The CARMENES search for exoplanets around M dwarfs: Occurrence rates of Earth-like planets around very low-mass stars (Corrigendum)
Kaminski, A. et al.
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2025
This section contains the publications database that collects IAC articles published in scientific journals. Please, click on the arrow to see full search filter and sort options: author, journal, year, etc..
It also provides access to IAC Preprints Repository here: https://research.iac.es/preprints/
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The ambiguous AT2022rze: changing-look AGN mimicking a supernova in a merging galaxy systemAT2022rze is a luminous, ambiguous transient located south-east of the geometric centre of its host galaxy at redshift $z = 0.08$. The host appears to be formed by a merging galaxy system. The observed characteristics of AT2022rze are reminiscent of active galactic nuclei (AGNs), tidal disruption events, and superluminous supernovae. The transientPessi, P. J. et al.
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The Alma catalogue of OB stars – III. A cross-match with Gaia DR3 and an extension based on new spectral classificationsWe present the third installment of the Alma Luminous Star catalogue, aimed at creating the most comprehensive and clean sample of Galactic massive stars. This update extends the sample by adding approximately 2000 OB stars, incorporating astrometric and photometric data from the Gaia Data Release 3 (DR3) alongside spectroscopic information fromPantaleoni González, M. et al.
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Technetium-rich M stars: Prime diagnostics of recent third dredge-up events on the asymptotic giant branchContext. Technetium (Tc)-rich M stars have been known for more than 45 years. However, the origin of Tc in these stars, particularly its detection without the concomitant detection of other s-process elements, which are typically produced during asymptotic giant branch (AGB) s-process nucleosynthesis, remains poorly understood. Technetium was firstShetye, Shreeya et al.
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Strong spectral features from asymptotic giant branch stars in distant quiescent galaxiesDating the ages and weighting the stellar populations in galaxies are essential steps when studying galaxy formation through cosmic times. Evolutionary population synthesis models with different input physics are used for this purpose. Moreover, the contribution from the thermally pulsing asymptotic giant branch (TP-AGB) stellar phase, which peaksShiying Lu et al.
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Square Kilometre Array Science Data Challenge 3a: foreground removal for an EoR experimentWe present and analyse the results of the Science Data Challenge 3a (SDC3a, https://sdc3.skao.int/challenges/foregrounds), an epoch of reionization (EoR) foreground-removal exercise organized by the Square Kilometre Array Observatory (SKAO) on SKA simulated data. The challenge ran for 8 months, from 2023 March to October. Participants were providedBonaldi, A. et al.
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102025