Preprints in 2023
PP 023103
Chasing the break: Tracing the full evolution of a black hole X-ray binary jet with multi-wavelength spectral modeling
(1) University of Colorado, Boulder, USA y IAC
PP 023102
The Hubble Tension Survey: A Statistical Analysis of the 2012-2022 Measurements
(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 China Academy of Sciences at Purple Mountain Observatory, Nanjing 210023
and National Astronomical Observatories, Beijing 100012, China;
(5) ULL
PP 023101
Fast infrared winds during the radio-loud and X-ray obscured stages of the black hole transient GRS 1915+105
IAC, ULL, INAF-Brera, Oxford University, Cape Town University, Curtin university, CEFCA-Teruel and Cambridge University.
PP 023100
The IACOB project X. Large-scale quantitative spectroscopic analysis of Galactic blue supergiants
(1) Universidad de La Laguna, (2) Instituto de Astrofísica de Canarias, (3) Universität Innsbruck, (4) LMU München
PP 023099
Stellar mass is not the best predictor of galaxy metallicity. The gravitational potential-metallicity relation $Φ\rm ZR$
(1) Dpto. de Física Teórica y del Cosmos, Universidad de Granada, Spain, (2) Instituto Carlos I de Física Teórica y computacional, Universidad de Granada, (3) IAC, (4) Dep. Astrofísica, ULL, (5) Universidad Nacional Autónoma de México, Instituto de Astronomía, Ensenada, BC, México
PP 023098
Catalogue of BRITE-Constellation targets I. Fields 1 to 14 (November 2013 - April 2016)
* Innsbruck University
** ULL/IAC
PP 023097
Stellar populations and origin of thick disks in AURIGA simulations
(1) Max Planck Institute for Astronomy, (2) Instituto de Astrofísica de Canarias, (3) Universidad de La Laguna, (4) Astrophysics Research Institute (5) Institute for Computational Cosmology, Durham University, (6) Instituto de Investigación Multidisciplinar en Ciencia y Tecnología, Universidad de La Serena, (7) Universidad de La Serena, (8) Dipartimento di Fisica e Astronomia "Augusto Righi”, Università di Bologna, (9) Max-Planck-Institut für Astrophysik
PP 023096
CONCERTO: instrument and status
(1) Istituto de Astrofísica de Canarias, Departamento de Astrofísica, Universidad de La Laguna and other international istitutes
PP 023094
The WHaD diagram: Classifying the ionizing source with one single emission line
(1) Instituto de Astronomía, Universidad Nacional Autonóma de México, A.P. 70-264, 04510, México, CDMX, (2) Instituto de Astrofísica de Canarias, La Laguna, Tenerife, E-38200, Spain,(3) Instituto de Radioastronomía and Astrofísica (IRyA-UNAM), 3-72 (Xangari), 8701, Morelia, Mexico, (4) Departamento de Astrofísica, Universidad de La Laguna, Spain, (5) Department of Astronomy, Indiana University, Bloomington, IN 47405, USA
PP 023093
An extended Lyman $α$ outflow from a radio galaxy at z=3.7?
(1) Università di Torino, (2) INAF-Osservatorio Astrofisico di Torino, (3) IAC, (4) ULL
PP 023092
Isolated Neutron Stars
1) Instituto de Astrofı́sica de Canarias, E-38205 La Laguna, Spain;
2) Departamento de Astrofı́sica, Universidad de La Laguna, E-38206 La Laguna Spain;
3) Institute of Space Sciences (ICE, CSIC), Campus UAB, Carrer de Can Magrans s/n,E-08193, Barcelona, Spain;
3) Scuola Universitaria Superiore IUSS Pavia, Palazzo del Broletto, piazza della Vittoria 15, I-27100, Pavia, Italy;
4) INAF-Istituto di Astrofisica Spaziale e Fisica Cosmica di Milano, via A. Corti 12,
I-20133, Milano, Italy.
PP 023091
The omnipresent flux-dependent optical dips of the black hole transient Swift J1357.2-0933
(1) Instituto de Astrofísica de Canarias, (2) Departamento de Astrofísica, Universidad de La laguna, (3) School of Physics and Astronomy, Monash University, (4) Center for Astrophysics and Space Science, New York University Abu Dhabi, (5) New York University Abu Dhabi, (6) INAF, Osservatorio Astronomico di Brera, (7) Anton Pannekoek Institute for Astronomy, University of Amsterdam, (8) European Southern Observatory, (9) Faulkes Telescope Project, School of Physics and Astronomy, Cardiff University, (10) Astrophysics Research Institute, Liverpool John Moores University.
