Astronomy & Astrophysics

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Extragalactic astronomy

Euclid Quick Data Release (Q1)

Euclid Quick Data Release (Q1). The Strong Lensing Discovery Engine C: Finding lenses with machine learning

Received: 14 March 2025 / Accepted: 11 June 2025
DOI: https://doi.org/10.1051/0004-6361/202554542
Euclid Quick Data Release (Q1)

Euclid Quick Data Release (Q1). The strong-lensing discovery engine d: Double-source-plane lens candidates

Received: 14 March 2025 / Accepted: 01 June 2025
DOI: https://doi.org/10.1051/0004-6361/202554543
Euclid Quick Data Release (Q1)

Euclid Quick Data Release (Q1). A first view of the star-forming main sequence in the Euclid Deep Fields

Received: 17 March 2025 / Accepted: 05 May 2025
DOI: https://doi.org/10.1051/0004-6361/202554576

Catalogs and data

Euclid Quick Data Release (Q1)
Free Access

Euclid Quick Data Release (Q1). From images to multi-wavelength catalogues: The Euclid MERge Processing Function

Received: 17 March 2025 / Accepted: 15 May 2025
DOI: https://doi.org/10.1051/0004-6361/202554586

Extragalactic astronomy

Euclid Quick Data Release (Q1)

Euclid Quick Data Release (Q1). Photometric redshifts and physical properties of galaxies through the PHZ processing function

Received: 17 March 2025 / Accepted: 28 April 2025
DOI: https://doi.org/10.1051/0004-6361/202554588

Catalogs and data

Euclid Quick Data Release (Q1)
Free Access

Euclid Quick Data Release (Q1). From spectrograms to spectra: The SIR spectroscopic processing function

Received: 18 March 2025 / Accepted: 17 May 2025
DOI: https://doi.org/10.1051/0004-6361/202554627

Free Access
Erratum

Hot Rocks Survey. II. The thermal emission of TOI-1468 b reveals a bare hot rock (Corrigendum)

Received: 27 June 2025 / Accepted: 27 June 2025
DOI: https://doi.org/10.1051/0004-6361/202556143e

    Letters to the Editor

    Free Access

    Unveiling a protoplanet candidate embedded in the HD 135344B disk with VLT/ERIS

    Received: 11 March 2025 / Accepted: 13 June 2025
    DOI: https://doi.org/10.1051/0004-6361/202554472
    Free Access

    Magnetospheric magnetic reconnection in high-mass young stellar objects and its possible relation to methanol maser flares

    Received: 01 April 2025 / Accepted: 14 June 2025
    DOI: https://doi.org/10.1051/0004-6361/202554974
    Free Access

    Impact of the Tayler magnetic instability on the surface abundance of boron in massive stars

    Received: 15 April 2025 / Accepted: 23 June 2025
    DOI: https://doi.org/10.1051/0004-6361/202555163
    Free Access

    Experimental confirmation of barrierless reactions between HeH^+ and deuterium atoms suggests a lower abundance of the first molecules at very high redshifts

    Received: 28 April 2025 / Accepted: 16 June 2025
    DOI: https://doi.org/10.1051/0004-6361/202555316

    Astrophysical processes

    The Chinese Pulsar Timing Array data release I. Single pulsar noise analysis

    Received: 09 October 2024 / Accepted: 02 May 2025
    DOI: https://doi.org/10.1051/0004-6361/202452550

    Orbit design for mitigating interstellar scattering effects in Earth-space very long baseline interferometry observations of Sagittarius A*

    Received: 18 October 2024 / Accepted: 09 April 2025
    DOI: https://doi.org/10.1051/0004-6361/202452668

    An unusual type-I X-ray burst from the neutron star X-ray binary IGR J17591--2342: A possible double-photospheric radius-expansion burst

    Received: 10 February 2025 / Accepted: 16 June 2025
    DOI: https://doi.org/10.1051/0004-6361/202554099

    Common envelopes in massive stars. III. The obstructive role of radiation transport in envelope ejection

    Received: 27 March 2025 / Accepted: 23 May 2025
    DOI: https://doi.org/10.1051/0004-6361/202554782

    Euclid: Early Release Observations -- The surface brightness and colour profiles of the far outskirts of galaxies in the Perseus cluster

    Received: 28 March 2025 / Accepted: 06 May 2025
    DOI: https://doi.org/10.1051/0004-6361/202554838

    How the spin-phase variability of cyclotron lines shapes the pulsed fraction spectra: Insights from 4U 1538-52

    Received: 10 April 2025 / Accepted: 19 June 2025
    DOI: https://doi.org/10.1051/0004-6361/202555112

    Cosmology (including clusters of galaxies)

    Galaxy formation with wave/fuzzy dark matter: The core-halo structure and the solitonic imprint

    Received: 19 April 2024 / Accepted: 31 May 2025
    DOI: https://doi.org/10.1051/0004-6361/202450443

    Detecting low-mass haloes with strong gravitational lensing. II: Constraints on the density profiles of two detected subhaloes

    Received: 17 July 2024 / Accepted: 25 May 2025
    DOI: https://doi.org/10.1051/0004-6361/202451546

    Caught in the cosmic web: Environmental effects on subhalo abundance and internal density profiles

    Received: 13 September 2024 / Accepted: 19 June 2025
    DOI: https://doi.org/10.1051/0004-6361/202452246

    Simulation-based inference benchmark for weak lensing cosmology

    Received: 29 September 2024 / Accepted: 20 March 2025
    DOI: https://doi.org/10.1051/0004-6361/202452410

    KiDS-Legacy: Covariance validation and the unified OneCovariance framework for projected large-scale structure observables

    Received: 12 October 2024 / Accepted: 16 March 2025
    DOI: https://doi.org/10.1051/0004-6361/202452592

    UNIONS: A direct measurement of intrinsic alignment with BOSS/eBOSS spectroscopy

    Received: 13 December 2024 / Accepted: 14 April 2025
    DOI: https://doi.org/10.1051/0004-6361/202453442

    The imprint of cosmic voids from the DESI Legacy Survey DR9 Luminous Red Galaxies in the Planck 2018 lensing map through spectroscopically calibrated mocks

    Received: 20 December 2024 / Accepted: 14 April 2025
    DOI: https://doi.org/10.1051/0004-6361/202453562

    Euclid preparation. LXXII. Three-dimensional galaxy clustering in configuration space. 1. Two-point correlation function estimation

    Received: 28 January 2025 / Accepted: 18 June 2025
    DOI: https://doi.org/10.1051/0004-6361/202553927

    Weak lensing mass-richness relation of redMaPPer clusters in LSST DESC DC2 simulations

    Received: 11 February 2025 / Accepted: 08 June 2025
    DOI: https://doi.org/10.1051/0004-6361/202554107

    Intrinsic galaxy alignments in the KiDS-1000 bright sample: Dependence on colour, luminosity, morphology, and galaxy scale

    Received: 14 February 2025 / Accepted: 20 May 2025
    DOI: https://doi.org/10.1051/0004-6361/202554134

    Selection function of clusters in Dark Energy Survey year 3 data from cross-matching with South Pole Telescope detections

