Preprints in 2021
PP 021099
Gradients of chemical abundances in the Milky Way from HII regions: distances derived from Gaia EDR3 parallaxes and temperature inhomogeneities
(1) Instituto de Astrofísica de Canarias (IAC), E-38205 La Laguna, Spain
(2) Departamento de Astrofísica, Universidad de La Laguna, E-38206 La Laguna, Spain
(3) Instituto de Astronomía, Universidad Nacional Autónoma de México, Ap. 70-264, 04510 CDMX, México
(4) Department of Astronomy, The University of Texas at Austin, 2515 Speedway, Stop C1400, Austin, TX 78712, USA
PP 021098
HARMONI view of the host galaxies of active galactic nuclei around cosmic noon: Resolved stellar morpho-kinematics and the MBH-σ⋆ relation
(1) Instituto de Astrofísica de Canarias (IAC), (2) Dpto. de Astrofísica, Universidad de La Laguna, (3) Leiden Observatory, Leiden University, (4) Centro de Astrobiología (CSIC-INTA), (5) Department of Physics, University of Oxford, (6) Institute of Space Sciences (ICE, CSIC), (7) Institut d’Estudis Espacials de Catalunya (IEEC)
PP 021097
The post-common-envelope binary central star of the planetary nebula Ou 5: a doubly-eclipsing post-red-giant-branch system
(1) IAC, (2) ULL
PP 021093
Learning to do multiframe wavefront sensing unsupervised: Applications to blind deconvolution
(1) IAC, (2) ULL, (3) MPS
PP 021092
The diverse cold molecular gas contents, morphologies and kinematics of type-2 quasars as seen by ALMA
(1) IAC, (2) ULL, (3) INAF/Trieste, (4) OAN-IGN, (5) CAB/CSIC-INTA/ESAC Campus, (6) Institute of Theoretical Astrophysics, University of Oslo, (7) University of Sheffield, (8) University of Hertfordshire, (9) CAB/CSIC-INTA
PP 021091
Exploring the s-process history in the Galactic disk: Cerium abundances and gradients in Open Clusters from the OCCAM/APOGEE sample
Several institutions from North and South America and Europe (including IAC and ULL)
PP 021090
APOGEE detection of N-rich stars in the tidal tails of Palomar 5
Several institutions from North and South America and Europe (including IAC and ULL)
PP 021089
MUSE spectroscopy of planetary nebulae with high abundance discrepancies
(1) Instituto de Astrofísica de Canarias, Spain, (2) Universidad de La Laguna, Spain, (3) Instituto de Astronomía, UNAM, Mexico, (4) University College London, UK, (5) European Southern Observatory, Germany, (6) Universidade Federal Itajubá, Brazil, (7) Gran Telescopio Canarias, Spain
PP 021088
Rapid contraction of giant planets orbiting the 20 million-years old star V1298 Tau
(1) IAC, (2) ULL, (3) INAF - Torino, (4) INAF - Palermo, (5) CAB - Torrejón, (6) CSIC, (7) INAF - Padova, (8) Universita degli studi di Padova, (9) INAOE, (10) Monash University, (11) CSIC-IAA, (12) CAUP, (13) University of Cambridge, (14) Institute for Space Astrophysics and Planetology, (15) CAHA, (16) CAB - Villanueva de la Cañada, (17) Universite de Liége, (18) AIP, (19) Universität Heidelberg, (20) Georg-August-Universität Göttingen, (21) Institut de Ciencies de l’Espai, (22) IEEC
PP 021087
The throughput calibration of the VERITAS telescopes
(1) Physics Department, Columbia University, New York, NY 10027,
USA
(2) Center for Astrophysics | Harvard & Smithsonian, Cambridge, MA
02138, USA
(3) Department of Physics, Washington University, St. Louis, MO
63130, USA
(4) Physics Department, California Polytechnic State University, San
Luis Obispo, CA 94307, USA
(5) Department of Astronomy and Astrophysics, 525 Davey Lab, Pennsylvania State University, University Park, PA 16802, USA
(6) Department of Physics and Astronomy, Barnard College, Columbia
University, NY 10027, USA