PP 023089
UltraCompCAT: a comprehensive Catalogue of Ultra-Compact and Short Orbital Period X-ray Binaries
(1) IAC, (2) ULL, (3) ESO
PP 023088
An infrared FWHM-$K_2$ correlation to uncover highly-reddened quiescent black holes
(1) IAC, (2) ULL, (3) ESO, (4) Pontificia Universidad Católica de Chile, (5) Texas Tech University
PP 023087
Matter ejections behind the highs and lows of the transitional millisecond pulsar PSR J1023+0038
Istituto de Astrofisca de Canarias (IAC), Departamento de Astrofísica, Universidad de La Laguna and other international institutes
PP 023086
Sub-second infrared variability from the archetypal accreting neutron star 4U 1728-34
Istituto de Astrofisica de Canarias, Departamento de Astrof´ısica, Universidad de La Laguna and other international istitutes
PP 023085
Shedding far-ultraviolet light on the donor star and evolutionary state of the neutron-star LMXB Swift J1858.6-0814
* Istituto Astrofisico de Canarias,
Departamento de Astrofísica, Universidad de La Laguna (ULL)
PP 023084
Deep X-Ray and Radio Observations of the First Outburst of the Young Magnetar Swift J1818.0-1607
(1)ICE-CSIC, (2)IEEC, (3)IAC, (4)ULL
PP 023083
The orbital period, black hole mass and distance to the X-ray transient GRS 1716-249 (=N Oph 93)
(1) Instituto de Astrofisica de Canarias, 38205 La Laguna, Tenerife, Spain
(2) Departamento de Astrofisica, Universidad de La Laguna, E-38206 La Laguna, Tenerife, Spain
(3) Cerro Tololo Inter-American Observatory, NSF’s National Optical-Infrared Astronomy Research Laboratory, Casilla 603, La Serena, Chile
(4) Department of Physics, Astrophysics, University of Oxford, Denys Wilkinson Building, Keble Road, Oxford OX1 3RH, UK
(5) Department of Physics and Astronomy, University of Southampton, Southampton SO17 1BJ, UK
(6) Department of Astrophysics/IMAPP, Radboud University, PO Box 9010, 6500 GL Nijmegen, The Netherlands
(7) SRON, Netherlands Institute for Space Research, Sorbonnelaan 2, 3584 CA, Utrecht, The Netherlands
(8) School of Physics, Trinity College Dublin, The University of Dublin, Dublin 2, Ireland
PP 023082
Constraining stellar and orbital co-evolution through ensemble seismology of solar-like oscillators in binaries systems –– A census of oscillating red-giants and main-sequence stars in Gaia DR3 binaries
* IAC & ULL
PP 023081
Self-Supervised Clustering on Image-Subtracted Data with Deep-Embedded Self-Organizing Map
(1) Monash University, (2) OzGrav, (3) University of Warwick, (4) IGDORE, (5) University of Sheffield, (6) University of Leicester, (7) Armagh Observatory & Planetarium, (8) NARIT, (9) University of Turku, (10) University of Manchester, (11) University of Portsmouth, (12) IAC, (13) ULL
PP 023080
Neutron star mass estimates from gamma-ray eclipses in spider millisecond pulsar binaries
(1) MPI for Gravitational physics, (2) Leibniz Universitat Hannover, (3) Jodrell Bank, (4) NRL, (5) MPI- for Radioastronomy, (6) NCRA, (7) Laboratoire Leprince-Ringuet, (8) SARAO, (9) Université d’Orléan, (10) CNRS, (11) Cornell University, (12) Hubble Fellowship Program Einstein Postdoctoral Fellow, (13) NRL, (14) University of Sheffield, (15) IAC, (16) University College Cork, (17) ULL, (18) University of Virginia, (19) NRAO, (20) Eureka Scientific, (21) Université de Bordeaux, (22) OzGrav, (23) Swinburne University of Technology, (24) New York University Abu Dhabi, (25) West Virginia University, (26) Observatoire de Paris
PP 023079
H-beta spectroscopy of the high-inclination black hole transient Swift J1357.2-0933 during quiescence
(1) Università di Palermo, (2) IAC, (3) ULLl (4) INAF/IASF, (5) ESO
PP 023078
Panning for gold, but finding helium: discovery of the ultra-stripped supernova SN2019wxt from gravitational-wave follow-up observations
