Preprints in 2025
PP 025160
Tales of stellar and binary co-evolution, told by stellar oscillations - Binary demographics and their impact on stellar mass, orbits, and age estimates in main-sequence and red-giant stars
ULL & IAC
PP 025159
Magnetic Flux Cancellation in the Solar Atmosphere through 3D Realistic Numerical Modeling
(1) Instituto de Astrofisica de Canarias, (2) Departamento de Astrofisica, Universidad de La Laguna, (3) Lockheed Martin Solar and Astrophysics Laboratory, (4) SETI Institute, (5) Rosseland Centre for Solar Physics, University of Oslo, (6) Institute of Theoretical Astrophysics, University of Oslo
PP 025158
A Morpho-kinematic Study of Galactic High-ADF PNe Based on the VLT/UVES Deep Spectroscopy
(1) NAOC, China, (2) U. Hong Kong, China, (3) IAC, Spain, (4) ULL, Spain, (5) Beijing Normal University, China, (6) Yunnan University, China
PP 025157
Identification of new Galactic symbiotic stars with SALT - II. New discoveries and characterization of the sample
(1) IAC, (2) Astronomical Institute of Charles University, Czech Republic, (3) Nicolaus Copernicus Astronomical Center, Polish Academy of Sciences, Poland, (4) Kleinkaroo Observatory, South Africa, (5) Astronomical Observatory, University of Warsaw, Poland
PP 025156
Silicate emission in a type-2 quasar: JWST/MIRI constraints on torus geometry and radiative feedback
(1) IAC, (2) ULL, (3) CAB, (4) University of South Carolina, (5) University of Southampton
PP 025155
Blending-induced beating and emission in the symbiotic star Terz V 2513
(1) IAC, (2) Astronomical Institute of Charles University, Czech Republic, (3) Nicolaus Copernicus Astronomical Center, Polish Academy of Sciences, Poland, (4) Universidad de La Laguna, Spain, (5) Kleinkaroo Observatory, South Africa, (6) Astronomical Observatory, University of Warsaw, Poland
PP 025154
ExoClock Project IV: A homogeneous catalogue of 620 updated exoplanet ephemerides
(1) University College London, (2) Department of Physics, Aristotle University of Thessaloniki, (3)Instituto de Astrofísica de Canarias, (4) Universidad de La Laguna, and others
PP 025153
ASASSN-24fw: Candidate gas-rich circumsecondary disk occultation of a main-sequence star
(1) Johns Hopkins University, (2) Institute for Advanced Study, Princeton, USA, (3) Apache Point Observatory and New Mexico State University, USA, (4) Moscow State University, (5) IAC, (6) Astronomical Institute of Charles University, (7) Imperial College London, (8) Gemini Observatory/NSF’s NOIRLab, Chile
PP 025152
Electron densities from [S II] lines significantly overestimate the impact of ionised AGN outflows
(1) University of Hertfordshire, (2) University of Edinburgh, Royal Observatory, (3) University of Sheffield, (4) IAC, (5) ULL
PP 025151
The lack of fast rotators in Cyg OB2. I. Insights from spectral reclassification of its B0 population.
(1) Instituto de Astrofísica de Canarias, (2) Universidad de La Laguna, (3) Gran Telescopio Canarias
PP 025150
MHD waves with mixed properties/Alfvén waves with pressure variations: a review
(1) Centre for mathematical Plasma Astrophysics, KU Leuven; (2) Instituto de Astrofísica de Canarias; (3) Universidad de La Laguna; (4) Universitat de les Illes Balears; (5) Institute of Applied Computing & Community Code (IAC3).
PP 025149
PyEMILI: A New Generation Computer-aided Spectral Line Identifier – II. Emission-line Identification and Plasma Diagnostics of A Sample of Gaseous Nebulae
(1) NAOC, China, (2) U. Hong Kong, China, (3) IAC, Spain, (4) ULL, Spain, (5) STScI, USA, (6) U. California, USA
PP 025148
GravSphere2: A higher-order Jeans method for mass-modeling spherical stellar systems
Instituto de Astrofísica de Canarias, Universidad de La Laguna, University of Surrey, Leibniz-Institut für Astrophysik Potsdam (AIP),
Institut für Physik und Astronomie, Universität Potsdam
PP 025147
Peculiarities in the infrared emission of PAH-C60 adducts
(1) IUdEA-ULL; (2) LPMC - Université de Tunis El Manar; (3) IAC-ULL; (4) IQCC -Universitat de Girona; (5) CIGUS CITIC - University of A Coruña; (6) CSIC; (7) Universitat de Barcelona; (8) Taif University
PP 025146
Impact of AGN and nuclear star formation on the ISM turbulence of galaxies: Insights from JWST/MIRI spectroscopy
(1) CAB, (2) Universidade Federal de Santa Maria, (3) IAC, (4) ULL
PP 025145
Shock-driven heating in the circumnuclear star-forming regions of NGC 7582: Insights from JWST NIRSpec and MIRI/MRS spectroscopy
(1) University of Oxford, (2) IAC, (3) ULL
PP 025144
Galaxy Activity, Torus and Outflow Survey (GATOS) X: Molecular gas clumpiness under the influence of AGN
(1) OAN, (2) IAC, (3) ULL
PP 025143
In space there will be no need to scream - Limits to the presence of giant planets in the $ζ^2$ Ret system
1 - Instituto de Astrofísica de Canarias, 2 - Universidad de La Laguna
PP 025142
Spindown of massive main sequence stars in the Milky Way
(1) Argelander-Institut für Astronomie, Universität Bonn (2) IAC/ULL
PP 025141
GATOS IX: A Detailed Assessment and Treatment of Emission Line Contamination in JWST/MIRI Images of Nearby Seyfert Galaxies
(1) University of Newcastle, (2) IAC, (3) ULL
PP 025140
GATOS. VIII. On the physical origin of the extended MIR emission in AGN
(1) University of South Carolina, (2) IAC, (3) ULL
PP 025139
Theoretical Diagnostics for the Physical Conditions in Active Galactic Nuclei under the View of JWST
(1) UTSA, (2) MPE, (3) IAC, (4) ULL
PP 025138
An observational study of rotation and binarity of Galactic O-type runaway stars
(1) ICCUB, (2) IAC/ULL
PP 025137
An accurate measure of the size of dark matter halos using the size of galaxies
Instituto de Astrofísica de Canarias
Universidad de La Laguna
PP 025136
Compositional characterisation of asteroid (84) Klio with JWST
(1) IAC, (2) ULL, (3) Space Telescope Science Institute, (4) Institute of Space Sciences and Technologies of Asturias, (5) Florida Space Institute, University of Central Florida, (6) Observatorio Nacional do Rio de Janeiro, (7) Northern Arizona University, (8) Caltech/IPAC, (9) Amentum, NASA Johnson Space Center
