activity
20152026
most citedUncovering the true periods of the young sub-Neptunes orbiting TOI-2076

45 citations · 221 across the 19 of their papers we have counts for

collaborators

23 papers

astro-ph.GA2026

The JWST Proto-PAH project: Aromatic backbones with extensive aliphatic substitution account for both the aromatic and aliphatic emission

N. Clark, E. Peeters, J. Cami +18

We find that the aromatic and aliphatic emission bands in four carbon-rich post-asymptotic giant branch stars with class D emission arise from a single carrier population: extensiv…

astro-ph.SR2026

The JWST Proto-PAH Project: Detection of the methyl radical CH in the highly evolved C-rich object SMP LMC 011

Jialu Li, D. A. García-Hernández, A. Manchado +17

We report the first detection of the neutral methyl radical CH in a highly evolved C-rich object, SMP LMC 011, using JWST MIRI/MRS. CH is well fitted by an excitation tempe…

astro-ph.SR2026

Late-Time Evolution of the Massive Stellar Merger M101 OT2015-1

Marco A. Gómez-Muñoz, Nadejda Blagorodnova, Tomasz Kamiński +6

Luminous red novae (LRNe) are astronomical transients arising from unstable mass transfer and common envelope phases in close binary systems, culminating in stellar mergers. Their…

astro-ph.SR2026

Detection of unidentified molecular pure rotational lines in C-rich PNe I. The fullerene-containing PN IC 418

T. Huertas-Roldán, J. P. Fonfría, J. Alcolea +7

Molecular emission is observed in a wide variety of astrophysical environments, yet a substantial fraction of spectral features detected at mm wavelengths remains unidentified. Ide…

astro-ph.HE2026

A Faint Progenitor System for the Faint Supernova 2024vjm

Erez A. Zimmerman, Avishay Gal-Yam, Paul J. Groot +68

Type Ia Supernovae (SNe Ia) are well known for their role as standardizable cosmological candles. Their uniformity is credited to their single origin as thermonuclear explosions of…

astro-ph.SR2025★ 1 cited

Hot springs and dust reservoirs: JWST reveals the dusty, molecular aftermath of extragalactic stellar mergers

Viraj Karambelkar, Mansi Kasliwal, Ryan M. Lau +7

We present James Webb Space Telescope (JWST) observations of four Luminous Red Novae (LRNe): dusty, extragalactic transients from stellar mergers following common-envelope evolutio…

astro-ph.SR2025

An attempt to determine the magnetic field configuration in the planetary nebula K 3-35 with ALMA

L. Sabin, Q. Zhang, L. F. Miranda +1

We examined dust polarisation within the planetary nebula (PN) K 3-35 using the Atacama Large Millimeter/Submillimeter Array (ALMA). This investigation aimed to identify and trace…

astro-ph.IM2024★ 1 cited

CHEOPS in-flight performance: A comprehensive look at the first 3.5 years of operations

A. Fortier, A. E. Simon, C. Broeg +128

CHEOPS is a space telescope specifically designed to monitor transiting exoplanets orbiting bright stars. In September 2023, CHEOPS completed its nominal mission and remains in exc…

astro-ph.GA2024

Planetary Nebulae of the Large Magellanic Cloud I: A multiwavelength analysis

Silvia Tosi, Flavia Dell'Agli, Devika Kamath +5

Planetary nebulae (PNe) have three main components: a central star (CS), ionised gas and dust in the nebula. Each of them contains critical chemical fingerprints of their evolution…

astro-ph.SR2024★ 4 cited

Hydrogenated amorphous carbon grains as an alternative carrier of the 913m plateau feature in the fullerene planetary nebula Tc 1

M. A. Gómez-Muñoz, D. A. García-Hernández, R. Barzaga +2

Fullerenes have been observed in several astronomical objects since the discovery of C in the mid-infrared (mid-IR) spectrum of the planetary nebula (PN) Tc 1. It has been s…

astro-ph.SR2024

An ultraviolet spectral study of fullerene-rich planetary nebulae

M. A. Gómez-Muñoz, D. A. García-Hernández, A. Manchado +2

Several planetary nebulae (PNe) have been found to contain both polycyclic aromatic hydrocarbon (PAH-like) species and fullerenes (C) distinguished by their mid-infrared emi…

astro-ph.SR2023

Infrared spectral fingerprint of neutral and charged endo- and exohedral metallofullerenes