(1) Instituto de Astrofísica de Canarias IAC, Spain, (2) Departamento de Astrofísica, Universidad de La Laguna, Spain
PP 023077
An almost dark galaxy with the mass of the Small Magellanic Cloud
(1) IAC, (2) ULL, (3) STScI, (4) IAA, (5) U of Toronto, (6) CEFCA, (7) Royal Military College of Canada, (8) Queens University, (9)Swinburne, (10) OKC, Stockholm University, (11) U of Padova, (12) Princeton, (13) Kapteyn
PP 023076
QUIJOTE scientific results - XIII. Intensity and polarization study of the microwave spectra of supernova remnants in the QUIJOTE-MFI wide survey: CTB 80, Cygnus Loop, HB 21, CTA 1, Tycho and HB 9
(1) IAC (2) ULL (3) Univ. Córdoba (4) CSIC
PP 023075
QUIJOTE Scientific Results -- XVII. Studying the Anomalous Microwave Emission in the Andromeda Galaxy with QUIJOTE-MFI
(1) IAC (2) ULL (3) CSIC
PP 023074
The orbital period of the recurrent nova V2487 Oph revealed
(1) Instituto de Astrofísica de Canarias IAC, Spain, (2) Departamento de Astrofísica, Universidad de La Laguna, Spain, (3) ESO, Chile, (4) INAF, Padova, Italy, (5) Institute of Space Sciences (ICE, CSIC), Barcelona, Spain, (6) University of Warwick, UK, (7) Institut d'Estudis Espacials de Catalunya (IEEC), Barcelona, Spain, (8) Universitat Politécnica de Catalunya, Barcelona, Spain
PP 023073
Dust from evolved stars: a pilot analysis of the AGB to PN transition
(1) INAF-OAR; (2) Roma Tre Univ.; (3) Macquire Univ.; (4) NSF’s NOIRLab; (5) INFN; (6) IAC-ULL
PP 023072
Infrared spectral fingerprint of neutral and charged endo- and exohedral metallofullerenes
(1) IAC-ULL; (2) UAM-IAdChem-IFIMAC; (3) LSR-HK Univ. ; (4) CSISC; (5) UAM-IAdChem-IMDEA_Nano
PP 023071
Obscuration beyond the nucleus: infrared quasars can be buried in extreme compact starbursts
(1) Durham University, (2) IAC, (3) ULL
PP 023070
A new discovery space opened by eROSITA: Ionised AGN outflows from X-ray selected samples
(1) UNIBO, (2) INAF-Osservatorio di Astrofisica e Scienza dello Spazio, (3) IAC, (4) ULL
PP 023069
The GW Vir instability strip in the light of new observations of PG 1159 stars. Discovery of pulsations in the central star of Abell 72 and variability of RX J0122.9-7521
(1) NCAC, (2) IAC, (3) ULL, (4) NOT
PP 023068
The [CII] 158 micron emission line as a gas mass tracer in high redshift quiescent galaxies
(1) IAC, (2) ULL, (3) Université Paris-Saclay, CEA, (4) MPIA, (5) Pontificia Universidad Católica de Valparaíso, Chile
PP 023067
Investigating the impact of quasar-driven outflows on galaxies at redshift 0.3-0.4
(1) ULL; (2) IAC; (3) University of Sheffield, UK
PP 023066
Mapping the stellar population and gas excitation of MaNGA galaxies with MEGACUBES. Results for AGN versus control sample
(1) Universidade Federal do Rio Grande do Sul; (2) Laboratório Interinstitucional de e-Astronomia - LIneA; (3) IAC; (4) ULL
PP 023065
Complex AGN feedback in the Teacup galaxy. A powerful ionised galactic outflow, jet-ISM interaction, and evidence for AGN-triggered star formation in a giant bubble
(1) Pontificia Universidad Católica de Chile; (2) Scuola Normale Superiore Pisa; (3) INAF - Arcetri; (4) Institute of Astronomy, Cambridge; (5) INAF - Capodimonte; (6) Millennium Institute of Astrophysics, Chile, (7) Newcastle University, UK; IAC, (8) ULL
PP 023064
To clump or not to clump The impact of wind inhomogeneities on the optical and NIR spectroscopic analysis of massive OB stars
1 Departamento de Física, Ingeniería de Sistemas y Teoría de la Señal, Universidad de Alicante, Carretera de San Vicente s/n, E03690, San Vicente del Raspeig
2 Departamento de Física Aplicada, Facultad de Ciencias, Universidad de Alicante, Carretera de San Vicente s/n, E03690, San Vicente del Raspeig, Spain
