Preprints in 2017
PP 017133
P-REx: The Piston Reconstruction Experiment for Infrared Interferometry
(1)Max-Planck-Institute for Astronomy (MPIA), (2)Instituto de Astrofísica de Canarias, (3)Departamento de Astrofísica Universidad de La Laguna
PP 017132
The CARMENES search for exoplanets around M dwarfs - HD 147379b: A nearby Neptune in the temperate zone of an early-M dwarf
(1) IAC
PP 017131
HADES RV Programme with HARPS-N at TNG. VII. Rotation and activity of M-Dwarfs from time-series high-resolution spectroscopy of chromospheric indicators
(1) IAC, (2) UniGe
PP 017130
J0815+4729: A chemically primitive dwarf star in the Galactic Halo observed with Gran Telescopio Canarias
Instituto de Astrofísica de Canarias
Univsersidad de La laguna. Departamento de Astrofísica.
Consejo Superior de investigaciones Científicas
PP 017129
A deep narrowband survey for planetary nebulae at the outskirts of M33
(1)IAC, (2) ULL, (3)GranTeCan
PP 017128
A view of the H-band light-element chemical patterns in Globular Clusters under the AGB self-enrichment scenario
Several institutions from USA and Europe (including IAC and ULL)
PP 017127
A Photometric Study of Globular Clusters Observed by the APOGEE Survey
Several institutions from USA and Europe (including IAC and ULL)
PP 017126
STELLAR POPULATION SYNTHESIS OF STAR FORMING CLUMPS IN GALAXY PAIRS AND NON-INTERACTING SPIRAL GALAXIES
(1)Instituto de Astronomía,Universidad Nacional Autónoma de México,
04510, D. F., México (2)Department of Physics & Astronomy,East Tennessee State University,(3)Instituto de Astrofísica de Canarias,C/ Vía Láctea s/n,38200 La Laguna, Tenerife, Spain(4)Departamento de Astrofísica,
Universidad de La Laguna,Tenerife, Spain(5)Consejo Superior de
Investigaciones Científicas,Spain 6CONACYT Research Fellow - Instituto de Radioastronomía y Astrofísica,Universidad Nacional Autónoma de México,58190 Morelia, México (7) Instituto de Ciencias Nucleares,
Universidad Nacional Autónoma de México,04510, D. F., México
PP 017125
On the Origin of Diffuse Ionized Gas in the Antennae Galaxy
(1) Leibniz-Institut für Astrophysik Potsdam (AIP), (2) Instituto de Astrofísica de Canarias (IAC), (3) Universidad de La Laguna, (4) CRAL, Univ Lyon 1, (5) Observatoire de Genève, (6) Institut für Astrophysik Göttingen, (7) ETH Zürich, (8) Leiden Observatory, (9) Universität Potsdam
PP 017124
Seismic probing of the first dredge-up event through the eccentric red-giant/red-giant spectroscopic binary KIC9163796
* IAC / ULL
PP 017123
The RoPES project with HARPS and HARPS-N. I. A system of super-Earths orbiting the moderately active K-dwarf HD 176986
(1)Instituto de Astrofísica de Canarias, (2)Observatoire Astronomique de l’Université de Genève, (3)Universidad de La Laguna, (4)Consejo Superior de Investigaciones Científicas, (5)Instituto de Astrofísica e Ciências do Espaço, (6)Universidade do Porto, (7)INAF - Osservatorio Astronomico di Capodimonte
PP 017122
Modeling Radial Velocities and Eclipse Photometry of the Kepler Target KIC 4054905: an Oscillating Red Giant in an Eclipsing Binary
1 CEA, Paris-Saclay; 2 NMSU; 3 IAC
PP 017121
Elemental Abundances of Kepler Objects of Interest in APOGEE. I. Two Distinct Orbital Period Regimes Inferred from Host Star Iron Abundances
Several institutions from USA and Europe (including IAC and ULL)
PP 017120
The IACOB project. V. Spectroscopic parameters of the O-type stars in the modern grid of standards for spectral classification
(1)Instituto de Astrofísica de Canarias, E-38200 La Laguna, Tenerife,Spain.
(2)Departamento de Astrofísica, Universidad de La Laguna, E-38205 La Laguna, Tenerife, Spain.
(3)Departamento de Física y Astronomía, Universidad de la Serena, Av.Juan Cisternas 1200 Norte, La Serena, Chile.
(4)Universitätssternwarte, Scheinerstr. 1, D-81679 München, Germany.
(5)Department of Astronomy, University of Michigan, 1085 S. University Avenue, Ann Arbor, MI 48109-1107, USA.
(6)Centro de Astrobiología (INTA-CSIC), Departamento de Astrofísica.Ctra. Torrejón a Ajalvir km.4, E-28850 Torrejón de Ardoz (Madrid),Spain.
(7)Centro de Astrobiología, CSIC-INTA, campus ESAC, camino bajo del castillo s/n, E-28692 Madrid, Spain.
(8)Departamento de Física, Ingeniería de Sistemas y Teoría de la Señal,Escuela Politécnica Superior, Universidad de Alicante, Carretera deSan Vicente del Raspeig s/n, 03690 San Vicente del Raspeig, Alicante, Spain.
(9)Instituto de Investigación Multidisciplinar en Ciencia y Tecnología,Universidad de La Serena, Raúl Bitrán 1305, La Serena, Chile.
