a sample…
Spin polarizabilities of the proton by measurement of Compton double-polarization observables
D. Paudyal, P. P. Martel, G. M. Huber +90
The Compton double-polarization observable has been measured for the first time in the resonance region using a circularly polarized photon beam incident on a lo…
Cross Section for measured at Mainz/A2
W. J. Briscoe, M. Hadzimehmedovi, A. E. Kudryavtsev +89
The differential cross section evaluated for 27 energy bins span the photon-energy range 290-813 MeV (W = 1.195-1.553 GeV) and the pion c.m. polar production angles,…
Predicting the light-front holographic TMDs of the pion
Mohammad Ahmady, Chandan Mondal, Ruben Sandapen
We predict the twist-2 Transverse Momentum Dependent parton distribution functions (TMDs) of the pion, namely the unpolarized quark TMD, , and the transversely p…
Measurement of the beam-helicity asymmetry in photoproduction of pairs on carbon, aluminum, and lead
V. Sokhoyan, S. Prakhov, A. Fix +88
The beam-helicity asymmetry was measured, for the first time, in photoproduction of pairs on carbon, aluminum, and lead, with the A2 experimental setup at MAMI. The result…
The Non-m-Positive Dimension of a Positive Linear Map
Nathaniel Johnston, Benjamin Lovitz, Daniel Puzzuoli
We introduce a property of a matrix-valued linear map that we call its "non-m-positive dimension" (or "non-mP dimension" for short), which measures how large a subspace can be…
LARgE Survey. I. Dead Monsters: the Massive End of the Passive Galaxy Stellar Mass Function at Cosmic Noon
Liz Arcila-Osejo, Marcin Sawicki, Stephane Arnouts +3
We introduce the largest to date survey of massive quiescent galaxies at redshift z~1.6. With these data, which cover 27.6 deg^2, we can find significant numbers of very rare objec…
Magnetic OB[A] Stars with TESS: probing their Evolutionary and Rotational properties (MOBSTER) - I. First-light observations of known magnetic B and A stars
A. David-Uraz, C. Neiner, J. Sikora +21
In this paper we introduce the MOBSTER collaboration and lay out its scientific goals. We present first results based on the analysis of nineteen previously known magnetic O, B and…
Diverse Variability of O and B Stars Revealed from 2-minute Cadence Light Curves in Sectors 1 and 2 of the TESS Mission: Selection of an Asteroseismic Sample
May G. Pedersen, Sowgata Chowdhury, Cole Johnston +18
Uncertainties in stellar structure and evolution theory are largest for stars undergoing core convection on the main sequence. A powerful way to calibrate the free parameters used…