3 Instituto de Astrofísica de Canarias, 38206 La Laguna, Tenerife, Spain.
4 Departamento de Astrofísica, Universidad de La Laguna, E-38205 La Laguna, Tenerife, Spain.
5 LMU München, Universitäts-Sternwarte, Scheinerstr. 1, 81679, München, Germany
PP 023063
Revisiting constraints on the photon rest mass with cosmological fast radio bursts
(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) Instituto de Astrofísica de Canarias, E-38205 La Laguna, Tenerife, Spain; (4) PIFI-Visiting Scientist 2023 of China Academy of Sciences at Purple Mountain Observatory, Nanjing 210023 and National Astronomical Observatories, Beijing 100012, China; (5) Departamento de Astrofísica, Universidad de La Laguna, E-38206 La Laguna, Tenerife, Spain
PP 023062
Unveiling optical signatures of outflows in accreting white dwarfs
(1) IAC, (2) ULL, (3) Monash University, Australia
PP 023061
Supermassive black hole wake or bulgeless edge-on galaxy? II: Order-of-magnitude analysis of the two physical scenarios
(1) IAC, (2) Departamento Astrofísica ULL
PP 023060
RXCJ1111.6+4050 galaxy cluster: the observational evidence of a transitional fossil group
(1) IAC; (2) Dpto de Astrofísica (ULL); (3) Ludwig-Maximilian-University (Germany); (4) Max-Planck-Institut für extraterrestrische Physik (Germany); (5) Dpto Fisica, Sapienza University of Rome (Italy)
PP 023059
X-Shooting ULLYSES: massive stars at low metallicity. I. Project Description
(1) Armagh Observatory (2) IAC (3) ULL
PP 023058
The B-type Binaries Characterisation Programme II. VFTS 291: A stripped star from a recent mass transfer phase
(1) Leuven (2) IAC (3) ULL
PP 023057
QUIJOTE scientific results -- X. Spatial variations of Anomalous Microwave Emission along the Galactic plane
Instituto de Astrofísica de Canarias, E-38200 La Laguna, Tenerife, Spain
Departamento de Astrofísica, Universidad de La Laguna, E-38206 La Laguna, Tenerife, Spain
Institut d’Astrophysique de Paris, UMR 7095, CNRS & Sorbonne Université, 98 bis boulevard Arago, 75014, Paris, France
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.
Universidad de Cantabria, Departamento de Ingeniería de Comunicaciones, Edificio Ingenieria de Telecomunicación, Plaza de la Ciencia no 1, 39005 Santander, Spain 6Astrophysics Group, Cavendish Laboratory, University of Cambridge, J J Thomson Avenue, Cambridge CB3 0HE, UK
Kavli Institute for Cosmology, University of Cambridge, Madingley Road, Cambridge CB3 0HA, UK
Instituto de Física de Cantabria (IFCA), CSIC-Univ. de Cantabria, Avda. los Castros, s/n, E-39005 Santander, Spain
Departamento de Física Moderna, Universidad de Cantabria, Avda. de los Castros s/n, 39005 Santander, Spain
Consejo Superior de Investigaciones Científicas, E-28006 Madrid, Spain
Departamento de Física. Facultad de Ciencias. Universidad de Córdoba. Campus de Rabanales, Edif. C2. Planta Baja. E-14071 Córdoba, Spain
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 023056
Everything that glitters is not gold: V1315 Cas is not a dormant black hole
(1) ESO, (2) IAC, (3) ULL, (4) NOT
PP 023055
The truncation of the disk of NGC 4565: Detected up to z=4 kpc, with star formation, and affected by the warp
(1) IAC, (2) ULL, (3) University of New South Wales, (4) ASTRO 3D, (5) CEFCA, (6) Monash University, (7) NASA, (8) Bay Area Environmental Research Institute, (9) KIPAC, (10) University of Groningen
PP 023054
The AMIGA sample of isolated galaxies. XIV. Disc breaks and interactions through ultra-deep optical imaging
(1) IAC, (2) ULL, (3) IAA, (4) University of Groningen, (5) UCLA, (6) Universidad de Granada, (7) ESA NEO Coordination Centre, (8) GMV, (9) Universidad de Antofagasta
PP 023053
Mapping non-axisymmetric velocity fields of external galaxies
(1) Centro Richerche Enrico Fermi, (2) Universitá di Roma, (3) ULL, (4) IAC
PP 023052
Iluminación solar y el calendario aborigen en Cuevas del Barranco de La Angostura (Agüimes, Gran Canaria)
(1) ULPGC, (2) IAC-ULL
PP 023051
Can cuspy dark matter dominated halos hold cored stellar mass distributions?
