Preprints in 2026
PP 026134
Gaia FGK benchmark stars Abundances of n-capture elements of the third version
Instituto de Astrofísica de Canarias, C. Vía Láctea, s/n, 38205 La Laguna, Santa Cruz de Tenerife, Spain.
Universidad de La Laguna, Dpto. Astrofísica, Av. Astrofísico Francisco Sánchez, 38206 La Laguna, Santa Cruz de Tenerife, Spain
PP 026133
Stellar nucleosynthesis in the era of large surveys: S-process-polluted binaries in GALAH DR4
(1) IAC, (2) ULL ,(3) INAF-Torino, (4) IvS-KU Leuven, (5) VIU, (6) ULB, (7) University of Cambridge, (8) UDP
PP 026132
Ionized Gas Kinematics and Star-forming Clumps in Extremely Metal-poor Galaxies
(1) IAC
(2) Universidad de La Laguna, E-38206 La Laguna, Spain
(3) Isaac Newton Group of Telescopes, Apartado 321, E-38700 Santa Cruz de La Palma, Tenerife, Spain
(4) CEFCA, Unidad Asociada al CSIC, Plaza San Juan 1, 44001 Teruel, Spain,
(5) Katonah, NY 10536, USA
PP 026131
An improvement to the spatial discretisation in the Astrophysical Weighted Particle Hydrodynamics method
(1) Instituto de Astrofísica de Canarias, (2) Universidad de La Laguna
PP 026130
First L-type substellar object discovered in the vicinity of the embedded cluster NGC 2023
(1) Instituto de Astrofísica de Canarias, (2) Universidad de La Laguna, Departamento de Astrofísica (3) Laboratoire d’Astrophysique de Bordeaux, CNRS and Université de Bordeaux (4) Institut universitaire de France (IUF) (5) Astrobiology Research Unit, Université de Liège, (6) Department of Earth, Atmospheric and Planetary Science, Massachusetts Institute of Technology, (7) Department of Physics and Astronomy, The University of Western Ontario, (8) Institute for Earth and Space Exploration, The University of Western Ontario
PP 026129
The DESIRED strong-line calibrations: I. New empirical metallicity relations for the local and high-redshift Universe
(1) INAOE, Mexico, (2) IA-UNAM, CDMX, Mexico, (3) IAC, Spain, (4) ULL, Spain, (5) U. Edinbourgh, UK, (6) IA-UNAM, Ensenada, Mexico, (7) ICF-UNAM, Mexico, (8) CIEMAT, Spain, (9) U. Heidelberg, Germany, (10) MAO-NASU, Ukraine, (11) IAA, Spain
PP 026128
X-Shooter view of planetary nebulae microstructures I: The case of NGC 7009 knots
(1) IAASARS-NOA, Greece; (2) U. Patras, Greece; (3) IAC, Spain; (4) ULL, Spain; (5) Obs. Valongo, Brazil
PP 026127
A two-stage settling of the Milky Way disk revealed by precise ChronoGal ages
(1) IAC, (2) ULL, (3) Universidad de Granada, (4) Instituto Carlos I de Física Teórica y Computacional, (5) INAF, (6) INFN, (7) University of Victoria, (8) Korea University
PP 026126
Dynamics of tidal dwarf galaxies in the system Arp 72
(1) INAOE, (2) CEFCA, (3) Unidad Asociada CEFCA-IAA, (4) East Tennessee State University, (5) North-West University, (6) NITheCS, (7) ULL, (8) IAC
PP 026125
Proto-Planetary Nebulae Are Not the Precursors of Planetary Nebulae With Close Binary Central Stars
(1) Valparaiso, (2) IAC, (3) ULL
PP 026124
Spectral classification of OB-type stars using tree-based ensemble methods and evaluation of their explainability
(1) Universidad Nacional Autonoma de Honduras, (2) IAC/ULL, (3) Universidad Mayor Chile, (4) Univ. Politécinca de Valencia, (5) ESO
PP 026123
The Physics of the Nebular Phase in Black Hole X-ray Binaries: Modelling V404 Cygni
IAC, ULL, CEFCA and Oxford University
PP 026122
A homogeneous three-dimensional view of Molecular Cloud kinematics out to 2.5 kpc. Using Young Stellar Objects and Open Clusters as complementary tracers
Universidade da Coruña, ISTA, IAC, ULL, UB, UCCUB, IEEC, U. Lund
PP 026121
Signatures of rocky debris accretion in AF-Type planet hosts
(1)INAF - Osservatorio astronomico di Palermo, Italy
(2) Centro de Astrobiología (CAB) CSIC-INTA, Spain
(3)Institute of Applied Computing & Community Code (IAC3). University of the Balearic Islands, Spain
(4) Departamento de Física Teórica y del Cosmos, Universidad de Granada,Spain
(5) Instituto de Astrofísica de Canarias, Spain
PP 026120
The JWST Proto-PAH Project: Detection of the methyl radical CH3 in the highly evolved C-rich object SMP LMC 011
(1) IAC-ULL; (2) CSIC; (3) Western Ontario Univ.
