Preprints in 2018
PP 018127
A homogeneous analysis of globular clusters from the APOGEE survey with the BACCHUS code. I. The Northern clusters
Several institutions from North and South America and Europe (including IAC and ULL)
PP 018126
Kepler-730: A hot Jupiter system with a close-in, transiting, Earth-sized planet
Several institutions from North and South America and Europe (including IAC and ULL)
PP 018125
The complex evolution of the X-ray binary transient MAXI J1807+132 along the decay of its discovery outburst
(1) Instituto de Astrofísica de Canarias, (2) Departamento de Astrofísica, Universidad de La Laguna, (3) New York University Abu Dhabi, (4) SRON, Netherlands Institute for Space Research, (5) Jodrell Bank Centre for Astrophysics, (6) Department of Astrophysics/IMAPP, (7) Faulkes Telescope Project, School of Physics, and Astronomy, Cardiff University, (8) Astrophysics Research Institute, Liverpool John Moores University
PP 018123
Title:APOGEE [C/N] Abundances Across the Galaxy: Migration and Infall from Red Giant Ages
Several institutions from North and South America and Europe (including IAC and ULL)
PP 018122
No unique solution to the seismological problem of standing kink MHD waves
(1) Instituto de Astrofisica de Canarias, E-38205, La Laguna, Tenerife, Spain
(2) Departamento de Astrofisica, Universidad de La Laguna, E-38206, La Laguna, Tenerife, Spain
(3) Centre for mathematical Plasma Astrophysics, Department of Mathematics, KU Leuven Celestijnenlaan 200B bus 2400, B-3001 Leuven, Belgium
PP 018121
Title:A candidate super-Earth planet orbiting near the snow line of Barnard's star
(1) IAC
PP 018120
Non-axisymmetric models of galaxy velocity maps
(1) Museo Storico della Fisica e Centro Studi e Ricerche Enrico Fermi, Rome, Italy; (2) Istituto dei Sistemi Complessi, CNR, Rome, Italy; (3) Istituto Nazionale Fisica Nucleare, Dip. Fisica, Univ. “Sapienza”, Rome, Italy; (4) Univ. Oulu, Astronomy Research Unit, Finland; (5) IAC; (6) ULL
PP 018119
BAM: Bias Assignment Method to generate mock catalogs
Instituto de Astrof´ısica de Canarias, Departamento de Astrofísica, Universidad de La Laguna, National Astronomy Observatories, Chinese Academy of Science, Kavli Institute for Particle Astrophysics and Cosmology, Stanford University, SLAC National Accelerator Laboratory
PP 018118
Gaia-DR2 extended kinematical maps. Part I: Method and application
(1) IAC; (2) ULL; (3) Museo Storico della Fisica e Centro Studi e Ricerche Enrico Fermi, Rome, Italy; (4) Istituto dei Sistemi Complessi, Rome, Italy; (5) Dipartimento di Fisica, Univ. di Roma “Sapienza”, Italy
PP 018117
Spiral Structure in Barred galaxies. Observational constraints to spiral arm formation mechanisms
1. Instituto de Astrofísica de Canarias, Tenerife, Spain. 2. Departamento de Astrofísica, Universidad de La Laguna, Tenerife, Spain 3. Gran Telescopio CANARIAS, La Palma, Spain 4 Astrophysics Research Centre, Liverpool John Moores University, UK 5. Reserach Center for Astronomy, Academy of Athens,Greece Greece.
PP 018115
The Second APOKASC Catalog: The Empirical Approach
Several institutions from North and South America and Europe (including IAC and ULL)
PP 018114
Temporal and spatial scales for coronal heating by Alfven wave dissipation in transverse loop oscillations
(1) Departament de Física, Universitat de les Illes Balears (UIB), E-07122, Spain, (2) Institute of Applied Computing & Community Code (IAC3), UIB, Spain, (3) Instituto de Astrofísica de Canarias, E-38205 La Laguna, Tenerife, Spain, (4) Departamento de Astrofísica, Universidad de La Laguna, E-38206 La Laguna, Tenerife, Spain
PP 018113
On the post-common-envelope central star of the planetary nebula NGC 2346
(1) Sheffield, (2) ING, (3) IAC, (4) ULL, (5) ESO, (6) Leuven
PP 018112
A headless tadpole galaxy: the high gas-phase metallicity of the ultra-diffuse galaxy UGC2162
((1) Instituto de Astrofisica de Canarias, Spain, (2) Departamento de Astrofisica, Universidad de La Laguna, Spain, (3) IBM Research Division, T.J. Watson Research Center, USA, (4) Department of Physics & Astronomy, Vassar College, NY, USA, (5) Center for Astrophysics and Gravitation - CENTRA/SIM Departamento de Fisica, Instituto Superior Tecnico, Universidade de Lisboa, Portuga, (6) Departamento de Engenharia Fisica, Faculdade de Engenharia, Universidade do Porto, Portugal, (7) Instituto de Astrofisica de Andalucia - CSIC, Granada, Spain)
PP 018111
An imaging spectroscopic survey of the planetary nebula NGC 7009 with MUSE
(1) European Southern Observatory,
(2) Instituto de Astrofísica de Canarias (IAC),