(1) Instituto de Astrofisica de Canarias, La Laguna, Spain, (2) Astrophysics Department, Universidad de La Laguna, (3) CeBio y Departamento de Ciencias Basicas, Universidad Nacional del Noroeste de la Prov. de Buenos Aires, UNNOBA, CONICET, Junin, Argentina
PP 023050
Bayesian evidence for two slow-wave damping models in hot coronal loops
(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) Centre for Fusion, Space and Astrophysics, Physics Department, University of Warwick, Coventry CV4 7AL, United Kingdom
(4) Engineering Research Institute “Ventspils International Radio Astronomy Centre (VIRAC)” of Ventspils University of Applied Sciences, Inzenieru iela 101, Ventspils, LV-3601, Latvia
(5) Centro de Investigacion en Astronomía, Universidad Bernardo O’Higgins, Avenida Viel 1497, Santiago, Chile
PP 023048
Disk galaxies are self-similar: the universality of the HI-to-Halo mass ratio for isolated disks
(1) Université de Strasbourg, CNRS, Observatoire Astronomique de Strasbourg, (2) Laboratoire de Phisique et de Chimie de l'Environnement, Université Joseph Ki-Zerbo, Burkina Faso, (3) IAC, (4) ULL
PP 023046
Ask The Machine: Systematic detection of wind-type outflows in low-mass X-ray binaries
(1) IAC, (2) ULL, (3) LERMA
PP 023045
Solar-like oscillations in $γ$ Cephei A as seen through SONG and TESS
(1) Aarhus University, (2) IAC/ULL
PP 023044
A calibration point for stellar evolution from massive star asteroseismology
(1) KULeuven, (2) IAC/ULL
PP 023043
iNNterpol: High-precision interpolation of stellar atmospheres with a deep neural network using a 1D convolutional auto encoder for feature extraction
(1) Instituto de Astrofísica de Canarias, España; (2) Universidad de La Laguna, España
PP 023042
On the origin of the planetary nebula M 1-16. A morphokinematic and chemical analysis
(1) Instituto de Astrofísica de Canarias, España; (2) Universidad de La Laguna, España; (3) Instituto de Astronomía, UNAM, Ensenada, Mexico; (4) Universidad de Sonora, Mexico; (5) Instituto Tecnológico de Ensenada, Mexico
PP 023041
The massive relic galaxy NGC 1277 is dark matter deficient. From dynamical models of integral-field stellar kinematics out to five effective radii
(1) Universidad de La Laguna, (2) IAC, (3) University of Oxford, (4) Universidad de Valladolid, (5) Universidade de Lisboa, (6) INAOE, (7) CONACYT, (8) Ludwig-Maximilians-Universität, (9) National Academy of Sciences of Ukraine, (10) Complutense de Madrid, (11) IPARCOS, (12) Max Planck Institute for Astronomy
PP 023040
AGN feedback in action in the molecular gas ring of the Seyfert galaxy NGC7172
(1) CAB, (2) OAN, (3) Instituto de Física Fundamental, CSIC, (4) MPE, (5) LERMA, Observatoire de Paris, (6) University of Alaska Anchorage, (7) IAC, (8) ULL
PP 023039
Flare, Warp, Satellite, and Truncation: the ultra-thin galaxy UGC11859
(1) Instituto de Astronomía, Facultad de Ciencias, Universidad de Valparaíso, Gran Bretaña 1111, Playa Ancha, Valparaíso, Chile (2) Valencian International University, (VIU)I, Valencia, Spain (3) NASA Ames Research Center, Moffett Field, CA 94035, USA (4) Bay Area Environmental Research Institute, Moffett Field, California CA 94035, USA (5) Kavli Institute for Particle Physics and Cosmology (KIPAC), Stanford University, Stanford, CA 94305, USA, (6) Instituto de Astrofísica de Canarias, C/ Vía Láctea s/n, E-38205, La Laguna Tenerife, Spain (7) Facultad de Física, Universidad de La Laguna, Avda. Astrofísico Fco. Sánchez s/n 38200 La Laguna, Tenerife, Spain
PP 023038
Density biases and temperature relations for DESIRED HII regions
(1) Universidad de Heidelberg, (2) IAC, (3) ULL, (4) Universidad de Edimburgo, (5) Universidad Nacional Autónoma de México
PP 023037
The role of grain size in AGN torus dust models
(1) Instituto de Radioastronomía y Astrofísica (IRyA), (2) IAC, (3) ULL, (4) CAB, (5) University of Southampton, (6) University of Oxford
PP 023036
Temperature inhomogeneities cause the abundance discrepancy in H II regions
(1) Universidad de Heidelberg, (2) IAC, (3) ULL, (4) Universidad Nacional Autónoma de México
PP 023034
A radio-jet driven outflow in the Seyfert 2 galaxy NGC 2110?
