90 citations · 149 across the 5 of their papers we have counts for
5 papers
ACRONYM IV: Three New, Young, Low-mass Spectroscopic Binaries
Laura Flagg, Evgenya L. Shkolnik, Alycia Weinberger +4
As part of our search for new low-mass members of nearby young moving groups (YMG), we discovered three low-mass, spectroscopic binaries, two of which are not kinematically associa…
Investigating the multiwavelength behaviour of the flat spectrum radio quasar CTA 102 during 2013-2017
F. D'Ammando, C. M. Raiteri, M. Villata +94
We present a multiwavelength study of the flat-spectrum radio quasar CTA 102 during 2013-2017. We use radio-to-optical data obtained by the Whole Earth Blazar Telescope, 15 GHz dat…
Asteroid Photometry from the Transiting Exoplanet Survey Satellite: A Pilot Study
A. McNeill, M. Mommert, D. E. Trilling +2
The {\it Transiting Exoplanet Survey Satellite} (TESS) searches for planets transiting bright and nearby stars using high-cadence, large-scale photometric observations. Full Frame…
Asteroid pairs: a complex picture
P. Pravec, P. Fatka, D. Vokrouhlický +45
We studied 93 asteroid pairs. We estimated times elapsed since separation of pair members that are between 7*10^3 and a few 10^6 yr. We derived the rotation periods for all the pri…
Non-Vestoid candidate asteroids in the inner main belt
Dagmara Oszkiewicz, Brian A. Skiff, Nick Moskovitz +5
Most Howardite-Eucrite-Diogenite (HED) meteorites (analogs to V-type asteroids) are thought to originate from asteroid (4) Vesta. However, some HEDs show distinct oxygen isotope ra…