(3) Universidad de La Laguna, Dpto. Astrofísica,
(4) Dept. of Physics and Astronomy, University College London,
(5) Department of Physics and Astronomy, University of Denver,
(6) Dept. of Physics and Astronomy, University College London,
(7) Jodrell Bank Centre for Astrophysics,
(8) Laboratory for Space Research, University of Hong Kong,
(9) Instituto de Astronomía, Universidad Católica del Norte,
(10) Institut für Astro- und Teilchenphysik, Leopold–Franzens Universität Innsbruck,
(11) Leiden Observatory, University of Leiden,
(12) Oberkasseler Straße 130, D-40545 Düsseldorf, Germany
(13) Okayama Observatory, Kyoto University Honjo,
PP 018110
The CARMENES search for exoplanets around M dwarfs: The warm super-Earths in twin orbits around the mid-type M dwarfs Ross 1020 (GJ 3779) and LP 819-052 (GJ 1265)
(1) Instituto de Astrofísica de Canarias, Tenerife (2) Dept. Astrofísica, Universidad de La Laguna, Tenerife (3) Max-Planck-Institut für Astronomie, Heidelberg (4) Institut für Astrophysik, Göttingen (5) Institut de Ciències de l’Espai, Barcelona (6) Institut d’Estudis Espacials de Catalunya, Barcelona (7) Centro de Astrobiología, Madrid (8) Instituto de Astrofísica de Andalucía, Granada (9) Landessternwarte, Heidelberg (10) Centro Astronómico Hispano-Alemán, Observatorio Astronómico de Calar Alto (11) Departamento de Astrofísica y Ciencias de la Atmósfera, Universidad Complutense de Madrid, Madrid (12) Thüringer Landessternwarte Tautenburg (13) Hamburger Sternwarte, Hamburg (14) School of Geosciences, Raymond and Beverly Sackler Faculty of Exact Sciences, Tel Aviv
PP 018109
'Climatological Study for the Cherenkov Telescope Array North Site at the Canary Islands I: Temperature, Precipitation, and Relative Humidity
Instituto de Astrofísica de Canarias
Universidad de La Laguna
PP 018108
Real-time multiframe blind deconvolution of solar images
((1) Instituto de Astrofisica de Canarias, (2) University of La Laguna, (3) Institute for Solar Physics, Dept. of Astronomy, Stockholm University, (4) Kiepenheuer-Institut für Sonnenphysik)
PP 018107
Nearly 100% of the sky is covered by Lyman-α emission around high redshift galaxies
(1) Leibniz-Institut fur Astrophysik Potsdam (AIP),
(2) Univ Lyon, Univ Lyon1, Ens de Lyon, CNRS, Centre de Recherche Astrophysique de Lyon,
(3) Leiden Observatory, Leiden University,
(4) Instituto de Astrofísica e Ciencias do Espacio, Universidade do Porto, CAUP
(5) Department of Physics, ETH Zurich,
(6) Institut fur Physik und Astronomie, Universität Potsdam,
(7) Institut de Recherche en Astrophysique et Planetologie (IRAP), Université de Toulouse, CNRS,
(8) Department of Astronomy, Stockholm University, AlbaNova University Centre,
(9) Instituto de Astrofísica de Canarias (IAC),
(10) Universidad de La Laguna, Dpto. Astrofísica
PP 018106
Evolved stars in the Local Group galaxies - III. AGB and RSG stars in Sextans A
(1) IAC-ULL; (2) OAR-INAF; (3)STSI
PP 018105
On Kelvin–Helmholtz and parametric instabilities driven by coronal waves
(1) Department of Mathematics, CEMPS, University of Exeter, Exeter, EX4 4QF U.K.
(2) Department of Applied Mathematics, School of Mathematics, University of Leeds, Leeds, LS2 9JT, U.K.
(3) Instituto de Astrof ́ısica de Canarias, V ́ıa La ́ctea s/n, E-38205 La Laguna, Tenerife, Spain
(4) Departamento de Astrof ́ısica, Universidad de La Laguna, E-38206 La Laguna, Tenerife, Spain
(5) Department of Applied Mathematics and Theoretical Physics, University of Cambridge, Wiberforce Road, CB3 0WA U.K.
PP 018104
The 1989 and 2015 outbursts of V404 Cygni: a global study of wind-related optical features
IAC, ULL and several other.
PP 018103
Gaia DR2 Proper Motions of Dwarf Galaxies within 420 kpc: Orbits, Milky Way Mass, Tidal Influences, Planar Alignments, and Group Infall
(1) IAC,(2) Universidad de La Laguna, (3) University of California, Irvine, (4) University of Virginia, (5) Space Telescope Science Institute, (6) John Hopkins University, (7) University of Arizona
PP 018102
Oxygen and silicon abundances in Cygnus OB2: Chemical homogeneity in a sample of OB slow rotators
(1) Instituto de Astrofísica de Canarias, 38200 La Laguna, Tenerife, Spain.
(2) Departamento de Astrofísica, Universidad de La Laguna, 38205 La Laguna, Tenerife, Spain.
(3) ESO, Karl-Schwarzschild-Strasse 2, 85748 Garching bei München, Germany.
(4) Centro de Astrobiología (CSIC/INTA), 28850 Torrejón de Ardoz, Madrid, Spain.
(5) Astronomisches Rechen-Institut, Zentrum für Astronomie der Universität Heidelberg, Mönchhofstr 12–14, 69120 Heidelberg, Germany.
