Preprints in 2024
PP 024124
Milky Way dark matter distribution or MOND test from vertical stellar kinematics with Gaia DR3
(1) IAC; (2) ULL
PP 024123
Orbit determination of visual binary systems observed with CST telescope in 2010-2013
(1) Federación Extremeña de Astronomía, C/José Ruíz Azorín, 14, 4º D, Mérida 06800, Spain
(2) IAC, DA-ULL
(3) Grupo de Observadores Astronómicos de Tenerife (GOAT), Spain
(4) Astronomical Observatory MPC J-48, C/San Pancracio, no 26, Urb. Mackay, La Laguna (Tenerife) E-38205, Spain
(5) Agupación Astronómica de Tenerife, PO box 10644, E-38080, Tenerife, Spain
(6) Sociedad para el Estudio y el Conocimiento de la Astronomía (SECAT), Tenerife, Spain
PP 024122
A wiggling filamentary jet at the origin of the blazar multi-wavelength behaviour
(1) INAF OATO, Italy; (2) IAC; (3) ULL Dpto Astrofisica
PP 024121
Multiwavelength picture of the misaligned BL Lac object 3C 371
(1) Instituto Astrofísica Andalucia, Spain; (2) Istituto Nazionale di Fisica Nucleare, Sezione di Padova, Italy; (3) INAF-Osservatorio Astrofisico di Torino, Italy; (4) Deparment of Astronomy, Univ. Geneva (Swtzerland); (5) IAC; (6) ULL, Dpto Astrofisica (Spain)
PP 024120
The Baryonic Mass Estimates of the Milky Way Halo in the form of High Velocity Clouds
(1) Department of Physics, School of Natural Sciences (SNS), National University of Sciences and Technology (NUST), Islamabad, Pakistan; (2) IAC; (3) ULL; (4) Department of Mathematics and Physics “Ennio De Giorgi”, University of Salento, Lecce, Italy; (5) INFN and INAF, Sezione di Lecce, Lecce, Italy
PP 024118
New constraints on the central mass contents of Omega Centauri from combined stellar kinematics and pulsar timing
Instituto de Astrofísica de Canarias, Universidad de La Laguna, Laboratoire d'Annecy-le-Vieux de Physique Théorique, University of Surrey
PP 024117
Unequivocal detection of the tidal deformation of a red giant in a binary system via interferometry
(1) ESO-Garching, (2) Astronomical Institute of Charles University, (3) IAC
PP 024116
Molecular gas stratification and disturbed kinematics in the Seyfert galaxy MCG-05-23-16 revealed by JWST and ALMA
(1) IAC; (2) ULL
PP 024114
CHEX-MATE: Dynamical masses for a sample of 101 Planck Sunyaev-Zeldovich selected galaxy clusters
(1) Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Italy
(2) INFN, Sezione di Bologna, Italy
(3) Université Côte d’Azur, Observatoire de la Côte d’Azur, CNRS, Laboratoire Lagrange, Bd de l’Observatoire, Nice Cedex, France
(4) IAC
(5) Dpto. de Astrofísica, Univ. de La Laguna, Tenerife, Spain
PP 024113
Identifying new high-confidence polluted white dwarf candidates using Gaia XP spectra and Self-Organizing Maps
(1)Universidade da Coruña (2)IAC
PP 024112
Constraining the overcontact phase in massive binary evolution -- III. Period stability of known B+B and O+B overcontact systems
(1)ESO-Chile, (2) Ku Leuven, (3)IAC, (4) ULL, (5)Royal Observatory of Belgium
PP 024111
Gas flows in the central region of the Seyfert galaxy NGC 4593 with MUSE
(1) University of Nairobi, (2) IAC, (3) ULL, (4) University of South Africa, (5) CSIC
PP 024110
KISS: instrument description and performance
1Laboratoire de Physique Subatomique et de Cosmologie, Universit´e Grenoble Alpes, CNRS/IN2P3, 53, avenue des Martyrs, Grenoble,
France
2Instituto de Astrof´ısica de Canarias, C/V´ıa L´actea s/n, E-38205 La Laguna, Tenerife, Spain
3Departamento de Astrof´ısica, Universidad de La Laguna, E-38206 La Laguna, Tenerife, Spain
4Institut N´eel, CNRS and Universit´e Grenoble Alpes, France
5Aix Marseille Universit´e, CNRS, LAM (Laboratoire d’Astrophysique de Marseille) UMR 7326, 13388, Marseille, France
6Dipartimento di Fisica, Sapienza Universit`a di Roma, Piazzale Aldo Moro 5, I-00185 Roma, Italy
7Centro de Astrobiolog´ıa (CSIC-INTA), Torrej´on de Ardoz, 28850 Madrid, Spain
8Imperial College London, Blackett Lab, Prince Consort Road, London SW7 2AZ, UK
9Astronomy Instrumentation Group, University of Cardiff, UK
10Univ. Grenoble Alpes, CNRS, IPAG, F-38000 Grenoble, France
11Consejo Superior de Investigaciones Cient´ıficas, E-28006 Madrid, Spain
PP 024109
Accretion properties of X-ray AGN: Evidence for radiation-regulated obscuration with redshift-dependent host galaxy contribution
(1) Durham University, (2) National Observatory of Athens, (3) IAC, (4) ULL
PP 024108
Scrutinising evidence for the triggering of Active Galactic Nuclei in the outskirts of massive galaxy clusters at z~1
(1) National Observatory of Athens, (2) University of Southampton, (3) IAC, (4) ULL
PP 024107
Observational constraints on the stellar recycled gas in active galactic nuclei feeding
(1) Universidade Federal do Rio Grande do Sul, (2) Shanghai Astronomical Observatory, (3) IAC, (4) ULL, (5) MPE, (6) Newcastle University.
