output
20062023
most citedStudy of the gp-->etap reaction with the Crystal Ball detector at the Mainz Microtron(MAMI-C)

126 citations

Showing 2019Show all

7 papers · 1 filter

math.CO2019

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…

hep-ph20198 cited

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…

astro-ph.SR20197 cited

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…

astro-ph.SR2019125 cited

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…

astro-ph.GA20199 cited

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…

astro-ph.SR201958 cited

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…