PP 026119
SPAMMS: 3D spectroscopic modelling of stellar surfaces. II. Implementation of Kurucz and TLUSTY model atmospheres
(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) Institute of Astronomy, KU Leuven, Celestijnlaan 200D, 3001 Leuven, Belgium
(4) Leuven Gravity Institute, KU Leuven, Celestijnenlaan 200D, box 2415, 3001 Leuven, Belgium
PP 026118
Spectral evolution of hot hybrid white dwarfs: II. Photometry
(1) Heidelberg, (2) IAC, (3) ULL, (4) Potsdam, (5) Tubingen
PP 026117
Classifying white dwarfs from multi-object spectroscopy surveys with machine learning
(1) Warwick, (2) IAC, (3) ULL
PP 026116
AT 2022csn: A Photometrically Peculiar Optical/UV Tidal Disruption Event in a Type II AGN
[1] Tel Aviv University, [2] IAC, [3] ULL
PP 026115
Bridging integrated-light and resolved-star studies of Local Group dwarf spheroidals. A novel use of deep imaging based on amateur telescopes
(1) Instituto de Astrofísica de Canarias, Vía Láctea S/N, E-38205 La Laguna, Spain (2) Departamento de Astrofísica, Universidad de La Laguna, E-38206 La Laguna, Spain (3) Institute of Space Sciences (ICE, CSIC), Campus UAB, Carrer de Can Magrans, s/n, 08193 Barcelona, Spain (4) Parc Astronòmic Muntanyes de Prades, C/ Muralla, 3 43364, Prades, Tarragona, Spain
PP 026114
The Physics of the Nebular Phase in Black Hole X-ray Binaries: Modelling V404 Cygni
(1) Instituto de Astrofísica de Canarias, E-38205 La Laguna, Tenerife, Spain
(2) Departamento de astrofísica, Universidad de La Laguna, E-38206 La Laguna, Tenerife, Spain
(3) Centro de Estudios de Física del Cosmos de Aragón (CEFCA), Plaza San Juan 1, 44001 Teruel, Spain
(4) Astrophysics Subdepartment, Department of Physics, University of Oxford, Keble Road, Oxford, OX13RH, UK
PP 026113
Serendipitous discovery of an almost-dark galaxy in the Virgo Cluster
(1) Instituto de Astrofísica de Canarias, Vía Láctea S/N, E-38205 La Laguna, Spain
(2) Departamento de Astrofísica, Universidad de La Laguna, E-38206 La Laguna, Spain
(3) Kapteyn Astronomical Institute, University of Groningen, P.O. Box 800, 9700AV Groningen, The Netherlands
(4) Leibniz-Institut für Astrophysik Potsdam (AIP), An der Sternwarte 16, 14482 Potsdam, Germany
(5) Department of Astronomy and the DiRAC Institute, University of Washington, 3910 15th Avenue, NE, Seattle, WA 98195, USA
(6) Bernoulli Institute of Mathematics, Computer Science and Artificial Intelligence, University of Groningen, Groningen, The Netherlands
(7) Institute of Space Sciences (ICE, CSIC), Campus UAB, Carrer de Can Magrans, s/n, E-08193 Barcelona, Spain
(8) Light Bridges, Observatorio del Teide, Carretera del Observatorio s/n, E-38500 Guimar, Tenerife, Canarias, Spain
PP 026112
The explosive growth of the Messier 74 galaxy. A galaxy doubling its size in less than a Gigayear
(1) IAC, (2) ULL, (3) Light Bridges S.L., (4) University of Padova
PP 026111
The Quasar Feedback Survey: Ionised Outflows in type 2 QSOs with MUSE data
(1)IAC, (2) ULL,(3) Newcastle University UK, (4) ESO Germany, (5) UFSM Brazil, (6)
INAF – Osservatorio Astrofisico di Arcetri Italy, (7) Scuola Normale Superiore Italy,
(8) University of Hertfordshire UK, (9) Flatiron Institute USA, (10) Ludwig-Maximilians-Universität Germany, (11) University of Oslo Norway, (12) Centro de Astrobiología (CAB) Spain, (13) International Gemini Observatory/NSF NOIRLab USA, (14) INAF – Osservatorio di Astrofisica e Scienza dello Spazio di Bologna Italy, (15) University of Sheffield UK, (16) Max Planck Institut für Astrophysik Germany
PP 026110
The Multi-phase Biconical Outflow in the local IR-Luminous Merger IRASF01364-1042
(1) European Southern Observatory, Chile, (2) Joint ALMA Observatory, Chile, (3) Max-Planck-Institut für Radioastronomie, Germany, (4) IPAC, California Institute of Technology, USA, (5) University of California, Irvine, USA, (6) IAC, (7) ULL, (8) Ritter Astrophysical Research Center and Department of Physics and Astronomy, University of Toledo, USA (9) National Radio Astronomy Observatory, Charlottesville, USA, (10) Department of Astronomy, University of Virginia, Charlottesville, USA, (11) Department of Astronomy, University of Geneva, Switzerland, (12) Instituto de Estudios Astrofísicos, Facultad de Ingeniería y Ciencias, Universidad Diego Portales, Chile, (13) Department of Physics \& Astronomy, University of British Columbia, Canada, (13) Hiroshima Astrophysical Science Center, Hiroshima University, Japan, (14) Occidental College, Physics Department, USA, (15) Leiden Observatory, Leiden University, The Netherlands, (16) Instituto de Alta Investigación, Universidad de Tarapacá, Chile, (17) European Space Agency, c/o STScI, USA, (18) Centre for Astrophysics Research, University of Hertfordshire, UK, (19) Steward Observatory, University of Arizona, USA, (20) School of Sciences, European University Cyprus, Cyprus, (21) Institute of Astrophysics, Foundation for Research and Technology-Hellas (FORTH), Greece, (22) Department of Physics, University of Crete, Greece, (23) Department of Astronomy, University of Florida, USA, (24) Research School of Astronomy and Astrophysics, Australian National University, Australia, (25) Research School of Astronomy and Astrophysics, Australian National University, Weston Creek, ACT 2611, Australia, (26) ARC Centre of Excellence for All Sky Astrophysics in 3 Dimensions (ASTRO 3D), Australia, (27) W. M. Keck Observatory, USA, (28) Institute for Astronomy, University of Hawaii, USA
PP 026109
QUIJOTE scientific results - XX. Commissioning and First Results from the Thirty and Forty Gigahertz Instrument (TFGI)
(1) LPSC, (2) IAC, (3) ULL
PP 026108
GATOS: Distinct Feedback Modes in AGN Central Regions Revealed by Spatially Resolved JWST Spectroscopy
(1) UTSA, USA; (2) IAC, (3) ULL
PP 026107
The IACOB project XVIII. Prevalence of short-period binaries among Galactic helium rich O-type stars
(1) IAC, (2) Departamento de astrofísica, ULL, (3) IALP, CONICET–UNLP, (4) Facultad de Ciencias Astronómicas y Geofísicas, UNLP, (5) ESO-Chile, (6) CAB
PP 026106
The symphony of pulsations and binarity among massive stars using HERMES spectroscopy and TESS photometry
(1) Newcastle University (2) IAC/ULL
PP 026105
Multiplicity of Massive Stars at Low Metallicity: Early Results from the BLOeM Campaign
(1) School of Physics and Astronomy, Tel Aviv University, (2) Anton Pannekoek Institute for Astronomy, University of Amsterdam, (3) IAC/ULL