(7) Department of Physics and Astronomy, Purdue University, West
Lafayette, IN 47907, USA
(8) Department of Physics and Astronomy and the Bartol Research Institute, University of Delaware, Newark, DE 19716, USA
(9) School of Physics and Astronomy, University of Minnesota, Minneapolis, MN 55455, USA
(10) Department of Physics, California State University - East Bay, Hayward, CA 94542, USA
(11) DESY, Platanenallee 6, 15738 Zeuthen, Germany
(12) Physics Department, McGill University, Montreal, QC H3A 2T8,
Canada
(13) Santa Cruz Institute for Particle Physics and Department of Physics,
University of California, Santa Cruz, CA 95064, USA
(14) Department of Physics and Astronomy, University of Utah, Salt
Lake City, UT 84112, USA
(15) Department of Physics and Astronomy, University of Alabama,
Tuscaloosa, AL 35487, USA
(16) Department of Physics and Astronomy, University of Iowa, Van
Allen Hall, Iowa City, IA 52242, USA
(17) School of Physics, National University of Ireland Galway, University Road, Galway, Ireland
(18) Department of Physics, Engineering Physics, and Astronomy,
Queen’s University, Kingston, ON K7L 3N6, Canada
(19) Institute of Physics and Astronomy, University of Potsdam, 14476
Potsdam-Golm, Germany
(20) School of Physics, University College Dublin, Belfield, Dublin 4,
Ireland
(21) Department of Physical Sciences, Munster Technological University, Bishopstown, Cork, T12 P928, Ireland
(22) Department of Physics and Astronomy, University of California,
Los Angeles, CA 90095, USA
(23) Department of Physics and Astronomy, Iowa State University,
Ames, IA 50011, USA
(24) Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas (CIEMAT), Av. Complutense, 40, E-28040 Madrid, Spain
(25) Instituto de Astrofísica de Canarias, E-38205 La Laguna, Tenerife,
Spain
(26) Universidad de La Laguna, Dept. Astrofísica, E-38206 La Laguna,
Tenerife, Spain
PP 021086
Do AGN triggering mechanisms vary with radio power? II. The importance of mergers as a function of radio power and optical luminosity
(1) University of Sheffield, (2) University of Hertfordshire, (3) University of Manitoba, Canada, (4) University of Wisconsin-Madison, USA, (5) IAC, (6) ULL, (7) University of Victoria, Canada, (8) University of Leeds, (9) Tel Aviv University.
PP 021085
The Influence of 10 Unique Chemical Elements in Shaping the Distribution of Kepler Planets
Several institutions from North and South America and Europe (including IAC and ULL)
PP 021084
First models of s process in AGB stars of solar metallicity for the stellar evolutionary code ATON with a novel stable explicit numerical solver
(1) Konkoly Obs.; (2) IAC-ULL; (3) INAF-OAR; (4) XCP-LANL
PP 021083
Observations with KIDs Interferometer Spectrum Survey(KISS)
Aix Marseille Univ, Univ. Grenoble Alpes, Instituto de Astrofísica de Canarias, Universidad de La Laguna, Sapienza Università di Roma, Centro de Astrobiología (CSIC-INTA), University of Cardiff
PP 021082
The ionised and molecular mass of post-common-envelope planetary nebulae. The missing mass problem
(1) OAN Madrid, (2) IAC, (3) ULL, (4) OAN Alcala de Henares, (5) UCL
PP 021081
TESS Eclipsing Binary Stars. I. Short cadence observations of 4584 eclipsing binaries in Sectors 1-26
(1) Villanova, (2) IAC, (3) ULL
PP 021080
Orientación solar del Traianeum de Italica (Santiponce, Sevilla, España)
(1) Universidad de Sevila, (2) IAC
PP 021079
Evidence of multithermal nature of spicular downflows. Impact on solar atmospheric heating
(1) RoCS, (2) ITA, (3) IAC, (4) ULL, (5) LMSAL, (6) (BAERI)
PP 021078
APOGEE Chemical Abundance Patterns of the Massive Milky Way Satellites