PP 018101
Prospects for Measurements with Strange Hadrons at LHCb
1
Instituto Galego de F´ısica de Altas Enerx´ıas (IGFAE), Santiago de Compostela, Spain
2Cavendish Laboratory, University of Cambridge, Cambridge, United Kingdom
3
INFN-Sezione di Cagliari, Cagliari, Italy
4
INFN-Sezione di Napoli, Napoli, Italy
5Oliver Lodge Laboratory, University of Liverpool, Liverpool, United Kingdom
6LPNHE, Sorbonne Universit´e, Universit´e Paris Diderot, CNRS/IN2P3, Paris, France
7
INFN-Sezione di Firenze, Firenze, Italy
8Laboratoire d’Annecy-le-Vieux de Physique Th´eorique , Annecy Cedex, France
9
Institute for Theoretical Particle Physics (TTP), Karlsruhe Institute of Technology, Kalsruhe, Germany
10Institute for Nuclear Physics (IKP), Karlsruhe Institute of Technology, Kalsruhe, Germany
11School of Physics and Astronomy, University of Birmingham, Birmingham, United Kingdom
12INFN-Sezione di Frascati, Frascati, Italy
13Laboratoire de l’Accelerateur Lineaire (LAL), Orsay, France
14Instituto de Astrof´ısica de Canarias, La Laguna, Tenerife, Spain
15CERN, CH-1211, Geneva 23, Switzerland
16Physik-Institut, Universit¨at Z¨urich, Z¨urich, Switzerland
PP 018100
A clockwork solution to the flavor puzzle
- Theoretical Physics Department, CERN, 1211 Geneva 23, Switzerland
- PRISMA Cluster of Excellence & Mainz Institute for Theoretical Physics, Johannes Gutenberg
University, 55099 Mainz, Germany
- Centre for Mathematical Sciences, Plymouth University, PL4-8AA Plymouth, UK
dJožef Stefan Institute, Jamova 39, 1000 Ljubljana, Slovenia
- Faculty of Mathematics and Physics, University of Ljubljana, Jadranska 19, 1000 Ljubljana,
Slovenia
- Instituto de Astrofísica de Canarias, C/ Vía Láctea, s/n E38205 - La Laguna (Tenerife), España
- Department of Physics, University of Cincinnati, Cincinnati, Ohio 45221,USA
PP 018099
Fast spectrophotometry of WD 1145+017
1. Instituto de Astrofísica de Canarias, 38205 La Laguna, Tenerife, Spain
2. Departamento de Astrofísica, Universidad de La Laguna, 38206 La Laguna, Tenerife, Spain
3. Department of Physics, University of Warwick, Coventry CV4 7AL, UK
4. Center for Exoplanets and Habitability, University of Warwick, Coventry CV4 7AL, UK
5. Lund Observatory, Department of Astronomy & Theoretical Physics, Lund University, Box 43, SE-221 00 Lund, Sweden
PP 018098
Chemistry in the dIrr galaxy Leo A
(1) Instituto de Astronomía, UNAM, Mexico, (2) Instituto de Ciencias Nucleares, UNAM, Mexico, (3) IAC, Spain, (4) Dep. Astrofisica, ULL, Spain
PP 018097
The Origin of the 300 km s^-1 Stream Near Segue 1
Several institutions from North and South America and Europe (including IAC and ULL)
PP 018096
APOGEE data releases 13 and 14: data and analysis
Several institutions from North and South America and Europe (including IAC and ULL)
PP 018095
APOGEE data releases 13 and 14: stellar parameter and abundance comparisons with independent analyses
Several institutions from North and South America and Europe (including IAC and ULL)
PP 018094
The Double Dust Envelopes of R Coronae Borealis Stars
(1) UC; (2) LSU; (3)SSI; (4) LJL-KU; (5) IAC-ULL; (6) IIA; (7) SPA-CU ; (8) SU
PP 018093
The Open Cluster Chemical Abundances and Mapping Survey: II. Precision Cluster Abundances for APOGEE using SDSS DR14
Several institutions from North and South America and Europe (including IAC and ULL)
PP 018092
A comprehensive comparison between APOGEE and LAMOST: Radial Velocities and Atmospheric Stellar Parameters
Several institutions from North and South America and Europe (including IAC and ULL)
PP 018091
When Nature Tries to Trick Us
(1) ESO, (2) IAC, (3) ULL, (4) UCL, (5) Las Campanas, (6) SAAO, (7) SALT, (8) ESO Chile, (9) Univ Andres Bello, (10) GTC, (11) OAN
PP 018090
The short orbital period binary star at the heart of the planetary nebula M 3-1
(1) IAC, (2) ULL, (3) ESO, (4) NCAC, (5) SALT, (6) SAAO, (7) OAN, (8) GTC
PP 018089
Confirmation of the link between central star binarity and extreme abundance discrepancy factors in planetary nebulae
(1) University College London, UK, (2) IAC, Tenerife, Spain, (3) ULL, Tenerife, Spain, (4) ESO, Garching, germany, (5) GTC, La Palma, Spain
PP 018088
Measuring masses in low mass X-ray binaries via X-ray spectroscopy: the case of MXB 1659-298
Max-Planck-Institut fur Extraterrestrische Physik (MPE), Universita Roma Tre, IAC, ULL
PP 018087
Integrated-light analyses vs. colour-magnitude diagrams - II. Leo~A, an extremely young dwarf in the Local Group
1- Instituto de Astrof\'isica de Canarias, Calle V\'ia L\'actea s/n, E-38205 La Laguna, Tenerife, Spain