PP 026104
You're Gonna Need a Bigger Core: Calibrating Massive Star Models against Galactic OB-type Stars
(1) Max Planck Institute for Astrophysics (2) ESO/Chile, (3) IAC/ULL
PP 026103
The IACOB project XIX. Revisiting massive-star evolution with empirical TAMS constraints: updated models, overshoot calibration, and the population of blue supergiants
(1) Observatoire de Genève, (2) ESO/Chile, (3) IAC/ULL
PP 026102
The s-process at Subsolar Metallicity: Insights from High-Resolution Infrared Spectroscopy of Magellanic Cloud Planetary Nebulae
(1) U. of West Georgia, (2) U. of Texas at Austin, (3) Los Alamos National Laboratory, (4) Konkoly Observatory, (5) ELTE Eötvös Loránd University, (6) Monash University, (7) U. of Naples, (8) INAF Observatory Astronomico d'Abruzzo, (9) The NuGrid Collaboration, (10) Instituto de Astrofísica de Canarias, (11) U. de La Laguna, (12) Georgia Institute of Technology
PP 026101
Constraining the shape of dark matter haloes using only starlight II. Tests of the technique with objects of known gravitational potential
(1) Instituto de Astrofisica de Canarias, La Laguna, Tenerife, E-38200, 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, Roque Saenz Pena 456, Junin, Argentina, (4) Department of Astronomy, University of Virginia, 530 McCormick Road, Charlottesville, VA 22904, USA
PP 026100
Introducing AuriGLOBES: The effects of compressive tides, compact object-induced mass loss, and size evolution on modelling globular clusters
(1) Instituto de Astrofísica de Canarias,
(2) Departamento de Astrofísica, Universidad de La Laguna,
(3) Astrophysics Research Institute, Liverpool John Moores University,
(4) Instituto Galego de Física de Altas Enerxías, Universidade de Santiago de Compostela
(5) Canadian Institute for Theoretical Astrophysics (CITA), University of Toronto
(6) Department of Physics & Astronomy, McMaster University
PP 026099
The first dusty galaxies across 6≲z≲14: Blue monsters, red monsters, and the bimodality of dust content in early galaxies
INAOE, IAC, Academia Checa
PP 026098
Superorbital variability in the quiescent black hole X-ray transient A0620-00
(1) IAC, (2) ULL, (3) Harvard & Smithsonian, (4) New York University Abu Dhabi, (5) Instituto Argentino de Radioastronomía, (6) Universidad Nacional de La Plata, (7) Faulkes Telescope Project, (8) The Schools’ Observatory, Liverpool John Moores University
PP 026097
K 1-6 is a photoionised ISM nebula shaped by a fast-moving hot white dwarf in a triple system
(1) IAC, (2) Astronomical Institute of Charles University, Czech Republic, (3) Universidad de La Laguna, Spain, (4) ESO, Germany, (5) Landessternwarte Heidelberg, Germany, (6) University of Texas Rio Grande Valley, USA, (7) Université Paris-Saclay, CEA, CNRS, AIM, France, (8) The University of Hong Kong, (9) Jodrell Bank Centre for Astrophysics, The University of Manchester, (10) Silesian University in Opava, Czech Republic, (11) Astronomical Institute of the Czech Academy of Sciences, (12) Deep Space Imaging Network, United Kingdom
PP 026096
Symbiotic binaries in the Gaia data. II. Symbiotic candidates from general variability classification in DR3
(1) IAC, (2) Astronomical Institute of Charles University, (3) Southern Spectroscopic Project Observatory Team, (4) Nicolaus Copernicus Astronomical Center, Polish Academy of Sciences, Poland, (5) Universidad de La Laguna, Spain
PP 026095
Symbiotic binaries in the Gaia data. I. Known symbiotics in DR3 and FPR
(1) IAC, (2) Astronomical Institute of Charles University
PP 026094
SpecFANN: Spectral Fitting via Artificial Neural Networks I. A deep learning based fastwind emulator and fitting suite
(1) IAC/ULL
PP 026093
How large can galaxies be? Ultra-deep imaging of IC 1101, the most extended known galaxy
(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-38205 La Laguna, Tenerife, Spain
(3) Departamento de Física Teórica, Atómica y Óptica, Universidad de Valladolid, 47011 Valladolid, Spain
(4) Laboratory for Disruptive Interdisciplinary Science (LaDIS), Universidad de Valladolid, 47011 Valladolid, Spain
(5) Instituto de Astrofísica e Ciências do Espaço, Universidade de Lisboa, OAL, Tapada de Ajuda, PT1349-018 Lisbon, Portugal
(6) Institute of Space Sciences (ICE, CSIC), Campus UAB, Carrer de Can Magrans, s/n, 08193 Barcelona, Spain
(7) School of Physics, University of New South Wales (UNSW Sydney), Sydney, NSW 2052, Australia
(8) Centro de Estudios de Física del Cosmos de Aragón (CEFCA), Plaza San Juan 1, E-44001 Teruel, Spain
(9) Departamento de Física, Universidad de Córdoba, Campus de Rabanales, Edificio Albert Einstein, E-14071 Córdoba, Spain
PP 026092
Multiplicity of Massive stars in the Milky Way (M3W). I. Project description, UNWIND, application to GLS 11 448, and DIB catalog
(1) CAB-CSIC, Spain, (2) Univ. La Plata, Argentina, (3) IAC/ULL, Spain
PP 026091
The Stellar Observations Network Group (SONG) -- A Legacy Archive of Stellar Time-Domain Spectroscopy
(1) Stellar Astrophysics Centre (SAC), Denmark, (2) IAC/ULL, Spain
PP 026090
Investigating the electron temperature of [Ar IV] in planetary nebulae using the DESIRED database
(1) IAC, Spain, (2) ULL, Spain, (3) IA-UNAM, Mexico, (4) ICF-UNAM, Mexico, (5) IA-UNAM, Ensenada, Mexico, (6) INAOE, Mexico, (7) NAOC, China, (8) UCAS, China, (9) Xinjiang Astronomical Obs., China, (10) U. Hong Kong, China
PP 026089
HI-bearing dark galaxies predictions from constrained Local Group simulations: how many and where to find them
(1) ULL, (2) IAC, (3) AIP, (4) Universidad de Sevilla, (5) INAF, (6) Universidad Autónoma de Madrid, (7) CIAFF, (8) International Centre for Radio Astronomy Research
PP 026088
GroundBIRD: First On-Sky Responsivity Calibration at the Teide Observatory
(1) IAC, (2) Korea University
PP 026087
Hints of enhanced magnetic activity after the intermediate rotation period gap as traced by the chromospheric Ca ii infrared triplet
(1) Instituto de Astrofísica de Canarias, (2) Universidad de La Laguna, (3) Lowell Observatory, (4) Instituto de Astrofísica e Ciências do Espaço Universidade do Porto, (5) Departamento de Física e Astronomia Universidade do Porto, (6) Université Paris-Saclay, (7) Space Telescope Science Institute
PP 026086
SN 2021lwz: Another exotic, luminous, and fast-evolving optical stripped-envelope supernova?