PP 024105
A sub-Earth-mass planet orbiting Barnard's star: No evidence of transits in TESS photometry
(1) Instituto de Astrofísica de Canarias, 38205 La Laguna, Spain
(2) Departamento de Astrofísica, Universidad de La Laguna, 38206 La La-
guna, Spain
(3) Light Bridges S. L., 35004 Las Palmas de Gran Canaria, Spain
(4) Consejo Superior de Investigaciones Científicas (CSIC), 28006
Madrid, Spain
(5) INAF - Osservatorio Astrofisico di Torino, Via Osservatorio 20, 10025
Pino Torinese, Italy
(6) Centro de Astrobiología (CAB), CSIC-INTA, ESAC campus, Camino
Bajo del Castillo s/n, 28692 Villanueva de la Cañada, Spain
(7) Instituto de Astrofísica e Ciências do Espaço, CAUP, Universidade do
Porto, Rua das Estrelas, 4150-762 Porto, Portugal
(8) Departamento de Física e Astronomia, Faculdade de Ciências, Univer-
sidade do Porto, Rua do Campo Alegre, 4169-007 Porto, Portugal
(9) Instituto de Astrofísica e Ciências do Espaço, Faculdade de Ciências
da Universidade de Lisboa, Campo Grande, 1749-016 Lisboa, Portugal
(10) Centro de Astrofísica da Universidade do Porto, Rua das Estrelas,
4150-762 Porto, Portugal
PP 024104
A sub-Earth-mass planet orbiting Barnard's star
(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) Consejo Superior de Investigaciones Científicas, Spain
(4) Observatoire de Genève, Département d’Astronomie, Université de
Genève, Chemin Pegasi 51b, 1290 Versoix, Switzerland
(5) Instituto de Astrofísica e Ciências do Espac̃o, CAUP, Universidade
do Porto, Rua das Estrelas, 4150-762, Porto, Portugal
(6) Departamento de Física e Astronomia, Faculdade de Ciências, Uni-
versidade do Porto, Rua do Campo Alegre, 4169-007, Porto, Portu-
gal
(7) Centro de Astrofísica da Universidade do Porto, Rua das Estrelas,
4150-762 Porto, Portugal
(8) Centro de Astrobiología (CAB), CSIC-INTA, ESAC campus,
Camino Bajo del Castillo s/n, E-28692, Villanueva de la Cañada
(Madrid), Spain
(9) INAF - Osservatorio Astronomico di Trieste, via G. B. Tiepolo 11,
I-34143, Trieste, Italy
(10) IFPU–Institute for Fundamental Physics of the Universe, via Beirut
2, I-34151 Trieste, Italy
(11) INAF - Osservatorio Astrofisico di Torino, Strada Osservatorio 20,
I-10025, Pino Torinese (TO), Italy
(12) ESO - European Southern Observatory, Av. Alonso de Cordova
3107, Vitacura, Santiago, Chile
(13) Département de Physique, Institut Trottier de Recherche sur les
Exoplanètes, Université de Montréal, Montréal, Québec, H3T 1J4,
Canada
(14) INAF - Osservatorio Astronomico di Palermo, Piazza del Parla-
mento 1, I-90134 Palermo, Italy
(15) Instituto de Astrofísica e Ciências do EspaÇo, Faculdade de Ciên-
cias da Universidade de Lisboa, Campo Grande, 1749-016, Lisboa,
Portugal
(16) Light Bridges S. L., Avda. Alcalde Ramírez Bethencourt, 17, E-
35004, Las Palmas de Gran Canaria, Canarias, Spain
(17) Departamento de Física de la Tierra y Astrofísica & IPARCOS-
UCM (Instituto de Física de Partículas y del Cosmos de la UCM),
Facultad de Ciencias Físicas, Universidad Complutense de Madrid,
E-28040 Madrid, Spain
(18) Center for Space and Habitability, University of Bern,
Gesellschaftsstrasse 6, 3012 Bern, Switzerland
(19) Weltraumforschung und Planetologie, Physikalisches Institut, Uni-
versity of Bern, Gesellschaftsstrasse 6, 3012 Bern, Switzerland
(20) Subaru Telescope, National Astronomical Observatory of Japan, 650
N Aohoku Place, Hilo, HI 96720, USA
(21) Hamburger Sternwarte, Gojenbergsweg 112, 21029 Hamburg, Ger-
many
PP 024103
Cloudy modeling suggests a diversity of ionization mechanisms for diffuse extraplanar gas
(1) University of Oulu, (2) University of Hertfordshire, (3) ULL, (4) IAC
PP 024102
CONCERTO at APEX On-sky performance in continuum
Aix Marseille Univ, CNRS, CNES, LAM, Marseille, France
2 Department of Physics and Astronomy, University of the Western Cape, Robert Sobukhwe Road, Bellville, 7535, South Africa
3 Instituto de Astrofísica de Canarias, E-38205 La Laguna, Tenerife, Spain
4 Departamento de Astrofísica, Universidad de La Laguna (ULL), E-38206 La Laguna, Tenerife, Spain
5 Astronomy Instrumentation Group, University of Cardiff, The Parade, CF24 3AA, United Kingdom
6 Instituto de Estudios Astrofísicos, Facultad de Ingeniería y Ciencias, Universidad Diego Portales, Av. Ejército 441, Santiago, Chile
7 Univ. Grenoble Alpes, CNRS, Grenoble INP, Institut Néel, 38000 Grenoble, France
8 Université de Strasbourg, CNRS, Observatoire astronomique de Strasbourg, UMR 7550, 67000 Strasbourg, France
9 Univ. Grenoble Alpes, CNRS, Grenoble INP, LPSC-IN2P3, 53, avenue des Martyrs, 38000 Grenoble, France
10 European Southern Observatory, Karl Schwarzschild Straße 2, 85748 Garching, Germany
11 Univ. Grenoble Alpes, CNRS, IPAG, 38400 Saint Martin d’Héres, France
12 Instituto de Radioastronomía Milimétrica (IRAM), Granada, Spain
13 LESIA, Observatoire de Paris, PSL Research University, CNRS, Sorbonne Universit´e, UPMC Univ. Paris 06, Univ. Paris Diderot,
Sorbonne Paris Cit´e, 5 place Jules Janssen, 92195 Meudon, France
14 Instituto de Física y Astronomía, Universidad de Valparaíıso, Avda. Gran Bretaña 1111, Valparaíso, Chile
PP 024101
The Galaxy Activity, Torus, and Outflow Survey (GATOS). (VI): Polycyclic Aromatic Hydrocarbon Emission in the Central Regions of Three Seyferts
(1) UTSA, (2) IAC, (3) ULL
PP 024100
The Galaxy Activity, Torus, and Outflow Survey (GATOS). V: Unveiling PAH survival and resilience in the circumnuclear regions of AGN with JWST
(1) CAB/INTA, (2) IAC, (3) ULL
PP 024099
The Galaxy Activity, Torus, and Outflow Survey (GATOS). (IV): Exploring Ionized Gas Outflows in Central Kiloparsec Regions of GATOS Seyferts
(1) UTSA, (2) IAC, (3) ULL
PP 024098
Unveiling the shape: a multi-wavelength analysis of the galaxy clusters Abell 76 and Abell 1307
(1) IAC
(2) DA, ULL
(3) Dipartamento di Fisica, Milano Bicocca University, I20-126 Milano, Italy
(4) Max-Planck-Institut für Physik, Boltzmannstr. 8, D-85748, Garching, Germany
(5) Universitäts-Sternwarte München, Fakultät für Physik, Ludwig-Maximilian-Universität München, Scheinerstr. 1, D-81679
München, Germany
(6) Max-Planck-Institut für extraterrestrische Physik, Gießenbachstraße 1, D-85748 Garching, Germany
PP 024097
The mass of the white dwarf in YY Dra (=DO Dra): Dynamical measurement and comparative study with X-ray estimates
ULL/IAC
PP 024096
Black hole X-ray binary A0620$\unicode{x2013}$00 in quiescence: hints of Faraday rotation of near-infrared and optical polarization?