Several institutions from North and South America and Europe (including IAC and ULL)
PP 021077
Solar surges related to UV bursts: Characterization through k-means, inversions and density diagnostics
(1) IAC, (2) ULL, (3) RoCS, (4) ITA, (5), Universita degli Studi di Catania (6) INAF, (7) LMSAL, (8) BAERI, (9) Stanford
PP 021076
Physically motivated fit to mass surface density profiles observed in galaxies
((1) Instituto de Astrofisica de Canarias, La Laguna, Tenerife, Spain, (2) Departamento de Astrofisica, Universidad de La Laguna, (3) CeBio y Departamento de Ciencias Basicas, Universidad Nacional del Noroeste Prov. de Buenos Aires, UNNOBA, CONICET, Junin, Argentina)
PP 021075
Accurate sky signal reconstruction for ground-based spectroscopy with kinetic inductance detectors
Aix Marseille Univ, Univ. Grenoble Alpes, Univ. Grenoble Alpes, Instituto de Astrofísica de Canarias, Universidad de La Laguna, Sapienza Università di Roma, Centro de Astrobiología (CSIC-INTA), University of Cardiff, Univ. Grenoble Alpes
PP 021074
A young spectroscopic binary in a quintuple system part of the Local Association
(1) IAC, (2) ULL, (3) IEC-CSIC, (4) IEEC, (5) UCM, (6) Department of Physic, University of Warwick, (7) Centre for Exoplanets an Habitability, Warwick, (8) Max-Planck-Insitut, Göttingen, (9) LCO
PP 021073
Surface Brightness Fluctuations to constrain secondary stellar populations: Revealing very low-metallicity stars in massive galaxies.
(1)Instituto de Astrofísica de Canarias (IAC),
(2) Departamento de Astrofísica Universidad de La Laguna
(3) Centro de Astrobiología (CSIC/INTA)
(4) Centro de Estudios de Física del Cosmos de Aragón
PP 021072
Modeling the unresolved NIR-MIR SEDs of local (z<0.1) QSOs
(1) Korea Astronomy and Space Science Institute, (2) IRyA/UNAM, (3) Yonsei University, (4) GTC, (5) University of Oxford, (6) IAC, (7) ULL
PP 021071
The Missing Link? Discovery of Pulsations in the Nitrogen-rich PG 1159 Star PG 1144+005
(1) NCAC Poland, (2) IAC, (3) ULL, (4) SAAO
PP 021070
Gas and dust from extremely metal-poor AGB stars
(1): INAF-OAR; (2) Univ. Roma Tre; (3) Kavli Inst., Tokyo; (4): INAF-IAPS; (5) Univ. Padova; (6) Konkly Obs.; (7) IAC-ULL;
PP 021069
Failed-transition outbursts in black hole low-mass X-ray binaries
(1) University of Southampton; (2) Kapteyn Astronomical Institute, University of Groningen; (3) IAC; (4) Universidad de La Laguna; (5) University of Turku; (6) KTH Royal Institute of Technology and Stockholm University; (7) Space Research Institute of the Russian Academy of Sciences
PP 021068
Double-lined spectroscopic binaries in the APOGEE DR16 and DR17 data
Several institutions from North and South America and Europe (including IAC and ULL)
PP 021067
Catching dual AGN activity and kiloparsec-scale outflows in IRAS 20210+1121
(1) INAF/Roma, (2) ASI/Roma, (3) INAF/Milano, (4) IAC, (5) ULL
PP 021066
Symbiotic Stars in the APOGEE Survey: The Case of LIN 358 and SMC N73 (LIN 445a)
Several institutions from North and South America and Europe (including IAC and ULL)
PP 021065
A new radio census of neutron star X-ray binaries
Several international institutions including IAC/ULL
PP 021064
El espacio ordenado. Paisaje, orientaciones y astronomía en los albores de la época ibérica en Mazaleón (Teruel)
(1) IAC, (2) Dirección General de Cultura y Patrimonio, Gobierno de Aragón, (3) Investigador independiente
PP 021063
The BINGO Project V: Further steps in Component Separation and Bispectrum Analysis
Various
PP 021062
The BINGO Project IV: Simulations for mission performance assessment and preliminary component separation steps