1 Instituto de Astrofísica de Canarias, Vía Láctea, 38205 La Laguna, Tenerife, Spain
2 Universidad de La Laguna, Departamento de Astrofísica, 38206 La Laguna, Tenerife, Spain
3 The Oskar Klein Centre, Department of Astronomy, Stockholm University, AlbaNova, SE-10691 Stockholm, Sweden
4 Astrophysics Research Institute, Liverpool John Moores University, Liverpool Science Park IC2, 146 Brownlow Hill,
Liverpool L3 5RF, UK
5 Konkoly Observatory, CSFK, Konkoly-Thege M. út 15-17, Budapest 1121, Hungary
6 Department of Optics & Quantum Electronics, University of Szeged, Dóm tér 9, Szeged 6720, Hungary
7 ELTE Evös Loránd University, Gothard Astrophysical Observatory, 9700 Szombathely Szent Imre h. u. 112, Hungary
8 Center for Interdisciplinary Exploration and Research in Astrophysics (CIERA), Northwestern University, 1800 Sherman Ave,
Evanston, IL 60201, USA
9 Graduate Institute of Astronomy, National Central University, 300 Jhongda Road, 32001 Jhongli, Taiwan
10 Finnish Centre for Astronomy with ESO (FINCA), FI-20014 University of Turku, Finland
11 Department of Physics and Astronomy, FI-20014 University of Turku, Finland
12 GRANTECAN, Cuesta de San José s/n, 38712 Breña Baja, La Palma, Spain
13 Geneva Observatory, University of Geneva, Chemin Pegasi 51, CH-1290 Versoix, Switzerland
14 Max-Planck-Institut für extraterrestrische Physik, Giessenbachstr. 1, 85748 Garching, Germany
15 Kavli Institute for Cosmology, University of Cambridge, Madingley Road, CB3 0HA Cambridge, UK
16 Institute of Astronomy, University of Cambridge, Madingley Road, CB3 0HA Cambridge, UK
17 Miller Institute for Basic Research in Science, 206B Stanley Hall, Berkeley, CA 94720, USA
18 Department of Astronomy, University of California, Berkeley, CA 94720-3411, USA
19 Caltech Optical Observatories, California Institute of Technology, Pasadena, CA 91125, USA
20 IPAC, California Institute of Technology, 1200 E. California, Blvd, Pasadena, CA 91125, USA
21 Division of Physics, Mathematics, and Astronomy, California Institute of Technology, Pasadena, CA 91125, USA
22 Cahill Center for Astrophysics, California Institute of Technology, MC 249-17, 1200 E California Boulevard, Pasadena,
CA 91125, USA
PP 026084
Not So Isolated: Green Pea Galaxies in Overdense Environments revealed by VLT/MUSE
(1) INAF–Osservatorio Astronomico di Roma, (2) IAA, (3) Observatorio de Calar Alto, (4) Observatório Nacional/MCTIC, Rio de Janeiro, Brazil, (5) Department of Astronomy, Stockholm University, Sweden, (6) Department of Astrophysics, University of Vienna, (7) IAC, (8) Depart. Astrofisica, ULL
PP 026083
Dense, multi-phase accretion disk atmosphere in the low-luminosity state of black hole transientV4641 Sgr
Oxford Astrophysics (and other international institutions including IAC, ULL)
PP 026082
Solar vortex detection methods in MHD simulations: Impact of magnetic field and spatial resolution
(1) IAC, (2) ULL, (3) Institute of Chemical Kinetics and Combustion, Russia
PP 026081
Resolving SLX 1744-299 and SLX 1744-300 in the hard X-ray band: implications for their ultracompact nature
(1,2) IAC, ULL
PP 026080
Kinematic detection of dusty outflows from AGN: PAH kinematics of type 2 quasars with JWST/MIRI spectroscopy
(1) University of California San Diego, (2) IAC, (3) ULL, (4) IRyA, (5) IFF, (6) CAB
PP 026079
Improving constraints on primordial non-Gaussianity from Quaia with a new cosmological observable: angular redshift fluctuations
(1) Instituto de Astrofísica de Canarias (IAC)
(2) Universidad de La Laguna (ULL)
(3) MTA–CSFK LSS Research Group
(4) Konkoli Observatory
(5) University of Oxford
(6) Institute d'Astrophysique Spatiale (CNRS)
(7) Kavli Institute for Cosmology (Cambridge)
(8) Kavli Institute for Particle Astrophysics and Cosmology (Stanford University)
PP 026078
Clumpy Disk, Interloper, or Merger? Nature of a Distant Galaxy Pair at 5 kpc Projected Separation
(1) University of California Irvine, (2) University of California Riverside,
(3) IPAC, (4) Department of Astronomy, The University of Texas at Austin, (5) Cosmic Frontier Center, The University of Texas at Austin, (6) IAC, (7) ULL,
(8) ESO, (9) Joint ALMA Observatory, (10) Max-Planck-Institut fur Radioastronomie, (11) Australian National University, (12) ARC Centre of Excellence for All Sky Astrophysics in 3 Dimensions (ASTRO 3D), (13) The Observatories of the Carnegie Institution for Science, (14) W. M. Keck Observatory
PP 026077
Blowing star formation away in AGN hosts (BAH) -- V: The Feeding-Feedback Cycle in local AGNs as reveled by their stellar populations
(1) Universidade Federal do Rio Grande do Sul, (2) Universidade Federal de Santa Maria,(3) Johns Hopkins University, (4) IAC, (5) ULL, (6) University of Hertfordshire,
(7) University of North Carolina at Chapel Hill
PP 026076
The Multi-phase Biconical Outflow in the local IR-Luminous Merger IRASF01364-1042
(1) ESO, (2) Joint ALMA Observatory, (3) Max-Planck-Institut für Radioastronomie, (4) IPAC,
(5) University of California Irvine, (6) IAC, (7) ULL, (8) University of Toledo, (9) NRAO, (10) University of Virginia, (11) University of Geneva, (12) Universidad Diego Portales, (13) University of British Columbia, (14) Hiroshima University, (15) Occidental College, (16) Leiden Observatory, (17) Universidad de Tarapacá, (18) European Space Agency, (19) University of Hertfordshire, (20) Steward Observatory, (21) European University Cyprus, (22) Foundation for Research and TechnologyHellas (FORTH), (23) University of Crete, (24) University of Florida,
