most citedPhysics Of Eclipsing Binaries. II. Towards the Increased Model Fidelity

326 citations · 439 across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph.SR201754 cited

The Most Massive Heartbeat: An In-depth Analysis of ι Orionis

Herbert Pablo, N. D. Richardson, J. Fuller +17

ι Ori is a well studied massive binary consisting of an O9 III + B1 III/IV star. Due to its high eccentricity (e = 0.764) and short orbital period (P orb = 29.13376 d), it has been…

astro-ph.SR2016

Magnetic B stars observed with BRITE: Spots, magnetospheres, binarity, and pulsations

G. A. Wade, D. H. Cohen, C. Fletcher +16

Magnetic B-type stars exhibit photometric variability due to diverse causes, and consequently on a variety of timescales. In this paper we describe interpretation of BRITE photomet…

astro-ph.SR20164 cited

Pulsations and outbursts in Be stars: Small differences - big impacts

D. Baade, Th. Rivinius, A. Pigulski +12

New high-cadence observations with BRITE covering many months confirm that coupled pairs of nonradial pulsation modes are widespread among early-type Be stars. With the difference…

astro-ph.SR20161 cited

Preparing and correcting extracted BRITE observations

B. Buysschaert, H. Pablo, C. Neiner

Extracted BRITE lightcurves must be carefully prepared and corrected for instrumental effects before a scientific analysis can be performed. Therefore, we have created a suite of P…

astro-ph.SR201632 cited

Combining BRITE and ground-based photometry for the Beta Cephei star Nu Eridani: impact on photometric pulsation mode identification and detection of several g modes

G. Handler, M. Rybicka, A. Popowicz +12

We report a simultaneous ground and space-based photometric study of the Beta Cephei star Nu Eridani. Half a year of observations have been obtained by four of the five satellites…

astro-ph.SR2016326 cited

Physics Of Eclipsing Binaries. II. Towards the Increased Model Fidelity

Andrej Prša, Kyle E. Conroy, Martin Horvat +6

The precision of photometric and spectroscopic observations has been systematically improved in the last decade, mostly thanks to space-borne photometric missions and ground-based…