Various
PP 021059
The BINGO Project I: Baryon Acoustic Oscillations from Integrated Neutral Gas Observations
Universidade de São Paulo, Max-Planck-Institut für Astrophysik, Technische Universität München, Yangzhou University, Instituto Nacional de Pesquisas Espaciais, University College London, Rhodes University, Univ. Federal de Campina Grande, Universidade de Brasília, Shanghai Jiao Tong University, Shanghai Jiao Tong University, Institute for BasicScience (IBS), Shanghai Astronomical Observatory, The University of Manchester, Université Paris Diderot, Université Paris Saclay, University of Science and Technology of China, Center for Research and Development in Mathematics and Applications – CIDMA, MIT Kavli Institute for Astrophysics and Space Research, University of KwaZulu-Natal, NAOC-UKZN Computational Astrophysics Centre (NUCAC), Institut d’Astrophysique Spatiale, Orsay (CNRS-INSU), Instituto de Astrofísica de Canarias, Universidad de La Laguna
PP 021058
A forecast of the sensitivity on the measurement of the optical depth to reionization with the GroundBIRD experiment
Korea University, IAC, ULL, High Energy Accelerator Research Organization (KEK), Japan Aerospace Exploration Agency (JAXA), Institute of Space and Astronautical Science (ISAS), Kavli Institute for the Physics and Mathematics of the Universe The University of Tokyo, The Graduate University for Advanced Studies (SOKENDAI) Miura District, Kyoto University, The Institute of Physical and Chemical Research (RIKEN)
PP 021057
Resolving the circumstellar environment of the Galactic B[e] supergiant star MWC 137. II. Nebular kinematics and stellar variability
(6) IAC, (7) ULL
PP 021056
The Galaxy Activity, Torus and Outflow Survey (GATOS): II. Torus and polar dust emission in nearby Seyfert galaxies
(1) CAB, (2) OAN, (3) University of Southampton, (4) University of Oxford, (5) IAC, (6) ULL
PP 021055
The Galaxy Activity, Torus and Outflow Survey (GATOS) I. ALMA images of dusty molecular tori in Seyfert galaxies
(1) OAN, (2) CAB, (3) IAC, (4) ULL
PP 021054
Revisiting the distance to radio Loops I and IV using Gaia and radio/optical polarization data
California Institute of Technology, University of Manchester, IAC, ULL
PP 021053
Molecular gas and star formation within 12 strong galactic bars observed with IRAM-30m
(1) Instituto de Astrofísica de Canarias; (2) Departamento de Astrofísica, Universidad de La Laguna; (3) Department for Physics, Engineering Physics and Astrophysics, Queen’s University; (4) Departamento de Física Teórica y del Cosmos, Campus de Fuentenueva, Universidad de Granada; (5) Instituto Carlos I de Física Teórica y Computacional, Facultad de Ciencias, Granada; (6) Observatoire de Paris, LERMA, Collège de France, CNRS, PSL University, Sorbonne University; (7) SKA Organization; (8) Joint ALMA Observatory; (9) Universidad Internacional de Valencia (VIU); (10) SUPA, Institute for Astronomy, Royal Observatory; (11) UK Astronomy Technology Centre, Royal Observatory; (12) Instituto de Astrofísica de Andalucía (IAA-CSIC)
PP 021051
Exploring nine simultaneously occurring transients on April 12th 1950
(1) Nordita, (2) IAC, (3) Center for Laser Awareness, (4) GRANTECAN, (5) CSIC/INTA, (6) Spanish Virtual Observatory, (7) Main Astronomical Observatory of the NAS of Ukraine, (8) University of Delaware, (9) Aryabhatta Research Institute of Observational Sciences
PP 021050
The OTELO survey: the star formation rate evolution of low-mass galaxies
(1) IAC, (2) ULL, (3) CSIC/INTA, (4) ASPID, (5) ISDEFE (ESAC)/ESA
PP 021049