    Received: 18 February 2025 / Accepted: 03 June 2025
    DOI: https://doi.org/10.1051/0004-6361/202554177

    Unbiased estimates of the shapes of haloes using the positions of satellite galaxies

    Received: 24 February 2025 / Accepted: 27 May 2025
    DOI: https://doi.org/10.1051/0004-6361/202554244

    NIKA2 Cosmological Legacy Survey. Blind detection of galaxy clusters in the COSMOS field via the Sunyaev-Zel’dovich effect

    Received: 10 March 2025 / Accepted: 02 June 2025
    DOI: https://doi.org/10.1051/0004-6361/202554450

    The ESPRESSO Redshift Drift Experiment. I. High-resolution spectra of the Lyman-α forest of QSO J052915.80-435152.0

    Received: 12 March 2025 / Accepted: 27 May 2025
    DOI: https://doi.org/10.1051/0004-6361/202554502

    A view of the CIZA J2242.8+5301 galaxy cluster at very low radio frequencies

    Received: 13 March 2025 / Accepted: 18 April 2025
    DOI: https://doi.org/10.1051/0004-6361/202554521

    Central galaxy alignments. Dependence on the mass and the large-scale environment

    Received: 17 March 2025 / Accepted: 10 June 2025
    DOI: https://doi.org/10.1051/0004-6361/202554593

    Intra-cluster light as a dynamical clock for galaxy clusters: Insights from the MAGNETICUM, IllustrisTNG, Hydrangea, and Horizon-AGN simulations

    Received: 26 March 2025 / Accepted: 02 June 2025
    DOI: https://doi.org/10.1051/0004-6361/202554777

    Flashlights: Prospects for constraining the initial mass function around cosmic noon with caustic-crossing events

    Received: 03 April 2025 / Accepted: 07 June 2025
    DOI: https://doi.org/10.1051/0004-6361/202555023

    Reconstructing the epoch of reionisation with Planck PR4

    Received: 17 April 2025 / Accepted: 23 June 2025
    DOI: https://doi.org/10.1051/0004-6361/202555196

    Extragalactic astronomy

    The brightest GRB ever detected: GRB,221009A as a highly luminous event at z=0.151

    Received: 15 February 2023 / Accepted: 09 June 2024
    DOI: https://doi.org/10.1051/0004-6361/202346146

    The ALMA-CRISTAL survey: Extended CII emission in an interacting galaxy system at z ∼ 5.5

    Received: 04 March 2024 / Accepted: 09 May 2025
    DOI: https://doi.org/10.1051/0004-6361/202449843

    The vertical structure of the stellar disk in NGC 551

    Received: 18 April 2024 / Accepted: 03 June 2025
    DOI: https://doi.org/10.1051/0004-6361/202450431

    MIDIS. Near-infrared rest-frame morphology of massive galaxies at 3<z<5 in the Hubble eXtreme Deep Field

    Received: 01 July 2024 / Accepted: 06 May 2025
    DOI: https://doi.org/10.1051/0004-6361/202451330

    Differences in the physical properties of satellite galaxies within relaxed and disturbed galaxy groups and clusters

    Received: 05 August 2024 / Accepted: 27 May 2025
    DOI: https://doi.org/10.1051/0004-6361/202451801

    Narrow-line AGN selection in CEERS: Spectroscopic selection, physical properties, and X-ray and radio analysis

    Received: 11 August 2024 / Accepted: 07 February 2025
    DOI: https://doi.org/10.1051/0004-6361/202451860

    The VVV near-IR galaxy catalogue of the southern Galactic disc

    Received: 10 September 2024 / Accepted: 23 June 2025
    DOI: https://doi.org/10.1051/0004-6361/202452197

    Mocking integral field unit observations and metallicity diagnostics from cosmological simulations

    Received: 12 September 2024 / Accepted: 27 May 2025
    DOI: https://doi.org/10.1051/0004-6361/202452226

    Unveiling multiple physical processes on a cluster galaxy at z=0.3 using JWST

    Received: 23 September 2024 / Accepted: 04 June 2025
    DOI: https://doi.org/10.1051/0004-6361/202452348

    Quenching of galaxies at cosmic noon. Understanding the effect of the environment

    Received: 29 September 2024 / Accepted: 22 May 2025
    DOI: https://doi.org/10.1051/0004-6361/202452406

    Reconstructing galaxy star formation histories from COSMOS2020 photometry using simulation-based inference

    Received: 01 October 2024 / Accepted: 28 April 2025
    DOI: https://doi.org/10.1051/0004-6361/202452457

    Strömgren photometric metallicity map of the Magellanic Cloud stars using Gaia DR3--XP spectra

    Received: 07 October 2024 / Accepted: 04 June 2025
    DOI: https://doi.org/10.1051/0004-6361/202452510

    The GECKOS survey: Identifying kinematic sub-structures in edge-on galaxies

    Received: 05 November 2024 / Accepted: 12 June 2025
    DOI: https://doi.org/10.1051/0004-6361/202452891

    MUSE observations of dwarf galaxies and a stellar stream in the M 83 group

    Received: 08 November 2024 / Accepted: 21 April 2025
    DOI: https://doi.org/10.1051/0004-6361/202452923

    Peering into the heart of 3CR radio galaxies. A very long baseline interferometry perspective on optical-radio classifications at parsec scales

    Received: 15 November 2024 / Accepted: 25 May 2025
    DOI: https://doi.org/10.1051/0004-6361/202453018

    The effect of measurement uncertainties on the inferred stability of planes of satellite galaxies

    Received: 20 November 2024 / Accepted: 07 May 2025
    DOI: https://doi.org/10.1051/0004-6361/202453087

    Investigating the relation between the environment and internal structure of massive elliptical galaxies using strong lensing

    Received: 30 November 2024 / Accepted: 11 April 2025
    DOI: https://doi.org/10.1051/0004-6361/202453239

    Decoding the molecular torus of NGC 1068. Insights into its structure and kinematics from high-resolution ALMA observations

    Received: 09 December 2024 / Accepted: 01 May 2025
    DOI: https://doi.org/10.1051/0004-6361/202453363

    The intermediate-mass black hole 2XMM J123103.2+110648: A varying disc accretion rate during possible X-ray quasi-periodic eruptions?

