activity
19992026
most citedSolar System objects observed with TESS -- First data release: bright main-belt and Trojan asteroids from the Southern Survey

91 citations · 1.4k across the 47 of their papers we have counts for

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Showing 2015Show all

6 papers · 1 filter

astro-ph.SR2015★ 64 cited

Extensive Spectroscopy and Photometry of the Type IIP Supernova 2013ej

G. Dhungana, R. Kehoe, J. Vinko +32

We present extensive optical (, , and open CCD) and near-infrared () photometry for the very nearby Type IIP SN ~2013ej extending from +1 to +461 days after…

astro-ph.HE2015★ 30 cited

The early phases of the type Iax supernova SN 2011ay

Tamás Szalai, József Vinkó, Krisztián Sárneczky +7

We present a detailed study of the early phases of the peculiar supernova 2011ay based on BVRI photometry obtained at Konkoly Observatory, Hungary, and optical spectra taken with t…

astro-ph.EP2015★ 16 cited

Physical properties of the extreme centaur and super-comet candidate 2013 AZ60

A. Pál, Cs. Kiss, J. Horner +12

We present estimates of the basic physical properties -- including size and albedo -- of the extreme Centaur 2013 AZ60. These properties have been derived from optical and thermal…

astro-ph.SR2015★ 15 cited

A new sdO+dM binary with extreme eclipses and reflection effect

A. Derekas, P. Nemeth, J. Southworth +10

We report the discovery of a new totally-eclipsing binary (RA=06:40:29.11; Dec=+38:56:52.2; J=2000.0; Rmax=17.2 mag) with an sdO primary and a strongly irradiated red dwarf compani…

astro-ph.SR2015★ 49 cited

Overtone and multi-mode RR Lyrae stars in the globular cluster M3

J. Jurcsik, P. Smitola, G. Hajdu +15

The overtone and multi-mode RR Lyrae stars in the globular cluster M3 are studied using a 200-d long, and time-series photometry obtained in 2012. 70\% of the…

astro-ph.EP2015★ 29 cited

Main-Belt Asteroids in the K2 Engineering Field of View

R. Szabó, K. Sárneczky, Gy. M. Szabó +6

Unlike NASA's original Kepler Discovery Mission, the renewed K2 Mission will stare at the plane of the Ecliptic, observing each field for approximately 75 days. This will bring new…