PP 017119
12C/13C isotopic ratios in red-giant stars of the open cluster NGC 6791
Several institutions from USA and Europe (including IAC and ULL)
PP 017118
Low-frequency photospheric and wind variability in the early-B supergiant HD 2905
(1) IAC & ULL, Spain (2) KULeuven, Belgium (3) Univ. Innsbruck, Austria (4) SAC, Denmark
PP 017117
New massive members of Cygnus OB2
(1) Instituto de Astrofísica de Canarias, E-38200 La Laguna, Tenerife, Spain; (2) Departamento de Astrofísica, Universidad de La Laguna, E-38205 La Laguna, Tenerife, Spain; (3) ESO, Karl-Schwarzschild-Strasse 2, 85748 Garching bei München, Germany; (4) Astronomisches Rechen-Institut, Zentrum für Astronomie der Universität Heidelberg, Mönchhofstr 12–14, 69120 Heidelberg, Germany; (5) Instituto de Astrofísica de Andalucía-CSIC, 18008 Granada, Spain.
PP 017116
Disentangling the Galactic Halo with APOGEE: II. Chemical and Star Formation Histories for the Two Distinct Populations
Several institutions from USA and Europe (including IAC and ULL)
PP 017115
Disentangling the Galactic Halo with APOGEE: I. Chemical and Kinematical Investigation of Distinct Metal-Poor Populations
Several institutions from USA and Europe (including IAC and ULL)
PP 017114
A new method of measuring center-of-mass velocities of radially pulsating stars from high-resolution spectroscopy.
(1) Instituto de Astrofísica de Canarias, E-38200 La Laguna, Tenerife, Spain; (2) Departamento de Astrofísica, Universidad de La Laguna, E-38206 La Laguna, Tenerife, Spain;
(3) INAF - Osservatorio Astrofisico di Arcetri, Largo Enrico Fermi 5, 50125 Firenze, Italy;
(4) Crimean Federal University, 295007, Vernadsky av. 4, Simferopol, Crimea;
(5) INAF-Osservatorio Astronomico di Bologna, Via Gobetti 93/3, I-40129 Bologna, Italy;
(6) Space Research Institute, Austrian Academy of Sciences, Schmiedlstrasse 6, A-8042 Graz, Austria
PP 017113
A 100 kpc nebula associated with the Teacup fading quasar
(1) CAB, (2) UAM, (3) GTC, (4) Universidade do Porto, (5) IAC, (6) ULL, (7) NRAO
PP 017112
Embedded AGN and star formation in the central 80 pc of IC 3639
1. Instituto de Astrofísica de Canarias (IAC)
2. Universidad de La Laguna (ULL)
3. Max-Planck-Institut für Radioastronomie (MPIfR)
PP 017111
Large-Amplitude Longitudinal Oscillations Triggered by the Merging of Two Solar Filaments: Observations and Magnetic Field Analysis
(1) Instituto de Astrofísica de Canarias, E-38200 La Laguna, Tenerife, Spain
(2) Departamento de Astrofísica, Universidad de La Laguna, E-38206 La Laguna, Tenerife, Spain
(3) Key Laboratory for Dark Matter and Space Science, Purple Mountain Observatory, CAS, Nanjing 210008, China
(4) School of Astronomy and Space Science, University of Science and Technology of China, Hefei, Anhui 230026, China
(5) Observatoire de Paris, LESIA, UMR8109 (CNRS), 92195 Meudon Principal Cedex, France
(6) Department of Physics, DSB Campus, Kumaun University, Nainital–263001, India
(7) NASA Goddard Space Flight Center, Code 671, Greenbelt,
MD 20771, USA
PP 017110
The First APOKASC Catalog of Kepler Dwarf and Subgiant Stars
Several institutions from USA and Europe (including IAC and ULL)
PP 017109
Quantifying the AGN-driven outflows in ULIRGs (QUADROS) I: VLT/Xshooter observations of 9 nearby objects
(1)University of Sheffield, (2)IAC, (3)ULL, (4)ASTRON
PP 017108
The shape of oxygen abundance profiles explored with MUSE: evidence for widespread deviations from single gradients
(1) Instituto de Astrofísica de Andalucía (CSIC), Glorieta de la Astronomía s/n, Aptdo. 3004, E-18080 Granada, Spain; (2) Dpto. de Física Teórica y del Cosmos, Universidad de Granada, Facultad de Ciencias (Edificio Mecenas), E-18071 Granada, Spain; (3) Instituto de Astrofísica de Canarias, Calle Vía Láctea s/n, E-38205 La Laguna, Tenerife, Spain; (4) Universidad de La Laguna, Dpto. Astrofísica, E-38206 La Laguna, Tenerife, Spain
PP 017107
SPICA and the Chemical Evolution of Galaxies: The Rise of Metals and Dust
(1) IAC, (2) ULL, (3) INAF-IAPS
PP 017106
The very faint hard state of the persistent neutron star X-ray binary SLX 1737-282 near the Galactic centre
1; Instituto de Astrofísica de Canarias (IAC), Vía Láctea s/n, La Laguna 38205, S/C de Tenerife, Spain
2; Departamento de Astrofísica, Universidad de La Laguna, La Laguna, E-38205, S/C de Tenerife, Spain
3; Max–Planck–Institut für extraterrestrische Physik, D-85748 Garching, GermanyNicolaus 4; Copernicus Astronomical Center, Polish Academy of Sciences, Bartycka 18, PL-00-716 Warsaw, Poland
PP 017105
The Role of Stellar Radial Motions in Shaping Galaxy Surface Brightness Profiles
(1) Instituto de Astrofísica de Canarias (2) Departamento de Astrofísica, Universidad de La Laguna (3) E.A. Milne Centre for Astrophysics, University of Hull (4) Joint Institute for Nuclear Astrophysics, Center for the Evolution of the Elements (JINA-CEE) (5) Departamento de Física Teórica y del Cosmos, Universidad de Granada (6) Instituto Carlos I de Física Teórica y computacional, Universidad de Granada (7) Departamento de Física Teórica, Universidad Autónoma de Madrid
PP 017104
A hybrid type Ia supernova with an early flash triggered by helium-shell detonation
(1) Uni. Tokyo, (2) Kavli Insitute, (3) Uni. Kyoto, (4) State Univ. New Jersey, (5) NOAJ, (6) Univ. Washington, (7) CSIC, (8) Aarhys Uni., (9) Liverpool John Moores, (10) Swinburne, (11) ESO, (12) Texas A&M, (13) IAC, (14) ULL
PP 017103
Where does galactic dust come from?