PP 025135
Optimization procedure of the baffle of the GroundBIRD Telescope to mitigate stray light
(1) Tohoku University, (2) IAC, (3) ULL, (4) University of Tsukuba, (5) Korea University, (6) Kyoto University, (7) RIKEN, (8) Imperial College Londo
PP 025134
GroundBIRD Telescope: Systematics Modelization of MKID Arrays Response
(1) Korea University, (2) IAC, (3) ULL, (4) University of Tsukuba, (5) RIKEN, (6) Graduate School of Science, Yoshidahonmachi, (7) Imperial College London, (8) SRON
PP 025133
CONCERTO: forward modeling of interferograms for calibration
(1) LAM, (2) IPAG, (3) IAC, (4) ULL, (5) Univ. Grenoble Alpes (6) Astronomy Instrumentation Group, (7) Instituto de Estudios Astrofísicos Universidad Diego Portales(8) Univ. Grenoble Alpes(9) Université de Strasbourg, CNRS, Observatoire astronomique de Strasbourg (10) ESO (11) IRAM (12) Department of Physics and Astronomy, University of the Western Cape, (13) ESO Vitacura (14) Instituto de Física y Astronomía, Universidad de Valparaíıso, (15) Department of Astronomy, University of Illinois
PP 025132
Molecular gas stratification and disturbed kinematics in the Seyfert galaxy MCG-05-23-16 revealed by JWST and ALMA
(1) IAC, (2) ULL
PP 025131
JWST reveals the diversity of nuclear obscuring dust in nearby AGN: nuclear isolation of MIRI/MRS datacubes and continuum spectral fitting
(1) IRyA, (2) Clearwater, Florida, (3) CAB, (4) University of South Carolina, (5) KIPAC, (6) IAC, (7) ULL
PP 025130
Scattered synchrotron emission and a giant torus revealed in polarized light in the nearest radio galaxy Centaurus A
(1) Université de Strasbourg, (2) Université de Liège, (3) CAS/China, (4) University of Science and Technology of China, (5) University of California, Santa Barbara, (6) STScI, (7) Durham University, (8) IAC, (9) ULL, (10) ESO Chile
PP 025129
TOI-283 b: A transiting mini-Neptune in a 17.6-day orbit discovered with TESS and ESPRESSO
(1) Instituto de Astrofísica de Canarias (IAC), E-38205 La Laguna, Tenerife, Spain. (2) Departamento de Astrofísica, Universidad de La Laguna (ULL), E-38206 La Laguna, Tenerife, Spain.
PP 025128
The GECKOS Survey: Resolved, multiphase observations of mass-loading and gas density in the galactic wind of NGC 4666
(1) Centre for Astrophysics and Supercomputing, Swinburne University of Technology, (2) ARC Centre of Excellence for All Sky Astrophysics in 3 Dimensions (ASTRO 3D), (3) Instituto de Astrofísica de Canarias, (4) Departamento de Astrofísica, Universidad de La Laguna
Departamento de Astrofísica, Universidad de La Laguna
PP 025127
A Kinematic History of Stellar Encounters with Beta Pictoris
Centro de Astrobiología (CAB) CSIC-INTA, Departamento de Física de la Tierra y Astrofísica, Facultad de Ciencias Físicas, Universidad Complutense de Madrid, Institute of Science and Technology Austria (ISTA), Lund Observatory, Division of Astrophysics, Department of Physics, Lund University, Instituto de Astrofísica de Canarias, Universidad de La Laguna (ULL))
PP 025126
Beyond diagnostic-diagrams: A critical exploration on the classification of ionization processes
(1) Instituto de Astronomía, Universidad Nacional Autonóma de México, A.P. 106, Ensenada 22800, BC, Mexico, (2) Instituto de Astrofísica de Canarias, La Laguna, Tenerife, E-38200, Spain, (3) Departamento de Astrofísica, Universidad de La Laguna, Spain, (4) Instituto de Radioastronomía and Astrofísica (IRyA-UNAM), 3-72 (Xangari), 8701, Morelia, Mexico, (5) Instituto de Astrofísica de Andalucía (IAA-CSIC), Granada, E-18008, Spain
PP 025125
Constraints on dark matter models from the stellar cores observed in ultra-faint dwarf galaxies: Self-interacting dark matter
(1) IAC, (2) Departamento de Astrofisica, Universidad de La Laguna, Spain
PP 025124
A second low-mass planet orbiting the nearby M-dwarf GJ 536
(1) IAC, (2) ULL, (3) Université Aix Marseille, (4) Université de Genevè, (5) Light Bridges S. L., (6) Università di Padova, (7) CSIC, (8) NASA JPL
PP 025123
Possible Evidence for the Presence of Volatiles on the Warm Super-Earth TOI-270 b
(19) IAC
PP 025122
Stellar-activity analysis of the nearby M dwarf GJ 526. Multi-dimensional Gaussian-process modelling of RV, FWHM and S-index
(1) IAC, (2) ULL, (3) CSIC, (4) Light Bridges S.L.
PP 025121
Quantifying thermal water dissociation in the dayside photosphere of WASP-121 b using NIRPS
IAC, ULL, CSIC, +Many
PP 025120
Atmospheric composition and circulation of the ultra-hot Jupiter WASP-121b with joint NIRPS, HARPS and CRIRES+ transit spectroscopy
(4) Light Bridges S. L., (5) IAC, (6) ULL, (21) CSIC
PP 025119
TOI-2322: two transiting rocky planets close to the stellar rotation period and its first harmonic
(2) IAC, (3) ULL
PP 025118
Blind search for activity-sensitive lines in the near-infrared using HARPS and NIRPS observations of Proxima and Gl 581
IAC, ULL, CSIC, +Many
PP 025117
A comprehensive study on radial velocity signals using ESPRESSO: Pushing precision to the 10 cm/s level
(12) IAC, (13) ULL
PP 025115
The ESPRESSO transmission spectrum of HD$\,$189733$\,$b : Extracting the planetary sodium and lithium signatures amid stellar contamination
(14) IAC, (15) ULL
PP 025114
Diving into the planetary system of Proxima with NIRPS -- Breaking the metre per second barrier in the infrared
IAC, ULL, CSIC, +Many
PP 025113
NIRPS joining HARPS at ESO 3.6 m. On-sky performance and science objectives
IAC, ULL, CSIC, +Many
PP 025112
Hydride ion continuum hides absorption signatures in the NIRPS near-infrared transmission spectrum of the ultra-hot gas giant WASP-189b
IAC, ULL, CSIC, +Many
PP 025111
NIRPS detection of delayed atmospheric escape from the warm and misaligned Saturn-mass exoplanet WASP-69b
IAC, ULL, CSIC, +Many
PP 025110
Two neighbours of the ultra-short-period Earth-sized planet K2-157 b in the warm Neptunian savanna
(17) IAC, (18) ULL
PP 025109
The ESPRESSO Redshift Drift Experiment I -- High-resolution spectra of the Lyman-$α$ forest of QSO J052915.80-435152.0
(11) IAC, (12) ULL
PP 025108