(1) University of Turku, (5) IAC/ULL
PP 024095
Rapid Mid-Infrared Spectral-Timing with JWST. I. The prototypical black hole X-ray Binary GRS 1915+105 during a MIR-bright and X-ray-obscured state
(1) Univ. Southampton, (39( IAC
PP 024094
Dust beyond the torus: Revealing the mid-infrared heart of local Seyfert ESO 428-G14 with JWST/MIRI
(1) University of Newcastle, (2) IAC, (3) ULL
PP 024093
Deciphering the imprint of AGN feedback in Seyfert galaxies: Nuclear-scale molecular gas deficits
(1) OAN, (2) IAC, (3) ULL
PP 024092
A study of interacting galaxies from the Arp-Madore Catalogue: Triggering of star formation and nuclear activity
(1) IAC, (2) ULL, (3) Universidade Federal do Rio Grande do Sul, (4) Instituto de Astronomia, Geofísica e Ciências Atmosféricas da USP, (5) Universidade Federal de Santa Maria
PP 024091
Coronal heating
(1) Instituto de Astrofísica de Canarias; (2) Departamento de Astrofísica, Universidad de La Laguna; (3) Center for mathematical Plasma Astrophysics, KU Leuven
PP 024090
Secondary bias through cosmic time II: Reconstructing halo properties using clustering information
Instituto de Astrofísica de Canarias, Universidad T´ecnica Federico Santa María, Chile
PP 024089
HD 110067 c has an aligned orbit: Measuring the Rossiter-McLaughlin effect inside a resonant multi-planet system with ESPRESSO
(1) ESO, (2) IAC, (3) ULL, (4) NOT
PP 024087
Planetary nebulae seen with TESS: New and revisited short-period binary central star candidates from Cycles 1 to 4
(1) OAN, (2) CAB, (3) IAC, (4) ULL, (5) NOT
PP 024086
Recovering chemical bimodalities in observed edge-on stellar disks: insights from AURIGA simulations
(1) IAC, (2) ULL, (3) Max Planck Institute for Astronomy, (4) Liverpool John Moores University, (5) Durham University
PP 024085
High-resolution observations of recurrent jets from an arch filament system
(1) Rosseland Centre for Solar Physics.
(2) Institute of Theoretical Astrophysics.
(3) LIRA, Observatoire de Paris.
(4) Centre for mathematical Plasma Astrophysics.
(5) School of Physics and Astronomy.
(6) Instituto de Astrofísica de Canarias.
(7) Departamento de Astrofísica, ULL.
(8) Sorbonne Université, École Polytechnique.
PP 024084
Constraints on the in situ and ex situ stellar masses in nearby galaxies obtained with artificial intelligence
(1) IAC
(2) University of Vienna
(3) Max Planck Institute
PP 024083
An ALMA CO(1-0) survey of the 2Jy sample: large and massive molecular disks in radio AGN host galaxies
(1) University of Sheffield, (2) ASTRON, (3) Kapteyn Astronomical Institute, (4) IAC, (5) ULL
PP 024082
A biconical ionised gas outflow and evidence for positive feedback in NGC 7172 uncovered by MIRI/JWST
(1) Centro de Astrobiología (CAB), CSIC-INTA; (2) IAC; (3) ULL
PP 024081
QUIJOTE scientific results -- XVIII. New constraints on the polarization of the Anomalous Microwave Emission in bright Galactic regions: ρ Ophiuchi, Perseus and W43
(1) Instituto de Astrofísica de Canarias, E-38200 La Laguna, Tenerife, Spain
(2) Departamento de Astrofísica, Universidad de La Laguna, E-38206 La Laguna, Tenerife, Spain
(3) Imperial College London, Blackett Lab, Prince Consort Road, London SW7 2AZ, UK
(4) Institut d’Astrophysique de Paris, UMR 7095, CNRS & Sorbonne Université, 98 bis boulevard Arago, 75014 Paris, France
(5) Laboratoire de Physique Subatomique et de Cosmologie, Université Grenoble Alpes, CNRS/IN2P3, 53 Avenue des Martyrs, Grenoble, France
(6) Consejo Superior de Investigaciones Científicas, E-28006 Madrid, Spain
(7) Universidad de Cantabria, Departamento de Ingeniería de Comunicaciones, Edificio Ingenieria de Telecomunicación, Plaza de la Ciencia 1, 39005 Santander, Spain
(8) Astrophysics Group, Cavendish Laboratory, University of Cambridge, J J Thomson Avenue, Cambridge CB3 0HE, UK
(9) Kavli Institute for Cosmology, University of Cambridge, Madingley Road, Cambridge CB3 0HA, UK
(10) Instituto de Física de Cantabria (IFCA), CSIC-Univ. de Cantabria, Avda. los Castros, s/n, E-39005 Santander, Spain
(11) Departamento de Física Moderna, Universidad de Cantabria, Avda. de los Castros s/n, 39005 Santander, Spain
(12) CNRS-UCB International Research Laboratory, Centre Pierre Binétruy, IRL2007, CPB-IN2P3, Berkeley, CA 94720, USA
(13) Jodrell Bank Centre for Astrophysics, Alan Turing Building, Department of Physics & Astronomy, School of Natural Sciences, The University of Manchester, Oxford Road, Manchester, M13 9PL, U.K.