(1) INAF - Osservatorio Astronomico di Roma, via Frascati 33, 00078 Monte Porzio Catone, Roma, Italy
(2 )Dipartimento di Fisica, ‘Sapienza’ Universit`a di Roma, Piazzale Aldo Moro 5, 00185, Roma, Italy
(3) Instituto de Astrofisica de Canarias, Via Lactea, E-38205 La Laguna, Tenerife, Spain
(4) Departamento de Astrofisica, Universidad de La Laguna (ULL), E-38206 La Laguna, Spain
(5) INAF/Osservatorio Astrofisico di Arcetri, Largo E. Femi 5, 50125 Firenze, Italy
PP 017102
A unified model for age-velocity dispersion relations in Local Group galaxies: Disentangling ISM turbulence and latent dynamical heating
(1) Max-Planck Institut f\ddot{u}r Astronomie, Heidelberg, Germany, (2) Max-Planck Institut f\ddot{u}r Extraterrestrische Physik, Garching, Germany, (3) Department of Physics & Astronomy, Piscataway, NJ 08854, USA, (4) Instituto de Astrofısica de Canarias, La Laguna, Spain, (5) Departamento de Astrofısica, Universidad de La Laguna, Spain, (6) Leibniz-Institut fr Astrophysik Potsdam, Potsdam, Germany, (7) Grinnell College Physics Department, Grinnell, USA, (8) School of Physical Sciences, University of Tasmania, Australia, (9) Institute of Astronomy, University of Cambridge, Cambridge, UK
PP 017101
What is the Milky Way outer halo made of? High resolution spectroscopy of distant red giants
(1) Instituto de Astrofisica de Canarias, calle Via Lactea s/n, E-38205 La Laguna, Tenerife, Spain, (2) Universidad de La Laguna, Dpto. Astrofisica, E-38206 La Laguna, Tenerife, Spain, (3) EPFL, Observatoire de Sauverny, CH-1290 Versoix, Switzerland, (4) GEPI, Observatoire de Paris, CNRS, Universit\'e de Paris Diderot, F-92195, Meudon, Cedex, France, (5), University of Texas at Austin, McDonald Observatory, USA, (6) Instituto Milenio de Astrofisica, Santiago, Chile, (7) Departamento de Fisica, Facultad de Ciencias Exactas, Universidad Andres Bello, Av. Fernandez Concha 700, Las Condes, Santiago, Chile, (8) Vatican Observatory, V00120 Vatican City State, Italy, (9) Departamento de Astronomia, Universidad de Chile, Camino el Observatorio 1515, Las Condes, Santiago, Chile, Casilla 36-D, (10) Leibniz-Institut f\"ur Astrophysik Potsdam (AIP), An der Sternwarte 16, 14482 Potsdam, Germany
PP 017100
Dissecting the long-term emission behaviour of the BL Lac object Mrk 421
Osservatorio Astrofisico di Torino, (2) IAC, (3) Dpto. Astrofisica ULL, (4) Astronomical Institute, St. Petersburg State University, (5) Pulkovo Observatory, (6) Steward Observatory, University of Arizona,
(7) INAF, Istituto di Radioastronomia di Bologna
PP 017099
C/O ratios in planetary nebulae with dual-dust chemistry from faint optical recombination lines
(1) IAC, Spain, (2) ULL, Spain, (3) IA-UNAM, Mexico, (4) Konkoly Observatory, Hungary, (5) Monash Univ., Australia, (6) ANU, Australia, (7) INAOE, Mexico
PP 017097
ALMA imaging of C2H emission in the disk of NGC1068
(1) Instituto de Astrofísica de Canarias, (2) Universidad de La Laguna, Departamento de Astrofísica,
PP 017096
Red Supergiants as Cosmic Abundance Probes: massive star clusters in M83, and the mass-metallicity relation of nearby galaxies
(1) Astrophysics Research Institute, Liverpool John Moores University, Liverpool Science Park ic2,