(1) CAB, (2) OAN, (3) University of Oxford, (4) CAB, (5) IAC, (6) ULL, (7) MPE, (8) Newcastle University, (9) University of Southampton, (10) STScI, (11) UTSA, (12) NAOJ, (13) Instituto de Física Fundamental, CSIC
PP 023033
ALMA High-Level Data Products: Submillimetre counterparts of SDSS quasars in the ALMA footprint
1) ESO, Karl-Schwarzschild-Str. 2, 85748 Garching bei München, Germany
2) Nanyang Technological University, 50 Nanyang Avenue, 639798 Singapore
3) Astronomical Institute, Czech Academy of Sciences, Bocní II 1401, 141 00 Prague, Czech Republic
4) Instituto de Astrofísica de Canarias, E-38205 La Laguna, Tenerife, Spain
5) Departamento de Astrofísica, Universidad de La Laguna, E-38206 La Laguna, Tenerife, Spain
6) Joint ALMA Observatory, Alonso de Córdova 3107, Vitacura 763-0355, Santiago, Chile
7) European Southern Observatory, Alonso de Córdova 3107, Vitacura, Casilla 19001, Santiago de Chile, Chile
PP 023032
The IACOB project. IX. Building a modern empirical database of Galactic O9-B9 supergiants: Sample selection, description, and completeness
(1) Universidad de La Laguna, (2) Instituto de Astrofísica de Canarias, (3) Universität Innsbruck, (4) Universidad de Alicante
PP 023031
Catalog of Planetary Nebulae detected by GALEX and corollary optical surveys
(1) IAC, (2) ULL, (3) JHU, (4) CSIC
PP 023030
Super-massive black hole wake or bulgeless edge-on galaxy?
(1) IAC, (2) Dept. Astrofisica, ULL
PP 023029
Fuzzy dark matter confronts rotation curves of nearby dwarf irregular galaxies
Instituto de Astrofísica de Canarias; Departamento de Astrofísica, Universidad de La Laguna; Dipartimento di Fisica e Astronomia Galileo Galilei, Università di Padova; INFN-Padova; INAF-Padova
PP 023028
The optical behaviour of BL Lacertae at its maximum brightness levels: a blend of geometry and energetics
(1) INAF, Osservatorio Astrofisico di Torino, Italy
(2) Institute for Astrophysical Research, Boston University, USA
(3) Astronomical Institute, St. Petersburg State University, Russia
(4) Instituto de Astrofisica de Canarias, La Laguna, Spain
(5) Departamento Astrofisica - Universidad de La Laguna, Spain
PP 023027
DESI Mock Challenge: Halo and galaxy catalogs with the bias assignment method
Instituto de Astrofìsica de Canarias
Universidad de la Laguna
Institue for Astronomy, Royal Observatory, University of Edinburgh, UK
Tata Institue of Fundamental Research, India.