    Received: 12 December 2024 / Accepted: 08 June 2025
    DOI: https://doi.org/10.1051/0004-6361/202453423

    Euclid: Early Release Observations of diffuse stellar structures and globular clusters as probes of the mass assembly of galaxies in the Dorado group

    Received: 19 December 2024 / Accepted: 23 June 2025
    DOI: https://doi.org/10.1051/0004-6361/202453534

    Variable stars in Local Group galaxies VII. New insights into the Leo II dSph

    Received: 20 December 2024 / Accepted: 12 May 2025
    DOI: https://doi.org/10.1051/0004-6361/202453567

    Tracing ongoing quenching in jellyfish galaxies at z∼0.35

    Received: 31 December 2024 / Accepted: 23 May 2025
    DOI: https://doi.org/10.1051/0004-6361/202453646

    The ionisation structure and chemical history in isolated H ii regions of dwarf galaxies with integral field unit. I. The Sagittarius dwarf irregular galaxy

    Received: 03 January 2025 / Accepted: 22 May 2025
    DOI: https://doi.org/10.1051/0004-6361/202553678

    The SRG/eROSITA all-sky survey. Subaru/HSC-SSP weak-lensing mass measurements for eRASS1 galaxy clusters

    Received: 09 January 2025 / Accepted: 12 June 2025
    DOI: https://doi.org/10.1051/0004-6361/202553708

    TP-AGB stars and stellar population properties of a post-starburst galaxy at z∼2 through optical and near-infrared spectroscopy with JWST

    Received: 13 January 2025 / Accepted: 21 May 2025
    DOI: https://doi.org/10.1051/0004-6361/202553736

    Mapping reionization bubbles in JWST era. II. Inferring the position and characteristic size of individual bubbles

    Received: 14 January 2025 / Accepted: 27 May 2025
    DOI: https://doi.org/10.1051/0004-6361/202553756

    Spatially resolved spectrophotometric SED modeling of NGC 253's central molecular zone. I. Star formation in extragalactic giant molecular clouds

    Received: 25 January 2025 / Accepted: 14 May 2025
    DOI: https://doi.org/10.1051/0004-6361/202553897

    Gas outflows in two recently quenched galaxies at z=4 and 7

    Received: 27 January 2025 / Accepted: 19 May 2025
    DOI: https://doi.org/10.1051/0004-6361/202553908

    Insight into the physical processes that shape the metallicity profiles in galaxies

    Received: 03 February 2025 / Accepted: 23 May 2025
    DOI: https://doi.org/10.1051/0004-6361/202554013

    CHANG-ES. XXXVI. The thin and thick radio discs

    Received: 05 February 2025 / Accepted: 15 May 2025
    DOI: https://doi.org/10.1051/0004-6361/202554046

    Simulating nearby disc galaxies on the main star formation sequence. II. The gas structure transition in low and high stellar mass discs

    Received: 06 February 2025 / Accepted: 05 May 2025
    DOI: https://doi.org/10.1051/0004-6361/202554056

    First polarization study of the M87 jet and active galactic nuclei at submillimeter wavelengths with ALMA

    Received: 14 February 2025 / Accepted: 04 April 2025
    DOI: https://doi.org/10.1051/0004-6361/202554140

    The rich JWST spectrum of the western nucleus of Arp 220: Shocked hot core chemistry dominates the inner disc

    Received: 14 February 2025 / Accepted: 14 May 2025
    DOI: https://doi.org/10.1051/0004-6361/202554141

    The MUSE view of the Sculptor galaxy: Survey overview and the luminosity function of planetary nebulae

    Received: 14 February 2025 / Accepted: 10 June 2025
    DOI: https://doi.org/10.1051/0004-6361/202554144

    Investigating the chemical link between H2CO and CH3OH within the central molecular zone of NGC 253

    Received: 17 February 2025 / Accepted: 13 May 2025
    DOI: https://doi.org/10.1051/0004-6361/202554156

    The S-PLUS Fornax Project (S+FP): Mapping Halpha+[N II] emission in 77 Fornax galaxy members reaching ∼4 Rvir

    Received: 17 February 2025 / Accepted: 19 May 2025
    DOI: https://doi.org/10.1051/0004-6361/202554159

    Accretion onto supermassive and intermediate-mass black holes in cosmological simulations

    Received: 18 February 2025 / Accepted: 16 May 2025
    DOI: https://doi.org/10.1051/0004-6361/202554174

    Distinguishing ram pressure from tidal interactions: Size-shape difference measure

    Received: 19 February 2025 / Accepted: 16 June 2025
    DOI: https://doi.org/10.1051/0004-6361/202554190

    The MUSE view of ram pressure stripped galaxies in clusters: The GASP sample

    Received: 20 February 2025 / Accepted: 27 May 2025
    DOI: https://doi.org/10.1051/0004-6361/202554200

    CEERS: Possibly forging the first dust grains in the universe. A population of galaxies with spectroscopically derived extremely low dust attenuation (GELDA) at 4.0 < z ≲ 11.4

    Received: 22 February 2025 / Accepted: 07 May 2025
    DOI: https://doi.org/10.1051/0004-6361/202554231

    The VMC survey. LII. Data release #7. Complete survey data and data from additional programmes

    Received: 25 February 2025 / Accepted: 25 April 2025
    DOI: https://doi.org/10.1051/0004-6361/202554254

    GA-NIFS: Mapping z≃3.5 AGN-driven ionized outflows in the COSMOS field

    Received: 26 February 2025 / Accepted: 09 May 2025
    DOI: https://doi.org/10.1051/0004-6361/202554281

    A physically motivated galaxy size definition across different state-of-the-art hydrodynamical simulations

    Received: 27 February 2025 / Accepted: 02 June 2025
    DOI: https://doi.org/10.1051/0004-6361/202554290

    Puzzling radial gradients of K-band absorption features in the giant elliptical galaxy M87

    Received: 28 February 2025 / Accepted: 02 June 2025
    DOI: https://doi.org/10.1051/0004-6361/202554315

    An LBT view of the co-rotating group of galaxies around NGC 2750: Deep imaging and new satellite candidates

    Received: 04 March 2025 / Accepted: 20 June 2025
    DOI: https://doi.org/10.1051/0004-6361/202554365

    Spectral indices in active galactic nuclei as seen by Apertif and LOFAR

    Received: 04 March 2025 / Accepted: 27 May 2025
    DOI: https://doi.org/10.1051/0004-6361/202554375

    The galaxy-halo connection of disc galaxies over six orders of magnitude in stellar mass

    Received: 05 March 2025 / Accepted: 27 May 2025
    DOI: https://doi.org/10.1051/0004-6361/202554381

    MaNGA AGN dwarf galaxies (MAD). III. The role of mergers and environment in active galactic nucleus activity in dwarf galaxies

    Received: 05 March 2025 / Accepted: 07 June 2025
    DOI: https://doi.org/10.1051/0004-6361/202554387

    Investigating the Hi distribution and kinematics of ESO444-G084 and [KKS2000]23: New insights from the MHONGOOSE survey

    Received: 06 March 2025 / Accepted: 01 June 2025
    DOI: https://doi.org/10.1051/0004-6361/202554391

    An improved Seyfert-low ionization nuclear emission-line region classification line in the [N ii] BPT diagram

    Received: 09 March 2025 / Accepted: 23 May 2025
    DOI: https://doi.org/10.1051/0004-6361/202554434

    The polarization of the synchrotron radiation from a recollimated jet: Application to high-energy BL Lacs

    Received: 12 March 2025 / Accepted: 04 June 2025
    DOI: https://doi.org/10.1051/0004-6361/202554490

    The formation and evolution of supermassive disks in IllustrisTNG

    Received: 13 March 2025 / Accepted: 28 June 2025
    DOI: https://doi.org/10.1051/0004-6361/202554509

    The changing impact of radio jets as they evolve: The view from the cold gas

    Received: 14 March 2025 / Accepted: 12 June 2025
    DOI: https://doi.org/10.1051/0004-6361/202554536