146 Brownlow Hill, Liverpool, L3 5RF, UK.
(2) Institute for Astronomy, University of Hawaii, 2680 Woodlawn Drive, Honolulu, HI, 96822, USA
(3) Laboratoire d'astrophysique, Ecole Polytechnique F ́eed ́erale de Lausanne (EPFL), Observatoire, 1290, Versoix, Switzerland
(4)Max-Planck Institute for Astronomy, 69117, Heidelberg, Germany
(5)Laboratoire Univers et Particules de Montpellier, Universit ́e de Montpellier 2, CNRS, F-34095 Montpellier, France
(6) UK Astronomy Technology Centre, Royal Observatory Edinburgh, Blackford Hill, Edinburgh., EH9 3HJ, UK
(7) Instituto de Astrofsica de Canarias, E-38205 La Laguna, Tenerife, Spain; Universidad de La Laguna, Dpto Astrofsica, E-38206 La
Laguna, Tenerife, Spain and
(8) Institute for Astronomy, Royal Observatory Edinburgh, Blackford Hill, Edinburgh., EH9 3HJ, UK
PP 017095
NuSTAR + XMM-Newton monitoring of the neutron star transient AX J1745.6-2901
Max-Planck-Institut fur Extraterrestrische Physik, Giessenbachstrasse, D-85748, Garching, Germany;
Dipartimento di Matematica e Fisica, Universita` Roma Tre, Via della Vasca Navale 84, I-00146, Roma, Italy;
Instituto de Astrof ́ısica de Canarias, 38205 La Laguna, Tenerife, Spain;
Departamento de astrof ́ısica, Univ. de La Laguna, E-38206 La Laguna, Tenerife, Spain;
Columbia Astrophysics Laboratory, Columbia University, New York, NY 10027, USA;
California Institute of Technology, 1200, E. California Blvd., Pasadena, CA 91125, USA;
PP 017094
Target Selection for the SDSS-IV APOGEE-2 Survey
Several institutions from USA and Europe (including IAC and ULL)
PP 017093
NuSTAR + XMM-Newton monitoring of the neutron star transient AX J1745.6-2901
Max-Planck-Institut fur Extraterrestrische Physik, Giessenbachstrasse, D-85748, Garching, Germany;
Dipartimento di Matematica e Fisica, Universita` Roma Tre, Via della Vasca Navale 84, I-00146, Roma, Italy;
Instituto de Astrof ́ısica de Canarias, 38205 La Laguna, Tenerife, Spain;
Departamento de astrof ́ısica, Univ. de La Laguna, E-38206 La Laguna, Tenerife, Spain;
Columbia Astrophysics Laboratory, Columbia University, New York, NY 10027, USA;
California Institute of Technology, 1200, E. California Blvd., Pasadena, CA 91125, USA;
PP 017092
Young LMC clusters: the role of red supergiants and multiple stellar populations in their integrated light and CMDs
(1) American University of Sharjah, UAE; (2) IAC; (3) ULL; (4) IAA; (5) University of Surrey, UK
PP 017091
HADES RV Programme with HARPS-N at TNG VI. GJ 3942 b behind dominant activity signals
(1) IAC
PP 017090
Tracing the stellar component of low surface brightness Milky Way Dwarf Galaxies to their outskirts I: Sextans
(1) Instituto de Astrofísica de Canarias (IAC)
(2) Departamento de Astrofísica, Universidad de La Laguna
(3) Institute of Astronomy, University of Cambridge
(4) Istituto di Astrofisica Spaziale e Fisica Cosmica di Bologna
(5) Sydney Institute for Astronomy, The University of Sydney
(6) Observatoire astronomique de Strasbourg, Université de Strasbourg
(7) NRC Herzberg Institute of Astrophysics, Dominion Astrophysical Observatory
(8) Kapteyn Astronomical Institute, University of Groningen
PP 017089
Mapping diffuse interstellar bands in the local ISM on small scales via MUSE 3D spectroscopy
(1) Institut für Physik und Astronomie, Universität Potsdam;
(2) Leibniz-Institut für Astrophysik Potsdam (AIP);
(3) Institut für Astrophysik, Georg-August-Universität Göttingen;
(4) GEPI, Observatoire de Paris;
(5) Instituto de Astrofísica de Canarias (IAC);
(6) Universidad de La Laguna, Dpto. Astrofísica;
(7) Leiden Observatory, Leiden University
PP 017088
Rise of the Titans: A Dusty, Hyper-Luminous "870 micron Riser" Galaxy at z~6
(1) Cornell, (2) ESO, (3) Edinburgh, (4) IAC, (5) Univ. La Laguna, (6) ICL, (7) UC Irvine, (8) Sussex, (9) Oxford, (10) RAL, (11) UBC, (12) MPIfR
PP 017087
Comparison of damping mechanisms for transverse waves in solar coronal loops
(1) IAC, (2) ULL
PP 017086
Photoionization instability of the Fe K absorbing plasma in the neutron star transient AX J1745.6-2901
Universita degli Studi Roma Tre; Max-Planck-Institut fur Extraterrestrische Physik; Instituto de Astrofísica de Canarias; Universidad de La Laguna; Univ. Grenoble Alpes
PP 017085
Nuclear obscuration in active galactic nuclei
(1) IAC, (2) ULL, (3) Pontificia Universidad Católica de Chile, (4) Peking University
PP 017084
Galaxy wide radio induced feedback in a radio quiet quasar
(1) CAB, (2) UAM, (3) GTC, (4) IAC, (5) ULL
PP 017083
The ESO Diffuse Interstellar Bands Large Exploration Survey: EDIBLES I. Project description, survey sample and quality assessment