(25) Australian National University, (26) ARC Centre of Excellence for All Sky Astrophysics in 3 Dimensions (ASTRO 3D), (27) W. M. Keck Observatory, (28) University of Hawaii
PP 026075
GOALS-JWST: resolved multiphase molecular gas in IRAS 20551-4250 using JWST and ALMA
(1) Centre for Astrophysics Research University of Hertfordshire, (2) Space Telescope Science Institute, (3) ESO, (4) Joint ALMA Observatory, (5) IPAC-Caltech,
(6) UCLA, (7) AURA for the European Space Agency, (8) University of Virginia, (9) National Radio Astronomy Observatory, (10) Caltech/IPAC, (11) Department of Physics and Astronomy UCI, (12)IAC, (13) ULL, (14) European Space Agency, (15) Ehime University, (16) Leiden Observatory, (17) School of Sciences European University Cyprus, (18) Foundation for Research and Technology-Hellas(FORTH), (19) University of Crete, (20) Hiroshima Astrophysical Science Center, (21) Steward Observatory, (22) Università di Padova, (23) University of Florida, (24) University of Geneva, (25) Universidad Diego Portales, (26) University of Hawaii, (27) University of Virginia
PP 026074
New Online Database of Symbiotic Variables: Catalog and Statistical Overview of Symbiotic Binaries
(1) IAC, (2) Astronomical Institute of Charles University, (3) P. J. Šafárik University in Košice
PP 026073
GATOS XIV: The first direct kinematic evidence of dusty outflows from AGN via PAH kinematics of local Seyfert galaxies with JWST
(1) University of Oxford, UK; (2) University of California at San Diego, USA; (3) IAC; (4) ULL
PP 026072
A comparative study of O, Ne, Cl, and Ar in HII regions and PNe of the Galactic disk: Temporal evolution of radial gradients?
(1) IA-UNAM, Cd. México, Mexico, (2) IAC, Spain, (3) ULL, Spain
PP 026071
ISOSCELES Project: II. Modelling galactic B-type stars for fast and $δ-$slow wind regimes
(1) Univ. Valparaiso, (2) Universidad Mayor, (3) Univ. La Plata, (4) IAC/ULL
PP 026070
Chromospheric condensation and heating in small-scale flaring events: Insights from GREGOR/GRIS and coordinated IRIS observations
1 INAF – Osservatorio Astrofisico di Catania, Via S. Sofia 78, 95123 Catania, Italy
2 INAF – Osservatorio Astronomico di Roma, Via Frascati 33, 00078 Monte Porzio Catone, Italy
3 INAF – Osservatorio Astronomico di Capodimonte, Salita Moiariello 16, 80131 Napoli, Italy
4 Instituto de Astrofísica de Canarias, Vía Láctea s/n, 38205 La Laguna, Tenerife, Spain
5 Departamento de Astrofísica, Universidad de La Laguna, 38205, La Laguna, Tenerife, Spain
6 INAF - Capodimonte Astronomical Observatory, Salita Moiariello 16, I 80131 Napoli, Italy; now at CMCC Foundation - Euro-
Mediterranean Center on Climate Change, Italy
PP 026069
Accessible does not mean exploitable: HiPERCAM reveals the ultra-fast rotation of 2022 OB5
(1) IAC, (2) ULL, (3) Light Bridges, (4) GRANTECAN
PP 026068
Accurate inner stellar density slopes from projected surface densities in galaxies
(1) IAC, (2) Departamento de Astrofisica, ULL, Spain
PP 026067
Analysis of the Gaia DR3 planetary nebula candidates and the possible symbiotic stars among them
(1) Southern Spectroscopic Project Observatory Team, (2) IAC, (3) Astronomical Institute of Charles University
PP 026066
Kepler Discovery of GW Vir Pulsations of the Central Star of Planetary Nebula Kn 61
(1) IAC, (2) ULL
PP 026065
A high-resolution X-ray view of the ultra-fast outflow in MAXI J1810-222
INAF-Palermo, IAC, ULL and other international institutions
PP 026064
X-ray luminous late-type giants: an overlooked population contributing to the Galactic ridge iron line emission
INAF-Brera, IAC, ULL and other international institutions
PP 026063
The DESIRED electron temperature relations in star-forming regions of the local Universe
(1) IAC, Spain, (2) ULL, Spain, (3) IA-UNAM, Mexico, (4) IfA, U. Edinburgh, UK, (5) IA-UNAM, Ensenada, Mexico, (6) CIEMAT, Spain, (7) INAOE, Mexico, (8) UNAH, Honduras
PP 026062
Photonic integrated circuits for astronomy: A formal description of an integrated photonics-based wavefront sensor (IP-WFS)
(1) IAC, (2) ULL
PP 026061
Accelerating 3D Non-LTE Synthesis with Graph Neural Networks
(1) Institut für Sonnenphysik, (2) Instituto de Astrofísica de Canarias, (3) Departamento de Astrofísica (ULL), (4) Institute of Theoretical Astrophysics (Univ. Oslo), (5) Rosseland Centre for Solar Physics (Univ. Oslo)
PP 026060
Mapping the Milky Way with Gaia Bp/Rp spectra-IV: the broken and asymmetric density profile of the stellar disk traced by a large sample of red clumps
(1) Institute of Astronomy and Physics, Inner Mongolia University, Hohhot, China; (2) National Astronomical Observatories, Chinese Academy of Sciences, Beijing, China; (3) IAC; (4) ULL; (5) School of Astronomy and Space Science, University of Chinese Academy of Sciences, Beijing, China; (6) South-Western Institute For Astronomy Research, Astronomy Building, Yunnan University, Chenggong District, Kunming, China; (7) Key Laboratory of Survey Science of Yunnan Province, Yunnan University, Kunming, Yunnan, China; (8) School of Astronomy and Space Science, Nanjing University, Nanjing, China; (9) Key Laboratory of Modern Astronomy and Astrophysics (Nanjing University), Ministry of Education, Nanjing, China
PP 026059
Accretion disc winds in X-ray binaries
(1,2) IAC, ULL; (3) ESO; (4) Durham University; (5) INAF-Brera; (6) Osaka University.