(14) Departamento de Física. Facultad de Ciencias. Universidad de Córdoba. Campus de Rabanales, Edif. C2. Planta Baja. E-14071 Córdoba, Spain
(15) Department of Physics, Xi’an Jiaotong-Liverpool University, 111 Ren’ai Road, Suzhou Dushu Lake Science and Education Innovation District, Suzhou Industrial Park, Suzhou 215123, P.R. China
PP 024080
Full abundance study of two newly discovered barium giants
(1)Universidad Diego Portales, (2) IAC, (3) ESO-Chile
PP 024079
Detection of the [C I] λ8727 emission line. Low-ionization structures in NGC 7009
(1) National Observatory of Athens, Greece, (2) U. Itajubá, Brazil, (3) ESO, Germany, (4) Obs. Valongo, Brazil, (5) IAC, Spain, (6) ULL, Spain
PP 024078
Gas-phase Fe/O and Fe/N abundances in star-forming regions. Relations between nucleosynthesis, metallicity and dust
(1) U. Heidelberg, (2) IAC, (3) IA-UNAM, (4) U. Bolonia, (5) Max Planck Institute for Astrophysics, Garching, (6) U. Gante, (7) U. Granada,
PP 024077
Unveiling the chemical fingerprint of phosphorus-rich stars II. Heavy-element abundances from UVES/VLT spectra
(1) IAC, (2) ULL, (3) Konkoly Observatory, (4) CSFK, MTA, (5) University of Hull, (6) Joint Institute for Nuclear Astrophysics, (7) The NuGrid Collaboration, (8) ELTE Eötvös Loránd University, (9) Monash University
PP 024076
A Microwave Blackbody Target for Cosmic Microwave Background Spectral Measurements in the 10-20GHz range
IAC, ULL
PP 024074
Rotational synchronisation of B-type binaries in 30 Doradus
(1) IAC, (2) ULL, (3) QUB Belfast, (4) Max-Planck-Institut für Astronomie, (5) Argelander-Institut für Astronomie der Universität Bonn, (6) STScI, (7) KU Leuen, (8) UKATC Edinburgh
PP 024073
Boron depletion in Galactic early B-type stars reveals two different main sequence star populations
(1) Argelander Institut für Astronomie, Bonn, (2) Max-Planck-Institut für Radioastronomie, Bonn, (3) IAC, (4) ULL, (5) STScI
PP 024072
Expanded Sample of Small Magellanic Cloud Ultraviolet Dust Extinction Curves: Correlations between the 2175 Å Bump, q_PAH, Ultraviolet Extinction Shape, and N(H I)/A(V)
(1) STScI, (2) Sterrenkundig Observatorium, Gent, (3) Department of Astronomy & Astrophysics, Villanova University, (4) Space Science Institute, (5) Department of Physics & Astronomy, Johns Hopkins University, (6) Department of Physics & Astronomy, Louisiana State University, (7) IAC, (8) ULL, (9) Steward Observatory, University of Arizon, (10) Department of Astronomy & Astrophysics, University of California, San Diego
PP 024071
Binarity at LOw Metallicity (BLOeM): I. A spectroscopic VLT monitoring survey of massive stars in the SMC
(1) Tel Aviv Univ, (2) ESO-Garching, (3) KU Leuven, (4) Univ of Sheffield ,(5) IAC ,(6) ULL
PP 024070
The PARSEC view of star formation in galaxy centres: from protoclusters to star clusters in an early-type galaxy
1 IAC, USM-Munich; 2 CIDA-Venezuela; 3 UMAM-Mexico; 4 CEFCA-Teruel; 5 USM-Munich, MPE-Garching
PP 024069
The stellar distribution in ultra-faint dwarf galaxies suggests deviations from the collision-less cold dark matter paradigm
(1) IAC, (2) Departamento de Astrofisica, ULL, (3) CeBio y Departamento de Ciencias Basicas, UNNOBA, CONICET, Junin, Argentina
PP 024068
MUSE spectroscopy of the high abundance discrepancy planetary nebula NGC 6153
(1) IAC, (2) ULL, (3) IA-UNAM, Mexico, (4) ICF-UNAM, Mexico, (5) U. Itajubá, Brazil, (6) U. Cardiff, UK, (7) ESO, Germany, (8) GTC
PP 024067
Application of the Eddington inversion method to constrain the dark matter halo of galaxies using only observed surface brightness profiles
(1) IAC, (2) ULL, (3)CeBio y Departamento de Ciencias Basicas, UNNOBA, CONICET, Junin, Argentina
PP 024066
Blue supergiants as a progenitor of intermediate-luminosity red transients
(1) National Astronomical Observatory of Japan
(2) Graduate Institute for Advanced Studies, SOKENDAI
(3) Monash University, Clayton, VIC 3800, Australia
(4) Instituto de Astrofisica de Canarias
(5) Universidad de La Laguna
PP 024065
LeMMINGs. Multi-wavelength constraints on the co-existence of nuclear star clusters and AGN in nucleated galaxies
ERAU, UCM, IAC, ULL, etc
PP 024063
The IACOB project XII. A new grid of northern standards for the spectral classification of B-type stars
Universidad de Alicante, IAC/ULL, NOT
PP 024062
PHANGS-HST catalogs for ∼ 100,000 star clusters and compact associations in 38 galaxies: I. Observed properties
(1) Steward Observatory, University of Arizona, (2) Space Telescope Science Institute, (3) Gemini Observatory/NSF’s NOIRLab, (4) Department of Physics and Astronomy, The Johns Hopkins University, (5) Institute of Astronomy, University of Cambridge, (6) Kavli Institute for Cosmology Cambridge, (7) Universit\'e C\ˆote d’Azur, Observatoire de la C\ˆote d’Azur, (8) University of Toledo, (9) Department of Physics and Astronomy, University of Wyoming, (10) Instituto de Astronom\'ıa, Universidad Nacional Aut\'onoma de M\'exico, (11) Department of Astronomy and Astrophysics, University of California, (12) Max-Planck-Institut f\¨ur Astronomie, (13) AURA for the European Space Agency (ESA), Space Telescope Science Institute, (14) Department of Astronomy, The Ohio State University,
(15) Department of Physics, University of Alberta, (16) European Southern Observatory, (17) Univ Lyon, (18) Research School of Astronomy and Astrophysics, Australian National University, (19) ARC Centre of Excellence for All Sky Astrophysics in 3 Dimensions (ASTRO 3D), (20) International Centre for Radio Astronomy Research, University of Western Australia, (21) University of Virginia Astronomy Department, (22) National Radio Astronomy Observatory, (23) Universit\¨at Heidelberg, Zentrum f\¨ur Astronomie, (24) Universit\¨at Heidelberg, Interdisziplin\¨ares Zentrum f\¨ur Wissenschaftliches Rechnen,
(25) Astronomisches Rechen-Institut, Zentrum f¨ur Astronomie der Universit¨at Heidelberg, (26) Instituto de Astrof\'ısica de Canarias, (27) Departamento de Astrof\'ısica, Universidad de La Laguna, (28) Instituto de Astrof\'ısica de La Plata, CONICET–UNLP, (29) Astronomy Department and Van Vleck Observatory, Wesleyan University, (30) Sub-department of Astrophysics, Department of Physics, University of Oxford.