    Constraints on the early Universe star formation efficiency from galaxy clustering and halo modeling of Halpha and [O III] emitters

    Received: 18 March 2025 / Accepted: 09 May 2025
    DOI: https://doi.org/10.1051/0004-6361/202554618

    X-ray investigation of the remarkable galaxy group Nest200047

    Received: 21 March 2025 / Accepted: 12 June 2025
    DOI: https://doi.org/10.1051/0004-6361/202554682

    The Close AGN Reference Survey (CARS). Long-term spectral variability study of the changing-look AGN Mrk 1018

    Received: 23 March 2025 / Accepted: 23 May 2025
    DOI: https://doi.org/10.1051/0004-6361/202554707

    Galaxy morphologies at cosmic noon with JWST : A foundation for exploring gas transport with bars and spiral arms

    Received: 24 March 2025 / Accepted: 11 June 2025
    DOI: https://doi.org/10.1051/0004-6361/202554725

    Explosion sites of SN 1994W-like transients

    Received: 27 March 2025 / Accepted: 22 May 2025
    DOI: https://doi.org/10.1051/0004-6361/202554795

    MICONIC: JWST/MIRI MRS reveals a fast ionized gas outflow in the central region of Centaurus A

    Received: 28 March 2025 / Accepted: 27 May 2025
    DOI: https://doi.org/10.1051/0004-6361/202554823

    Discovery and characterization of 25 new quasars at 4.6 < z < 6.9 from wide-field multiband surveys

    Received: 29 March 2025 / Accepted: 19 May 2025
    DOI: https://doi.org/10.1051/0004-6361/202554859

    ADF22+: A declining faint end in the far-infrared luminosity function in the SSA22 protocluster at z=3.09

    Received: 30 March 2025 / Accepted: 23 June 2025
    DOI: https://doi.org/10.1051/0004-6361/202554868

    Revealing a ribbon-like jet in OJ 287 with RadioAstron

    Received: 01 April 2025 / Accepted: 06 June 2025
    DOI: https://doi.org/10.1051/0004-6361/202554929

    Star formation at different stages of ram-pressure stripping as observed through far-ultraviolet imaging of 13 GASP galaxies

    Received: 01 April 2025 / Accepted: 19 May 2025
    DOI: https://doi.org/10.1051/0004-6361/202554945

    The GLASS-JWST Early Release Science programme: The NIRISS spectroscopic catalogue

    Received: 01 April 2025 / Accepted: 28 May 2025
    DOI: https://doi.org/10.1051/0004-6361/202554954

    Observational diversity of bright long-lived Type II supernovae

    Received: 01 April 2025 / Accepted: 02 June 2025
    DOI: https://doi.org/10.1051/0004-6361/202554988

    Deriving physical parameters of unresolved star clusters. IX. Sky background effects in the aperture photometry

    Received: 14 April 2025 / Accepted: 04 June 2025
    DOI: https://doi.org/10.1051/0004-6361/202555153

    Origin of the ring ellipticity in the black hole images of M87*

    Received: 21 April 2025 / Accepted: 14 May 2025
    DOI: https://doi.org/10.1051/0004-6361/202555235

    Revealing the intricacies of radio galaxies and filaments in the merging galaxy cluster Abell 2255. I. Insights from deep LOFAR-VLBI sub-arcsecond resolution images

    Received: 23 April 2025 / Accepted: 16 May 2025
    DOI: https://doi.org/10.1051/0004-6361/202555268

    Microlensing at cosmological distances: Event rate predictions in the Warhol arc of MACS 0416

    Received: 08 May 2025 / Accepted: 09 June 2025
    DOI: https://doi.org/10.1051/0004-6361/202555447

    Testing the ubiquitous presence of very high energy emission in gamma-ray bursts with the MAGIC telescopes

    Received: 09 May 2025 / Accepted: 27 June 2025
    DOI: https://doi.org/10.1051/0004-6361/202555468

    Delving into the depths of NGC 3783 with XRISM. I. Kinematic and ionization structure of the highly ionized outflows

    Received: 22 May 2025 / Accepted: 11 June 2025
    DOI: https://doi.org/10.1051/0004-6361/202555623

    Galactic structure, stellar clusters and populations

    The diverse physical origins of stars in the dynamically hot bulge: CALIFA versus IllustrisTNG

    Received: 28 June 2024 / Accepted: 09 December 2024
    DOI: https://doi.org/10.1051/0004-6361/202451292

    The great wave. Evidence of a large-scale vertical corrugation propagating outwards in the Galactic disc

    Received: 26 July 2024 / Accepted: 29 April 2025
    DOI: https://doi.org/10.1051/0004-6361/202451668

    Beyond the main sequence: Binary evolution pathways to blue stragglers in the Gaia era. I. Galactic open and globular clusters

    Received: 10 September 2024 / Accepted: 26 March 2025
    DOI: https://doi.org/10.1051/0004-6361/202452195

    High-resolution infrared spectroscopy of the dust-obscured metal-poor open cluster Trumpler 5

    Received: 10 October 2024 / Accepted: 07 May 2025
    DOI: https://doi.org/10.1051/0004-6361/202452561

    The completeness of the open cluster census towards the Galactic anticentre

    Received: 15 October 2024 / Accepted: 12 June 2025
    DOI: https://doi.org/10.1051/0004-6361/202452614

    A non-axisymmetric potential for the Milky Way disk

    Received: 19 November 2024 / Accepted: 09 May 2025
    DOI: https://doi.org/10.1051/0004-6361/202453077

    The Pristine Inner Galaxy Survey (PIGS). XI: Revealing the chemical evolution of the interacting Sagittarius dwarf galaxy

    Received: 09 December 2024 / Accepted: 14 May 2025
    DOI: https://doi.org/10.1051/0004-6361/202453354

    Time to Sparkler. Accurate ages of lensed globular clusters at z=1.4 with JWST photometry

    Received: 09 December 2024 / Accepted: 21 May 2025
    DOI: https://doi.org/10.1051/0004-6361/202453368

    Open clusters in the outer disc studied with GTC/MEGARA. Auner 1 and Berkeley 102

    Received: 13 December 2024 / Accepted: 10 June 2025
    DOI: https://doi.org/10.1051/0004-6361/202453444

    Magnetohydrodynamic turbulence and the associated spatial diffusion tensor of cosmic rays in dynamical galactic halos

    Received: 23 January 2025 / Accepted: 23 April 2025
    DOI: https://doi.org/10.1051/0004-6361/202553873

    Gaps in stellar streams as a result of globular cluster flybys. The case of Palomar 5

    Received: 27 January 2025 / Accepted: 26 May 2025
    DOI: https://doi.org/10.1051/0004-6361/202553923

    Reconstructing the Milky Way chemical map with the galactic chemical evolution tool OMEGA+ from SDSS-MWM

    Received: 29 January 2025 / Accepted: 29 May 2025
    DOI: https://doi.org/10.1051/0004-6361/202553951

    The PICS Project. I. The impact of metallicity and helium abundance on the bright end of the planetary nebula luminosity function