2- Departamento de Astrof\'isica, Universidad de La Laguna, E-38200 La Laguna, Tenerife, Spain
PP 018086
The Pristine Survey IV: Approaching the Galactic metallicity floor with the discovery of an ultra metal-poor star
(1) IAC
PP 018085
The first super-Earth Detection from the High Cadence and High Radial Velocity Precision Dharma Planet Survey
(1) IAC
PP 018084
Spectroscopic characterisation of the stellar content of ultra diffuse galaxies
(1) Instituto de Astrofísica de Canarias, Calle Vía Láctea s/n, E-38205 La Laguna, Tenerife, Spain
(2) Departamento de Astrofísica, Universidad de La Laguna, E-38200 La Laguna, Tenerife, Spain
(3) University of California Observatories, 1156 High Street, Santa Cruz, CA 95064, USA
(4) Max-Planck Institut f\"ur Astronomie, Konigstuhl 17, D-69117 Heidelberg, Germany
PP 018083
Stellar chemo-kinematics of the Cetus dwarf spheroidal galaxy
(1) IAC, Spain, (2) ULL, Spain, (3) MPIA, Heidelberg, Germany, (4) ESO, Garching, Germany, (5) Excellence Cluster Origin and Structure of the Universe, Garching, Germany, (6) Institute of Astronomy, Cambridge, UK, (7) Instituto de Astrofísica - PUC, Santiago, Chile (8) Millennium Institute of Astrophysics, Santiago, Chile, (9) Kapteyn Astronomical Institute, Groningen, Netherlands, (10) Institute of Physics, Laboratory of Astrophysics - EPFL, Sauverny, Switzerland, (11) GEPI, CNRS UMR 8111, Observatoire de Paris, Meudon, France
PP 018082
3D non-LTE corrections for Li abundance and 6Li/7Li isotopic ratio in solar-type stars I. Application to HD 207129 and HD 95456
(1) IAC
PP 018081
Self-Similar Approach for Rotating Magnetohydrodynamic Solar and Astrophysical Structures
(1) IAC, (2) ULL
PP 018080
Binary companions of evolved stars in APOGEE DR14: Search method and catalog of ~5,000 companions
Several institutions from North and South America and Europe (including IAC and ULL)
PP 018078
A chemical and kinematical analysis of the intermediate-age open cluster IC 166 from APOGEE and Gaia DR2
Several institutions from North and South America and Europe (including IAC and ULL)
PP 018077
The APOGEE-2 Survey of the Orion Star Forming Complex II: Six-dimensional structure
Several institutions from North and South America and Europe (including IAC and ULL)
PP 018076
Appearances can be deceiving: clear signs of accretion in the seemingly ordinary Sextans dSph
(1) Instituto de Astrofísica de Canarias (IAC)
(2) Departamento de Astrofísica, Universidad de La Laguna (ULL)
PP 018075
The low-luminosity accretion disc wind of the black hole transient V4641 Sagittarii
IAC, ULL, SRON-Utrecht, NASA-Washington D.C
PP 018074
Neutron-capture Elements in Planetary Nebulae: First Detections of Near-infrared [Te III] and [BrV] Emission Lines
(1) IAC, Spain, (2) ULL, Spain, (3) Western Michigan U., USA, (4) U. Texas, USA, (5) U. West Georgia, USA (6) U. Arizona, (7) CSIC-INTA, Spain, (8) GTC, Spain
PP 018073
On the optical counterparts of radio transients and variables
Sydney Institute for Astronomy, University of Oxford, University of Southampton, IAC, ULL
PP 018070
MUSE crowded field 3D spectroscopy in NGC300 I. First results from central fields
(1) Leibniz-Institut für Astrophysik Potsdam (AIP), (2) Institute for Astrophysics, University of Göttingen, (3) Astrophysics Research Institute, Liverpool John Moores University, (4) Instituto de Astrofísica de Canarias (IAC), (5) Universidad de La Laguna, (6) CRAL, Observatoire de Lyon, CNRS, (7) Department of Physics, ETH Zürich,
PP 018069
A Detection of Sgr A* in the far infrared
(1) MPE Garching, (2) IAC, (3) Universidad de La Laguna, (4) University of California, Berkeley
PP 018068
On the early evolution of Local Group dwarf galaxy types: star formation and supernova feedback
(1) INAF/OAS Bologna, Italy; (2) INFN, Sezione di Bologna, Italy; (3) IAC, Spain; (4) ULL, Spain; (5) AIP, Germany; (6) MPIA, Germany; (7) Center for Theoretical Astrophysics and Cosmology, Zurich, Switzerland; (8)
Institute for Astronomy, Edinburgh, UK; (9) Department of Physics, Guildford, UK
PP 018067
Testing tidal theory for evolved stars by using red-giant binaries observed by Kepler
1 Instituto de Astrofısica de Canarias, E-38200 La Laguna, Tenerife, Spain
2 Departamento de Astrof´ısica, Universidad de La Laguna, E-38206 La Laguna, Tenerife, Spain
3 IRFU, CEA, Universit´e Paris-Saclay, F-91191 Gif-sur-Yvette, France
4 Universit´e Paris Diderot, AIM, Sorbonne Paris Cit´e, CEA, CNRS, F-91191 Gif-sur-Yvette, France
5 LESIA, Observatoire de Paris, PSL Research Univ., CNRS, Univ. Pierre et Marie Curie, Univ. Paris Diderot, 92195 Meudon, France