PP 024061
Deriving the star formation histories of galaxies from spectra with simulation-based inference
1 Instituto de Astrofísica de Canarias, C/ Vía Láctea s/n, 38205 La Laguna, Tenerife, Spain
2 Departamento de Astrofísica, Universidad de La Laguna, 38200 La Laguna, Tenerife, Spain
3 Observatoire de Paris, LERMA, PSL University, 61 avenue de l’Observatoire, F-75014 Paris, France
4 Université Paris-Cité, 5 Rue Thomas Mann, 75014 Paris, France
5 Department of Physics, Faculty of Engineering and Physical Sciences, University of Surrey, GU2 7XH, Guildford, United Kingdom
PP 024060
Fast X-ray/IR observations of the black hole transient Swift~J1753.5--0127: from an IR lead to a very long jet lag
INAF - IASF Palermo, IAC, INAF, Turku, New York University Abu Dhabi, Nordita, Texas Tech University, University of Amsterdam, Università degli Studi di Roma, University of Oxford, Durham University, Università degli Studi di Cagliari, Southampton, Wheaton College, IRAP
PP 024059
Galaxies Ages with Redshift z=2 to 4: Stellar Population Synthesis for Candidates in FourStar Galaxy Evolution Survey
(1) Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing 210023, China; (2) School of Astronomy and Space Sciences, University of Science and Technology of China, Hefei 230026, China; (3) IAC; (4) PIFI-Visiting Scientist 2023 of Chinese Academy of Sciences; (5) ULL
PP 024058
GATOS: missing molecular gas in the outflow of NGC5728 revealed by JWST
(1) MPE, (2) IAC, (3) ULL
PP 024057
CONCERTO: Instrument model of Fourier transform spectroscopy, white-noise components
Aix Marseille Univ., CNRS, CNES, LAM, Marseille, France
Instituto de Astrofísica de Canarias, Santa Cruz de Tenerife, E-38205 La Laguna, Spain
Departamento de Astrofísica, Universidad de La Laguna (ULL), E-38206 La Laguna, Tenerife, Spain
Astronomy Instrumentation Group, University of Cardiff, The Parade, CF24 3AA, United Kingdom
Núcleo de Astronomía, Facultad de Ingeniería y Ciencias, Universidad Diego Portales, Av. Ejército 441, Santiago, Chile
Univ. Grenoble Alpes, CNRS, Grenoble INP, Institut Néel, 38000 Grenoble, France
Univ. Grenoble Alpes, CNRS, LPSC/IN2P3, 38000 Grenoble, France
European Southern Observatory, Karl Schwarzschild Straße 2, 85748 Garching, Germany
Univ. Grenoble Alpes, CNRS, IPAG, 38000 Grenoble, France
European Southern Observatory, Alonso de Cordova 3107, Vitacura, Santiago, Chile
PP 024056
Einasto gravitational potentials have difficulty to hold spherically symmetric stellar systems with cores
(1) IAC, (2) Departamento de Astrofísica, ULL
PP 024055
The Tully-Fisher relation and the Bosma effect
(1) Cenro Ricerche Enrico Fermi, (2) Universitá di Roma Sapienza, (3) Universitá di Roma, (4) IAC, (5) ULL
PP 024054
Constraining the top-light initial mass function in the extended ultraviolet disk of M83
(1) University of Oulu, (2) University of Hertfordshire, (3) IAC, (4) ULL
PP 024053
A fast neural emulator for interstellar chemistry
(1) IAC, (2) ULL, (3) Université Paris-Saclay, (4) OAN, (5) LAB, (6) CAB
PP 024052
From eruption to post-flare rain: A 2.5D MHD model
Instituto de Astrof\'{i}sica de Canarias, 38205 La Laguna, Tenerife, Spain.
Universidad de La Laguna, 38206 La Laguna, Tenerife, Spain.
Centre for mathematical Plasma-Astrophysics, Celestijnenlaan 200B, 3001 Leuven, KU Leuven, Belgium.
Rosseland Centre for Solar Physics, University of Oslo, Postboks 1029 Blindern, 0315 Oslo, Norway.
Institute of Theoretical Astrophysics, University of Oslo, Postboks 1029 Blindern, 0315 Oslo, Norway.
PP 024051
Deep HST imaging favors the bulgeless edge-on galaxy explanation for the hypothetical stellar wake created by a runaway supermassive black hole
(1) IAC, (2) Departamento de Astrofísica, Universidad de La Laguna
PP 024050
Hidden Gems on a Ring: Infant Massive Clusters and Their Formation Timeline Unveiled by ALMA, HST, and JWST in NGC 3351
(1) Department of Astrophysical Sciences, Princeton University,
(2) Department of Physics and Astronomy, McMaster University,
(3) Canadian Institute for Theoretical Astrophysics (CITA),
(4) Steward Observatory, University of Arizona,
(5) National Radio Astronomy Observatory,
(6) Space Telescope Science Institute,
(7) Instituto de Astrofisica de La Plata, CONICET–UNLP,
(8) Department of Physics, University of Alberta,
(9) Department of Astronomy, The Ohio State University,
(10) Center for Cosmology and Astroparticle Physics (CCAPP),
(11) Max-Planck-Institut f¨ur Astronomie,
(12) Department of Astronomy, University of Maryland,
(13) Department of Physics and Astronomy, University of Kansas,
(14) Department of Physics and Astronomy, University of Wyoming,
(15) AURA for the European Space Agency (ESA), Space Telescope Science Institute,
(16) Department of Physics and Astronomy, The Johns Hopkins University,
(17) Sub-department of Astrophysics, Department of Physics, University of Oxford,
(18) European Southern Observatory,
(19) Argelander-Institut f¨ur Astronomie, Universit¨at Bonn,
(20) Universit¨at Heidelberg, Zentrum f¨ur Astronomie, Institut f¨ur Theoretische Astrophysik,
(21) Cosmic Origins Of Life (COOL) Research DAO,
(22) Research School of Astronomy and Astrophysics, Australian National University,
(23) ARC Centre of Excellence for All Sky Astrophysics in 3 Dimensions (ASTRO 3D),
(24) International Centre for Radio Astronomy Research, University of Western Australia,
(25) Astrophysics Research Institute, Liverpool John Moores University,
(26) University of Virginia,
(27) Observatorio Astron´omico Nacional (IGN),
(28) Universit¨at Heidelberg, Interdisziplin¨ares Zentrum f¨ur Wissenschaftliches Rechnen,
(29) Center for Astrophysics | Harvard & Smithsonian,
(30) Max-Planck-Institut f¨ur extraterrestrische Physik,
(31) Sterrenkundig Observatorium, Universiteit Gent,
(32) Department of Physics and Astronomy, Rutgers, the State University of New Jersey,
(33) Center for Computational Astrophysics, Flatiron Institute,
(34) Instituto de Astrofisica de Canarias,
(35) Departamento de Astrofisica, Universidad de La Laguna,
(36) Department of Physics, University of Surrey,
(37) Institute of Physics, Laboratory for galaxy evolution and spectral modelling, EPFL.
PP 024049
Do spiral arms enhance star formation efficiency?