Bayesian evidence for a nonlinear damping model for coronal loop oscillations
(1) Instituto de Astrofísica de Canarias (IAC)
(2) Departamento de Astrofísica, Universidad de la Laguna (ULL)
PP 021048
Photoionized Herbig-Haro objects in the Orion Nebula through deep high-spectral resolution spectroscopy II: HH204
(1) IAC, Spain, (2) ULL, Spain, (3) IRyA, Mexico, (4) private affiliation, (5) U. Texas at Austin, USA
PP 021047
Origin of stellar prolate rotation in a cosmologically simulated faint dwarf galaxy
(1) IAC,
(2) ULL
(3) Institute of Physics, Laboratoire d’astrophysique, École Polytechnique Fédérale de Lausanne (EPFL), Observatoire
(4) GEPI, Observatoire de Paris, Université, PSL
PP 021046
Electron temperature fluctuations in Seyfert galaxies
(1 ) Universidade Federal de Santa Maria, (2) Universidade do Vale do Paraíba, (3) IAC, (4) ULL
PP 021045
Relation of internal attenuation, dust emission, and the size of spiral galaxies. Calibration at low-z and how to use it as a cosmological test at high-z
(1) IAC; (2) ULL
PP 021044
Baryon Acoustic Oscillations from Integrated Neutral Gas Observations: an instrument to observe the 21cm hydrogen line in the redshift range 0.13 $<$ z $<$ 0.45 -- status update
Instituto Nacional de Pesquisas Espaciais. Universidade de S ̃ao Paulo, Rhodes University, University College London, Universidade Federal de Campina Grande, Shanghai Jiao Tong University, Yangzhou University, University of Southern California, University of Manchester, Universidade Federal da Para ́ıba, University of Science and Technology of China, Universit ́e Paris Diderot, Max-Planck-Institut fr Astrophysik, Universit`a degli Studi di Roma Tor Vergata, , Technische Universit ̈at M ̈unchen, University of KwaZulu-Natal, Universit ́e Paris-Saclay, ETH Z ̈urich, Instituto de Astrof ́ısica de Canarias, Universidad de La Laguna, Phase2 Microwave Ltd., Universidade de Bras ́ılia, Bras ́ılia, Liao Ning Normal University, CTPU-IBS, Shanghai Jiao Tong University
PP 021043
History of the gas fuelling star formation in eagle galaxies
(1) Instituto de Astrofisica de Canarias, La Laguna, Tenerife, Spain,
(2) Departamento de Astrofisica, Universidad de La Laguna, Spain
PP 021042
CAPOS: The bulge Cluster APOgee Survey I. Overview and initial ASPCAP results
Several institutions from North and South America and Europe (including IAC and ULL)
PP 021041
The OTELO survey: Revealing a population of low-luminosity current/active star-forming galaxies at z∼0.9
(1) ASPID, (2) Centro de Astrobiología (CSIC/INTA), (3) ISDEFE for European Space Astronomy Centre (ESAC)/ESA, (4) Departamento de Física de la Tierra y Astrofísica, Instituto de Física de Partículas y del Cosmos, Universidad Complutense de Madrid, (5) IRAM, (6) Geneva Observatory, (7) RAL Space, STFC Rutherford Appleton Laboratory, (8) ESAC,European Space Astronomy Center,
(9) IAC, (10) Departamento de Astrofísica ULL, (11) IAA, (12) Departamento de Física, Escuela Superior de Física y Matemáticas, Instituto Politécnico Nacional, (13) Instituto de Astronomía, Universidad Nacional Autónoma de México,
(14) Instituto de Física de Cantabria, (15) Armagh Observatory and Planetarium,
(16) INAF, (17) Fundación Galileo Galilei
PP 021039
Optical spectral characterization of the gamma-ray blazars S4 0954+65,TXS 1515-273 and RX J0812.0+0237
(1) IAC, La Laguna, Tenerife, Spain
(2) Universidad de La Laguna (ULL), Dpto. de Astrofísica, Tenerife, Spain
(3) Fundación G. Galilei – INAF, La Palma, Spain
(4) Instituto de Alta Investigación, Universidad de Tarapacá, Chile
(5) Isaac Newton Group of Telescopes, La Palma, Spain