6 Department of Astronomy, University of Geneva, Chemin des Maillettes 51, 1290, Versoix, Switzerland
7 IRAP, UMR 5277, CNRS and Universit´e de Toulouse, 14 Av. E. Belin, 31400, Toulouse, France
8 Harvard-Smithsonian Center for Astrophysics, Cambridge, MA 02138, USA
9 Departamento de Fısica, Universidade Federal do Rio Grande do Norte, CEP: 59072-970 Natal, RN, Brazil
PP 018066
El equinoccio en el ritual ibérico. El santuario de La Malladeta (La Vila Joiosa, Alicante)
(1) IAC, (2) Vilamuseu
PP 018065
Evolved stars in the Local Group galaxies - II. AGB, RSG stars and dust production in IC10
(1) IAC-ULL; (2) OAR-INAF; (3) Univ. La Sapienza
PP 018064
Kepler-503b: An Object at the Hydrogen Burning Mass Limit Orbiting a Subgiant Star
Several institutions from USA and IAC/ULL
PP 018063
The Magnetic Response of the Solar Atmosphere to Umbral Flashes
(1) Queen's University Belfast, (2) Department of Physics and Astronomy, California State University Northridge, (3) Instituto de Astrofisica de Canarias, (4) ULL, (5) NSO, (6) HELP, Stanford University
PP 018062
44 New & Known M Dwarf Multiples In The SDSS-III/APOGEE M Dwarf Ancillary Science Sample
Several institutions from North and South America and Europe (including IAC and ULL)
PP 018061
MOLPOP-CEP: An Exact, Fast Code for Multi-Level Systems
(1) Instituto de Astrofisica de Canarias, (2) Departamento de Astrofisica, Universidad de La Laguna, (3) Department of Physics and Astronomy, University of Kentucky, (4) Astronomy Dept., University of California, Berkeley
PP 018060
Two planetary systems with transiting Earth-size and super-Earth planets orbiting late-type dwarf stars
(1) IAC
(2) GTC
PP 018059
An updated stellar census of the Quintuplet cluster
1. The Open University, Milton Keynes, UK,
2 IAC, 3 ULL,
4 University of Edinburgh, UK,
5 CSIC-INTA, Madrid, Spain
6 CSIC, Granada, Spain
7 Rochester Institute of Technology, NY, USA
PP 018058
The GTC exoplanet transit spectroscopy survey IX. Detection of Haze, Na, K, and Li in the super-Neptune WASP-127b
G. Chen (1,2,3), E. Palle (1,2), L. Welbanks (4), J. Prieto-Arranz (1,2), N. Madhusudhan (4), S. Gandhi (4), N. Casasayas-Barris (1,2), F. Murgas (1,2), L. Nortmann (1,2), N. Crouzet (1,2), H. Parviainen (1,2), and D. Gandolfi (5)
(1) IAC, (2) ULL, (3) Purple Mountain Observatory, (4) University of Cambridge, (5) Universita di Torino
PP 018057
Stellar and Planetary Characterization of the Ross 128 Exoplanetary System from APOGEE Spectra
Several institutions from North and South America and Europe (including IAC and ULL)
PP 018056
HD 89345: a bright oscillating star hosting a transiting warm Saturn-sized planet observed by K2
*IAC
PP 018055
NOEMA OBSERVATIONS OF A MOLECULAR CLOUD IN THE LOW-METALLICITY GALAXY KISO 5639
(1) IBM Research Division, T.J. Watson Research Center, NY, USA, (2) Institut de Radioastronomie Millimetrique, Domaine Universitaire, France, (3) Departamento de Astronomia, Universidad de Chile, Santiago, Chile, (4) Department of Physics & Astronomy, Vassar College, NY, USA, (5) IAC + ULL
PP 018054
Nonlinear seismic scaling relations
1: Vienna University, Austria 2: IAC, Spain 3: Sydney Universtity, Australia, 4: CEA Saclay, France
PP 018053
Calibrating the metallicity of M dwarfs in wide physical binaries with F-, G-, and K- primaries - I: High-resolution spectroscopy with HERMES: stellar parameters, abundances, and kinematics
(1) IAC
PP 018052
The Arches cluster revisited: II. A massive eclipsing spectroscopic binary in the Arches cluster
(1) The Open University, UK, (2) CSIC-INTA, Madrid, (3) IAC, (4) ULL, (5) Royal Observatory Edinburgh, UK, (6) University of Sheffield, UK, (7) UK ATC, Edinburgh, UK)
PP 018051
Disk-Like Chemistry of the Triangulum-Andromeda Overdensity as Seen by APOGEE
Several institutions from North and South America and Europe (including IAC and ULL)
PP 018050
The origin of the mid-infrared nuclear polarization of active galactic nuclei
(1) NASA/SOFIA, (2) IAC, (3) ULL
PP 018049
A search for Galactic runaway stars using Gaia Data Release 1 and Hipparcos proper motions
[1] CAB/CSIC, [2] IAC/ULL
PP 018048
Oscillating red giants in eclipsing binary systems: empirical reference value for asteroseismic scaling relation
* IAC
PP 018047
An Unusual Transient in the Extremely Metal-Poor Galaxy SDSS J094332.35+332657.6 (Leoncino Dwarf)
(1)Center for Astrophysics and Gravitation - CENTRA/SIM, Departamento de Física, Instituto Superior Técnico, Universidade de Lisboa, Av. Rovisco Pais 1, P-1049-001 Lisbon, Portugal, (2) 2Departamento de Engenharia Física, Universidade do Porto, Faculdade de Engenharia, Universidade do Porto, Rua Dr. Roberto Frias, s/n, P-4200-465,