PP 026058
Jet-driven shocks and turbulence in radio-loud Active Galactic Nuclei observed with JWST MIRI/MRS
(1) CAB, (2) Universidade Federal de Santa Maria, (3) IAC, (4) ULL
PP 026057
CONCERTO: forward modeling of interferograms for calibration
(1) LAM, (2) IPAG, (3) IAC, (4) IAC, (5) LPSC, (6) Institut Néel, (7) Cardiff Uni., (8) Univ. Diego Portales, (9) ESO, (10) Univ. Valparaiso
PP 026056
The IACOB project XVII. Nitrogen abundances in Galactic O-type stars: further hints for separating binary-interaction products from effectively single stars
(1) IAC, (2) Departamento de Astrofísica, ULL, (3)
LUPM, Université de Montpellier, (4) LMU Munich, Universitätssternwarte
PP 026055
The IACOB project: XVI. Surface helium abundances in Galactic O-type stars: indications for identifying binary interaction products
(1) IAC/ULL, (2) ESO/Chile, (3) Univ. Bonn, (4) Univ. Innsbruck, (5) Univ. La Plata, (6) USM, Munich, (7) CAB, (8) ICCUB, Univ. Barcelona
PP 026054
Decoupling the AGN outflow and star-forming disk kinematics in the nuclear region of NGC 7582 with JWST NIRSpec and MIRI/MRS
(1) University of Oxford, (2) IAC, (3) ULL
PP 026053
The impact of supermassive black holes on exoplanet habitability: I. Spanning the natural mass range
(1) Florida Institute of Technology, USA; (2) Tor Vergata University of Rome, Italy; (3) INAF, Italy; (4) INFN, Italy; (5) IAC, Spain; (6) ULL, Spain
PP 026052
Ancient 'ghost' planetary nebulae discovered with amateur telescopes
(1) AstroHenares, (2) IAC, (3) ULL, (4) OAN, (5) Heidelberg
PP 026050
Forecasting Synchrotron Spectral Parameters with QUIJOTE-MFI2 in combination with Planck and WMAP
(1) Instituto de Astrofísica de Canarias (2) Universidad de La Laguna, Dpto. Astrofísica
PP 026049
Extended coronal line emission and new clues to a possible dual AGN in the merger J1356+1026
(1) IAC, (2) ULL
PP 026048
The Galaxy Activity, Torus, and outflow Survey (GATOS) XIII: Coupling Driven H2 Excitation in Seyferts
(1) Department of Physics, University of Alaska Fairbanks; (2) University of Alaska Anchorage; (3) UTSA; (4) IAC, (5) ULL
PP 026046
A comparison of pendulum models for large-amplitude longitudinal prominence oscillations
(1) Instituto de Astrofisica de Canarias
(2) Departamento de Astrofísica, Universidad de La Laguna
PP 026044
Two hot pre-white dwarfs inside the red-giant-branch planetary nebula Pa 13 -- Double core evolution or common envelope-induced rejuvenation?
(1) Heidelberg, (2) IAC, (3) ULL
PP 026043
Automatic Detection of CMEs Using Synthetically-Trained Mask R-CNN
(1) Univ. Mendoza, (2) CNICT, (3) NASA Goddard, (4) Physics and Astronomy Dep. George Mason Univ (5) IAC
PP 026042
Chemical study of two starless cores in the B213/L1495 filament
(1) CAB, (2) ESAC, (3) OAN, (4) IGN, (5) IAC, (6) ULL
PP 026041
torchmfbd: A flexible multi-object, multi-frame blind deconvolution code
(1) IAC, (2) ULL, (3) Institute for Solar Physics, Stockholm Univ, (4) Institute of Theoretical Astrophysics, Univ of Oslo, (5) Rosseland Center for Solar Physics
PP 026040
Multi-height probing of horizontal flows in the solar photosphere
(1) Astronomical Observatory, Serbia, (2) Institute for Solar Physics, (3) Department of Astronomy, University of Belgrade, (4) HAO, (5) Univ. Winsconsin, (6) LASP, (7) Univ. Colorado Boulder, (8) NSO, (9) IAC, (10) ULL, (11) Environment and Climate Change Canada
PP 026039
Inference of horizontal velocity fields from the induction equation in the solar atmosphere. I. Analytical and numerical solutions in 2D
(1) Institut für Sonnenphysik, (2) Departamento de Astrofísica ULL, (3) IAC
PP 026038
Long-period magnetic activity in the K dwarf GJ 1137 and a new super-Earth on a 9-day orbit
(1) Sofia University "St Kliment Ohridski",
(2) IAC,
(3) ULL,
(4) Institute of Astronomy and National Astronomical Observatory, Bulgarian Academy of Sciences,
(5) Ss. Cyril and Methodius University in Skopje,
(6) Department of Physics, University of Warwick,
(7) Centre for Exoplanets and Habitability, University of Warwick,
(8) INAF-Osservatorio Astronomico di Roma,
(9) Università di Roma Tor Vergata,
(10) Sapienza Università di Roma,
(11) Consejo Superior de Investigaciones Científicas,
(12) Light Bridges S. L.,
(13) Università di Padova,
(14) Zentrum für Astronomie der Universtät Heidelberg,
PP 026037
Revisiting the Milky Way stellar long bar and the 3 kpc arm
(1) IAC; (2) ULL; (3) Institute of Astronomy and Physics, Inner Mongolia University, Hohhot, China; (4) NAOC-CAS, Beijing, China; (5) Local Universe and Time-Domain Astronomy Laboratory, China West Normal University, Nanchong, China; (6) Luoxiahong Institute of Astronomy, China West Normal University, Nanchong, China; (7) Dep. of Astronomy, China West Normal University, Nanchong, China
PP 026036
Mining the Kepler Field: Atmospheric Parameters, Bolometric Corrections, and Luminosities
(1) Instituto de Astrofísica de Canarias, (2) Universidad de La Laguna, (3) Lowell Observatory, (4) Instituto de Astrofísica e Ciências do Espaço Universidade do Porto, (5) Departamento de Física e Astronomia Universidade do Porto, (6) Université Paris-Saclay
