activity
19972026
most citedMAMBO Mapping of Spitzer c2d Small Clouds and Cores

625 citations · 7.7k across the 122 of their papers we have counts for

collaborators
Showing 2020Show all

7 papers · 1 filter

astro-ph.HE2020★ 12 cited

Long-term X-ray Variability of the Symbiotic System RT Cru based on Chandra Spectroscopy

A. Danehkar, M. Karovska, J. J. Drake +1

RT Cru belongs to the rare class of hard X-ray emitting symbiotics, whose origin is not yet fully understood. In this work, we have conducted a detailed spectroscopic analysis of X…

astro-ph.GA2020★ 60 cited

Preliminary Target Selection for the DESI Milky Way Survey (MWS)

Carlos Allende Prieto, Andrew P. Cooper, Arjun Dey +31

The DESI Milky Way Survey (MWS) will observe 8 million stars between mag, supplemented by observations of brighter targets under poor observing conditions. The s…

astro-ph.SR2020★ 8 cited

Li-rich giant stars under scrutiny: Binarity, magnetic activity and the evolutionary status after Gaia DR2

B. F. O. Gonçalves, J. S. da Costa, L. de Almeida +2

We present a study of the evolutionary state of a few lithium-rich giant stars based on the Gaia DR2 parallaxes and photometry. We also investigate the chromospheric activity, the…

astro-ph.EP2020★ 21 cited

Is the gap in the DS Tau disc hiding a planet?

Benedetta Veronesi, Enrico Ragusa, Giuseppe Lodato +6

Recent mm-wavelength surveys performed with the Atacama Large Millimeter Array (ALMA) have revealed protoplanetary discs characterized by rings and gaps. A possible explanation for…

astro-ph.EP2020★ 18 cited

HATS-47b, HATS-48Ab, HATS-49b and HATS-72b: Four Warm Giant Planets Transiting K Dwarfs

J. D. Hartman, Andrés Jordán, D. Bayliss +43

We report the discovery of four transiting giant planets around K dwarfs. The planets HATS-47b, HATS-48Ab, HATS-49b, and HATS-72b have masses of ,…

astro-ph.SR2020★ 2 cited

Investigating Opacity Modifications and Reaction Rate Uncertainties to Resolve the Cepheid Mass Discrepancy

Joyce A. Guzik, Ebraheem Farag, Jakub Ostrowski +4

Cepheid masses derived from pulsations or binary dynamics are generally lower than those derived from stellar evolution models. Recent efforts have been dedicated to investigating…