(1) Observatorio Astronómico Nacional (IGN),
(2) Department of Astronomy, The Ohio State University,
(3) Sterrenkundig Observatorium, Universiteit Gent,
(4) Max-Planck-Institut für Astronomie,
(5) INAF – Osservatorio Astrofisico di Arcetri,
(6) European Southern Observatory,
(7) Univ Lyon, Univ Lyon 1, ENS de Lyon, CNRS, Centre de Recherche
Astrophysique de Lyon UMR5574,
(8) Universität Heidelberg, Zentrum für Astronomie, Institut für The-
oretische Astrophysik,
(9) Universität Heidelberg, Interdisziplinäres Zentrum für Wis-
senschaftliches Rechnen,
(10) Department of Astrophysical Sciences, Princeton University,
(11) Università dell’Insubria,
(12) Department of Physics, University of Surrey,
(13) Sorbonne Université, Observatoire de Paris, Université PSL, CNRS,
LERMA,
(14) Max-Planck-Institut für extraterrestrische Physik,
(15) Cosmic Origins Of Life (COOL) Research DAO, coolresearch.io
(16) Argelander-Institut für Astronomie,
(17) Department of Physics and Astronomy, University of Wyoming,
(18) Research School of Astronomy and Astrophysics, Australian Na-
tional University,
(19) International Centre for Radio Astronomy Research, University of
Western Australia,
(20) Harvard-Smithsonian Center for Astrophysics,
(21) Department of Physics, Tamkang University,
(22) Leibniz-Institut for Astrophysik Potsdam (AIP),
(23) Institut de Radioastronomie Millimétrique (IRAM),
(24) Instituto de Astrofísica de Canarias,
(25) Departamento de Astrofísica, Universidad de La Laguna,
(26) Departamento de Astronomía, Universidad de Chile,
(27) Department of Physics, University of Alberta,
(28) Departamento de Física de la Tierra y Astrofísica, Universidad
Complutense de Madrid,
(29) School of Physics and Astronomy, University of St Andrews,
(30) Space Telescope Science Institute,
(31) Sub-department of Astrophysics, Department of Physics, University
of Oxford,
PP 024048
Age of massive galaxies at redshift 8
(1) IAC; (2) PIFI-Visiting Scientist 2023 of Chinese Academy of Sciences; (3) ULL; (4) Department of Physics, The Applied Math Program, and Department of Astronomy, The University of Arizona, AZ 85721, USA; (5) John Woodruff Simpson Fellow; (6) Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing 210023, China; (7) School of Astronomy and Space Sciences, University of Science and Technology of China, Hefei 230026, China
PP 024047
SiO maser polarization and magnetic field in evolved cool stars
UB, MPIfR, IRAP, IAC, LIPM, IRAP, LESIA
PP 024046
NLTE modelling of water-rich exoplanet atmospheres. Cooling and heating rates
(1) Université Paris-Saclay
(2) IAC
(3) Université Grenoble Alps
PP 024045
Solar multi-object multi-frame blind deconvolution with a spatially variant convolution neural emulator
IAC+ULL
PP 024044
The IACOB project XI. No increase of mass-loss rates over the bi-stability region
(1) University of La Laguna, (2) IAC, (3) NAOJ, (4) University of Innsbruck
PP 024043
A 20 kiloparsec bipolar Lyman $α$ outflow from a radio galaxy at z=2.95
(1) Università di Torino, (2) INAF - Osservatorio Astrofisico di Torino, (3) IAC, (4) ULL, (5) Scuola Normale Superiore Pisa
PP 024042
Towards an observationally motivated AGN dusty torus model. I. Dust chemical composition from the modeling of Spitzer spectra
(1) IRyA/UNAM, (2) Sterrenkundig Observatorium, Universiteit Gent, (3) KIPAC/Stanford University, (4) Astronomical Observatory of Belgrade, (5) IAC, (6) ULL
PP 024041
A Very-High-Energy Gamma-Ray View of the Transient Sky
(1) INAF—Osservatorio Astronomico di Roma, Via Frascati 33, I-00040 Monte Porzio Catone, Italy, (2) Instituto de Astrofísica de Canarias and Departamento de Astrofísica, Universidad de La Laguna, 38200 La Laguna, Tenerife, Spain
PP 024040
Ionised AGN outflows in the Goldfish galaxy -- The illuminating and interacting red quasar eFEDSJ091157.4+014327 at z $\sim$ 0.6
(1) Università di Bologna, (2) INAF-Osservatorio di Astrofisica e Scienza dello Spazio, (3) IAC, (4) ULL, (5) Leibniz-Institut für Astrophysik Potsdam
PP 024039
QSOFEED: The relationship between star formation and AGN Feedback
(1) IAC, (2) ULL, (3) University of Sheffield, UK, (4) University of California, Riverside, USA
PP 024038
The miniJPAS Survey: The radial distribution of star formation rates in faint X-ray active galactic nuclei
(1) Donostia International Physics Center (DIPC), (2) IAC, (3) ULL
PP 024037
Integral field spectroscopy supports atmospheric optics to reveal the finite outer scale of the turbulence
(1) IAC, (2) Departamento de Astrofísica, ULL
PP 024036
On the Pair-Instability Supernova origin of J1010+2358
(1)University of Florence
(2)Uppsala University
(3)IAC
PP 024035
Excitation mechanisms of C II optical permitted lines in ionized nebulae
(1) IAC, Spain, (2) Dep. Astrofísica, ULL, Spain, (3) U. Heidelberg, Germany, (4) IA-UNAM, México, (5) New York University, Abu Dhabi, UAE
PP 024034
Modelling of surface brightness fluctuation measurements: Methodology, uncertainty, and recommendations
(1) Instituto de Astrofísica de Canarias (IAC), E-38200 La Laguna, Tenerife, Spain, (2) Departamento de Astrofísica, Universidad de La Laguna, E-38205 Tenerife, Spain, (3) Centro de Astrobiología (CSIC/INTA), ESAC Campus, Camino Bajo del Castillo s/n, E-28692 Villanueva de la Cañada, Spain, (4) Centre for Astrophysics and Supercomputing, Swinburne University, John Street, Hawthorn VIC 3122, Australia
PP 024033
Observational Tests of Active Galactic Nuclei Feedback: An Overview of Approaches and Interpretation
(1) Newcastle University, UK; (2) IAC; (3) ULL
PP 024032
Chronology of our Galaxy from Gaia Colour-Magnitude Diagram-fitting (ChronoGal). I. The formation and evolution of the thin disk from the Gaia Catalogue of Nearby Stars
(1) Instituto de Astrofisica de Canarias; (2) Departamento de Astrofísica, Universidad de La Laguna (3) INAF-Astronomical Observatory of Abruzzo; (4) INFN, Sezione di Pisa; (5) Universidad de Granada, Departamento de Física Teórica y del Cosmos (6) Instituto Carlos I de Física Teórica y Computacional, Universidad de Granada; (7) Isaac Newton Group of Telescopes (8) Institute of Astronomy, Cambridge; (9) Leibniz-Institut für Astrophysik Potsdam (AIP); (10) Kapteyn Astronomical Institute, University of Groningen; (11) Université Côte d'Azur, Observatoire de la Côte d'Azur, CNRS (12) INAF - Osservatorio di Astrofisica e Scienza dello Spazio di Bologna.