PP 026035
WD 1054-226 revisited: a stable transiting debris system
(1)Observatoire Astronomique de l’Université de Genève; (2) Lund Observatory, Division of Astrophysics; (3)Departamento de Astrofísica, Universidad de La Laguna (ULL); (4) Instituto de Astrofísica de Canarias ; (5)McDonald Observatory
PP 026034
Electron densities and filling factors of extragalactic Hii regions: NGC 2403 and NGC 628
1Departamento de Física Teórica y del Cosmos, Campus de Fuentenueva, Edificio Mecenas, Universidad de Granada, E18071–Granada, Spain
2Instituto Carlos I de Física Teórica y Computacional, Facultad de Ciencias, E18071–Granada, Spain
3Institute for Astronomy, 2680 Woodlawn Drive, Honolulu, HI 96822, USA
4Instituto de Astrofísica de Canarias, E38205–La Laguna, Tenerife, Spain
5Departamento de Astrofísica, Universidad de La Laguna, Tenerife, Spain
PP 026033
Disc growth and vertical heating of lenticular galaxies in the Fornax cluster
(1)Astrophysics Research Institute, Liverpool John Moores University, 146 Brownlow Hill, Liverpool L3 5RF, UK
(2)Instituto de Astrofísica de Canarias, Calle Via Láctea s/n, 38200 La Laguna, Tenerife, Spain
(3)Depto. Astrofísica, Universidad de La Laguna, Calle Astrofísico Francisco Sánchez s/n, 38206 La Laguna, Tenerife, Spain
(4)Leibniz-Institut für Astrophysik Potsdam (AIP), An der Sternwarte 16, D-14482 Potsdam, Germany
PP 026032
The Average Age Map of the Galactic Bulge
(1) National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100101, People’s Republic of China;
(2) School of Astronomy and Space Science, University of Chinese Academy of Sciences, Beijing 100049, People’s Republic of China;
(3) IAC;
(4) ULL;
(5) PIFI-Visiting Scientist 2023 of Chinese Academy of Sciences at Purple Mountain Observatory, Nanjing 210023, and National Astronomical Observatories, Beijing 100012, People’s Republic of China;
(6) Institute for Frontiers in Astronomy and Astrophysics, Beijing Normal University, Beijing 100875, People’s Republic of China;
(7) Zhejiang Lab, Hangzhou 311121, People’s Republic of China;
(8) Local Universe and Time-Domain Astronomy Laboratory, China West Normal University, Nanchong 637002, People’s Republic of China;
(9) Luoxiahong Institute of Astronomy, China West Normal University, Nanchong 637002, People’s Republic of China;
(10) Department of Astronomy, China West Normal University, Nanchong 637002, People’s Republic of China;
(11) Shanghai Key Laboratory for Astrophysics, Shanghai Normal University, 100 Guilin Road, Shanghai 200234, People’s Republic of China
PP 026031
Optimization procedure of the baffle of the GroundBIRD Telescope to mitigate stray light
(1) Tohoku University, (2) IAC, (3) ULL, (4) Tsukuba University, (5) Korea University, (6) Kyoto University, (7) RIKEN, (8) Imperial College London
PP 026030
New Robotic Telescope: The big eye to observe the transient Universe
(1) IAC, (2) ULL, (3) Liverpool John Moores University (UK), (4) ICTEA, (5,6,7) Universidad de Oviedo
PP 026029
The 4 meter New Robotic Telescope project: an updated report
(1) IAC, (2) ULL, (3) Liverpool John Moores (UK), (4) ICTEA, (5) Yunnan Astronomical Observatories (China), (6) NAOC (China), (7) CSIC, (8) Shanghai Astronomical Observatory (China), (9) Purple Mountain Observatory (China), (10) Key Laboratory of Space Astronomy and Technology (China), (11) NIAOT (China)
PP 026028
The Nuclear Star Cluster of M 74: a fossil record of the very early stages of a star-forming galaxy
1 Instituto de Astrofísica de Canarias, calle Vía Láctea s/n, E-38205 La Laguna, Tenerife, Spain
2 Departamento de Astrofísica, Universidad de La Laguna, Avenida Astrofísico Francisco Sánchez s/n, E-38206 La Laguna, Spain
3 Max-Planck-Institut für Astronomie, Königstuhl 17, D-69117, Heidelberg, Germany
4 Université Côte d’Azur, Observatoire de la Côte d’Azur, CNRS, Laboratoire Lagrange, 06000, Nice, France
5 Department of Physics and Astronomy, University of Wyoming, Laramie, WY 82071, USA
6 Research School of Astronomy and Astrophysics, Australian National University, Mt Stromlo Observatory, Weston Creek, ACT
2611, Australia
7 Universität Heidelberg, Zentrum für Astronomie, Institut für Theoretische Astrophysik, Albert-Ueberle-Str 2, D-69120 Heidel-
berg, Germany
8 Universität Heidelberg, Interdisziplinäres Zentrum für Wissenschaftliches Rechnen, Im Neuenheimer Feld 205, D-69120 Heidel-
berg, Germany
9 Observatorio Astronómico Nacional (IGN), C/Alfonso XII, 3, E-28014 Madrid, Spain
10 UK ALMA Regional Centre Node, Jodrell Bank Centre for Astrophysics, Department of Physics and Astronomy, The University
of Manchester, Oxford Road, Manchester M13 9PL, UK
11 Astronomy Department, The Ohio State University, Columbus, Ohio, USA
12 Center for Cosmology and Astro-Particle Physics, The Ohio State University, Columbus, Ohio, USA
PP 026027
GroundBIRD Telescope: Systematics Modelization of MKID Arrays Response
(1) Korea University, (2) IAC, (3) ULL, (4) Tohoku University, (5) University of Tsukuba, (6) RIKEN, (7) Graduate School of Science, Yoshidahonmachi, (8) SRON