    Received: 31 January 2025 / Accepted: 12 June 2025
    DOI: https://doi.org/10.1051/0004-6361/202553974

    Evolution of star clusters with initial bulk rotation via N-body simulations

    Received: 10 February 2025 / Accepted: 20 May 2025
    DOI: https://doi.org/10.1051/0004-6361/202554093

    Chemical characterisation of small substructures in the local stellar halo

    Received: 24 February 2025 / Accepted: 23 May 2025
    DOI: https://doi.org/10.1051/0004-6361/202554252

    Comparing population synthesis models of compact double white dwarfs to electromagnetic observations

    Received: 27 February 2025 / Accepted: 09 May 2025
    DOI: https://doi.org/10.1051/0004-6361/202554302

    Probing the origins. II. Unravelling lithium depletion and stellar motion: Intrinsic stellar properties driving depletion, not kinematics

    Received: 27 February 2025 / Accepted: 21 May 2025
    DOI: https://doi.org/10.1051/0004-6361/202554305

    Structural parameters, chronological age, and dynamical age of the Large Magellanic Cloud globular cluster NGC 1754

    Received: 13 March 2025 / Accepted: 13 May 2025
    DOI: https://doi.org/10.1051/0004-6361/202554512

    GAMA 526784: The progenitor of a globular cluster-rich ultra-diffuse galaxy?. I. Star clusters, stellar body, and ionised gas properties

    Received: 24 March 2025 / Accepted: 21 May 2025
    DOI: https://doi.org/10.1051/0004-6361/202554733

    The Galactic bulge exploration V. The secular spherical and X-shaped Milky Way bulge

    Received: 28 March 2025 / Accepted: 23 June 2025
    DOI: https://doi.org/10.1051/0004-6361/202554819

    Chemo-dynamics of the stellar component of the Sculptor dwarf galaxy. II. Dynamical properties and dark matter halo density

    Received: 28 March 2025 / Accepted: 10 June 2025
    DOI: https://doi.org/10.1051/0004-6361/202554826

    Studying stellar populations in Omega Centauri with phylogenetics

    Received: 29 March 2025 / Accepted: 02 June 2025
    DOI: https://doi.org/10.1051/0004-6361/202554863

    Shaping Galactic habitability: Impact of stellar migration and gas giants

    Received: 05 April 2025 / Accepted: 22 June 2025
    DOI: https://doi.org/10.1051/0004-6361/202555050

    Interstellar and circumstellar matter

    Hot exozodiacal dust around Fomalhaut: The MATISSE perspective

    Received: 21 July 2024 / Accepted: 20 May 2025
    DOI: https://doi.org/10.1051/0004-6361/202451592

    BASIL: Fast broadband line-rich spectral-cube fitting and image visualization via Bayesian quadrature

    Received: 31 October 2024 / Accepted: 21 May 2025
    DOI: https://doi.org/10.1051/0004-6361/202452828

    Dancing on the grain: Variety of CO and its isotopologue fluxes as a result of surface chemistry and T Tauri disk properties

    Received: 19 December 2024 / Accepted: 17 June 2025
    DOI: https://doi.org/10.1051/0004-6361/202453529

    Discovery of the binary nature of the magnetospheric B-type star ρ Oph A

    Received: 04 February 2025 / Accepted: 09 May 2025
    DOI: https://doi.org/10.1051/0004-6361/202554023

    High-resolution APEX/LAsMA ^12CO and ^13CO (3-2) observation of the G333 giant molecular cloud complex. III. Decomposition of molecular clouds into multi-scale hub-filament structures

    Received: 08 February 2025 / Accepted: 18 June 2025
    DOI: https://doi.org/10.1051/0004-6361/202554080

    PDRs4All XIV. Probing CH out-of-plane bending modes of PAH molecules in the Orion Bar with JWST

    Received: 10 February 2025 / Accepted: 03 April 2025
    DOI: https://doi.org/10.1051/0004-6361/202554096

    PRODIGE -- envelope to disk with NOEMA: V. Low 12C/13C ratios for CH3OH and CH3CN in hot corinos

    Received: 11 February 2025 / Accepted: 27 May 2025
    DOI: https://doi.org/10.1051/0004-6361/202554104

    MINDS: The very low-mass star and brown dwarf sample. Detections and trends in the inner disk gas

    Received: 12 February 2025 / Accepted: 03 June 2025
    DOI: https://doi.org/10.1051/0004-6361/202554109

    A correlation between accretion and outflow rates for class II young stellar objects with full and transition disks

    Received: 25 February 2025 / Accepted: 21 May 2025
    DOI: https://doi.org/10.1051/0004-6361/202554259

    Dense clumps survive in the vicinity of R136 in 30 Doradus

    Received: 28 February 2025 / Accepted: 27 May 2025
    DOI: https://doi.org/10.1051/0004-6361/202554327

    Narrow absorption lines from intervening material in supernovae. II. Galaxy properties

    Received: 03 March 2025 / Accepted: 17 June 2025
    DOI: https://doi.org/10.1051/0004-6361/202554355

    JWST Observations of Young protoStars (JOYS). Overview of program and early results

    Received: 10 March 2025 / Accepted: 05 May 2025
    DOI: https://doi.org/10.1051/0004-6361/202554444

    Hierarchical fragmentation in hub-filament-system I18308 observed as part of the INFANT survey

    Received: 19 March 2025 / Accepted: 04 June 2025
    DOI: https://doi.org/10.1051/0004-6361/202554634

    FAUST. XXVI. The dust opacity spectral indices of protostellar envelopes bridge the gap between interstellar medium and disks

    Received: 19 March 2025 / Accepted: 06 June 2025
    DOI: https://doi.org/10.1051/0004-6361/202554645

    FAUST. XXV. A potential new molecular outflow in [BHB2007]11

    Received: 25 March 2025 / Accepted: 17 May 2025
    DOI: https://doi.org/10.1051/0004-6361/202554755

    Tracing the ejecta structure of supernova 1987A: Insights and diagnostics from 3D magnetohydrodynamic simulations

    Received: 29 March 2025 / Accepted: 02 May 2025
    DOI: https://doi.org/10.1051/0004-6361/202554862

    Impact of a binary companion in AGB outflows on CO spectral lines

    Received: 31 March 2025 / Accepted: 12 June 2025
    DOI: https://doi.org/10.1051/0004-6361/202554905

    Inner disc and circumplanetary material in the PDS 70 system: Insights from multi-epoch, multi-frequency ALMA observations

    Received: 01 April 2025 / Accepted: 04 June 2025
    DOI: https://doi.org/10.1051/0004-6361/202554959

    Studying the multiphase interstellar medium in the Large Magellanic Cloud with SRG /eROSITA. I. Analysis of diffuse X-ray emission

    Received: 01 April 2025 / Accepted: 27 June 2025
    DOI: https://doi.org/10.1051/0004-6361/202554971

    Rings and arcs around evolved stars. IV. Characterizing the physical properties of the rings around IC 418 with MUSE

    Received: 07 April 2025 / Accepted: 02 June 2025
    DOI: https://doi.org/10.1051/0004-6361/202555063