PP 024031
NLTE modelling of water-rich exoplanet atmospheres. Cooling and heating rates
(1) Université Paris-Saclay
(2) IAC
(3) Université Grenoble Alps
PP 024030
Optical variability of the blazar 3C 371: from minute to year timescales
(1) IAA, (2) IAC, (3) INAF-Osservatorio Astrofisico di Torino - Italia, (4) Universidad de La Laguna, Dpto Astrofisica
PP 024029
The effects of environment on galaxies' dynamical structures: From simulations to observations
(1) Shanghai Astronomical Observatory,
(2) School of Astronomy and Space Sciences,
(3) Max-Planck-Institut für Astronomie,
(4) University of Vienna,
(5) Università di Padova,
(6) INAF - Osservatorio Astronomico di Padova,
(7) INAF - Astronomical Observatory of Capodimonte,
(9) Instituto de Astrofísica de Canarias,
(10) Departamento de Astrofísica, Universidad de La Laguna.
PP 024028
MUSE view of PDS 456: kpc-scale wind, extended ionized gas and close environment
(1) Università degli Studi di Milano-Bicocca, (2) INAF – Osservatorio Astronomico di Trieste, (3) INAF – Osservatorio Astronomico di Roma, (4) IAC, (5) ULL
PP 024027
Small-scale magnetic flux emergence preceding a chain of energetic solar atmospheric events
(1) Instituto de Astrofísica de Canarias, (2) Universidad de La Laguna, (3) Rosseland Centre for Solar Physics, (4)
Institute of Theoretical Astrophysics, (5) Lockheed Martin Solar and Astrophysics Laboratory, (6) Bay Area Environmental Research Institute, (7) LPC2E, CNRS/CNES/University of Orléans
PP 024026
Nonlinear Wave Damping by Kelvin-Helmholtz Instability-induced Turbulence
(1) Department of Mathematics and Statistics, University of Exeter, Exeter, EX4 4QF UK
(2) Instituto de Astrofísica de Canarias, Vía Láctea S/N, E-38205 La Laguna, Tenerife, Spain
(3) Departamento de Astrofísica, Universidad de La Laguna, E-38206 La Laguna, Tenerife, Spain
(4) Department of Physics, Kyoto university, Kitashirakawa Oiwakecho Sakyoku Kyoto, 606-8502, Japan
PP 024025
ALMA reveals a compact and massive molecular outflow driven by the young AGN in a nearby ULIRG
(1) University of Sheffield, (2) IAC, (3) ULL, (4) ASTRON, (5) University of Groningen
PP 024024
AGN feedback in the Local Universe: multiphase outflow of the Seyfert galaxy NGC 5506
(1) Università degli Studi di Bologna, (2) INAF-OAS, (3) IAC, (4) ULL
PP 024023
Probing the roles of orientation and multi-scale gas distributions in shaping the obscuration of Active Galactic Nuclei through cosmic time
(1) University of Southampton, (2) IAC, (3) ULL
PP 024022
The influence of thermal pressure gradients and ionization (im)balance on the ambipolar diffusion and charge-neutral drifts
IAC, Departamento de Astrofísica ULL
PP 024021
Hydrogenated amorphous carbon grains as an alternative carrier of the 9-13μm plateau feature in the fullerene planetary nebula Tc 1
(1) Instituto de Astrofísica de Canarias,
(2) Universidad de La Laguna,
(3) Consejo Superior de Investigaciones Científicas
PP 024020
Baryonic properties of nearby galaxies across the stellar-to-total dynamical mass relation
(1) Instituto de Astrofísica de Canarias, (2) Universidad de La Laguna, (3) ESO-Garching, (4) University of Vienna
PP 024019
Ultra-deep imaging of NGC1052-DF2 and NGC1052-DF4 to unravel their origins
(1) IAC (2) ULL (3) Gemini Observatory (4) Kapteyn Astronomical Institute
PP 024018
Stellar halo density with LAMOST K and M giants
(1) IAC; (2) PIFI-Visiting Scientist 2023 of Chinese Academy of Sciences at Purple Mountain Observatory, Nanjing 210023, and National Astronomical Observatories, Beijing 100012; (3) ULL; (4) School of Physics and Astronomy, China West Normal University, 1 ShiDa Road, Nanchong 637002, China; (5)
Institute for Frontiers in Astronomy and Astrophysics, Beijing Normal University, Beijing 102206, China; (6) Key Laboratory of Space Astronomy and Technology, National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100101, China; (7) Dipartimento di Fisica e Astronomia, Universita di Padova, Vicolo dell’Osservatorio 3, 35122 Padova, Italy; (8) University of Chinese Academy of Sciences, Beijing 100049, China
PP 024017
Secondary halo bias through cosmic time I: Scaling relations and the connection with the cosmic web
Instituto de Astrofísica de Canarias (IAC), Universidad de La Laguna, Universidad Técnica Federico Santa María (UTFS
PP 024016
More fundamental than the fundamental metallicity relation: The effect of the stellar metallicity on the gas-phase mass-metallicity and gravitational potential-metallicity relations
(1) Dpto. de Física Teórica y del Cosmos, Facultad de Ciencias (Edificio Mecenas), Universidad de Granada, E-18071 Granada, Spain, (2) Instituto Carlos I de Física Teórica y computacional, Universidad de Granada, E-18071 Granada, Spain, (3) Universidad Nacional Autónoma de México, Instituto de Astronomía, AP 106, Ensenada 22800, BC, México, (4)
Instituto de Astrofísica de Canarias, E-38205 La Laguna, Tenerife, Spain, (5) Universidad de La Laguna, Dpto. Astrofísica, E-38206 La Laguna, Tenerife, Spain
PP 024015
TESS and ESPRESSO discover a super-Earth and a mini-Neptune orbiting the K-dwarf TOI-238