gr8stars I: A homogeneous spectroscopic study of bright FGKM dwarfs and a public library of their high-resolution spectra
(5) IAC, (6) ULL
PP 025105
TOI-512: Super-Earth transiting a K-type star discovered by TESS and ESPRESSO
(11) IAC, 12 (ULL)
PP 025103
Revisiting the multi-planetary system of the nearby star HD 20794: Confirmation of a low-mass planet in the habitable zone of a nearby G-dwarf
(1) Light Bridges S.L., (2) IAC, (3) ULL, (4) CSIC, +19
PP 025102
TESS Subgiant and Lower Red Giant Asteroseismology in the Continuous Viewing Zones
(1) University of Florida Gainesville, FL 32611, USA, (2) California State University, Los Angeles, CA 90032, USA, (3) Instituto de Astrofísica de Canarias (IAC), C/Via Láctea, s/n, E-38200 La Laguna, Tenerife, Spain, (4) Universidad de La Laguna (ULL), Departamento de Astrofísica, E-38206 La Laguna, Tenerife, Spain
PP 025101
Technetium-rich M Stars: Prime diagnostics of recent third dredge-up events on the Asymptotic Giant Branch
(1) KU Leuven, (2) Université Libre de Bruxelles, (3) IAC/ULL, (4) TU Wien
PP 025100
Scaling relations at the central regions of nearby galaxies
(1)Universidade de Sao Paulo
(2)Instituto de Astrofisica de Canarias
(3)Universidad de la Laguna
PP 025099
The GECKOS survey: Jeans anisotropic models of edge-on discs uncover the impact of dust and kinematic structures
(1) European Southern Observatory
(2) University of Sydney
(3) Instituto de Astrofísica de Canarias
(4) Departamento de Astrofísica, Universidad de La Laguna
PP 025098
The IACOB project XV. Updated calibrations of fundamental parameters of Galactic O-type stars
(1) IAC, (2) ULL
PP 025097
MONOS: Multiplicity Of Northern O-type Spectroscopic systems. III. New orbits and Gaia TESS analysis for 10 SB2E systems
(1) IAC, (2) ULL,(3) CAB-CSIC, (4) Instituto de Astrofísica de La Plata, CONICET-UNLP
PP 025096
Neural translation for Stokes inversion and synthesis
(1) IAC, (2) ULL, (3) Institute for Solar Physics, Stockholm University
PP 025095
Variability of Central Stars of Planetary Nebulae with the Zwicky Transient Facility. II. Long-Timescale Variables including Wide Binary and Late Thermal Pulse Candidates
(1) Caltech, (2) IAC, (3) ULL
PP 025094
Azimuthal offsets in spiral arms of nearby galaxies
(1) Observatorio Astronómico Nacional (IGN);
(2) Sterrenkundig Observatorium, Universiteit Gent;
(3) Max-Planck-Institut für extraterrestrische Physik;
(4)Instituto de Astrofísica de Canarias;
(5) Departamento de Astrofísica, Universidad de La Laguna
PP 025093
Large-scale variability in macroturbulence driven by pulsations in the rapidly rotating massive star Zeta Oph from high-cadence ESPRESSO spectroscopy and TESS photometry
(1) Newcastle University (2) IAC/ULL
PP 025092
Beyond the Nyquist frequency: Asteroseismic catalog of undersampled Kepler late subgiants and early red giants
(1) ENS Paris-Saclay, Université Paris-Saclay, 91190, Gif-sur-Yvette, France, (2) Université Paris-Saclay, Université Paris Cité, CEA, CNRS, AIM, F-91191, Gif-sur-Yvette, France, (3) Instituto de Astrofísica de Canarias (IAC), E-38205 La Laguna, Tenerife, Spain, (4) Institute of Science and Technology Austria (ISTA), Am Campus 1, 3400 Klosterneuburg, Austria, (5) Universidad de La Laguna (ULL), Departamento de Astrofísica, E-38206 La Laguna, Tenerife, Spain, (6) Department of Astronomy, The Ohio State University, Columbus, OH 43210, USA, (7) Institute of Space Sciences (ICE, CSIC), Carrer de Can Magrans S/N, E-08193, Cerdanyola del Vallès, Spain, (8) Institut d’Estudis Espacials de Catalunya (IEEC), Carrer Esteve Terradas, 1, Edifici RDIT, Campus PMT-UPC, E-08860, Castelldefels, Spain, (9) Department of Physics and Astronomy, California State University, Long Beach, Long Beach, CA 90840, USA, (10) Department of Astronomy, University of Florida, Gainesville, FL 32611, USA, (11) Department of Physics, The Ohio State University, Columbus, OH 43210, USA
PP 025091
Extreme cloud collisions in nearby barred galaxies
1 School of Physics and Astronomy, University of Nottingham, University Park, Nottingham NG7 2RD, UK
2 Astrophysics Research Institute, Liverpool John Moores University, IC2 Liverpool Science Park, 146 Brownlow Hill, L3 5RF, UK
3 Como Lake centre for AstroPhysics (CLAP), DiSAT, Universit`a dell’Insubria, via Valleggio 11, 22100 Como, Italy
4 Max-Planck-Institut f¨ur Astronomie, K¨onigstuhl 17, 69117 Heidelberg, Germany
5 Institute for Computational Cosmology, Department of Physics, Durham University, DH1 3LE, United Kingdom
6 European Southern Observatory, Karl-Schwarzschild 2, 85748 Garching bei Muenchen, Germany
7 Argelander-Institut f¨ur Astronomie, Universit¨at Bonn, Auf dem H¨ugel 71, 53121 Bonn, Germany
8 Institut f¨ur Theoretische Astrophysik, Zentrum f¨ur Astronomie der Universit¨at Heidelberg, Albert-Ueberle-Strasse 2, 69120
Heidelberg, Germany
9 Cosmic Origins Of Life (COOL) Research DAO, coolresearch.io
10 Univ Lyon, Univ Lyon 1, ENS de Lyon, CNRS, Centre de Recherche Astrophysique de Lyon UMR5574, 69230 Saint-Genis-Laval, France
11 Universit¨at Heidelberg, Interdisziplin¨ares Zentrum f¨ur Wissenschaftliches Rechnen, Im Neuenheimer Feld 225, 69120,
Heidelberg, Germany
12 Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, U.S.A
13 Elizabeth S. and Richard M. Cashin Fellow at Radcliffe Institute for Advanced Studies at Harvard University, 10 Garden Street, Cambridge, MA
14 Sterrenkundig Observatorium, Universiteit Gent, Krijgslaan 281 S9, B-9000 Gent, Belgium
15 Instituto de Astrof´ısica de Canarias, C/ V´ıa L´actea s/n, E-38205, La Laguna, Spain
16 Departamento de Astrof´ısica, Universidad de La Laguna, Av. del Astrof´ısico Francisco S´anchez s/n, E-38206, La Laguna, Spain
17 Observatorio Astron´omico Nacional (IGN), C/Alfonso XII 3, Madrid 28014, Spain
18 Sub-department of Astrophysics, Department of Physics, University of Oxford, Keble Road, Oxford OX1 3RH, UK
PP 025090
Spindown of massive main sequence stars in the Milky Way
(1) Argelander-Institut für Astronomie, Universität Bonn (2) IAC/ULL
