output
19922026
most citedSciPy 1.0--Fundamental Algorithms for Scientific Computing in Python

40.2k citations

Showing 2019 · astro-ph.EPShow all

42 papers · 2 filters

astro-ph.EP2019★ 63 cited

The widest H survey of accreting protoplanets around nearby transition disks

A. Zurlo, G. Cugno, M. Montesinos +6

The mechanisms of planet formation are still under debate. We know little about how planets form, even if more than 4000 exoplanets have been detected to date. Recent investigation…

astro-ph.EP2019★ 10 cited

XO-7 b: A transiting hot Jupiter with a massive companion on a wide orbit

Nicolas Crouzet, Brian F. Healy, Guillaume Hébrard +16

Transiting planets orbiting bright stars are the most favorable targets for follow-up and characterization. We report the discovery of the transiting hot Jupiter XO-7 b and of a se…

astro-ph.EP2019★ 67 cited

Shadowing and multiple rings in the protoplanetary disk of HD 139614

G. A. Muro-Arena, M. Benisty, C. Ginski +20

Shadows in scattered light images of protoplanetary disks are a common feature and support the presence of warps or misalignments between disk regions. These warps are possibly due…

astro-ph.EP2019★ 30 cited

TOI-132 b: A short-period planet in the Neptune desert transiting a G-type star

Matías R. Díaz, James S. Jenkins, Davide Gandolfi +45

The Neptune desert is a feature seen in the radius-mass-period plane, whereby a notable dearth of short period, Neptune-like planets is found. Here we report the {\it TESS} discove…

astro-ph.EP2019★ 28 cited

Gravity-Darkening Analysis of Misaligned Hot Jupiter MASCARA-4 b

John P. Ahlers, Ethan Kruse, Knicole D. Colon +17

MASCARA-4 b is a hot Jupiter in a highly-misaligned orbit around a rapidly-rotating A3V star that was observed for 54 days by the Transiting Exoplanet Survey Satellite (\tess). We…

astro-ph.EP2019★ 4 cited

Spitzer Space Telescope observations of bilobate comet 8P/Tuttle

O. Groussin, P. L. Lamy, M. S. P. Kelley +4

Comet 8P/Tuttle is a Nearly Isotropic Comet (NIC), whose physical properties are poorly known and could be different from those of Ecliptic Comets (EC) owing to their different ori…

astro-ph.EP2019★ 51 cited

The SOPHIE search for northern extrasolar planets. XVI. HD 158259: A compact planetary system in a near-3:2 mean motion resonance chain

N. C. Hara, F. Bouchy, M. Stalport +32

Since 2011, the SOPHIE spectrograph has been used to search for Neptunes and super-Earths in the Northern Hemisphere. As part of this observational program, 290 radial velocity mea…

astro-ph.EP2019★ 55 cited

WASP-127b transmission spectrum]{Abundance measurements of HO and carbon-bearing species in the atmosphere of WASP-127b confirm its super-solar metallicity

Jessica J. Spake, David K. Sing, Hannah R. Wakeford +14

The chemical abundances of exoplanet atmospheres may provide valuable information about the bulk compositions, formation pathways, and evolutionary histories of planets. Exoplanets…

astro-ph.EP2019★ 18 cited

HD 117214 debris disk: scattered-light images and constraints on the presence of planets

N. Engler, C. Lazzoni, R. Gratton +34

We performed observations of the Sco-Cen F star HD 117214 aiming at a search for planetary companions and the characterization of the debris disk structure. HD 117214 was observed…

astro-ph.EP2019★ 84 cited

VLT/SPHERE exploration of the young multiplanetary system PDS70

D. Mesa, M. Keppler, F. Cantalloube +51

Context. PDS 70 is a young (5.4 Myr), nearby (~113 pc) star hosting a known transition disk with a large gap. Recent observations with SPHERE and NACO in the near-infrared (NIR) al…

astro-ph.EP2019★ 21 cited

Near-Infrared Imaging of a Spiral in the CQ Tau Disk

Taichi Uyama, Takayuki Muto, Dimitri Mawet +28

We present -band Keck/NIRC2 imaging and -band Subaru/AO188+HiCIAO polarimetric observations of CQ Tau disk with a new spiral arm. Apart from the spiral feature our obs…

astro-ph.EP2019★ 47 cited

Exoplanet characterisation in the longest known resonant chain: the K2-138 system seen by HARPS