Kavli Institute for Particle Astrophysics and Cosmology, Stanford University
Shanghai Jiao Tong University, 800 Dongchuan Road, Shanghai
Department of Physics and Astronomy, Università degli Studi di Padova
Institute of Physics. Laboratory of astrophysics. École Polytechnique Fédérale de Lausanne
Department of Physics & Astronomy, University College London
nstituto de Física, Universidad Nacional Autónoma de México
Institut de Física d’Altes Energies, The Barcelona Institute of Science and Technology,
Lawrence Berkeley National Laboratory
Department of Physics, The Ohio State University
Department of Physics, Southern Methodist University
Institució Catalana de Recerca i Estudis Avançats
University of Michigan
National Astronomical Observatories, Chinese Academy of Sciences
PP 023026
Atomic Data Assessment with PyNeb: Radiative and Electron Impact Excitation Rates for [Fe II] and [Fe III]
(1) IVIC, Venezuela, (2) U. Heidelberg, (3) Western Michigan University, (4) IAC, (5) ULL, (6) IA-UNAM, Mexico
PP 023025
On the computation of interstellar extinction in photoionized nebulae
(1) IA-UNAM, Mexico, (2) GTC, (3) IAC, (4) ULL, (5) NOT, (6) Williams College, USA, (7) INAF-Arcetri, Italy, (8) CAB
PP 023024
On the dearth of C-enhanced metal-poor stars in the Galactic bulge
GEPI, Observatoire de Paris (France)
University of Florence (Italy)
Instituto de Astrofísica de Canarias (Spain)
PP 023023
Optical and near-infrared spectroscopy of the black hole transient 4U 1543-47 during its 2021 ultra-luminous state
(1) Instituto de Astrofísica de Canarias, (2) Universidad de La Laguna, (3) European Southern Observatory, (4) Osservatorio Astronomico di Brera, (5) University of Oxford, (6) Max-Planck-Institut fur Extraterrestrische Physik, (7) University of Warwick
PP 023022
The carbon star DY Persei may be a cool R Coronae Borealis variable
(1) IAC-ULL; (2) IIA India; (3) McDonal Obs. & UT; (4) TA-DPA Uppsala
PP 023021
Unveiling the chemical fingerprint of phosphorus-rich stars I. In the infrared region of APOGEE-2
(1) IAC, (2) ULL, (3) Konkoly Observatory, (4) CSFK, (5) University of Hull, (6) Joint Institute for Nuclear Astrophysics, (7) The NuGrid Collaboration, (8) ELTE Eötvös Loránd University, (9) Monash University, (10) NRC Herzberg
PP 023020
Optical polarization and spectral properties of the H-poor superluminous supernovae SN 2021bnw and SN 2021fpl
1) Instituto de Astrofisíca de Canarias, 38200 La Laguna,Tenerife, Canary Islands, Spain
2) Departamento de Astrofísica, Universidad de La Laguna (ULL), 38206 La Laguna, Tenerife, Spain
3) The Oskar Klein Centre, Department of Astronomy, Stockholm University, AlbaNova, SE-10691 Stockholm, Sweden
4) Konkoly Observatory, CSFK, Konkoly-Thege M. út 15-17, Budapest, 1121, Hungary
5) Department of Experimental Physics, Institute of Physics, University of Szeged, Dóm tér 9, Szeged, 6720 Hungary
6) ELTE Eötvös Loránd University, Gothard Astrophysical Observatory, Szombathely, Hungary
7) GRANTECAN: Cuesta de San José s/n, 38712 Breña Baja, La Palma, Spain
8) Geneva Observatory, University of Geneva, Chemin Pegasi 51, CH-1290 Versoix, Switzerland
9) Astronomy Centre, Department of Physics & Astronomy, University of Southampton, Southampton, SO17 1BJ, UK
10) Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge, CB3 0HA, UK
PP 023019
Planetary nebulae hosting accreting white dwarfs: A possible solution for the mysterious cut-off of Planetary Nebula Luminosity Function?
(1) NOA Greece, (2) IAC, (3) ULL, (4) NOT
PP 023018
Absence of nuclear polycyclic aromatic hydrocarbon emission from a compact starburst: The case of the type-2 quasar Mrk 477
(1) IAC, (2) ULL, (3) IRyA, (4) University of Oxford
PP 023017
Jet-induced molecular gas excitation and turbulence in the Teacup
(1) IAC, (2) ULL, (3) OAN, (4) Observatoire de Paris, LERMA, (5) Universitá di Trieste, (6) Savitribai Phule Pune University Campus, (7) The Australian National University, (8) University of Tsukuba
PP 023016
First BISTRO observations of the dark cloud Taurus L1495A-B10: the role of the magnetic field in the earliest stages of low-mass star formation
100 institutions including the IAC and the ULL.