PP 025088
Asteroseismology of the G8 subgiant beta Aquilae with SONG-Tenerife, SONG-Australia and TESS
(1) Aarhus University, (2) Sydney Institute for Astronomy, (3) IAC/ULL
PP 025087
High-Resolution Optical IFU Spectroscopy of the Complex Galaxy Merger II Zw 096
(1) Pontificia Universidad Católica de Chile, (2) Universidad de Tarapacá, Chile, (3) IAC, (4) ULL
PP 025086
Characterizing the roles of transitory obscured phases and inner torus in shaping the fractions of obscured AGN at cosmic noon
(1) University of Southampton, (2) IAC, (3) ULL
PP 025085
The orbital period and inclination of the neutron star X-ray transient MAXI J1807+132
(1) Instituto de Astrofísica de Canarias (IAC), Vía Láctea, La Laguna, E-38205, Santa Cruz de Tenerife, Spain
(2) Departamento de Astrofísica, Universidad de La Laguna, E-38206, Santa Cruz de Tenerife, Spain
(3) New York University Abu Dhabi, PO Box 129188, Abu Dhabi, UAE
(4) Center for Astrophysics and Space Science (CASS), New York University Abu Dhabi, PO Box 129188, Abu Dhabi, UAE
PP 025084
Euclid Quick Data Release (Q1) -- Spectroscopic search, classification and analysis of ultracool dwarfs in the Deep Fields
(1) Instituto de Astrofisica de Canarias, La Laguna, Spain;
(2) Universidad de La Laguna, Dpto. Astrofisica, La Laguna, Spain;
(3)Centro de Astrobiologia (INTA-CSIC),Villanueva de la Can ̃ada, Madrid, Spain;
(4) Department of Physics and Astronomy, Ohio University, USA;
(5) Department of Physics, International University, Ho Chi Minh City, Vietnam;
(6) Vietnam National University, Ho Chi Minh City, Vietnam;
(7) Department of Astronomy & Astrophysics, UC San Diego, USA
PP 025083
The slow evolution of dark matter halos from cusp to core naturally produces extended stellar core-like distributions
((1) Instituto de Astrofisica de Canarias, La Laguna, Tenerife, Spain, (2) Departamento de Astrofisica, Universidad de La Laguna, Spain, (3) CeBio y Departamento de Ciencias Basicas, Universidad Nacional del Noroeste de la Prov. de Buenos Aires, UNNOBA, CONICET, Junin, Argentina)
PP 025082
Probing Thin Winds in Massive OB Stars of the SMC with JWST/NIRSPEC Br-alpha Spectroscopy
(1) CAB-CSIC, (2) IAC/ULL, plus some other institutions
PP 025081
easyspec: An open-source Python package for long-slit spectroscopy
(1) Centro Brasileiro de Pesquisas Físicas, Brazil, (2) Dpto di Fisica, Università degli Studi di Torino, Italy, (3) Istituto Nazionale di Fisica Nucleare, Sezione di Torino, Italy, (4) INAF – Osservatorio Astrofisico di Torino, Italy (5) Consorzio Interuniversitario per la Fisica Spaziale (CIFS), Italy, (6) Department of Physics & Astronomy, Louisiana State University, USA, (7) East Asian Observatory, USA,
(8) Instituto de Astrofísica de Canarias, Spain, (9) Dpto de Astrofísica, Universidad de La Laguna, Spain
PP 025080
Stellar-activity analysis of the nearby M dwarf GJ 526. Multi-dimensional Gaussian-process modelling of RV, FWHM and S-index
(1) Instituto de Astrofísica de Canarias, (2) Departamento de Astrofísica, Universidad de La Laguna, (3) Consejo Superior de Investigaciones Científicas,
(4) Light Bridges S. L., (5) Dipartimento di Fisica e Astronomia "Galileo Galilei", Universitá di Padova, (6) Instituto de Astrofísica e Ciências do Espaço, CAUP, Universidade do Porto, (7) Departamento de Física de la Tierra y Astrofísica & IPARCOS-UCM, Facultad de Ciencias Físicas, Universidad Complutense de Madrid, (8) Centro de Astrobiología (CAB), CSIC-INTA, (9) Observatoire Astronomique de l’Université de Genève, (10) Departamento de Física e Astronomia, Faculdade de Ciências, Universidade do Porto, (11) INAF - Osservatorio Astrofisico di Torino, (12) INAF - Osservatorio Astrofisico di Trieste, (13) IFPU - Institute for Fundamental Physics of the Universe, (14) Centro de Astrofísica da Universidade do Porto
PP 025079
Characterising the short-orbital period X-ray transient Swift J1910.2-0546
(1) ESO, Chile, (2) IAC, Spain, (3) Departamento de Astrofísica, Universidad de La Laguna, Spain, (4) Department of Astrophysics/IMAPP, Radboud University Nijmegen, Netherlands, (5) SRON, Netherlands Institute for Space Research, Netherlands, (6) Max Planck Institute for Astronomy, Germany, (7) Astronomy, Engineering, and Physics Department, Fresno City College, USA, (8) Instituto de Alta Investigación, Universidad de Tarapacá, Chile, (9) School of Physics & Astronomy, University of Southampton, UK, (10) Astrophysics, Department of Physics, University of Oxford, UK, (11) Department of Physics, California State University, Fresno, USA, (12) Gran Telescopio Canarias, Spain, (13) Center for Astro, Particle and Planetary Physics, New York University Abu Dhabi, UAE
PP 025078
Constraining the TeV gamma-ray emission of SN 2024bch, a possible type IIn-L from a red supergiant progenitor. Multiwavelength observations and analysis of the progenitor
Many
PP 025077
The intracluster light as an estimator of the cluster mass profile
Instituto de Astrofísica de Canarias, Universidad de La Laguna
PP 025076
Identification of Nonlinear Damping of Transverse Loop Oscillations by KHI-induced Turbulence
1 Department of Mathematics and Statistics, University of Exeter, UK
2 Instituto de Astrofísica de Canarias, Spain
3 Departmento de Astrofísica, Universidad de La Laguna, Spain
PP 025075
A reference framework for extremely metal-poor OB star studies: calibrations for stellar parameters and intrinsic colours
(1) Centro de Astrobiología, (2) Institut für Astrophysik Göttingen, (3) IAC, (4) ULL
PP 025074
Binarity at LOw Metallicity (BLOeM): Enhanced multiplicity of early B-type dwarfs and giants at $Z=0.2\,{\rm Z}_\odot$
(1) MPIA, Heidelberg, (2) IAC, (3) ULL
PP 025073
Binarity at LOw Metallicity (BLOeM): Multiplicity of early B-type supergiants in the Small Magellanic Cloud
(1) Royal Observatory of Belgium (2) University of Liège (3) IAC, (4) ULL
PP 025072
NASIM: Revealing the low surface brightness Universe from legacy VISTA data
(1) IAC, (2) ULL, (3) University of Southampton, (4) CEFCA, (5) INAF, (6) IFPU
PP 025071