Oporto, Portugal, (3) Instituto Astrofísica de Canarias, La Laguna, Tenerife, Spain, (4) Departamento de Astrofísica, Universidad La Laguna
PP 018046
Quantifying the AGN-driven outflows in ULIRGs (QUADROS) II: evidence for compact outflow regions from HST [OIII] imaging observations
(1) University of Sheffield, (2) FIT, (3) University of Notre Dame, (4) IAC, (5) ULL
PP 018044
An Unusual Transient in the Extremely Metal-Poor Galaxy SDSS J094332.35+332657.6 (Leoncino Dwarf)
(1)Center for Astrophysics and Gravitation - CENTRA/SIM, Departamento de Física, Instituto Superior Técnico, Universidade de Lisboa, Av. Rovisco Pais 1, P-1049-001 Lisbon, Portugal, (2) 2Departamento de Engenharia Física, Universidade do Porto, Faculdade de Engenharia, Universidade do Porto, Rua Dr. Roberto Frias, s/n, P-4200-465,
Oporto, Portugal, (3) Instituto Astrofísica de Canarias, La Laguna, Tenerife, Spain, (4) Departamento de Astrofísica, Universidad La Laguna
PP 018043
The host galaxy of the gamma-ray-emitting narrow-line Seyfert 1 galaxy PKS 1502+036
(1) INAF-Istituto di Radioastronomia; (2) Instituto de Astrofísica de Canarias; (3) Departamento de Astrofísica, Universidad de La Laguna; (4)INAF-Osservatorio Astrofisico di Torino; (5) Department of Physics and Astronomy, University of Southampton;
PP 018042
The origin of the relation between metallicity and size in star-forming galaxies
((1) Instituto de Astrofisica de Canarias, La Laguna, Tenerife, Spain, (2) Departamento de Astrofisica, Universidad de La Laguna)
PP 018041
Circumnuclear star-formation and AGN activity: Clues from surface brightness radial profile of PAHs and [SIV]
(1) IRyA, (2) UNAM, (3) IAC, (4) ULL
PP 018040
Optical validation and characterization of Planck PSZ1 sources at the Canary Islands observatories. I. First year of ITP13 observations
(1) IAC, (2) DA, ULL, (3) University of KwaZulu-Natal (South Africa), (4) Universidad Andres Bello (Chile), (5) Tartu Observatory (Estonia), (6) Institut d'Astrophysique Spatiale, Universite Paris-Sud (Francia), (7) IRFU, CEA, Universite Paris-Saclay (Francia), (8) Universit\'e Paris Diderot, AIM, Sorbonne Paris Cite (Francia), (9) Max-Planck-Institut fur extraterrestrische Physik (Alemania), (10) Institute of Theoretical Astrophysics, University of Oslo (Noruega), (11) Astrophysics Group, Cavendish Laboratory (UK), (12) Kavli Institute for Cosmology (UK), (13) Universita degli Studi di Roma Tor Vergata (Italia), (14) Universite de Toulouse, UPS-OMP, Institut de Recherche en Astrophysique et Planetologie (IRAP) (Francia), (15) CNRS, IRAP (Francia), (16) IASF-Milano, Istituto Nazionale di Astrofisica (Italia), (17) ESO
PP 018039
Lucky Spectroscopy, an equivalent technique to Lucky Imaging. Spatially resolved spectroscopy of massive close visual binaries using the William Herschel Telescope
[1] CAB-CSIC/INTA, [2] Universidad de La Serena, [3] IAC/ULL
PP 018038
The VLT-FLAMES Tarantula Survey: XXVIII. Nitrogen abundances for apparently single dwarf and giant B-type stars with small projected rotational velocities
[1] QUB, [2] IAC/ULL
PP 018037
Fundamental parameters of massive stars in multiple systems: The cases of HD17505A and HD206267A
[1] Université de Liège, [2] KU Leuven, [3] IAC/ULL
PP 018036
An excess of massive stars in the local 30 Doradus starburst
[1] University of Oxford, [2] IAC/ULL
PP 018035
The emission and distribution of dust of the torus of NGC 1068
(1) SOFIA/NASA, (2) IAC, (3) ULL
PP 018034
Resolving the nuclear obscuring disk in the Compton-thick Seyfert galaxy NGC5643 with ALMA
(1) CAB, INTA/CSIC, (2) IAC, (3) ULL
PP 018033
The HADES RV Programme with HARPS-N@TNG VIII. Gl15A: A multiple wide planetary system sculpted by binary interaction
(1) IAC
PP 018032
GONG Catalog of Solar Filament Oscillations Near Solar Maximum
(1) Instituto de Astrofísica de Canarias, E-38200 La Laguna,Tenerife, Spain
(2) Departamento de Astrofísica, Universidad de La Laguna, E38206, La Laguna, Tenerife, Spain
(3) NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA
(4) Departament de Física, Universitat de les Illes Balears (UIB), E-07122 Palma de Mallorca, Spain
(5) Institute of Applied Computing & Community Code (IAC3), UIB, Spain
(6) Catholic University of America, Washington, DC 20064, US
PP 018031
Disk stars in the Milky Way detected beyond 25 kpc from its center
(1) IAC; (2) ULL; (3) Key Laboratory of Optical Astronomy, National Astronomical Observatories, Beijing, China; (4) University of Chinese Academy of Sciences, Beijing, China