PP 021038
The complex variability of blazars: Time-scales and periodicity analysis in S4 0954+65
(1) INAF, Osservatorio Astrofisico di Torino, Italy, (2) Astronomical Institute, St. Petersburg State University, Rusia (3) Pulkovo Observatory, St.-Petersburg, Rusia, (4) IAC
PP 021037
Homogeneous Analysis of Globular Clusters from the APOGEE Survey with the BACCHUS Code - III. ω Cen
Several institutions from North and South America and Europe (including IAC and ULL)
PP 021036
The dust-gas AGN torus as constrained from X-ray and mid-infrared observations
(1) IRyA-UNAM, (2) IA-UNAM, (3) IAA, (4) IAC, (5) ULL, (6) University of Oxford
PP 021035
Extreme Emission-Line Galaxies in SDSS. I. Empirical and model-based calibrations of chemical abundances
(1) IAA, (2) Universidad de La Serena, Chile, (3) IAC
PP 021034
X-ray binary accretion states in Active Galactic Nuclei? Sensing the accretion disc of supermassive black holes with mid-infrared nebular lines
(1) Istituto di Astrofisica e Planetologia Spaziali (INAF–IAPS, Rome, Italy; (2) IAC; (3) ULL
PP 021032
Testing the Limits of Precise Subgiant Characterization with APOGEE and Gaia: Opening a Window to Unprecedented Astrophysical Studies
Several institutions from North America (including IAC and ULL)
PP 021031
Numerical simulations of dark matter haloes produce polytropic central cores when reaching thermodynamic equilibrium
(1) IAC (2) Departmento de Astrofisica, Universidad de La Laguna
PP 021030
Optical nebular emission following the most luminous outburst of Aquila X-1
(1) Instituto de Astrofísica de Canarias, (2) Departamento de Astrofísica, Universidad de La Laguna, (3) Jodrell Bank Centre for Astrophysics, Department of Physics and Astronomy, The University of Manchester
PP 021029
APOGEE view of the globular cluster NGC 6544
Several institutions from North and South America and Europe (including IAC and ULL)
PP 021028
Joint Gas and Stellar Dynamical Models of WLM: An isolated dwarf galaxy within a cored, prolate DM halo
(1) Max-Planck Institut fur Astronomie, K ̈onigstuhl 17, D-69117 Heidelberg, Germany; (2) Instituto de Astrof ısica de Canarias, Calle Vıa Lactea s/n, E-38205 La Laguna, Tenerife, Spain; (3) Departamento de Astrof ısica, Universidad de La Laguna, E-38200 La Laguna, Tenerife, Spain; (4) Department of Astrophysics, University of Vienna, Turkenschanzstrasse 17, 1180 Vienna, Austria; (5) Department of Physics & Astronomy, Rutgers, The State University of New Jersey, 136 Frelinghuysen Rd, Piscataway, NJ 08854, USA; (6) Institute for Astronomy, University of Edinburgh, Royal Observatory, Blackford Hill, Edinburgh EH9 3HJ; (7) Department of Physics and Astronomy, University of Victoria, Victoria, BC V8W 3P2, Canada
PP 021027
Weighing stars from birth to death: mass determination methods across the HRD
* Graz Univ, Austria
** IAC, Tenerife
PP 021026
Fingerprints of Stellar Populations in the Near-Infrared: An Optimised Set of Spectral Indices in the JHK-Bands
(1) IAC, (2) ULL (3) INAF-Osservatorio Astronomico di Capodimonte
PP 021025
Dips and eclipses in the X-ray binary Swift J1858.6-0814 observed with NICER
(1) University of Southampton, (2)Instituto de Astrofísica de Canarias,
(3) Universidad de La Laguna,(+) Several international institutions
PP 021024
The APOGEE Data Release 16 Spectral Line List
Several institutions from North and South America and Europe (including IAC and ULL)
PP 021023
Evidence of intra-binary shock emission from the redback pulsar PSR J1048+2339
Several international institutions including IAC/ULL
PP 021022