    Interstellar water ice analogue properties as a function of temperature: Updated density, porosity, and infrared band strength

    Received: 09 April 2025 / Accepted: 05 June 2025
    DOI: https://doi.org/10.1051/0004-6361/202555090

    The HI-to-H_2 transition in the Draco cloud

    Received: 26 April 2025 / Accepted: 24 June 2025
    DOI: https://doi.org/10.1051/0004-6361/202555308

    Stellar structure and evolution

    Short- and long-term variations of the high mass accretion rate classical T Tauri star DR Tau

    Received: 12 February 2024 / Accepted: 06 May 2025
    DOI: https://doi.org/10.1051/0004-6361/202449576

    Magnetic activity of RS CVn stars based on TESS and LAMOST surveys

    Received: 23 August 2024 / Accepted: 12 May 2025
    DOI: https://doi.org/10.1051/0004-6361/202451962

    The impact of rotation on the stochastic excitation of stellar acoustic modes in solar-like pulsators

    Received: 02 September 2024 / Accepted: 12 February 2025
    DOI: https://doi.org/10.1051/0004-6361/202452093

    Collision-induced mass loss and mass gain on an extremely massive star. An analytical approach and a static proto-globular cluster test-case

    Received: 16 December 2024 / Accepted: 28 May 2025
    DOI: https://doi.org/10.1051/0004-6361/202453462

    The i-processes nucleosynthesis during the formation of He-rich hot-subdwarf stars

    Received: 20 December 2024 / Accepted: 28 March 2025
    DOI: https://doi.org/10.1051/0004-6361/202453572

    Red supergiant stars in binary systems. II. Confirmation of B-type companions of red supergiants in the Small Magellanic Cloud using Hubble ultraviolet spectroscopy

    Received: 24 December 2024 / Accepted: 29 April 2025
    DOI: https://doi.org/10.1051/0004-6361/202453607

    Light clusters as a possible source of crustal impurities: A quasi-particle approach

    Received: 21 January 2025 / Accepted: 25 May 2025
    DOI: https://doi.org/10.1051/0004-6361/202553838

    The model fitting of Gaia DR3 classical Cepheid light and radial velocity curves

    Received: 22 January 2025 / Accepted: 19 June 2025
    DOI: https://doi.org/10.1051/0004-6361/202553855

    The O,Vz stars in NGC 346: Distribution, stellar parameters, and insights into low-metallicity effects

    Received: 31 January 2025 / Accepted: 23 June 2025
    DOI: https://doi.org/10.1051/0004-6361/202553983

    Spectroscopic orbit and variability of the Be star V1624 Cyg = 28 Cyg

    Received: 19 February 2025 / Accepted: 19 May 2025
    DOI: https://doi.org/10.1051/0004-6361/202554185

    Unevolved Li-rich stars at low metallicity: A possible formation pathway through novae

    Received: 25 February 2025 / Accepted: 14 May 2025
    DOI: https://doi.org/10.1051/0004-6361/202554264

    Four ages of rotating stars in the rotation--activity relationship and gyrochronology

    Received: 05 March 2025 / Accepted: 08 June 2025
    DOI: https://doi.org/10.1051/0004-6361/202554379

    The Northern Cross Fast Radio Burst project. V. Search for transient radio emission from Galactic magnetars

    Received: 05 March 2025 / Accepted: 29 May 2025
    DOI: https://doi.org/10.1051/0004-6361/202554386

    X-ray polarization of Z-type neutron star low-mass X-ray binaries. I. Model-independent, time-resolved X-ray polarimetry

    Received: 17 March 2025 / Accepted: 26 May 2025
    DOI: https://doi.org/10.1051/0004-6361/202554573

    Reverse mass transfer and rejuvenation in the massive contact system

    Received: 18 March 2025 / Accepted: 26 May 2025
    DOI: https://doi.org/10.1051/0004-6361/202554603

    Asteroseismology of the G8 subgiant β Aquilae with SONG-Tenerife, SONG-Australia and TESS

    Received: 19 March 2025 / Accepted: 13 June 2025
    DOI: https://doi.org/10.1051/0004-6361/202554633

    Prompt stellar and binary black hole mergers in tight triples. Insights from chemically homogeneous evolution

    Received: 21 March 2025 / Accepted: 04 June 2025
    DOI: https://doi.org/10.1051/0004-6361/202554680

    Evolutionary models for the Very Massive Stars in the R136 cluster of 30 Doradus in the Large Magellanic Cloud

    Received: 26 March 2025 / Accepted: 17 June 2025
    DOI: https://doi.org/10.1051/0004-6361/202554758

    Massive stars exploding in a He-rich circumstellar medium. XI. Diverse evolution of five Ibn SNe 2020nxt, 2020taz, 2021bbv, 2023utc, and 2024aej

    Received: 26 March 2025 / Accepted: 16 June 2025
    DOI: https://doi.org/10.1051/0004-6361/202554768

    The VMC Survey. LIII. Anomalous Cepheids in the Magellanic Clouds: Period-luminosity relations in the near-infrared bands

    Received: 29 March 2025 / Accepted: 09 June 2025
    DOI: https://doi.org/10.1051/0004-6361/202554854

    Chemical composition of asymptotic giant branch stars in Galactic open clusters: Implications for the initial-final mass relation

    Received: 12 April 2025 / Accepted: 05 June 2025
    DOI: https://doi.org/10.1051/0004-6361/202555143

    Binarity at LOw Metallicity (BLOeM). Bayesian inference of natal kicks from inert black hole binaries

    Received: 23 April 2025 / Accepted: 23 June 2025
    DOI: https://doi.org/10.1051/0004-6361/202555274

    Testing the asteroseismic estimates of stellar radii with surface brightness--colour relations and Gaia DR3 parallaxes. III. Main-sequence stars

    Received: 19 May 2025 / Accepted: 13 June 2025
    DOI: https://doi.org/10.1051/0004-6361/202555572

    Stellar atmospheres

    X-Shooting ULLYSES: Massive stars at low metallicity. XIII. Testing the bi-stability jump in the Large Magellanic Cloud

    Received: 17 January 2025 / Accepted: 01 June 2025
    DOI: https://doi.org/10.1051/0004-6361/202553799

    Improving 1D stellar atmosphere models with insights from multi-dimensional simulations. II. 1D versus 3D model comparison for Wolf-Rayet stars

    Received: 13 February 2025 / Accepted: 20 May 2025
    DOI: https://doi.org/10.1051/0004-6361/202554125

    Unlocking the mystery of strontium synthesis in the early Galaxy through analysis of barium isotopes in very metal-poor stars

    Received: 08 April 2025 / Accepted: 05 June 2025
    DOI: https://doi.org/10.1051/0004-6361/202555073

    The Sun and the Heliosphere

    Data-driven MHD simulation of a sunspot-rotating active region leading to a solar eruption

    Received: 11 June 2023 / Accepted: 27 July 2023
    DOI: https://doi.org/10.1051/0004-6361/202347153

    Case study on the evolution of corotating interaction regions for the ``smiley coronal holes'': 0.3 to 1AU