Fuzzy dark matter fails to explain dark matter cores
(1) Tartu Observatory, University of Tartu, Observatooriumi 1, Toravere 61602, Estonia, (2) Keemilise ja Bioloogilise Füüsika Instituut, Rävala pst. 10, 10143 Tallinn, Estonia, (3) IAC
PP 025070
Revisiting symbiotic binaries with interferometry: II. New PIONIER data
(1) ESO-Garching, (2) IAC, (3) Astronomical Institute of Charles University
PP 025069
V Sge: Supersoft Source or Exotic Hot Binary? I. An X-Shooter campaign in the high state
(1) Finnish Centre for Astronomy with ESO (FINCA), University of Turku; (2) Department of Physics & Astronomy, University of Southampton; (3) Astrophysics, Department of Physics, University of Oxford; (4) Department of Physics, University of the Free State, South Africa; (5) Instituto de Astrofísica de Canarias (IAC); (6) Departamento de Astrofísica, Universidad de La Laguna, Spain
PP 025067
Assessing interstellar comet 3I/ATLAS with the 10.4 m Gran Telescopio Canarias and the Two-meter Twin Telescope
(1) UCM, (2) IAC, (3) ULL (4) Light Bridges (5) GRANTECAN
PP 025066
Discovery of SiC and Iron Dust Around AGB Stars in the very Metal-Poor Sextans A Dwarf Galaxy with JWST: Implications for Dust Production at High Redshift
*: IAC/ULL
PP 025065
NGC 663 as a laboratory for massive star evolution
[1] Universidad de Alicante, [2] Leibniz-Institut f\"ur Astrophysik Potsdam [3] IAC/ULL
PP 025064
The DBL Survey II: towards a mass-period distribution of double white dwarf binaries
(1) Warwick, (2) IAC, (3) ULL
PP 025063
The relationship between nuclear rings and the overall galaxy morphology
(1) IFAE, (2) ULL, (3) IAC, (4) Universitats-Sternwarte München
PP 025062
Dissecting NGC 3132: Tracing the mass-loss history of the southern ring planetary nebula
(1) IAASARS-NOA, Greece, (2) U. Patras, Greece, (3) U. Itajubá, Brazil, (4) U. Cardiff, UK, (5) IAC, Spain, (6) ULL, Spain, (7) O. Valongo, Brazil, (8) Leiden U., Netherlands, (9) LNA, Brazil
PP 025061
Nickel and Iron-rich clumps in planetary nebulae: New discoveries and emission line diagnostics
(1) IAASARS-NOA, Greece, (2) U. Patras, Greece, (3) U. tajubá, Brazil, (4) U. Cardiff, UK, (5) IAC, Spain, (6) ULL, Spain, (7) O. Valongo, Brazil, (8) LNA, Brazil, (9) Leiden U., Netherlands, (10) UWO, Canada, (11) IESE-UWO, Canada, (12) SETI Inst., USA
PP 025060
Deep survey of millimeter RRLs towards the planetary nebulae IC 418 and NGC 7027
(1) IAC-ULL; (2) OAN, IGN/CNIG; (3) Chalmers UoT; (4) IFF/CSIC; (5) FQA-ICCUB/UB
PP 025059
Kinematic misalignment as a driver of black hole activity in galaxies with external interactions
(1) University of Southampton, (2) DARK, (3) Universidade Federal do Rio Grande do Sul, (4) Australian National University, (5) ASTRO 3D, Australia, (6) IAC, (7) ULL
PP 025058
Binarity at LOw Metallicity (BLOeM): Pipeline-Determined Physical Properties of OB Stars
(1) IAC, (2) ULL
PP 025057
CGCS 6306, another X-ray-emitting asymptotic giant branch star confirmed to be a symbiotic binary
(1) IAC, (2) Astronomical Institute of Charles University, (3) Instituto de Astrofísica de Andalucía, (4) Universidad Nacional Autónoma de México, (5) Universidade de São Paulo
PP 025056
Chromospheric velocities in an M3.2 flare using He I 1083.0 nm and Ca II 854.2 nm
(1) Instituto de Astrofísica de Canarias (IAC), (2) Departamento de Astrofísica, Universidad de La Laguna, (3) Institute of Theoretical Astrophysics, University of Oslo, (4) Rosseland Centre for Solar Physics, University of Oslo, (5) Astronomical Institute of the University of Bern, (6) School of Physics and Astronomy, University of Glasgow, (7) UCL Mullard Space Science Laborator
PP 025055
Relatively young thick discs in low-mass star-forming late-type galaxies
(1) Max Planck Institute for Astronomy, (2) University of Heidelberg, (3) IAC, (4) ULL, (5) Liverpool John Moores University
PP 025054
Assessing the accuracy of the star formation rate measurements by direct star count in molecular clouds
(1) Max Planck Institute for Astronomy, (2) Max Planck Institute for Radioastronomy, (3) ULL, (4) IAC, (5) INAOE, (6) Lomonosov Moscow State University, (7) Cardiff University, (8) Yunnan University, (9) UCM, (10) Shanghai Astronomical Observatory, (11) Golestan University
PP 025053
The Intrinsic Flattening of Galaxy Disks
(1) Queen's University, (2) ULL, (3) IAC, (4) Université de Montréal, (5) Mila–Québec Artificial Intelligence Institute, (6) Ciela–Montréal Institute for Astrophysical Data Analysis and Machine Learning
PP 025052
Advancing accuracy in age determinations of old-disk stars using an oscillating red giant in an eclipsing binary
U. Bologna, IAC
PP 025051
Red supergiant stars in binary systems II. Confirmation of B-type companions of red supergiants in the Small Magellanic Cloud using Hubble ultra-violet spectroscopy
(1) CAB, (2) IAC, (3) Argelander Institute for Astronomy Bonn, (4) JHU, (5) Alicante, (6) European University of the Canarias
PP 025050
A study of sixty-one massive over-contact binary candidates from the OGLE survey of the Magellanic Clouds
(1) IAC, (2) Lund, (3) Argelander Institute for Astronomy, Bonn
PP 025049
Is the Symbiotic Recurrent Nova T CrB Late? Recent Photometric Evolution and Comparison with Past Pre-Outburst Behaviour
(1) IAC, (2) Astronomical Institute of Charles University, (3) Astronomical Observatory, University of Warsaw, (4) National Centre for Nuclear Research, (5) ULL, (6) Astronomical Institute, University of Wrocław
PP 025048
CHEX-MATE: exploring the kinematical properties of Planck galaxy clusters
(1) Dipartimento di Fisica G. Occhialini, Università degli Studi di Milano Bicocca (Italy)
(2) IAC
(3) DA-ULL
(4) INAF – Osservatorio di Astrofisica e Scienza dello Spazio di Bologna (Italy)
(5) INFN, Sezione di Bologna (Italy)
PP 025047
Decoding the molecular torus of NGC 1068: Insights into its structure and kinematics from high-resolution ALMA observations
(1) Leiden Observatory, (2) IAC, (3) ULL
PP 025046
Continuum, CO and Water vapour maps of the Orion Nebula. First millimetre spectral imaging with Concerto
