activity
20112022
most citedMOA-2011-BLG-293Lb: A test of pure survey microlensing planet detections

235 citations · 1.7k across the 36 of their papers we have counts for

collaborators

37 papers

astro-ph.SR2022★ 30 cited

The VLT-FLAMES Tarantula Survey: Observational evidence for two distinct populations of massive runaway stars in 30 Doradus

H. Sana, O. H. Ramírez-Agudelo, V. Hénault-Brunet +17

Two main scenarios have been proposed for origin of massive runaway stars -- dynamical ejection or release from a binary at the first core collapse -- but their relative contributi…

astro-ph.SR2022★ 7 cited

Distance and age of the massive stellar cluster Westerlund 1. II. The eclipsing binary W36

Danilo F. Rocha, Leonardo A. Almeida, Augusto Damineli +3

Westerlund 1 (Wd 1) is one of the most relevant star clusters in the Milky Way to study massive star formation, although it is still poorly known. Here, we used photometric and spe…

astro-ph.HE2022★ 98 cited

An X-ray quiet black hole born with a negligible kick in a massive binary within the Large Magellanic Cloud

Tomer Shenar, Hugues Sana, Laurent Mahy +35

Stellar-mass black holes are the final remnants of stars born with more than 15 solar masses. Billions are expected to reside in the Local Group, yet only few are known, mostly det…

astro-ph.SR2022★ 19 cited

Distance and age of the massive stellar cluster Westerlund 1. I. Parallax method using Gaia-EDR3

Felipe Navarete, Augusto Damineli, Aura E. Ramirez +2

Westerlund 1 (Wd 1) is one of the most massive young star clusters in the Milky Way. Although relevant for star formation and evolution, its fundamental parameters are not yet very…

astro-ph.SR2022★ 11 cited

Rotation signature of TESS B-type stars. A comprehensive analysis

L. F. Barraza, R. L. Gomes, Y. S. Messias +11

Stellar rotation is a fundamental observable that drives different aspects of stellar and planetary evolution. In this work, we present an unprecedented manifold analysis of 160 B-…

astro-ph.SR2022

An Isolated Stellar-Mass Black Hole Detected Through Astrometric Microlensing

Kailash C. Sahu, Jay Anderson, Stefano Casertano +90

We report the first unambiguous detection and mass measurement of an isolated stellar-mass black hole (BH). We used the Hubble Space Telescope (HST) to carry out precise astrometry…

astro-ph.SR2021★ 9 cited

Probing the low-mass end of the companion mass function for O-type stars

M. Reggiani, A. Rainot, H. Sana +6

Almost all massive stars are part of a binary system. Given the wide range of separations at which these companions are found, several observational techniques have been adopted to…

astro-ph.SR2021★ 42 cited

The B-type Binaries Characterisation Programme I. Orbital solutions for the 30 Doradus population

J. I. Villaseñor, W. D. Taylor, C. J. Evans +6

We present results from the B-type Binaries Characterisation (BBC) programme, a multi-epoch spectroscopic study of 88 early B-type binary candidates in the 30 Doradus region of the…

astro-ph.SR2021★ 34 cited

Constraining the Overcontact Phase in Massive Binary Evolution I. Mixing in V382 Cyg, VFTS 352, and OGLE SMC-SC10 108086

Michael Abdul-Masih, Hugues Sana, Calum Hawcroft +10

As potential progenitors of several exotic phenomena including gravitational wave sources, magnetic stars, and Be stars, close massive binary systems probe a crucial area of the pa…

astro-ph.SR2021★ 7 cited

Search for magnetic accretion in SW Sextantis systems

I. J. Lima, C. V. Rodrigues, C. E. Ferreira Lopes +9

SW Sextantis systems are nova-like cataclysmic variables that have unusual spectroscopic properties, which are thought to be caused by an accretion geometry having part of the mass…

astro-ph.SR2020

A search for rotation periods in 1000 TESS objects of interest

Bruno L. Canto Martins, Roseane L. Gomes, Yuri S. Messias +8

The high quality light curves from the Transiting Exoplanet Survey Satellite (TESS) represent a unique laboratory for the study of stellar rotation, a fundamental observable drivin…

astro-ph.SR2020

The Carina High-Contrast Imaging Project for massive Stars (CHIPS) I. Methodology and proof of concept on QZ Car ( HD93206)

A. Rainot, M. Reggiani, H. Sana +13

Massive stars like company. However, low-mass companions have remained extremely difficult to detect at angular separations () smaller than 1" (~1000-3000 au considering typical…

astro-ph.SR2020★ 13 cited

Exploratory Spectroscopy of Magnetic Cataclysmic Variables Candidates and Other Variable Objects II