(1) Université de Toulouse, UPS-OMP, IRAP, (2) CNRS, IRAP, (3) Department of Physics and Astronomy, (4) SETI Institute, (5) School of Astronomy, Institute for Research in Fundamental Sciences, (6) European Southern Observatory, (7) GEPI, Observatoire de Paris, (8) Instituto de Astrofísica de Canarias (IAC), (9) Universidad de La Laguna, Dpto. Astrofísica, (10) School of Chemistry, The University of Nottingham, (11) Royal Astronomical Society, (12) AAAS Science International, (13) UK Astronomy Technology Centre, Royal Observatory, (14) Instituut voor Sterrenkunde, KULeuven, (15) Sackler Laboratory for Astrophysics, Leiden Observatory, (16) Astrochemistry Laboratory, NASA Goddard Space Flight Center, (17) Department of Physics, The Catholic University of America, (18) Lennard-Jones Laboratories, Keele University, (19) ESTEC, ESA, (20) ICCM, (21) Anton Pannekoek Institute for Astronomy, University of Amsterdam, (22) George Washington University, (23) LERMA, Observatoire de Paris, (24) INAF - Osservatorio Astronomico di Cagliari, (25) NASA Ames Research Center, Space Science & Astrobiology Division, (26) Kapteyn Institute, University of Groningen
PP 017082
BALMER FILAMENTS IN TYCHO’S SUPERNOVA REMNANT: AN INTERPLAY BETWEEN COSMIC-RAY AND BROAD-NEUTRAL PRECURSORS
1Department of Particle Physics and Astrophysics, Faculty of Physics, The Weizmann Institute of Science, P.O. Box 26, Rehovot 76100, Israel
2Benoziyo Fellow, Email: sladja.ast@gmail.com, ORCID: 0000-0003-1416-8069
3Finnish Centre for Astronomy with ESO (FINCA), University of Turku, V¨ais¨al¨antie 20, FI-21500 Kaarina, Finland
4Max Planck Institute for Astronomy, K¨onigstuhl 17, D-69117, Heidelberg, Germany
5Instituto de Astrof´ısica de Canarias, V´ıa L´actea, La Laguna, Tenerife, Spain
6Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, U.S.A.
7INFN Gran Sasso Science Institute, viale F. Crispi 7, 67100 L’Aquila, Italy
8Department of Physics, Astronomy and Geosciences Towson University, Towson, MD 21252, U.S.A.
9Department of Physics and Astronomy, Rutgers University, 136 Frelinghuysen Road, Piscataway, NJ 08854, U.S.A.
10University of Bern, Center for Space and Habitability, Sidlerstrasse 5, CH-3012, Bern, Switzerland
PP 017081
The Pristine survey III: Spectroscopic confirmation of an efficient search for extremely metal-poor stars
(1)IAC
PP 017080
The kinematical behaviour of ORLs and CELs in Galactic planetary nebulae
(1) IA-UNAM, Mexico, (2) IAC, Spain, (3) ULL, Spain
PP 017078
The evolution of Galactic planetary nebula progenitors through the comparison of their nebular abundances with AGB yields
(1) INAF – Osservatorio Astronomico di Roma, (2) National Optical Astronomy Observatory, (3) Instituto de Astrofísica de Canarias, (4) Departamento de Astrofísica, ULL
PP 017077
The Magellanic Inter-Cloud Project (MAGIC) III: First spectroscopic evidence of a dwarf stripping a dwarf
(1) Instituto de Astrofísica de Canarias, Spain, (2) Departamento de Astrofísica, Universidad de La Laguna, Spain, (3) Research School of Astronomy and Astrophysics, Mount Stromlo Observatory, Australia, (4) Department of Physics, University of Surrey, UK, (5) Australian Astronomical Observatory, Australia, (6) Department of Physics and Astronomy, Macquarie University, Australia
PP 017076
Polarization of the changing-look quasar J1011+5442
(1) Université de Liège, (2) IAC, (3) ULL
PP 017075
The radial abundance gradient of oxygen towards the Galactic anti-centre
(1) IAC, (2) Departamento de Astrofísica, ULL, (3) University of Hong Kong
PP 017074
The open cluster King 1 in the second quadrant
(1) Instituto de Astrofísica de Canarias (2) Departamento de Astrofísica, Universidad de La Laguna (3) Departament de Física Quántica i Astrofísica, Institut Ciéncies Cosmos (ICCUB), Universitat de Barcelona (4) National Research Council
PP 017073
Atypical Mg-poor Milky Way field stars with globular cluster second-generation like chemical patterns
(1) Universidad de Concepción
(2) Instituto de Astrofísica de Canarias
PP 017071
Stellar disc truncations and extended haloes in face-on spiral galaxies
Univ. of Groningen, IAC, ULL
PP 017070
Mass-metallicity relation of dwarf galaxies and its dependency on time: clues from resolved systems and comparison with massive galaxies
(1) IAC, (2) ULL
PP 017069
The planetary nebula IC 4776 and its post-common-envelope binary central star
(1) NCAC, (2) IAC, (3) ULL, (4) GTC, (5) UCL, (6) OAN-IGN, (7) ESO
PP 017068
A mid-infrared statistical investigation of clumpy torus model predictions
(1) IFCA, (2) CAB, (3) University of Southampton, (4) UCM, (5) IAC, (6) ULL
PP 017067
Neutron-capture element abundances in the planetary nebula NGC 5315 from deep optical and near-infrared spectrophotometry
(1) IAC, Spain, (2) ULL, Spain, (3) U. West-Georgia, USA, (4) IA-UNAM,. Mexico, (5) PUC, Chile,(6) U. Michigan, USA, (7) JINA-CEE, USA
PP 017066
Flare activity and photospheric analysis of Proxima Centauri
(1) Main Astronomical Observatory of the National Academy of Sciences of Ukraine
(2) IAC
(3) Observatoire Astronomique de l’Université de Genève
PP 017065
New ultra metal-poor stars from SDSS: follow-up GTC medium-resolution spectroscopy
(1) IAC-ULL y (2) Observatoire de Paris-Meudon
PP 017064
Observational constraints to boxy/peanut bulge formation time
(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
PP 017063
Using binary statistics in Taurus-Auriga to distinguish between brown dwarf formation processes
(1) Clara-Fey Gymnasium Bonn
(2) Centro de Astrobiología (INTA-CSIC)
(3) Instituto de Astrofísica de Canarias (IAC)
(4) Universidad de La Laguna, Dpto. Astrofísica,
(5) Helmholtz-Institut für Kern- und Strahlenphysik, Univers
ity of Bonn
(6) Charles University in Prague.