PP 023015
The role of cooling induced by mixing in the mass and energy cycles of the solar atmosphere
(1) Department of Mathematics, 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
PP 023014
Mass models of the Milky Way and estimation of its mass from the GAIA DR3 data-set
(1) Centro Ricerche Enrico Fermi, Via Pansiperna 89a, 00184 Rome, Italy; (2) Istituto Nazionale Fisica Nucleare, Unità Roma 1, Dipartimento di Fisica, Universitá di Roma “Sapienza”, 00185 Rome, Italy; (3) Faculty of Mathematics, Physics, and Informatics, Comenius University, Mlynsk´a dolina, 842 48 Bratislava, Slovakia; (4) Dipartimento di Fisica, Universitá di Roma “Sapienza”, 00185 Rome, Italy; (5) IAC; (6) ULL
PP 023013
The miniJPAS survey: AGN & host galaxy co-evolution of X-ray selected sources
(1) Università di Bologna, (2) INAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, (3) DIPC, (4) IKERBASQUE, (5) University of Southampton, (6) National Observatory of Athens, (7) Durham University, (8) Ludwig-Maximilians-
Universität München, (9) Max-Planck-Institut für Astrophysik, (10) SISSA, (11) IAC, (12) ULL
PP 023012
The IACOB project VIII. Searching for empirical signatures of binarity in fast-rotating O-type stars
(1) Universite de Liege, (2) IAC/ULL, (3) CAB, (4) KULeuven
PP 023011
A black widow population dissection through HiPERCAM multi-band light curve modelling
(1) Jodrell Bank Centre for Astrophysics, Department of Physics and Astronomy, University of Manchester, Manchester, UK, (2) Instituto de Astrofísica de Canarias, La Laguna, Tenerife, Spain, (3) Departamento de astrofísica, Univ. de La Laguna, La Laguna, Tenerife, Spain, (4) Department of Physics, University College Cork, Cork, Ireland, (5) Max Planck Institute for Gravitational Physics, Albert Einstein Institute, Hannover, Germany, (6) Leibniz Universität Hannover, Hannover, Germany, (7) Department of Physics and Astronomy, University of Sheffield, Sheffield, UK, (8) LUTH, Observatoire de Paris, PSL Research University, CNRS, Meudon, France, (9) South African Radio Astronomy Observatory, South Africa, (10) Department of Physics, University of Warwick, Coventry, UK
PP 023010
The Pristine survey -- XX: GTC follow-up observations of extremely metal-poor stars identified from Pristine and LAMOST
(1) University of Cambridge (2) University of Florence (3) University of Victoria (4) IAC (5) Strasbourgh (6)Groningen
PP 023009
PISN-explorer: hunting the descendants of very massive first stars
(1) University of Florence, (2) INAF, (3) IAC, (4) GEPI, (5) Uppsala
PP 023008
The pristine nature of SMSS 1605$-$1443 revealed by ESPRESSO
(1)University of Florence, (2)IAC, (3)INAF, (4)GEPI, (5)CSIC-INTA, (6)Geneve, (7)Lisboa, (8)CAUP, (9)
PP 023007
The messy death of a multiple star system and the resulting planetary nebula as observed by JWST
(1) Macquarie University, (2) GRANTECAN, La Palma, Spain, (3) IAC, (4) ULL
PP 023006
QUIJOTE scientific results -- IX. Radio sources in the QUIJOTE-MFI wide survey maps
IFCA, ESAC, Univ Europea Madrid, IAC, ULL, Univ Wellington, CSIC, DICOM, Univ Cambridge, Kavli, Univ Cantabria, IAP, Univ Manchester, Univ Cordoba, CAS, NAOC-UKZN
PP 023005
QUIJOTE scientific results -- VIII. Diffuse polarized foregrounds from component separation with QUIJOTE-MFI
IFCA, Univ Cantabria, IAC, ULL, IAP, Univ Cambridge, Kavli, DICOM, ESAC, Universidad Europea Madrid, Univ Manchester, CSIC, Univ Cordoba, CAS, NAOC-UKZN
PP 023004
QUIJOTE Scientific Results -- VII. Galactic AME sources in the QUIJOTE-MFI Northern Hemisphere Wide-Survey
IAC, ULL, Univ Manchester, DICOM, Univ Cambridge, Kavli, IFCA, Univ Cantabria, IAP, CSIC, Univ Cordoba, CAS, NAOC-UKZN
PP 023003
QUIJOTE scientific results -- VI. The Haze as seen by QUIJOTE
IAC, ULL, IAP, IFCA, Univ Cantabria, Univ Manchester, Univ Cambridge, Kavli, DICOM, CSIC, Univ Cordoba, CAS, NAOC-UKZN
PP 023002
QUIJOTE scientific results -- V. The microwave intensity and polarisation spectra of the Galactic regions W49, W51 and IC443
IAC, ULL, CAS, NAOC-UKZN, IFCA, Univ Cambridge, Kavli, DICOM, Univ Cantabria, IAP, Univ Manchester, CSIC, Univ Cordoba
PP 023001
QUIJOTE scientific results -- IV. A northern sky survey in intensity and polarization at 10-20GHz with the Multi-Frequency Instrument
IAC, ULL, IAP, Univ Manchester, IFCA, Univ Cambridge, Kavli, CSIC, Univ Cordoba, DICOM, Univ Cantabria, ESAC, Univ Wellington, CAS, NAOC-UKZN