activity
20102026
most citedMINDS. Abundant water and varying C/O across the disk of Sz 98 as seen by JWST/MIRI

66 citations · 294 across the 16 of their papers we have counts for

collaborators

16 papers

astro-ph.EP2026

CAFE follow-up of TESS hot Jupiter candidates left behind: I. Five newly confirmed planets and a false positive

J. Lillo-Box, C. Cifuentes, O. Balsalobre-Ruza +56

Hot Jupiters are key targets for understanding planet formation, migration, and atmospheres. Yet, most ground-based follow-up resources for the TESS mission are focused on confirmi…

astro-ph.EP2024★ 23 cited

MINDS. JWST-MIRI reveals a peculiar CO-rich chemistry in the drift-dominated disk CX Tau

Marissa Vlasblom, Milou Temmink, Sierra L. Grant +20

Radial drift of icy pebbles can have a large impact on the chemistry of the inner regions of protoplanetary disks. Compact dust disks (50 au) are suggested to have a high…

astro-ph.EP2024★ 27 cited

MINDS. A multi-instrument investigation into the molecule-rich JWST-MIRI spectrum of the DF Tau binary system

Sierra L. Grant, Nicolas T. Kurtovic, Ewine F. van Dishoeck +26

Most stars form in multiple systems whose properties can significantly impact circumstellar disk evolution. We investigate the physical and chemical properties of the equal-mass, s…

astro-ph.SR2024

ExoplANETS-A: A VO database for host stars and planetary systems: The effect of XUV on planet atmospheres

M. Morales-Calderón, S. R. G. Joyce, J. P. Pye +12

ExoplANETS-A is an EU Horizon-2020 project with the primary objective of establishing new knowledge on exoplanet atmospheres. Intimately related to this topic is the study of the h…

astro-ph.EP2024★ 11 cited

The AstraLux-TESS high-spatial resolution imaging survey. Search for stellar companions of 215 planet candidates from TESS

J. Lillo-Box, M. Morales-Calderón, D. Barrado +6

Chance-aligned sources or blended companions can cause false positives in planetary transit detections or simply bias the determination of the candidate properties. In the era of h…

astro-ph.EP2024

Signs of magnetic star-planet interactions in HD 118203. TESS detects stellar variability that matches the orbital period of a close-in eccentric Jupiter-sized companion

A. Castro-González, J. Lillo-Box, A. C. M. Correia +4

Planetary systems with close-in giant planets can experience magnetic star-planet interactions that modify the activity levels of their host stars. The induced activity is known to…

astro-ph.EP2023★ 66 cited

MINDS. Abundant water and varying C/O across the disk of Sz 98 as seen by JWST/MIRI

Danny Gasman, Ewine F. van Dishoeck, Sierra L. Grant +41

MIRI/MRS on board the JWST allows us to probe the inner regions of protoplanetary disks. Here we examine the disk around the classical T Tauri star Sz 98, which has an unusually la…

astro-ph.EP2023★ 23 cited

Two Warm Neptunes transiting HIP 9618 revealed by TESS & Cheops

Hugh P. Osborn, Grzegorz Nowak, Guillaume Hébrard +126

HIP 9618 (HD 12572, TOI-1471, TIC 306263608) is a bright ( mag) solar analogue. TESS photometry revealed the star to have two candidate planets with radii of …

astro-ph.EP2022★ 23 cited

The KOBE experiment: K-dwarfs Orbited By habitable Exoplanets. Project goals, target selection and stellar characterization

J. Lillo-Box, N. C. Santos, A. Santerne +33

The detection of habitable worlds is one of humanity's greatest endeavors. So far, astrobiological studies show that one of the most critical components for life development is liq…

astro-ph.SR2022★ 39 cited

Lithium depletion boundary, stellar associations, and Gaia

F. J. Galindo-Guil, D. Barrado, H. Bouy +9

Stellar ages are key to improving our understanding of different astrophysical phenomena. However, many techniques to estimate stellar ages are highly model-dependent. The lithium…

astro-ph.SR2017★ 9 cited

Early phases in the stellar and substellar formation and evolution: Infrared and submillimeter data in the Barnard 30 dark cloud

D. Barrado, I. de Gregorio-Monsalvo, N. Huélamo +10

The early evolutionary stage of brown dwarfs are not very well characterized, specially during the embedded phase. To gain insight into the dominant formation mechanism of very low…

astro-ph.SR2013★ 50 cited

CoRoT 223992193: A new, low-mass, pre-main sequence eclipsing binary with evidence of a circumbinary disk

Edward Gillen, Suzanne Aigrain, Amy McQuillan +12

We present the discovery of CoRoT 223992193, a double-lined, detached eclipsing binary, comprising two pre-main sequence M dwarfs, discovered by the CoRoT space mission during a 23…

astro-ph.SR2013

The substellar content of the ONC

Holger Drass, Rolf Chini, Dieter Nürnberger +5

The Substellar Initial Mass Function (SIMF) of many star-forming regions is still poorly known but the detailed knowledge of its shape will help to distinguish among the substellar…

astro-ph.SR2012★ 16 cited

Potential Drivers of Mid-Infrared Variability in Young Stars: testing physical models with multi-epoch near-infrared spectra of YSOs in ρ Oph

Christopher M. Faesi, Kevin R. Covey, Robert Gutermuth +6

Recent studies have identified several young stellar objects (YSOs) which exhibit significant mid-infrared (mid-IR) variability. A wide range of physical mechanisms may be responsi…

astro-ph.SR2010

Young Stars in the Time Domain: A Cool Stars 16 Splinter Summary

Kevin R. Covey, Peter Plavchan, Fabienne Bastien +6

Variability is a defining characteristic of young stellar systems, and optical variability has been heavily studied to select and characterize the photospheric properties of young…

astro-ph.SR2010★ 7 cited

The low-mass diskless population of Corona Australis

Belén López Martí, Loredana Spezzi, Bruno Merín +4

We combine published optical and near-infrared photometry to identify new low-mass candidate members in an area of about 0.64 deg^2 in Corona Australis, using the S-parameter metho…