(7) Steward Observatory, The University of Arizona,
PP 017062
Rubidium and zirconium abundances in massive Galactic asymptotic giant branch stars revisited
(1)IAC, (2)ULL, (3)Laboratoire Univers et Particules de Montpellier, (4)CSIC, (5)Monash Centre for Astrophysics, (6)Konkoly Observatory
PP 017060
WHT follow-up observations of extremely metal-poor stars identified from SDSS and LAMOST
IAC-ULL
PP 017059
Evolution of the anti-truncated stellar profiles of S0 galaxies since z=0.6 in the SHARDS survey: I - Sample and Methods
1. IAC, 2. Dept. Astrofísica y CC. U. Complutense de Madrid, 3. Dept. Astrofísica ULL 4. CSIC 5. Centre Astrophysics & Supercomputing, U. Swinburne (Australia), 6.U.California, Berkeley, 7. Observatoire de Genève, Suiza 8. IFCA-CSIC.
PP 017058
An infrared view of AGN feedback in a type-2 quasar: the case of the Teacup galaxy
(1) IAC, (2) ULL, (3) CAB, (4) Pontificia Universidad Católica de Chile
PP 017057
HADES RV Programme with HARPS-N at TNG: V. A super-Earth on the inner edge of the habitable zone oft he nearby M-dwarf GJ 625
(1) Instituto de Astrofísica de Canarias, (2) Observatoire Astronomique de l’Université de Genève, (3) Universidad de La Laguna, Dpto. Astrofísica, (4) Consejo Superior de Investigaciones Científicas, (5) INAF - Osservatorio Astronomico di Palermo, (6) Institut de Ciènces de l’Espai, (7) INAF - Osservatorio Astrofisico di Catania, (8) INAF - Osservatorio Astrofisico di Torino, (9) INAF - Osservatorio Astronomico di Capodimonte, (10) INAF - Osservatorio Astronomico di Padova, (11) INAF - Osservatorio Astronomico di Trieste, (12) INAF - Osservatorio Astronomico di Brera, (13) Fundación Galileo Galilei - INAF
PP 017056
The Wolf-Rayet star population in the dwarf galaxy NGC 625
(1) IAC, (2) ULL, (3) AIP, (4) IAA-CSIC, (5) ESO, (6) EEZA-CSIC, (7) UG
PP 017055
Chemical abundances of 1111 FGK stars from the HARPS GTO planet search program II: Cu, Zn, Sr, Y, Zr, Ba, Ce, Nd and Eu
(1) IAC, ULL
PP 017054
Survival of the obscuring torus in the most powerful active galactic nuclei
(1) IFCA, (2) IAC, (3) ULL
PP 017053
Observational hints of radial migration in disc galaxies from CALIFA
(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
PP 017052
Search for rings and satellites around the exoplanet CoRoT-9b using Spitzer photometry
(1) IAC, ULL
PP 017051
A deeper view of the CoRoT-9 planetary system. A small non-zero eccentricity for CoRoT-9b likely generated by planet-planet scattering
Alonso, Deeg: IAC, ULL
PP 017049
A comparison between the soft X-ray and [O III] morphologies of active galactic nuclei
(1) Dark Cosmology Centre, (2) IRyA-UNAM, (3) IAC, (4) ULL, (5) UCM
PP 017048
Analysis of the Amplitude of the Sunyaev-Zel'dovich Effect out to Redshift z=0.8
(1) IAC & ULL
PP 017046
DeepVel: deep learning for the estimation of horizontal velocities at the solar surface
Instituto de Astrofísica de Canarias
PP 017045
Hints on the gradual re-sizing of the torus in AGN by decomposing IRS/Spitzer spectra
(1) CRyA, (2) IAA, (3) UCM, (4) IAC, (5) ULL, (6) CAB, (7) INAOE
PP 017044
The Correlation Between Mixing Length and Metallicity on the Giant Branch: Implications for Ages in the Gaia Era