PP 018030
3D Asymmetrical motions of the Galactic outer disk with LAMOST K giant stars
(1) Key Lab of Optical Astronomy, National Astronomical Observatories, Beijing, China; (2) University of the Chinese Academy of Sciences, Beijing, China; (3) IAC; (4) ULL; (5) LSST, Tucson (Arizona), USA
PP 018029
Age-resolved chemistry of red giants in the solar neighbourhood
Several institutions from North and South America and Europe (including IAC and ULL)
PP 018028
Chemical Abundances of Main-Sequence, Turn-off, Subgiant and red giant Stars from APOGEE spectra I: Signatures of Diffusion in the Open Cluster M67
Several institutions from North and South America and Europe (including IAC and ULL)
PP 018027
Heavy-element yields and abundances of Asymptotic Giant Branch models with a Small Magellanic Cloud metallicity
(1) Monash; (2) Konkoly Obs.; (3) Univ. Sao Paulo; (4) Mcquarie Univ; (5) AAO; (6) IAC-ULL
PP 018026
Signatures of the Galactic bar on stellar kinematics unveiled by APOGEE
(1)IAC, (2)ULL, (3)Space Telescope Science Institute, (4)Department of Physics and Astronomy, University of Utah, (5) Departamento de Astronomía, Universidad de Concepción, (6) Institut Utinam, CNRS UMR6213, Univ. Bourgogne Franche-Comté, OSU THETA , Observatoire de Besançon, (7)Institute of Cosmology and Gravitation, University of Portsmouth, (8)Haverford College, Department of Physics and Astronomy, (9)Departamento de Fsica, Facultad de Ciencias, Universidad de La Serena
PP 018025
Evolution of the anti-truncated stellar profiles of S0 galaxies since z = 0.6 in the SHARDS survey. II - Structural and photometric evolution-
1 Instituto de Astrofísica de Canarias, C/ Vía Láctea, E-38200 La Laguna, Tenerife, Spain e-mail: asborlaff@iac.es
2 Departamento de Astrofísica y CC. de la Atmósfera, Universidad Complutense de Madrid, E-28040 Madrid, Spain
3 Facultad de Física, Universidad de La Laguna, Avda. Astrofísico Fco. Sánchez s/n, 38200, La Laguna, Tenerife, Spain
4 Consejo Superior de Investigaciones Científicas, Spain
5 Observatoire de Paris, LERMA, PSL Research University, 61 Avenue de l’Observatoire, 75014, Paris, France
6 University of California, 501 Campbell Hall, Berkeley, CA 94720 Santa Cruz, USA
7 Observatoire de Genève, Université de Genève, 51 Ch. des Maillettes, 1290 Versoix, Switzerland
PP 018024
K2 photometry and HERMES spectroscopy of the blue supergiant rho Leo: rotational wind modulation and low-frequency waves
(1) KULeuven (2) IAC, ULL
PP 018023
Impact of young stellar components on quiescent galaxies: deconstructing cosmic chronometers
IAC, ULL
PP 018022
J0023+0307: A mega metal-poor dwarf star from SDSS/BOSS
Instituto de Astrofísica de Canarias
Departamento de Astrofísica de la universidad de La laguna
PP 018021
Local anti-correlation between star-formation rate and gas-phase metallicity in disk galaxies
((1) Instituto de Astrofisica de Canarias, Spain, (2) Departamento de Astrofisica, Universidad de La Laguna, Spain, (3) Center for Astrophysics and Gravitation - CENTRA/SIM, Universidade de Lisboa, Portugal, (4) Departamento de Engenharia Fisica, Universidade do Porto, Portugal, (5) Instituto de Astrofisica de Andalucia, Spain)
PP 018020
THE UPDATED BASTI STELLAR EVOLUTION MODELS AND ISOCHRONES: I. SOLAR SCALED CALCULATIONS
(1) Instituto de Astrofısica de Canarias, (2) Department of Astrophysics of University of La Laguna, (3) INAF-Osservatorio Astronomico d’Abruzzo, (4) Astrophysics Research Institute Liverpool John Moores University, (5) Dipartimento di Fisica e Astronomia - Universitá a degli Studi di Bologna, (6) INAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, (7) Kapteyn Astronomical Institute University of Groningen, (8) Stellar Astrophysics Centre Department of Physics and Astronomy Aarhus University
PP 018019
Identifying two groups of massive stars aligned in the l ∼ 38◦ Galactic direction
(1) Unidad de Astronomıa, Universidad de Antofagasta, Antofagasta, Chile.
(2) Instituto de Astrofısica de Canarias, c/Vıa Lactea s/n, 38205 La Laguna, Tenerife, Spain.
(3) Departamento de Astrofısica, Universidad de La Laguna, E-38205 La Laguna, Tenerife, Spain.
(4) Centro de Estudios de F ısica del Cosmos de Aragon (CEFCA), E-44001, Teruel, Spain.
(5) Departamento de Astrofısica, Universidad Complutense de Madrid, E-38040, Madrid, Spain.
(6) Centro de Astrobiologıa, CSIC-INTA. Ctra. Torrejon a Ajalvir km.4, E-28850 Torrejon de Ardoz, Madrid, Spain.
(7) Instituto de Fısica y Astronomıa, Facultad de Ciencias, Universidad de Valparaıso, Valparaıso, Chile.
(8) Millennium Institute of Astrophysics, MAS.