R. Barzaga, D. A. Garcia-Hernandez, S. Diaz-Tendero +5

Small metal-containing molecules have been detected and recognized as one of the hybrid species efficiently formed in space; especially in the circumstellar envelopes of evolved st…

astro-ph.EP2023★ 13 cited

TESS discovery of a super-Earth orbiting the M dwarf star TOI-1680

M. Ghachoui, A. Soubkiou, R. D. Wells +52

We report the discovery by the TESS mission of a super-Earth on a 4.8-d orbit around an inactive M4.5 dwarf (TOI-1680) validated by ground-based facilities. The host star is locate…

astro-ph.SR2023★ 7 cited

The origin of the planetary nebula M 1-16. A morphokinematic and chemical analysis

M. A. Gómez-Muñoz, R. Vázquez, L. Sabin +4

We investigated the origin of the Planetary Nebula (PN) M 1-16 using narrow-band optical imaging, and high- and low-resolution optical spectra to perform a detailed morpho-kinemati…

astro-ph.SR2023★ 16 cited

Catalog of Planetary Nebulae detected by GALEX and corollary optical surveys

M. A. Gómez-Muñoz, L. Bianchi, A. Manchado

Planetary nebulae (PNe) consist of an ionized envelope surrounding a hot central star (CSPN) that emits mostly at ultraviolet (UV) wavelengths. Ultraviolet observations, therefore,…

astro-ph.EP2023★ 33 cited

A super-Earth and a mini-Neptune near the 2:1 MMR straddling the radius valley around the nearby mid-M dwarf TOI-2096

F. J. Pozuelos, M. Timmermans, B. V. Rackham +72

Several planetary formation models have been proposed to explain the observed abundance and variety of compositions of super-Earths and mini-Neptunes. In this context, multitransit…

astro-ph.EP2023★ 18 cited

GJ 806 (TOI-4481): A bright nearby multi-planetary system with a transiting hot, low-density super-Earth

E. Palle, J. Orell-Miquel, M. Brady +63

One of the main scientific goals of the TESS mission is the discovery of transiting small planets around the closest and brightest stars in the sky. Here, using data from the CARME…

astro-ph.EP2022★ 45 cited

Uncovering the true periods of the young sub-Neptunes orbiting TOI-2076

Hugh P. Osborn, Andrea Bonfanti, Davide Gandolfi +93

Context: TOI-2076 is a transiting three-planet system of sub-Neptunes orbiting a bright (G = 8.9 mag), young ( Myr) K-type star. Although a validated planetary system, th…

astro-ph.EP2021★ 26 cited

TOI-2257 b: A highly eccentric long-period sub-Neptune transiting a nearby M dwarf

N. Schanche, F. J. Pozuelos, M. N. Günther +61

Thanks to the relative ease of finding and characterizing small planets around M dwarf stars, these objects have become cornerstones in the field of exoplanet studies. The current…

astro-ph.EP2021

A large sub-Neptune transiting the thick-disk M4V TOI-2406

R. D. Wells, B. V. Rackham, N. Schanche +71

Large sub-Neptunes are uncommon around the coolest stars in the Galaxy and are rarer still around those that are metal-poor. However, owing to the large planet-to-star radius ratio…

astro-ph.SR2020★ 9 cited

Wide binaries in Planetary Nebulae with Gaia DR2

I. González-Santamaría, M. Manteiga, A. Manchado +3

Gaia Data Release 2 (DR2) was used to select a sample of 211 central stars of planetary nebulae (CSPNe) with good quality astrometric measurements, that we refer to as GAPN, Golden…

astro-ph.EP2016★ 38 cited

Results from the 2014 November 15th multi-chord stellar occultation by the TNO (229762) 2007 UK

Gustavo Benedetti-Rossi, Bruno Sicardy, Marc W. Buie +26

We present results derived from the first multi-chord stellar occultation by the trans-Neptunian object (229762) 2007 UK, observed on 2014 November 15. The event was observ…

astro-ph.SR2015★ 10 cited

Morpho-kinematics of the planetary nebula NGC 3242: an analysis beyond its multiple-shell structure

M. A. Gómez-Muñoz, M. W. Blanco Cárdenas, R. Vázquez +3

In this paper we present the results of optical high-resolution imaging and spectroscopy of the complex planetary nebula (PN) NGC~3242. Our study is based on the analysis of the na…