Several institutions from USA and Europe (including IAC and ULL)
PP 017043
Triple system HD 201433 with a SPB star component seen by BRITE-Constellation: Pulsation, differential rotation, and angular momentum transfer
1 Institute for Astrophysics, University of Vienna, Türkenschanzstrasse 17, 1180 Vienna, Austria
2 Laboratoire AIM, CEA/DRF CNRS - Université Denis Diderot IRFU/SAp, 91191 Gif-sur-Yvette Cedex, France
3 Instituto de Astrofísica de Canarias, E-38200 La Laguna, Tenerife, Spain
4 Departamento de Astrofísica, Universidad de La Laguna, E-38206 La Laguna, Tenerife, Spain
5 Instytut Astronomiczny, Uniwersytet Wrocławski, Kopernika 11, 51-622 Wrocław, Poland
6 Institut für Kommunnikationsnetze und Satellitenkommunikation, Technical University Graz, Inffeldgasse 12, 8010 Graz, Austria
7 Instituut voor Sterrenkunde, K.U. Leuven, Celestijnenlaan 200D, 3001 Leuven, Belgium
8 Institute of Astronomy, Russian Academy of Sciences, Pyatnitskaya 48, 119017 Moscow, Russia
9 Special Astrophysical Observatory, Russian Academy of Sciences, 369167, Nizhnii Arkhyz, Russia
10 Nicolaus Copernicus Astronomical Center, ul. Bartycka 18, 00-716 Warsaw, Poland
11 Department of Physics and Astronomy, University of British Columbia, Vancouver, BC V6T1Z1, Canada
12 Département de physique and Centre de Recherche en Astrophysique du Québec (CRAQ), Université de Montréal, CP 6128, Succ.
Centre-Ville, Montréal, Québec, H3C 3J7, Canada
13 Institute of Automatic Control, Silesian University of Technology, Akademicka 16, 44-100 Gliwice, Poland
14 Department of Astronomy & Astrophysics, University of Toronto, 50 St. George Street, Toronto, Ontario, M5S 3H4, Canada
15 Department of Physics, Royal Military College of Canada, PO Box 17000, Station Forces, Kingston, Ontario, K7K 7B4, Canada
16 Institut für Astro- und Teilchenphysik, Universität Innsbruck, Technikerstrasse 25/8, 6020 Innsbruck, Austria
PP 017042
Identification of Near-Infrared [Se III] and [Kr VI] Emission Lines in Planetary Nebulae
(1) U. of West Georgia, USA, (2) IAC, Spain, (3) ULL, Spain, (4) IAA, Germany, (5) IA-UNAM, Mexico (6) U. Michigan, USA, (7) JINA-CEE, USA
PP 017041
Multi-filter transit observations of HAT-P-3b and TrES-3b with multiple Northern Hemisphere telescopes
(1) Instituto de Astrofísica de Canarias, (2) Universidad de La Laguna, Departamento de Astrofísica, (3) Observatorio Astronómico Nacional, Instituto de Astronomía (Universidad Nacional Autónoma de México, (4) Departamento de Física y Matemáticas (Universidad de Monterrey), (5) Instituto Nacional de Astrofísica, (6) SUPA, School of Physics and Astronomy, University of St Andrews, (7) Facultad de Ciencias Físico-Matemáticas, Puebla, (8) Dipartimento di Informatica, Bioingegneria, Robotica e Ingegneria dei Sistemi (DIBRIS), Universitá di Genova, (9) Universitá degli Studi dell'Insubria, (10) INAF-Osservatorio Astronomico di Brera, (11) Dipartimento di Fisica, Universitá degli studi di Genova, (12) Istituto Nazionale di Fisica Nucleare, (13) Dipartimento di Fisica, Universitá degli Studi di Trieste, (14) Kitt Peak National Observatory, (15) Observatorio Nacional MCTIC.
