activity
19982025
most citedWASP-12b: The hottest transiting planet yet discovered

399 citations · 2.7k across the 43 of their papers we have counts for

collaborators

43 papers

astro-ph.SR2025

Discovery of the pre-main-sequence eclipsing binary MML 48

Y. Gómez Maqueo Chew, L. Hebb, H. C. Stempels +12

We present the discovery of the eclipsing binary MML 48, which is a member of Upper Centaurus Lupus, has an associated age of 16 Myr, and is composed of two young, low-mass stars.…

astro-ph.SR2019★ 7 cited

Fundamental properties of the pre-main sequence eclipsing stars of MML 53 and the mass of the tertiary

Y. Gómez Maqueo Chew, L. Hebb, H. C. Stempels +7

We present the most comprehensive analysis to date of the Upper Centaurus Lupus eclipsing binary MML 53 (2.097892 d), and for the first time, confirm the bound-nature of the third…

astro-ph.SR2018★ 13 cited

S Coronae Australis -- a T Tauri Twin

Gösta F. Gahm, Peter P. Petrov, Larisa V. Tambovtseva +3

The star S CrA is a tight visual binary consisting of two classical T Tauri stars, both with outstanding spectral characteristics and brightness variations. High-resolution spectra…

astro-ph.IM2016★ 56 cited

EELT-HIRES the high-resolution spectrograph for the E-ELT

A. Marconi, P. Di Marcantonio, V. D'Odorico +70

The first generation of E-ELT instruments will include an optical-infrared High Resolution Spectrograph, conventionally indicated as EELT-HIRES, which will be capable of providing…

astro-ph.SR2014★ 27 cited

Magnetic field topology and chemical spot distributions in the extreme Ap star HD 75049

O. Kochukhov, N. Rusomarov, J. A. Valenti +7

Intermediate-mass, magnetic chemically peculiar (Ap) stars provide a unique opportunity to study the topology of stellar magnetic fields in detail and to investigate magnetically d…

astro-ph.SR2014★ 15 cited

Doppler Probe of Accretion onto a T Tauri star

Peter P. Petrov, Gösta Gahm, Gregory J. Herczeg +2

The YY Ori stars are T Tauri stars with prominent time-variable redshifted absorption components that flank certain emission lines. One of the brightest in this class is S CrA, a v…