(1) IPAG, (2) LPSC, (3) LAM, (4) Institut Néel, (5) Observatoire astronomique de Strasbourg, (6) ESO, (7) IRAM Granada, (8) IRAM Grenoble, (9) Universidad de Valparaíso, (10) MINGAL, (11) Laboratoire Lagrange, (12) Cardiff University, (13) AIM Paris-Saclay, (14) Sapienza Università di Roma, (15) IPM Tehran, (16) Centro de Astrobiología Madrid, (17) IAC, (18) Universidad de La Laguna, (19) University of the Western Cape, (20) National Observatory of Athens, (21) University of Athens, (22) Argonne National Laboratory, (23) LERMA Paris, (24) ICE-CSIC Barcelona, (25) ICREA Barcelona, (26) IRAP Toulouse, (27) Università di Roma ‘Tor Vergata’
PP 025045
Molecular gas excitation and outflow properties of obscured quasars at z~0.1
(1) IAC, (2) ULL, (3) OAN, (4) IFF
PP 025044
Evaluating quenching in cosmological simulations of galaxy formation with spectral covariance in the optical window
(1) Instituto de Astrofìsica de Canarias, C/ Vìa La ctea s/n, La Laguna, E-38200 La Laguna, Tenerife, Spain, (2) Departamento de Astrofsica, Universidad de La Laguna, E-38205 La Laguna, Tenerife, Spain, (3) Department of Physics and Astronomy, University College London, Gower Street, London WC1E 6BT, UK, (4) Facultad de Física, Universidad de Sevilla, Avda. Reina Mercedes s/n, Campus de Reina Mercedes, E-41012 Sevilla, Spain, (5) INAF- Osservatorio Astronomico di Brera, Via Brera 28, 20121, Milano, Italy, (6) Center for Computational Astrophysics, Flatiron Institute, New York, NY 10010, USA
PP 025043
Symbiotic stars in the era of modern ground- and space-based surveys
(1) IAC, (2) Astronomical Institute of Charles University
PP 025042
V4141 Sgr: Outflows and repeated outbursts
(1) IAC, (2) Astronomical Institute of Charles University, (3) Nicolaus Copernicus Astronomical Center, Polish Academy of Sciences, (4) Southern Spectroscopic Project Observatory Team, (5) Kleinkaroo Observatory
PP 025041
Three new 2+2 quadruple systems with changing inclination
(1) Astronomical Institute of Charles University, (2) Hvězdárna Jaroslava Trnky ve Slaném, (3) Czech Astronomical Society, (4) Institute of Physics of the Czech Academy of Sciences, (5) University of Texas Rio Grande Valley, (6) Silesian University, (7) IAC, (8) Private Observatory Jílové u Prahy
PP 025040
Signature of spin-down stalling in stellar magnetic activity. The case of the open cluster NGC 6811
(1) Universidade do Porto, (2) IAC, (3) ULL, (4) INAF Osservatorio Astrofisico di Catania, (5) Université Paris-Saclay
PP 025039
A super-Chandrasekhar mass type Ia supernova progenitor at 49 pc set to detonate in 23 Gyr
(1) University of Warwick, (2) IAC, (3) ULL, (4) NOT
PP 025038
The Local Group Symbiotic Star Population and its Tenuous Link with Type Ia Supernovae
(1) Valongo Observatory, Federal University of Rio de Janeiro, Brazil, (2) Astronomical Institute of Charles University, (3) IAC
PP 025037
JWST MIRI reveals the diversity of nuclear mid-infrared spectra of nearby type-2 quasars
(1) IAC, (2) ULL, (3) CAB, (4) IFF, (5) Kavli Institute for Cosmology, (6) Cavendish Laboratory, (7) UCL.
PP 025036
The OTELO survey: New evidence of downsizing from the specific star formation rates, stellar mass functions, and star formation histories of a sample of low-mass galaxies at 0.38
The OTELO survey: New evidence of downsizing from the specific star formation rates, stellar mass functions, and star formation histories of a sample of low-mass galaxies at 0.38
(1) IAC
(2) Departamento de Astrofísica, Universidad de La Laguna (ULL)
(3) Asociación Astrofísica para la Promoción de la Investigación, Instrumentación y su Desarrollo, ASPID,
(4) Institut de Radioastronomie Millimétrique (IRAM)
(5) Fundación Galileo Galilei–INAF,
(6) Astronomical Observatory Institute, Faculty of Physics and Astronomy, Adam Mickiewicz University, ul. Słoneczna
(7) Departamento de Física de la Tierra y Astrofísica, Instituto de Física de Partículas y del Cosmos, IPARCOS. Universidad Complutense de Madrid (UCM)
(8) Instituto de Física de Cantabria (CSIC-Universidad de Cantabria)
(9) Instituto de Astrofísica de Andalucía (CSIC)
(10) Centro de Astrobiología (CSIC/INTA)
(11) Instituto de Astronomía, Universidad Nacional Autónoma de México
(12) ISDEFE for European Space Astronomy Centre (ESAC)/ESA
(13) Space Science and Geospatial Institute (SSGI), Entoto Observatory and Research Center (EORC)
(14) Physics Department, Mbarara University of Science and Technology (MUST),
PP 025035
The Structure, Populations and Kinematics of the Milky Way central and inner Bulge with OGLE, APOGEE and Gaia data
(1) Department of Astronomy, China West Normal University, Nanchong, 637002, P. R. China; (2) Dipartimento di Fisica e Astronomia “Galileo Galilei”, Universitá degli Studi di Padova, Vicolo Osservatorio 3, I-35122, Padova, Italy; (3) IAC; (4) ULL; (5) Department of Astronomy, The Ohio State University, Columbus, OH 43210, USA; (6) Center for Cosmology and AstroParticle Physics, The Ohio State University, Columbus, OH 43210, USA
PP 025034
Convergence study of ambipolar diffusion in realistic simulations of magneto-convection
(1) Instituto de Astrofísica de Canarias, 38205 La Laguna, Tenerife, Spain; (2) Departamento de Astrofísica, Universidad de La Laguna, 38205, La Laguna, Tenerife, Spain
PP 025033
Generalized Te([O III])−Te(He I) Discrepancies in Ionized Nebulae: Possible Evidence of Case B Deviations and Temperature Inhomogeneities
(1) Instituto de Astronomía UNAM, (2) University of Minnesota, (3) Gonzaga University, (4) IAC, (5) Universität Heidelberg, (6) Northwestern University, (7) INAOE, (8) University of Edinburgh, (9) ING
PP 025032
TESS light curves and period changes in low-mass eclipsing binary BB Persei
(1) Astronomical Institute of Charles University, (2) Masaryk University, (3) Institute of Physics of the Czech Academy of Sciences, (4) Czech Astronomical Society, (5) Observatory in Holovousy, (6) Silesian University, (7) Mt. Suhora Observatory, (8) IAC, (9) University of Texas Rio Grande Valley