Alexandre S. Oliveira, Claudia V. Rodrigues, Murilo Martins +4

This is the second paper of a series presenting our search for magnetic Cataclysmic Variables (mCVs) among candidates selected mostly from the Catalina Real-Time Transient Survey (…

astro-ph.SR2019★ 67 cited

The Tarantula Massive Binary Monitoring: III. Atmosphere analysis of double-lined spectroscopic systems

L. Mahy, H. Sana, M. Abdul-Masih +17

Accurate stellar parameters of individual objects in binary systems are essential to constrain the effects of binarity on stellar evolution. These parameters serve as a prerequisit…

astro-ph.SR2019★ 49 cited

The Tarantula Massive Binary Monitoring. IV. Double-lined photometric binaries

L. Mahy, L. A. Almeida, H. Sana +10

A high fraction of massive stars are found to be binaries but only a few of them are reported as photometrically variable. By studying the populations of SB2 in the 30 Doradus regi…

astro-ph.SR2019★ 109 cited

Properties of OB star-black hole systems derived from detailed binary evolution models

N. Langer, C. Schürmann, K. Stoll +38

The recent gravitational wave measurements have demonstrated the existence of stellar mass black hole binaries. It is essential for our understanding of massive star evolution to i…

astro-ph.GA2019★ 205 cited

The Southern Photometric Local Universe Survey (S-PLUS): improved SEDs, morphologies and redshifts with 12 optical filters

C. Mendes de Oliveira, T. Ribeiro, W. Schoenell +142

The Southern Photometric Local Universe Survey (S-PLUS) is imaging ~9300 deg^2 of the celestial sphere in twelve optical bands using a dedicated 0.8 m robotic telescope, the T80-So…

astro-ph.SR2019★ 43 cited

Clues on the Origin and Evolution of Massive Contact Binaries: Atmosphere Analysis of VFTS 352

Michael Abdul-Masih, Hugues Sana, Jon Sundqvist +10

The massive O4.5 V + O5.5 V binary VFTS 352 in the Tarantula nebula is one of the shortest-period and most massive overcontact binaries known. Recent theoretical studies indicate t…

astro-ph.SR2019★ 15 cited

Orbital period variation of KIC 10544976: Applegate mechanism versus light travel time effect

Leonardo A. Almeida, Leandro de Almeida, Augusto Damineli +6

In recent years, several close post-common-envelope eclipsing binaries have been found to show cyclic eclipse timing variations (ETVs). This effect is usually interpreted either as…

astro-ph.SR2017★ 12 cited

HS 2231+2441: an HW Vir system composed by a low-mass white dwarf and a brown dwarf

Leonardo A. Almeida, Augusto Damineli, Cláudia V. Rodrigues +2

HW Vir systems are rare evolved eclipsing binaries composed by a hot compact star and a low-mass main-sequence star in a close orbit. These systems provide a direct way to measure…

astro-ph.EP2017★ 9 cited

Multi-band characterization of the hot Jupiters: WASP-5b, WASP-44b and WASP-46b

M. Moyano, L. A. Almeida, C. von Essen +2

We have carried out a campaign to characterize the hot Jupiters WASP-5b, WASP-44b and WASP-46b using multiband photometry collected at the Observatório do Pico Dos Dias in Brazil.…

astro-ph.SR2016★ 154 cited

The Tarantula Massive Binary Monitoring: I. Observational campaign and OB-type spectroscopic binaries

L. A. Almeida, H. Sana, W. Taylor +24

Massive binaries (MBs) play a crucial role in the Universe. Knowing the distributions of their orbital parameters (OPs) is important for a wide range of topics, from stellar feedba…

astro-ph.SR2016★ 23 cited

Exploratory Spectroscopy of Magnetic Cataclysmic Variables Candidates and Other Variable Objects

A. S. Oliveira, C. V. Rodrigues, D. Cieslinski +5

The increasing number of synoptic surveys made by small robotic telescopes, such as the photometric Catalina Real-Time Transient Survey (CRTS), represents a unique opportunity for…

astro-ph.SR2015★ 74 cited

Discovery of the massive overcontact binary VFTS 352: Evidence for enhanced internal mixing

L. A. Almeida, H. Sana, S. E. de Mink +15

The contact phase expected to precede the coalescence of two massive stars is poorly characterized due to the paucity of observational constraints. Here we report on the discovery…