(1) Instituto de Astrofísica de Canarias, (2) Departamento de Astrofísica, Universidad de La Laguna, (3) Hamburger Sternwarte, (4) Department of Physics, University of Warwick, (5) Centre for Exoplanets and Habitability, University of Warwick, (6) European Southern Observatory, (7) Observatoire astronomique de l’Université de Genève, (8) Instituto de Astrofísica e Ciências do Espaço, CAUP, Universidade do Porto, (9) Departamento de Física e Astronomia, Faculdade de Ciências, Universidade do Porto, (10) Département de Physique, Institut Trottier de Recherche sur les Exoplanètes, Université de Montréal, (11) Consejo Superior de Investigaciones Científicas (CSIC), (12) INAF – Osservatorio Astronomico di Trieste, (13) INAF – Osservatorio Astrofisico di Torino, (14) Centro de Astrobiología, CSIC-INTA, (15) Departamento de Física de la Tierra y Astrofísica & IPARCOSUCM (Instituto de Física de Partículas y del Cosmos de la UCM), Facultad de Ciencias Físicas, Universidad Complutense de Madrid, (16) Physics Institute of University of Bern, (17) Scuola Normale Superiore, Piazza dei Cavalieri 7, (18) NASA Ames Research Center, (19) Center for Astrophysics - Harvard & Smithsonian, (20) Centro de Astrofísica da Universidade do Porto, (21) INAF - Osservatorio Astronomico di Palermo, (22) Instituto de Astrofísica e Ciências do EspaÇo, Faculdade de Ciências da Universidade de Lisboa, (23) Light Bridges S. L., (24) Royal Astronomical Society, (25) Department of Physics and Kavli Institute for Astrophysics and Space Research, Massachusetts Institute of Technology, (26) Department of Earth, Atmospheric and Planetary Sciences, Massachusetts Institute of Technology, (27) Department of Aeronautics and Astronautics, MIT, (28) Department of Astrophysical Sciences, Princeton University, (29) SETI Institute, (30) Società Astronomica Lunae
PP 024014
Boron Abundances in Early B Dwarfs of the Galactic Open Cluster NGC 3293
(1) Space Telescope Science Insitute (2) Inst. f. Astronomie Bonn (3) Obs, Nacional, Rio de J. (4) IAC/ULL (5) Uni. Arizona
PP 024013
Characterising the intra-cluster light in The Three Hundred simulations
(1) Departamento de Física Teórica, UAM (2) IAC (3) ULL
PP 024012
Wolf 327b: A new member of the pack of ultra-short-period super-Earths around M dwarfs
(1) IAC, (2) ULL
PP 024011
An ultraviolet spectral study of fullerene-rich planetary nebulae
Instituto de Astrofísica de Canarias; Departamento de Astrofísica, Universidad de La Laguna; Consejo Superior de Investigaciones Científicas
PP 024010
A post-merger enhancement only in star-forming Type 2 Seyfert galaxies: the deep learning view
(1) University of Bath, (2) IAC, (3) ULL, (4) LERMA, Paris, (5) Durham University, (6) DIPC, (7) IKERBASQUE, (8) SISSA, (9) Università di Bologna, (10) INAF-Bologna, (11) University of Southampton
PP 024009
Ground-Based Photometric Follow-up for Exoplanet Detections with the PLATO Mission
(1) Instituto de Astrofísica de Canarias, (2) Universidad de La Laguna
PP 024008
Effects of density and temperature variations on the metallicity of Mrk71
(1) Universität Heidelberg, (2) IAC, (3) Instituto de Astronomía UNAM
PP 024007
Global Coronal Magnetic Field Estimation Using Bayesian Inference
(1) Aryabhatta Research Institute of Observational Sciences, 263001, Nainital, India; (2) Mahatma Jyotiba Phule Rohilkhand University, Bareilly - 243006, Uttar Pradesh, India; (3) Instituto de Astrof ́ısica de Canarias, E-38205 La Laguna, Tenerife, Spain; (4) Departamento de Astrof ́ısica, Universidad de La Laguna, E-38206 La Laguna, Tenerife, Spain
PP 024006
LSPE-STRIP on-sky calibration strategy using bright celestial sources
(a) Instituto de Astrofísica de Canarias, E-38200 La Laguna, Tenerife, Canary Islands, Spain
(b) Departamento de Astrofísica. Universidad de La Laguna (ULL), E-38206 La Laguna, Tenerife, Spain
(c) Dipartamento de Fisica, Università degli Studi di Milano, via Celoria, 16, 20133 Milano, Italy
(d) INFN–Sezione di Milano, Via Celoria 16, 20133 Milano, Italy
(e) Dipartimento di Fisica, Università di Milano - Bicocca, Piazza della Scienza 3, 20126 Milano, Italy
(f) INFN–Sezione di Milano Bicocca, Piazza della Scienza 3, 20126 Milano, Italy
(g) INAF–Osservatorio Astronomico di Trieste, Via G.B. Tiepolo 11, Trieste, Italy
(h) INAF–OAS Bologna, Via P. Gobetti 101, Bologna, Italy
(i) SISSA, Astrophysics Sector, via Bonomea 265, 34136, Trieste, Italy
(j) ASI, Via del Politecnico snc, 00133 Roma, Italy.
(k) Sub-department of Astrophysics, University of Oxford, Denys Wilkinson Building, Keble Road, Oxford OX1
PP 024005
Evidence for inflows and outflows in the nearby black hole transient Swift J1727.8-162
(1) IAC, (2) ULL
PP 024004
Accretion-induced flickering variability among symbiotic stars from space photometry with NASA TESS
1 Astronomical Institute, Charles University, Prague, Czechia; 2 IAC, Spain; 3 ULL, Spain; 4 Université Paris-Saclay, France;
* This paper presents the work, conducted during the stay of JM at the IAC through the IAC early-career visitor program in 2023A.
PP 024003
Deconvolution of JWST/MIRI Images: Applications to an AGN Model and GATOS Observations of NGC 5728
(1) UTSA, (2) IAC, (3) ULL
PP 024002
The Galaxy Activity, Torus, and Outflow Survey (GATOS). III: Revealing the inner icy structure in local AGN
(1) University of Oxford, (2) CAB, CSIC-INTA, (3) European University of Cyprus, (4) Instituto de Física Fundamental, Madrid, (5) MPE, Garching, (6) IRyA, (7) IAC, (8) ULL
PP 024001
Preparing for low surface brightness science with the Vera C. Rubin Observatory: A Comparison of Observable and Simulated Intracluster Light Fractions
(1) UNSW, (2) Leiden U., (3) EPFL, (4) Durham U., (5) U. Amsterdam, (6) U. Florida, (7) IAA-CSIC, (8) Observatório Nacional-MCTI, (9) U. Munich, (10) Korea Astronomy and Space Science Institute, (11) U. Arizona, (12) IAC, (13) ULL, (14) STScI, (15) MPIA, (16) INAF Capodimonte, (17) U. Naples, (18) Liverpool John Moores U., (19) Case Western Reserve U.