PP 018018
The star formation history of the Sextans dwarf spheroidal galaxy: a true fossil of the pre-reionization era
(1)(Instituto de Astrofísica de Canarias, Vía Láctea S/N, E-38200 La Laguna, Tenerife, Spain; Department of Astrophysics, University of La Laguna, E-38200 La Laguna, Tenerife, Canary Islands, Spain; Dipartimento di Fisica e Astronomia "Galileo Galilei", Universitá degli Studi di Padova, Vicolo dell'Osservatorio 3, I-35122 Padova, Italy), (2)(Instituto de Astrofísica de Canarias, Vía Láctea S/N, E-38200 La Laguna, Tenerife, Spain; Department of Astrophysics, University of La Laguna, E-38200 La Laguna, Tenerife, Canary Islands, Spain), (3)(INAF-Osservatorio Astronomico d'Abruzzo, Via M. Maggini, sn. 64100 Teramo, Italy; Instituto de Astrofísica de Canarias, Vía Láctea S/N, E-38200 La Laguna, Tenerife, Spain), (4)(Department of Astrophysics, University of La Laguna, E-38200 La Laguna, Tenerife, Canary Islands, Spain; Instituto de Astrofísica de Canarias, Vía Láctea S/N, E-38200 La Laguna, Tenerife, Spain), (5)(Dipartimento di Fisica e Astronomia "Galileo Galilei", Universitá degli Studi di Padova, Vicolo dell'Osservatorio 3, I-35122 Padova, Italy; INAF-Osservatorio Astronomico di Padova, Vicolo dell'Osservatorio 5, I-35122 Padova, Italy)
PP 018017
Massive stars in the SDSS-IV/APOGEE SURVEY. I- OB stars
Several institutions from North and South America and Europe (including IAC and ULL)
PP 018016
StarHorse: A Bayesian tool for determining stellar masses, ages, distances, and extinctions for field stars
Several institutions from USA and Europe (including IAC and ULL)
PP 018015
The l5780 and l5797 diffuse interstellar bands in the Antennae Galaxy as seen by MUSE
(1) Instituto de Astrofísica de Canarias, (2) Universidad de La Laguna, (3) Leibniz-Institut für Astrophysik Potsdam, (4) Institut für Physik und Astronomie, Universität Potsdam
PP 018013
Extracting cosmological information from the angular power spectrum of the 2MASS Photometric Redshift catalogue
Instituto de Astrofísica de Canarias, s/n, E-38205, La Laguna, Tenerife, Spain
Departamento de Astrofísica, Universidad de La Laguna, E-38206, La Laguna, Tenerife, Spain
Leiden Observatory, Leiden University, Niels Bohrweg 2, NL-2333 CA Leiden, The Netherlands
National Centre for Nuclear Research, Astrophysics Division, P.O. Box 447, 90-950 L´od´z, Poland
5Janusz Gil Institute of Astronomy, University of Zielona G´ora, ul. Licealna 9, 65-417 Zielona G´ora, Poland
Dipartamento di Fisica, Universit´a degli Studi Roma Tre, Via della Vasca Navale 84, Rome 00146, Italy
INFN Sezione di Roma 3, Via della Vasca Navale 84, Rome 00146, Italy
INAF, Osservatorio Astronomico di Roma, Monte Porzio Catone, Italy
PP 018012
The Bulge Metallicity Distribution from the APOGEE Survey
(1) University of Virginia
(2) Instituto de Astrofísica de Canarias
(3) Universidad de La Laguna
(4) Max-Planck-Institut für Astronomie,
(5) Institut Utinam
(6) University of Washington
(7) University of Utah
(8) University of Toronto
(9) Dunlap Institute for Astronomy and Astrophysics
(10) Observatório Nacional
(11) Steward Observatory
(12) Laboratório Interinstitucional de e-Astronomia —
LIneA
(13) Osservatorio Astronomico di Padova
(14) ELTE Eötvös Loránd University
(15) National Optical Astronomy Observatories
(16) Liverpool John Moores University
(17) Université Côte d’Azur
(18) University of Texas at Austin
PP 018011
New insights into the outflows from R Aquarii
(1) Tartu Obs., (2) Univ. of Tartu (3) GTC, (4) IAC, (5) ULL, (6) Kapteyn Instituut, (7) OAN, (8) Terroux Obs., (9) QUB, (10) NOT, (11) Leiden Obs., (12) CNRS
PP 018010
The Metal-poor non-Sagittarius (?) Globular Cluster NGC 5053: Orbit and Mg, Al and Si Abundances
Several institutions from USA and Europe (including IAC and ULL)
PP 018009
Machine learning in APOGEE: Unsupervised spectral classification with K-means
Instituto de Astrofísica de Canarias,
Departamento de astrofísica, Universidad de La Laguna,
Instituto de Física de Cantabria
PP 018008
Precision determination of corotation radii in galaxy disks: Tremaine-Weinberg v. Font-Beckman for NGC 3433
(1) Instituto de Astrofísica de Canarias, c/Vía Láctea, s/n, E38205, La Laguna, Tenerife, Spain; jeb@iac.es,
jfont@iac.es, asborlaff@iac.es, bgarcia@iac.es (2) Departamento de Astrofísica, Universidad de La Laguna, Tenerife, Spain. (3 )Consejo Superior de Investigaciones Científicas, Spain
PP 018006
A new look inside Planetary Nebula LoTr 5: A long-period binary with hints of a possible third component
(1) Univ de Valparaiso, (2) ESO Chile, (3) Univ Leuven, (4) IAC, (5) ULL, (6) INTA-CSIC, (7) IAA
PP 018005
GTC/CanariCam mid-IR imaging of the fullerene-rich Planetary Nebula IC 418: searching for the spatial distribution of fullerene-like molecules
(1) IAC-ULL; (2) OAN; (3) CSIC; (4) ESAC; (5) UAM; (6) IA-UNAM
PP 018004
Revisiting the Stellar Velocity Ellipsoid - Hubble type relation: observations versus simulations
(1) Instituto de Astrofísica de Canarias, (2) Depto. Astrofísica, Universidad de La Laguna (ULL), (3) Astrophysics Research Institute, Liverpool John Moores University, (4) European Southern Observatory, (5) Max-Planck-Institut für Astronomie
PP 018003
Evidence of a truncated spectrum in the angular correlation function of the cosmic microwave background
(1) Department of Physics, The Applied Math Program, and Department of Astronomy, The University of Arizona, USA; (2) IAC, (3) ULL
PP 018002
Non-grey dimming events of KIC 8462852 from GTC spectrophotometry
(1) Instituto de Astrofísica de Canarias, (2) Universidad de La Laguna, (3) Louisiana State University