PP 025031
Alpha-element abundance patterns in star-forming regions of the local Universe
(1) IAC, Spain, (2) ULL, Spain, (3) IA-UNAM, Mexico, (4) U.Edimbourgh, UK, (5) INAOE, Mexico, (6) ING, La Palma, Spain
PP 025030
The properties of the obscuring material of an AGNs sample from mid-IR and X-ray simultaneous fitting
(1) IAC, (2) ULL, (3) IRyA-UNAM, (4) IA-UNAM
PP 025029
Chlorine abundances in star-forming regions of the local Universe
(1) IAC, Spain, (2) ULL, Spain, (3) UNAM, Mexico (4) IfA, UK, (5) INAOE, México, (6) ING, Spain
PP 025028
Integral field spectroscopy of the planetary nebula NGC 3242 and the puzzling nature of its low ionization structures
(1) IAASARS, Greece, (2)U. Patras, Greece, (3) IAC, Spain, (4) ULL, Spain, (5)O. Valongo, Brazil, (6) Cardiff U., UK, (7) U. F. Itajubá, Brazil, (8) U. N. Córdova, Argentina, (9) LNA, Brazil, (10) Leiden Obs. Netherlands
PP 025027
HADES RV Programme with HARPS-N at TNG. XVI. A super-Earth in the habitable zone of the GJ 3998 multi-planet system
(1) Instituto de Astrofísica de Canarias, (2) Universidad de La Laguna, (3) Light Bridges S. L., (4) Consejo Superior de Investigaciones Científicas, (5) INAF - Palermo, (6) Institut de Ciències de l’Espai, (7) Institut d’Estudis Espacials de Catalunya, (8) INAF - Torino, (9) Departamento de Física de la Tierra y Astrofísica & IPARCOS-UCM, (10) INAF - Catania
PP 025026
A physically motivated galaxy size definition across different state-of-the-art hydrodynamical simulations
(1) Instituto de Astrofísica de Canarias, Calle Via Láctea s/n, E-38206 La Laguna, Tenerife, Spain
(2) Universidad de La Laguna, Avda. Astrofísico Fco. Sánchez, E-38205 La Laguna, Tenerife, Spain
(3) Astrophysics Research Institute, Liverpool John Moores University, 146 Brownlow Hill, Liverpool, L3 5RF, U
(4) Department of Physics and Astronomy, University of California, Riverside, 900 University Avenue, Riverside, CA 92521, USA
(5) New York University Abu Dhabi, PO Box 129188 Abu Dhabi, United Arab Emirates
(6) Center for Astrophysics and Space Science (CASS), New York University Abu Dhabi
(7) Max-Planck-Institut für Astronomie, Königstuhl 17, D-69117 Heidelberg, Germany
(8) Leibniz-Institut für Astrophysik Potsdam (AIP), An der Sternwarte 16, D-14482 Potsdam, Germany
(9) Departamento de Física Teórica, Módulo 15, Facultad de Ciencias, Universidad Autónoma de Madrid, 28049 Madrid, Spain
(10) Centro de Investigación Avanzada en Física Fundamental (CIAFF), Facultad de Ciencias, Universidad Autónoma de Madrid,
28049 Madrid, Spain
(11) International Centre for Radio Astronomy Research, University of Western Australia, 35 Stirling Highway, Crawley, Western
Australia 6009, Australia
PP 025025
Spatially resolved circumnuclear coronal [Fe VII] emission in nearby Seyfert galaxies
(1) ULL, (2) IAC, (3) National Centre for Nuclear Research
PP 025024
The Complete Spitzer Survey of Stellar Structure in Galaxies (CS4G)
(1) Instituto de Astrofísica de Canarias, c/ Vía Láctea s/n, E-38205, La Laguna, Tenerife, Spain
(2) Departamento de Astrofísica, Universidad de La Laguna, E-38206, La Laguna, Tenerife, Spain
(3) Space Physics and Astronomy Research Unit, University of Oulu, Pentti Kaiteran katu 1, FI-90014 Oulu, Finland
(4) Departamento de Física de la Tierra y Astrofísica, Universidad Complutense de Madrid, E-28040 Madrid, Spain
(5) Centre of Astrophysics Research, School of Physics, Astronomy and Mathematics, University of Hertfordshire, Hatfield, UK
(6) Department of Physics and Astronomy, University of Alabama, Box 870324, Tuscaloosa, AL 35487, USA
(7) IPAC, Mail Code 314-6, Caltech, 1200 E. California Blvd., Pasadena, CA 91125, USA
(8) Max-Planck-Institut für Extraterrestriche Physik, Giessenbach-Str. 1, D-85748 Garching, Germany
(9) Aix Marseille Univ, CNRS, CNES, LAM, Marseille, France
(10) Centre for Extragalactic Astronomy, Department of Physics, Durham University, South Road, Durham DH1 3LE, UK
(11) MMT Observatory, University of Arizona, 933 N Cherry Ave, Tucson AZ 85721
(12) Kavli Institute for Astronomy and Astrophysics, Peking University, 12 Beijing 100871, P. R. China
(13) Department of Astronomy, School of Physics, Peking University, Beijing 100871, P. (14) University of Louisville, Department of Physics and Astronomy, 102 Natural Science Building, 40292, KY Louisville, USA
(15) Finnish Centre of Astronomy with ESO (FINCA), Vesilinnantie 5, FI-20014 University of Turku, Finland
(16) Specim, Spectral Imaging Ltd., Elektroniikkatie 13, FI-90590 Oulu, Finland
(17) Department of Astronomy and Atmospheric Sciences, Kyungpook National University, Daegu 702-701, Republic of Korea
(18) Department of Physics and Astronomy, Stony Brook University, Stony Brook, NY 11794-3800, USA
(19) Normet Oy, Elektroniikkatie 8, FI-90590 Oulu, Finland
(20) The Observatories, Carnegie Institution for Science, 813 Santa Barbara Street, Pasadena, CA 91101, USA
(21) Department of Astronomy \& Astrophysics, University of Chicago, 5640 South Ellis Avenue, Chicago, IL 60637, USA
(22) Observatório do Valongo, Universidade Federal do Rio de Janeiro, Rio de Janeiro, Brazil
(23) Kapteyn Astronomical Institute, University of Groningen, PO Box 800, NL-9700 AV Groningen, the Netherlands
(24) Observatorio Astronómico Nacional (IGN), C/Alfonso XII, 3, E28014 Madrid, Spain
(25) NASA Headquarters Mary W. Jackson Building, 300 E Street SW, Washington, DC 20546, USA
(26) Steward Observatory and Department of Astronomy, University of Arizona, 933 N. Cherry Ave., Tucson, AZ 85721, USA
PP 025023
JWST/MIRI Study of the Enigmatic Mid-Infrared Rings in the Planetary Nebula NGC 1514
(1) JPL, (2) OAN, (3) IAC, (4) ULL, (5) NOT, (6) NSF NOIRLAB, (7) IAA
PP 025022
Search for new Galactic Wolf-Rayet stars using Gaia DR3. I. Candidate selection and the follow-up of the bright sample
(1) Southern Spectroscopic Project Observatory Team, (2) IAC, (3) Astronomical Institute of Charles University
PP 025021
JWST/MIRI detection of [Ne V] and [Ne VI] in M83: Evidence for the long sought-after AGN?