T. A. Lopez, S. C. C. Barros, A. Santerne +36

The detection of low-mass transiting exoplanets in multiple systems brings new constraints to planetary formation and evolution processes and challenges the current planet formatio…

astro-ph.EP2019★ 59 cited

Planet Hunters TESS I: TOI 813, a subgiant hosting a transiting Saturn-sized planet on an 84-day orbit

N. L. Eisner, O. Barragán, S. Aigrain +47

We report on the discovery and validation of TOI 813b (TIC 55525572 b), a transiting exoplanet identified by citizen scientists in data from NASA's Transiting Exoplanet Survey Sate…

astro-ph.EP2019★ 11 cited

First resolved observations of a highly asymmetric debris disc around HD 160305 with VLT/SPHERE

Clément Perrot, Philippe Thebault, Anne-Marie Lagrange +36

Context. Direct imaging of debris discs gives important information about their nature, their global morphology, and allows us to identify specific structures possibly in connectio…

astro-ph.EP2019★ 46 cited

An Exo-Kuiper Belt and An Extended Halo around HD 191089 in Scattered Light

Bin Ren, Élodie Choquet, Marshall D. Perrin +70

We have obtained Hubble Space Telescope STIS and NICMOS, and Gemini/GPI scattered light images of the HD 191089 debris disk. We identify two spatial components: a ring resembling K…

astro-ph.EP2019★ 55 cited

Nearly Polar orbit of the sub-Neptune HD3167 c: Constraints on a multi-planet system dynamical history

Shweta Dalal, Guillaume Hébrard, Alain Lecavelier des Étangs +5

We present the obliquity measurement, that is, the angle between the normal angle of the orbital plane and the stellar spin axis, of the sub-Neptune planet HD3167 c, which transits…

astro-ph.EP2019★ 5 cited

Kepler Object of Interest Network III. Kepler-82f: A new non-transiting $21 M_\bigoplus$ planet from photodynamical modelling

J. Freudenthal, C. von Essen, A. Ofir +13

Context. The Kepler Object of Interest Network (KOINet) is a multi-site network of telescopes around the globe organised for follow-up observations of transiting planet candidate K…

astro-ph.EP2019★ 10 cited

A multi-wavelength study of the debris disc around 49 Cet

Nicole Pawellek, Attila Moór, Julien Milli +17

In a multi-wavelength study of thermal emission and scattered light images we analyse the dust properties and structure of the debris disc around the A1-type main sequence star 49~…

astro-ph.EP2019★ 27 cited

Determining mass limits around HD163296 through SPHERE direct imaging data

D. Mesa, M. Langlois, A. Garufi +33

HD163296 is a Herbig Ae/Be star known to host a protoplanetary disk with a ringed structure. To explain the disk features, previous works proposed the presence of planets embedded…

astro-ph.EP2019★ 35 cited

The B-Star Exoplanet Abundance Study: a co-moving 16-25 Mjup companion to the young binary system HIP 79098

Markus Janson, Ruben Asensio-Torres, Damien Andre +13

Wide low-mass substellar companions are known to be very rare among low-mass stars, but appear to become increasingly common with increasing stellar mass. However, B-type stars, wh…

astro-ph.EP2019★ 13 cited

MASCARA-3b: A hot Jupiter transiting a bright F7 star in an aligned orbit

M. Hjorth, S. Albrecht, G. J. J. Talens +12

We report the discovery of MASCARA-3b, a hot Jupiter orbiting its bright (V = 8.33) late F-type host every days in an almost circular orbit ($e = 0.050^{+0.020…

astro-ph.EP2019★ 10 cited

From Centaurs to comets - 40 years

Nuno Peixinho, Audrey Thirouin, Stephen C. Tegler +4

In 1977, while Apple II and Atari computers were being sold, a tiny dot was observed in an inconvenient orbit. The minor body 1977 UB, to be named (2060) Chiron, with an orbit betw…

astro-ph.EP2019★ 57 cited

Optical polarized phase function of the HR\,4796A dust ring

J. Milli, N. Engler, H. M. Schmid +24

The scattering properties of the dust originating from debris discs are still poorly known. The analysis of scattered light is however a powerful remote-sensing tool to understand…

astro-ph.EP2019★ 37 cited

The meteorite flux of the last 2 Myr recorded in the Atacama desert

A. Drouard, J. Gattacceca, A. Hutzler +11

The evolution of the meteorite flux to the Earth can be studied by determining the terrestrial ages of meteorite collected in hot deserts. We have measured the terrestrial ages of…