Chemodynamically Characterizing the Jhelum Stellar Stream with APOGEE-2
Several institutions from North and South America and Europe (including IAC and ULL)
PP 021021
The R136 star cluster dissected with Hubble Space Telescope/STIS. II. Physical properties of the most massive stars in R136
(1) University of Sheffield, (2) IAC/ULL
PP 021020
Lucky spectroscopy, an equivalent technique to Lucky Imaging: II. Spatially-resolved intermediate-resolution blue-violet spectroscopy of 19 close massive binaries using the William Herschel Telescope
(1) CAB-INTA, (2) IAC/ULL
PP 021019
Mapping the core of the Tarantula Nebula with VLT-MUSE II. The spectroscopic Hertzsprung-Russell diagram of OB stars in NGC 2070
(1) Leibniz-Institut für Astrophysik Potsdam, (2) IAC/ULL
PP 021018
Convective core sizes in rotating massive stars: I. Constraints from solar metallicity OB field stars
(1) Observatoire de Geneve, (2) IAC/ULL
PP 021017
The OTELO survey: Faint end of the luminosity function of [OII], emitters at
The OTELO survey: Faint end of the luminosity function of [OII], emitters at =1.43
(1) Instituto de Astrofísica de Canarias (IAC), (2) Departamento de Astrofísica, Universidad de La Laguna (ULL), (3) Instituto de Radioastonomía Milimétrica (IRAM), (4) Asociación Astrofísica para la Promoción de la Investigación, Instrumentación y su Desarrollo, ASPID, (5) Centro de Astrobiología (CSIC/INTA), (6) Instituto de Astronomía, Universidad Nacional Autónoma de México, (7) Departamento de Física de la Tierra y Astrofísica, Instituto de Física de Partículas y del Cosmos, IPARCOS. Universidad Complutense de Madrid, (8) DARK, Niels Bohr Institute, University of Copenhagen, (9) Instituto de Física de Cantabria (CSIC-Universidad de Cantabria), (10) Instituto de Astrofísica de Andalucía, (11) ISDEFE for European Space Astronomy Centre (ESAC)/ESA, (12) Instituto de Astronomía, Universidad Nacional Autónoma de México, (13) Fundación Galileo Galilei, Telescopio Nazionale Galileo, (14) Departamento de Física, Escuela Superior de Física y Matemáticas, Instituto Politécnico Nacional
PP 021016
Exact semianalytical calculation of rotation curves with Bekenstein-Milgrom nonrelativistic MOND
(1) IAC, (2) ULL
PP 021015
Carbon dust in the evolved born-again planetary nebulae A30 and A78
(1) IRA-UNAM; (2) IAA; (3) CUCEI; (4) IAC-ULL; (5)IPA-Postdam
PP 021014
An enquiry on the origins of N-rich stars in the inner Galaxy basedon APOGEE chemical compositions
Several institutions from North and South America and Europe (including IAC and ULL)
PP 021013
On the nature of VX Sagitarii: Is it a TZO, a RSG or a high-mass AGB star?
(1) Instituto de Astrofísica e Ciências do Espaço, Universidade do Porto, CAUP, Rua das Estrelas, 4150-762 Porto, Portugal
(2) 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, Spain
(3) Instituto de Astrofísica de Canarias (IAC), 38205 La Laguna, Tenerife, Spain
(4) Universidad de La Laguna (ULL), Departamento de Astrofísica, 38206 La Laguna, Tenerife, Spain
(5) Departamento de Física Aplicada, Facultad de Ciencias, Universidad de Alicante, Carretera de San Vicente s/n, E03690, San
Vicente del Raspeig, Spain
(6) 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, 28040 Madrid, Spain
PP 021012
Multiplicity among the cool supergiants in the Magellanic Clouds
(1) Instituto de Astrofísica de Canarias, E-38205 La Laguna, Tenerife, Spain
(2) Universidad de La Laguna, Dpto. Astrofísica, E-38206 La Laguna, Tenerife, Spain
(3) Departamento de Física, Ingeniería de Sistemas y Teoría de la Señal, Universidad de Alicante, E-03690 San Vicente del Raspeig, Alicante, Spain.