    Received: 20 November 2024 / Accepted: 30 May 2025
    DOI: https://doi.org/10.1051/0004-6361/202453096

    Detecting in situ directional discontinuities in the Solar Wind at Mercury's orbit

    Received: 17 February 2025 / Accepted: 13 June 2025
    DOI: https://doi.org/10.1051/0004-6361/202554165

    Coriolis force acting on near-surface horizontal flows during simulations of flux emergence produces a tilt angle consistent with Joy’s law on the Sun

    Received: 25 February 2025 / Accepted: 12 June 2025
    DOI: https://doi.org/10.1051/0004-6361/202554253

    Presenting 28 years of Sun-as-a-star extreme ultraviolet light curves from SOHO EIT

    Received: 01 April 2025 / Accepted: 23 June 2025
    DOI: https://doi.org/10.1051/0004-6361/202554946

    Entropy proxy inversions as tracers of the evolution of physical conditions at the base of the solar convective envelope

    Received: 02 May 2025 / Accepted: 04 June 2025
    DOI: https://doi.org/10.1051/0004-6361/202555366
    Free Access
    Erratum

    Erratum. Electron and proton peak intensities as observed by a five-spacecraft fleet in solar cycle 25

    Received: 05 June 2025 / Accepted: 21 June 2025
    DOI: https://doi.org/10.1051/0004-6361/202555825e

    Planets, planetary systems, and small bodies

    Dark skies of the slightly eccentric WASP-18 b from its optical-to-infrared dayside emission

    Received: 31 May 2024 / Accepted: 01 May 2025
    DOI: https://doi.org/10.1051/0004-6361/202450939

    Reanalysis of the Huygens GCMS dataset. II. Trace species in Titan's lower atmosphere

    Received: 11 July 2024 / Accepted: 28 March 2025
    DOI: https://doi.org/10.1051/0004-6361/202451466

    Disk Evolution Study Through Imaging of Nearby Young Stars (DESTINYS): Evidence of planet-disk interaction in the 2MASSJ16120668-3010270 system

    Received: 24 July 2024 / Accepted: 07 May 2025
    DOI: https://doi.org/10.1051/0004-6361/202451647

    Planets and planetary systems


    Planets, planetary systems, and small bodies

    The KELT-7b atmospheric thermal-inversion conundrum revisited with CHEOPS, TESS, and additional data

    Received: 10 October 2024 / Accepted: 21 May 2025
    DOI: https://doi.org/10.1051/0004-6361/202452560

    The TOI-2427 system: Two close-in planets orbiting a late K-dwarf star

    Received: 15 October 2024 / Accepted: 22 May 2025
    DOI: https://doi.org/10.1051/0004-6361/202452620

    The HOSTS survey: Suspected variable dust emission and constraints on companions around theta,Boo

    Received: 18 October 2024 / Accepted: 07 May 2025
    DOI: https://doi.org/10.1051/0004-6361/202452653

    Cloud and haze parameterization in atmospheric retrievals: Insights from Titan's Cassini data and JWST observations of hot Jupiters

    Received: 26 November 2024 / Accepted: 19 May 2025
    DOI: https://doi.org/10.1051/0004-6361/202453186

    Non-transiting exoplanets as a means of understanding star-planet interactions in close-in systems

    Received: 17 January 2025 / Accepted: 17 May 2025
    DOI: https://doi.org/10.1051/0004-6361/202553791

    A 3D model simulation of hydrogen chloride photochemistry on Mars: Comparison with satellite data

    Received: 23 January 2025 / Accepted: 26 May 2025
    DOI: https://doi.org/10.1051/0004-6361/202553872

    Predicting the surface age of chondritic S-type asteroids using the space weathering features in reflectance spectra: Small data machine learning

    Received: 18 February 2025 / Accepted: 26 May 2025
    DOI: https://doi.org/10.1051/0004-6361/202554173

    Interior redox state effects on the stability of secondary atmospheres and observational manifestations: LP 791-18,d as a case study for outgassing rocky exoplanets

    Received: 19 February 2025 / Accepted: 02 June 2025
    DOI: https://doi.org/10.1051/0004-6361/202554192

    MINDS: Water reservoirs of compact planet-forming dust discs. A diversity of H_2O distributions

    Received: 21 February 2025 / Accepted: 20 May 2025
    DOI: https://doi.org/10.1051/0004-6361/202554213

    Non-local thermodynamical equilibrium atmospheric modelling of the ultra-hot Jupiter WASP-178b and comparison with UV and optical observations

    Received: 24 February 2025 / Accepted: 30 May 2025
    DOI: https://doi.org/10.1051/0004-6361/202554240

    A high geometric albedo for LTT9779b points toward a metal-rich atmosphere and silicate clouds

    Received: 27 February 2025 / Accepted: 12 June 2025
    DOI: https://doi.org/10.1051/0004-6361/202554303

    Evaluating the contribution of Tianwen-4 mission to Jupiter's gravity field estimation using inter-satellite tracking

    Received: 09 March 2025 / Accepted: 13 June 2025
    DOI: https://doi.org/10.1051/0004-6361/202554439

    Shock effects of Fa_50 iron-rich olivine: Spectral and microstructural implications for Mars and Phobos

    Received: 12 March 2025 / Accepted: 19 May 2025
    DOI: https://doi.org/10.1051/0004-6361/202554497

    Late gas released in the young Kuiper belt could have significantly contributed to the carbon enrichment of the atmospheres of Neptune and Uranus

    Received: 21 March 2025 / Accepted: 02 June 2025
    DOI: https://doi.org/10.1051/0004-6361/202554691

    Two neighbours of the ultra-short-period Earth-sized planet K2-157 b in the warm Neptunian savanna

    Received: 25 March 2025 / Accepted: 25 April 2025
    DOI: https://doi.org/10.1051/0004-6361/202554736

    Orbit and atmosphere of HIP 99770 b through the eyes of VLTI/GRAVITY

    Received: 26 March 2025 / Accepted: 19 June 2025
    DOI: https://doi.org/10.1051/0004-6361/202554766

    The survivorship bias of protoplanetary disc populations. Internal photoevaporation causes an apparent increase in the median total disc mass with time

    Received: 26 March 2025 / Accepted: 06 May 2025
    DOI: https://doi.org/10.1051/0004-6361/202554771

    The ESPRESSO transmission spectrum of HD 189733 b. Extracting the planetary sodium and lithium signatures amid stellar contamination

    Received: 27 March 2025 / Accepted: 17 June 2025
    DOI: https://doi.org/10.1051/0004-6361/202554785

    Planet Earth in reflected and polarized light. II. Refining contrast estimates for rocky exoplanets with ELT and HWO

    Received: 28 March 2025 / Accepted: 02 June 2025
    DOI: https://doi.org/10.1051/0004-6361/202554831

    JWST mid-infrared spectroscopy of centaurs and small trans-Neptunian objects: Linking the inner and outer Solar System

    Received: 08 April 2025 / Accepted: 28 May 2025
    DOI: https://doi.org/10.1051/0004-6361/202555084

    Evolution of ejecta in the (65803) Didymos system driven by the fast-spin primary. Stability conditions, mass transfer, and orbiting disk