(1) STScI, USA; (2) IAC; (3) ULL
PP 025020
Unveiling the warm molecular outflow component of type-2 quasars with SINFONI
(1) SISSA, (2) IAC, (3) ULL
PP 025019
The GECKOS Survey: Identifying kinematic sub-structures in edge-on galaxies
1 European Southern Observatory,
2 ARC Centre of Excellence for All Sky Astrophysics in Three Di-
mensions (ASTRO-3D)
3 School of Physics, University of New South Wales,
4 Centre for Extragalactic Astronomy, Durham University,
5 National Research Council of Canada,
6 Centre for Astrophysics and Supercomputing, Swinburne University
of Technology,
7 Astrophysics Research Institute, Liverpool John Moores University,
8 Sub-department of Astrophysics, Department of Physics, University
of Oxford,
9 Max-Planck-Institut für Extraterrestrische Physik,
10 International Centre for Radio Astronomy Research (ICRAR), The
University of Western Australia,
11 Research School of Astronomy and Astrophysics, Australian Na-
tional University,
12 Sydney Institute for Astronomy, School of Physics, The Uni-
versity of Sydney,
13 Observatoire de Paris,
14 Collège de France,
15 Cardiff Hub for Astrophysics Research & Technology, School of
Physics & Astronomy, Cardiff University,
16 Instituto de Astrofísica de Canarias,
17 Departamento de Astrofísica, Universidad de La Laguna,
18 Institute for Computational Cosmology, Department of Physics,
Durham University,
19 Homer L. Dodge Department of Physics & Astronomy, University
of Oklahoma,
20 Research Centre for Astronomy, Macquarie University, 21 European Southern Observatory, Chile,
22 Universidade Cidade de São Paulo/Universidade Cruzeiro do Sul,
23 Universitäts-Sternwarte, Fakultät für Physik, Ludwig-Maximilians-
Universität München,
24 Department of Astrophysics, University of Vienna,
25 Department of Physics and Astronomy, University of Utah
PP 025018
Revisiting symbiotic binaries with interferometry. I. The PIONIER archival collection
(1) IAC, (2) Astronomical Institute of Charles University, (3) ESO-Garching
PP 025017
A comprehensive Gaia view of ellipsoidal and rotational red giant binaries
(1) Université Côte d’Azur, (2) IAC, (3) ULL
PP 025016
Magnetic activity evolution of solar-like stars: II. $S_{\rm ph}$-Ro evolution of Kepler main-sequence targets
(1) IAC, (2) ULL, (3) Universidade do Porto, (4) Space Telescope Science Institu, (5) Université Paris-Saclay, (6) Rosseland Centre for Solar Physic, (7) Osservatorio Astrofisico di Catania, (8) Vanderbilt University,(9) Ohio State University, (10) University of Hawai‘i
PP 025015
Kepler meets Gaia DR3: Homogeneous extinction-corrected color-magnitude diagram and binary classification
(1) IAC, (2) ULL, (3) Université Paris-Saclay, (4) Ohio State University, (5) Universidade do Porto, (6) Karl-Franzens Universität Graz, (7) University of Sydney, (8) Flatiron Institute, (9) Charles University
PP 025014
The Galaxy Activity, Torus, and Outflow Survey (GATOS). VII. The 20-214 $μ$m imaging atlas of active galactic nuclei using SOFIA
(1) University of Texas at San Antonio, (2) University of South Carolina, (3) CAB, (4) IAC, (5) ULL
PP 025013
The Galaxy Activity, Torus, and Outflow Survey (GATOS): VI. Black hole mass estimation using machine learning
(1) Observatoire de Paris, LERMA; (2) IAC, (3) ULL
PP 025012
A Link Between White Dwarf Pulsars and Polars: Multiwavelength Observations of the 9.36-Minute Period Variable Gaia22ayj
(1) Caltech; (2) Finnish Centre for Astronomy with ESO (FINCA); (3) IAC; (4) ULL
PP 025011
The IACOB project XIV. New clues on the location of the TAMS in the massive star domain
(1) IAC/ULL, (2) ESO, (3) Universität Innsbruck, (4) Observatoire de Geneve, (5) MPIA-Heidelberg
PP 025010
Improving the stellar age determination through joint modeling of binarity and asteroseismology -- Grid modeling of the seismic red-giant binary KIC 9163796
(1) IAC; (2) ULL ; (3) MPIA; (4) Radboud University; (5) KU Leuven; (6) California State University; (7) INAF - Abruzzo; (8) INFN - Pisa; (9) CEA
(10) University of Graz (11) University of Sydney; (12) Graz University of Technology; (13) University of New South Wales
PP 025009
Constraining the shape of dark matter haloes using only starlight. I. A new technique and its application to the galaxy Nube
(1) IAC, (2) ULL, (3)
PP 025008
State-dependent signatures of jets and winds in the optical and infrared spectrum of the black hole transient GX 339$-$4
IAC, ULL and other international institutions
PP 025007
Accretion disc winds imprint distinct signatures in the optical variability spectrum of black hole transients
(1) IAC; (2) ULL; (3) University of Southampton
PP 025006
Signs of `Everything Everywhere All At Once' formation in low surface brightness globular cluster-rich dwarf galaxies
(1) IAC; (2) ULL; (3) CAS; (4) ASTRO 3D; (5) UCSC; (6) SJSU; (7) ESO
PP 025005
Detection of binary companions below the diffraction limit with lucky imaging
(1) IAC (2) ULL (3)UC (4) NOT
PP 025004
The IACOB project XIII. Helium enrichment in O-type stars as a tracer of past binary interaction
(1) Instituto de Astrofísica de Canarias, c/Vía Láctea, s/n, E-38205 La Laguna, Tenerife, Spain
(2) Departamento de Astrofísica, Universidad de La Laguna, E-38206 La Laguna, Tenerife, Spain
(3) Argelander Institut für Astronomie, Auf dem Hügel 71, DE-53121 Bonn, Germany
(4) Center for Computational Astrophysics, Division of Science, National Astronomical Observatory of Japan, 2-21-1, Osawa, Mitaka, Tokyo 181-8588, Japan
(5) Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, DE-53121 Bonn, Germany
(6) LMU Munich, Universitätssternwarte, Scheinerstrasse 1, 81679 München, Germany
PP 025003
Implications of the intriguing constant inner mass surface density observed in dark matter halos
IAC
PP 025002
X-Shooting ULLYSES: Massive stars at low metallicity -- V. Effect of metallicity on surface abundances of O stars
(1) Université Montpellier, (2) ULL/IAC
PP 025001
X-Shooting ULLYSES: Massive Stars at Low Metallicity X. Physical Parameters and Feedback of Massive Stars in the LMC N11 B Star-Forming Region
(1) Universität Potsdam, (2) ULL/IAC