PP 021011
An intermediate-age alpha-rich Galactic population in K2
Several institutions from North and South America and Europe (including IAC and ULL)
PP 021010
A tidally tilted sectoral dipole pulsation mode in the eclipsing binary TIC 63328020
(5) IAC, (6) ULL
PP 021009
Probing 3D and NLTE models using APOGEE observations of globular cluster stars
(1) IAC-ULL; (2) ELTE
PP 021008
The OTELO survey as a morphological probe. Last ten Gyr of galaxy evolution. The mass--size relation up to z=2
1 Instituto de Astrofísica de Canarias, E-38205 La Laguna, Tenerife, Spain
2 Universidad de La Laguna, Dept. Astrofísica, E-38206 La Laguna, Tenerife, Spain
3 Instituto de Radioastronomía Milimétrica (IRAM), Av. Divina Pastora 7, Núcleo Central, E-18012 Granada, Spain
4 Asociación Astrofísica para la Promoción de la Investigación, Instrumentación y su Desarrollo, ASPID, E-38205 La Laguna,
Tenerife, Spain
5 Depto. Astrofísica, Centro de Astrobiología (INTA-CSIC), ESAC Campus, Camino Bajo del Castillo s/n, 28692, Villanueva de la
Cañada, Spain
6 Ethiopian Space Science and Technology Institute (ESSTI), Entoto Observatory and Research Center (EORC), Astronomy and
Astrophysics Research Division, PO Box 33679, Addis Abbaba, Ethiopia
7 Instituto de Astrofísica de Andalucía, CSIC, E-18080, Granada, Spain
8 ISDEFE for European Space Astronomy Centre (ESAC)/ESA, P.O. Box 78, E-28690, Villanueva de la Cañada, Madrid, Spain
9 Instituto de Astronomía, Universidad Nacional Autónoma de México, Apdo. Postal 70-264, 04510 Ciudad de México, Mexico
10 Department of Astronomy & Astrophysics, University of Toronto, Canada
11 Departamento de Física, Escuela Superior de Física y Matemáticas, Instituto Politécnico Nacional, México D.F., Mexico
12 Departamento de Física de la Tierra y Astrofísica, Facultad CC Físicas, Instituto de Física de Partículas y del Cosmos, IPARCOS,
Universidad Complutense de Madrid
13 Instituto de Física de Cantabria (CSIC-Universidad de Cantabria), E-39005 Santander, Spain
14 Armagh Observatory and Planetarium, College Hill, Armagh BT61 9DG, Northern Ireland, UK
15 Fundación Galileo Galilei - INAF Rambla José Ana Fernéndez Pérez, 7, 38712 Breña Baja, TF - Spain
16 Telescopio Nazionale Galileo Roque de Los Muchachos Astronomical Observatory 38787 Garafia, TF, Spain
PP 021007
The star formation history of Eridanus II: on the role of SNe feedback in the quenching of ultra-faint dwarf galaxies
(1) IAC; 2 (ULL); 3 (Kapteyn); 4 (STScI), 5 (INAF), 6 (CTIO), 7 (U. Zurich),8 (U. La Serena), 9 (U. Victoria), 10 (U. Oslo), 11 (U. Colorado)
PP 021006
A prediction on the age of thick discs as a function of the stellar mass of the host galaxy
(1) ULL, (2) IAC
PP 021005
A Modified Kwee─Van Woerden Method for Eclipse Minimum Timing with Reliable Error Estimates
IAC
PP 021004
Photoionized Herbig-Haro objects in the Orion Nebula through deep high-spectral resolution spectroscopy I: HH529II and III
Instituto de Astrofísica de Canarias (IAC), E-38205 La Laguna, Spain
Departamento de Astrofísica, Universidad de La Laguna, E-38206 La Laguna, Spain
Instituto de Radioastronomía y Astrofísica, Universidad Nacional Autónoma de México, Apartado Postal 3-72, 58090 Morelia, Michoacán, México
Calle Camino Real 64, Icod el Alto, Los Realejos, 38414, Tenerife, Spain
PP 021003
Towards a more complete sample of binary central stars of planetary nebulae with Gaia
(1) IoA Cambridge, (2) IAC, (3) ULL, (4) ESO, (5) UCL
PP 021002
The APOGEE Library of Infrared SSP Templates (A-LIST): High-Resolution Simple Stellar Population Spectral Models in the H-Band
Several institutions from North and South America and Europe (including IAC and ULL)
PP 021001
The Similarity of Abundance Ratio Trends and Nucleosynthetic Patterns in the Milky Way Disk and Bulge
Several institutions from North and South America and Europe (including IAC and ULL)