    Received: 11 April 2025 / Accepted: 18 June 2025
    DOI: https://doi.org/10.1051/0004-6361/202555138

    Burned to ashes: How the thermal decomposition of refractory organics in the inner protoplanetary disc impacts the gas-phase C/O ratio

    Received: 15 April 2025 / Accepted: 23 May 2025
    DOI: https://doi.org/10.1051/0004-6361/202555164

    Is ozone a reliable proxy for molecular oxygen? II. The impact of N_2O on the O2-O3 relationship for Earth-like atmospheres

    Received: 24 April 2025 / Accepted: 27 May 2025
    DOI: https://doi.org/10.1051/0004-6361/202555289

    Celestial mechanics and astrometry

    Testing gravity with wide binaries. 3D velocities and distances of wide binaries from Gaia and HARPS

    Received: 11 April 2025 / Accepted: 31 May 2025
    DOI: https://doi.org/10.1051/0004-6361/202555115

    Atomic, molecular, and nuclear data

    Free Access

    UV photodissociation of H_2^+ in interstellar radiation fields: Shape resonances and astrophysical implications

    Received: 31 March 2025 / Accepted: 12 June 2025
    DOI: https://doi.org/10.1051/0004-6361/202554904
    Free Access

    Gas-phase formation and photochemistry of large cyano-containing polycyclic aromatic hydrocarbon clusters

    Received: 08 April 2025 / Accepted: 19 June 2025
    DOI: https://doi.org/10.1051/0004-6361/202555079

    Astronomical instrumentation

    Free Access

    LISA test-mass charging. Particle flux modeling, Monte Carlo simulations, and induced effects on the sensitivity of the observatory

    Received: 19 November 2024 / Accepted: 31 May 2025
    DOI: https://doi.org/10.1051/0004-6361/202453076
    Free Access

    NIRPS joining HARPS at ESO 3.6m. On-sky performance and science objectives

    Received: 07 December 2024 / Accepted: 04 June 2025
    DOI: https://doi.org/10.1051/0004-6361/202453341
    Free Access

    Full-link optical differential piston-sensing strategy towards extremely large segmented telescopes

    Received: 16 January 2025 / Accepted: 07 May 2025
    DOI: https://doi.org/10.1051/0004-6361/202553787
    Free Access

    The polarimetric response of the Nançay Radio Telescope and its impact on precision pulsar timing

    Received: 28 January 2025 / Accepted: 07 May 2025
    DOI: https://doi.org/10.1051/0004-6361/202553929
    Free Access

    The Solar Orbiter merged magnetic field

    Received: 24 March 2025 / Accepted: 08 June 2025
    DOI: https://doi.org/10.1051/0004-6361/202554731
    Free Access

    Observation of the Crab Nebula with the Single-Mirror Small-Size Telescope stereoscopic system at low altitude

    Received: 25 April 2025 / Accepted: 31 May 2025
    DOI: https://doi.org/10.1051/0004-6361/202555292

    Catalogs and data

    Free Access

    The eROSITA DR1 variability catalogue

    Received: 26 January 2024 / Accepted: 11 June 2025
    DOI: https://doi.org/10.1051/0004-6361/202449355
    Free Access

    A comprehensive search for hot subdwarf stars using Gaia and TESS. ll. Uncovering new pulsators and close binary systems

    Received: 14 October 2024 / Accepted: 16 June 2025
    DOI: https://doi.org/10.1051/0004-6361/202452606
    Free Access

    The survey of DA double white dwarf candidates based on DESI EDR

    Received: 21 January 2025 / Accepted: 22 May 2025
    DOI: https://doi.org/10.1051/0004-6361/202553834
    Free Access

    HOLISMOKES XVI. Lens search in HSC-PDR3 with a neural network committee and post-processing for false-positive removal

    Received: 07 March 2025 / Accepted: 19 June 2025
    DOI: https://doi.org/10.1051/0004-6361/202554425
    Free Access

    Galaxies OBserved as Low-luminosity Identified Nebulae (GOBLIN): Catalog of 43,000 high-probability dwarf galaxy candidates in the UNIONS survey

    Received: 12 March 2025 / Accepted: 23 May 2025
    DOI: https://doi.org/10.1051/0004-6361/202554501
    Free Access

    Identifying misclassified meteor showers in the IAU MDC database. Reclassification proposal

    Received: 19 March 2025 / Accepted: 16 May 2025
    DOI: https://doi.org/10.1051/0004-6361/202554647
    Free Access

    Magnitude-limited catalogue of unresolved white dwarf-main sequence binaries from Gaia DR3

    Received: 22 March 2025 / Accepted: 18 May 2025
    DOI: https://doi.org/10.1051/0004-6361/202554700
    Free Access

    DAWN JWST Archive: Morphology from profile fitting of over 340,000 galaxies in major JWST fields. Morphology evolution with redshift and galaxy type

    Received: 13 May 2025 / Accepted: 28 May 2025
    DOI: https://doi.org/10.1051/0004-6361/202555504

    Numerical methods and codes

    Free Access

    A numerical approach for modelling the polarisation signals of strong resonance lines with partial frequency redistribution. Applications to two-term atoms and plane-parallel atmospheres

    Received: 21 November 2024 / Accepted: 12 May 2025
    DOI: https://doi.org/10.1051/0004-6361/202453107
    Free Access

    Uncertainty estimation for time series classification. Exploring predictive uncertainty in transformer-based models for variable stars

    Received: 11 December 2024 / Accepted: 30 April 2025
    DOI: https://doi.org/10.1051/0004-6361/202453388
    Free Access

    Observational mapping of the mass discrepancy in eclipsing binaries. A new self-contained framework for concurrent analysis of photometric and spectroscopic time series

    Received: 24 December 2024 / Accepted: 29 April 2025
    DOI: https://doi.org/10.1051/0004-6361/202453605
    Free Access

    Navigating AGN variability with self-organizing maps

    Received: 23 January 2025 / Accepted: 12 June 2025
    DOI: https://doi.org/10.1051/0004-6361/202553866
    Free Access

    DRAGyS - A comprehensive tool for extracting scattering phase functions in protoplanetary disks. Disk ring adjusted geometry yields scattering phase function

    Received: 06 February 2025 / Accepted: 26 May 2025
    DOI: https://doi.org/10.1051/0004-6361/202554058
    Free Access

    From few to many maps: A fast map-level emulator for extreme augmentation of cosmic microwave background systematics datasets

    Received: 14 March 2025 / Accepted: 10 June 2025
    DOI: https://doi.org/10.1051/0004-6361/202554540
    Free Access

    Role of diffusive and nondiffusive grain-surface processes in cold cores: Insights from the PEGASIS three-phase astrochemical model

    Received: 24 March 2025 / Accepted: 23 April 2025
    DOI: https://doi.org/10.1051/0004-6361/202554717
    Free Access

    Simulation-based inference with neural posterior estimation applied to X-ray spectral fitting. II. High-resolution spectroscopy with Athena X-IFU

    Received: 18 April 2025 / Accepted: 05 June 2025
    DOI: https://doi.org/10.1051/0004-6361/202555215