PP 026026
QUIJOTE-TFGI polarization calibration - Ground characterization and on-sky validation with Tau A and the Moon
(1) IAC (2) ULL (3) IFCA (4) WPI
PP 026024
A dedicated survey of fast-rotating near-Earth asteroids with the Two-meter Twin Telescope. I. Observational strategy and first results
(1) IAC, (2) ULL, (3) Light Bridges
PP 026023
The dependence of triggering mechanisms on radio AGN sub-types: the role of galaxy mergers
(1) University of Sheffield, UK; (2) IAC; (3) ULL
PP 026022
Ubiquitous yet forgotten: Broad absorptions in the optical spectra of low-mass X-ray binaries
(1) IAC, (2) ULL
PP 026021
Self-Consistent Direct Method for Chemical Abundances in High-z Galaxies with JWST
(1) Univeristy of Edinburgh, (2) IA-UNAM, (3) IAC, (4) Universtität Heidelberg, (5) INAOE
PP 026020
Signatures of Damping Nonlinear Oscillations by KHI-induced Turbulence in Synthetic Observations
(1) Centre for mathematical Plasma Astrophysics, Department of Mathematics, KU Leuven, Leuven, BE-3001, Belgium
(2) Department of Mathematics and Statistics, University of Exeter, Exeter, EX4 4QF, UK
(3) Instituto de Astrofísica de Canarias, Vía Láctea S/N, E-38205 Laguna, Tenerife, Spain
(4) Departmento de Astrofísica, Universidad de La Laguna, E-38206 Laguna, Tenerife, Spain
PP 026019
JWST spectra are consistent with the edge-on star-forming galaxy scenario for the "runaway supermassive black hole"
(1) IAC, (2) Departamento de Astrofisica, ULL, (3) Instituto de Astronomia, Universidad Nacional Autonoma de M exico, Ensenada, Mexico, (5) Institute of Space Sciences (ICE, CSIC), Campus UAB, Barcelona, Spain
PP 026018
X-Shooting ULLYSES: massive stars at low metallicity: XII. The clumped winds of O-type (super)giants in the Large Magellanic Cloud
(1) Anton Pannekoek Institute for Astronomy, University of Amsterdam, (2) IAC/ULL
PP 026017
The lack of fast rotators in Cyg OB2. I. Insights from spectral reclassification of its B0 population
IAC/ULL
PP 026016
The Gaia-ESO Survey: Projected Rotational Velocities of B stars in the Carina Nebula
(1) Observatório Nacional (ON)-MCTI (2) ULL/IAC
PP 026015
QSOFEED: Investigating warm molecular, low- and high-ionization atomic gas in six type-2 quasars with GTC/EMIR
(1) IAC; (2) ULL; (3) Università degli Studi di Torino; (4) INAF - Osservatorio Astrofisico di Torino; (5) ESO Chile
PP 026014
Lord of LRDs: Insights into a "Little Red Dot" with a low-ionization spectrum at z = 0.1
(1) Kavli Institute for Cosmology, University of Cambridge; (2) Cavendish Laboratory, University of Cambridge; (3) University of Hertfordshire; (4) Institute of Astronomy, University of Cambridge; (5) UCL; (6) IAC; (7) ULL
PP 026013
Search for Faint Lone Double-Peaked Ha Lines as IMBH Signatures in the MUSE Deep Field
(1) IAC, (2) Departamento de Astrofísica, ULL, (3) INAF-Osservatorio Astronomico di Capodimonte, Via Moiariello 16, 80131 Napoli, Italy
PP 026011
Appraising the Necklace: A post-common-envelope carbon dwarf inside an apparently carbon-poor planetary nebula
IAC, ULL
PP 026010
Dynamical mass of a solar-like oscillator at the main-sequence turnoff from Gaia astrometry & ground-based spectroscopy
(IAC/ULL)
PP 026008
The DESIRED temperature-metallicity relations in star-forming regions: probing the Galactic radial and azimuthal metallicity distributions
(1) UNAH, Honduras, (2) IA-UNAM, Mexico, (3) IAC, Spain, (4) ULL, Spain
PP 026007
WEAVE imaging spectroscopy of NGC 6720: an iron bar in the Ring
(1) U. Cardiff, UK, (2) University College London, UK, (3) IAC, Spain, (4) ULL, Spain, (5) CAB, Spain
PP 026006
Polarization echoes from past nuclear activity in the quasi-periodic eruption source GSN 069
(1) FORTH, Greece, (2) IAA, (3) Université de Liège, (4) CAB, (5) Université de Strasbourg, (6) IAC, (7) ULL
PP 026005
Evidence of Feedback Effects in Low-luminosity Active Galactic Nuclei Revealed by JWST Spectroscopy
(1) UTSA, (2) IAC, (3) ULL
PP 026004
Evidence of the amino acids Tyrosine and Phenylalanine in the interstellar material of IC348 in Perseus
1 Instituto de Astrofísica de Canarias, Via Lactea s/n, 38200 La Laguna, Tenerife, Spain
2 Universidad Politécnica de Cartagena C/ Campus Muralla del Mar, E-30202 Cartagena, Murcia, Spain
PP 026003
GATOS XI: Excess dust heating in the Narrow Line Regions of nearby AGN revealed with JWST/MIRI
(1) University of Newcastle, (2) IAC, (3) ULL
PP 026002
Early Mosques in Al-Andalus: two singular examples of eighth-century CE Muslim architecture on the margins of the Islamic world
(1) Universitat Autònoma de Barcelona, (2) Universitat d'Alacant, (3) Diputació de Castelló, (4) Instituto de Historia, CSIC, (5) ULL-IAC
PP 026001
Inferring physical parameters of solar filaments from simultaneous longitudinal and transverse oscillations
(1) Aryabhatta Research Institute of Observational Sciences, India
(2) Department of Applied Physics, Mahatma Jyotiba Phule Rohilkhand University, India
(3) Instituto de Astrofísica de Canarias, Spain
(4) Departamento de Astrofísica, Universidad de La Laguna, Spain