PP 017040
The infrared to X-ray correlation spectra of unobscured type 1 active galactic nuclei
(1) IAC, (2) ULL, (3) Durham University, (4) California Institute of Technology
PP 017039
SWEET-Cat update and FASMA. A new minimization procedure for stellar parameters using high-quality spectra
(1) Instituto de Astrofísica e Ciências do Espaço, Universidade do Porto, CAUP, Rua das Estrelas, 4150-762 Porto, Portugal
(2) Departamento de Física e Astronomia, Faculdade de Ciências, Universidade do Porto, Rua Campo Alegre, 4169-007 Porto, Portugal
(3) Instituto de Radioastronomía y Astrofísica, IRyA, UNAM, Campus Morelia, A.P. 3-72, 58089 Michoacán, Mexico
(4) Centre for Exoplanet Science, SUPA, School of Physics and Astronomy, University of St Andrews, St Andrews KY16 9SS, UKSUPA, School of Physics and Astronomy, University of St Andrews, St Andrews KY16 9SS, UK
(5) Depto. Astrofísica, Universidad de La Laguna (ULL), E-38206 La Laguna, Tenerife, Spain
(6) Instituto de Astrofísica de Canarias, E-38205 La Laguna, Tenerife, Spain
PP 017038
Characterisation of the radial velocity signal induced by rotation in late-type dwarfs
(1) IAC, (2) UniGe, (3) INAF
PP 017037
Lithium abundance and rotation of seismic solar analogues - Solar and stellar connection from Kepler and Hermes observations
1 Laboratoire AIM, CEA/DRF - CNRS - Univ. Paris Diderot - IRFU/SAp, Centre de Saclay, 91191 Gif-sur-Yvette Cedex, France e-mail: paul.beck@cea.fr
2 Departamento de Física, Universidade Federal do Rio Grande do Norte, 59072-970 Natal, RN, Brazil
3 Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, USA
4 Instituut voor Sterrenkunde, KU Leuven, B-3001 Leuven, Belgium
5 Space Science Institute, 4750 Walnut street Suite 205, Boulder, CO 80301, USA
6 Instituto de Astrofísica de Canarias, E-38200 La Laguna, Tenerife, Spain
7 Departamento de Astrofísica, Universidad de La Laguna, E-38206 La Laguna, Tenerife, Spain
8 High Altitude Observatory, National Center for Atmospheric Research, P.O. Box 3000, Boulder, CO 80307-3000, USA
9 Department of Physics, Montana State University, Bozeman, MT 59717-3840, USA
10 Dpto. Astrofísica, Facultad de CC. Físicas, Universidad Complutense de Madrid, E-28040 Madrid, Spain
11 Laboratoire Lagrange, Université de Nice Sophia-Antipolis, UMR 7293, CNRS, Observatoire de la Côte d’Azur, Nice, France
12 Stellar Astrophysics Centre, Aarhus University, Ny Munkegade 120, 8000 Aarhus C, Denmark
PP 017036
Spin alignment of stars in old open clusters
1 Laboratoire AIM Paris-Saclay, CEA/DRF — CNRS — Universite ́ Paris Diderot, IRFU/SAp Centre de Saclay, F-91191 Gif-sur-Yvette Cedex, France
2 Instituto de Astrof ́ısica de Canarias, E-38200 La Laguna, Tenerife, Spain
3 Departamento de Astrof ́ısica, Universidad de La Laguna, E-38205 La Laguna, Tenerife, Spain
4 INAF - Osservatorio Astrofisico di Catania, Via S. Sofia 78, I-95123 Catania, Italy
5 Space Science Institute, 4750 Walnut street Suite 205, Boulder, CO 80301, USA
6 Sydney Institute for Astronomy (SIfA), School of Physics, University of Sydney, Sydney, New South Wales 2006, Australia
7 Stellar Astrophysics Centre, Department of Physics and Astronomy, Aarhus University, Ny Munkegade 120, DK-8000 Aarhus C, Denmark
8 Universite ́ Grenoble Alpes, IPAG, F-38000 Grenoble, France; CNRS, IPAG, F-38000 Grenoble, France
PP 017035
Uncovering the host galaxy of the gamma-ray emitting narrow-line Seyfert 1 galaxy FBQS J1644+2619
(1) INAF-Istituto di Radioastronomia, (2) IAC, (3) ULL, (4) INAF-Osservatorio Astrofisico di Torino, (5) University of Southampton
PP 017034
The GTC exoplanet transit spectroscopy survey. VII. Detection of sodium in WASP-52b's cloudy atmosphere
(1) IAC, (2) ULL, (3) PMO
PP 017033
Links between quasi-periodic oscillations and accretion states in neutron star low mass X-ray binaries
(1) Oxford, (2) University of Amsterdam, (3) ESAC-Madrid, (4) IAC, (5) ULL, (6) University of Cagliari
PP 017032
The long-period binary central stars of the planetary nebulae NGC 1514 and LoTr 5
(1) IAC, (2) ULL, (3) KU Leuven, (4) Univ. de Valparaiso, (5) ESAC, (6) ISDEFE, (7) Macquarie University, (8) AAARC Macquarie University
PP 017031
The GTC exoplanet transit spectroscopy survey. V. A spectrally-resolved Rayleigh scattering slope in GJ 3470b
(1) IAC, (2) ULL, (3) PMO, (4) Thüringer Landessternwarte Tautenburg, (5) Visiting scientist at IAC
PP 017030
Physical Properties of superbubbles in the Antennae Galaxies
1. IAC. 2. ULL 3. Instituto de Astronomía, UNAM, 4. CSIC 5. Instituto de Ciencias Nucleares, UNAM.
PP 017029
The VLT-FLAMES Tarantula Survey XXVI: Properties of the O-dwarf population in 30 Doradus
(1) Universidad de La Serena, (2) IAC-ULL
PP 017028
Kepler sheds new and unprecedented light on the variability of a blue supergiant: gravity waves in the O9.5Iab star HD 188209
(1) KULeuven
(2) IAC, ULL
PP 017027
First Detection of Sign-reversed Linear Polarization from the Forbidden [OI] 630.03 nm Line
(1) High Altitude Observatory, (2) IAC
PP 017026
Swift and SALT observations of the Multiple Outbursts of MAXI J1957+032
(1) Instituto de Astrofísica de Canarias, (2) Universidad de La Laguna, (3) University of Southampton, (4) South African Astronomical Observatory, (5) INAR-Osservatorio Astronomico di Roma
PP 017025
Search for exoplanets around pulsating stars of A-F type in Kepler Short Cadence data and the case of KIC 8197761
(1) Astronomical Observatory of the Jagiellonian University, Poland, (2) NCAC, Poland, (3) IAC, (4) ULL, (5) KU Leuven
PP 017024
AGB and SAGB stars: modelling dust production at solar metallicity
(1) IAC-ULL; (2) OAR; (3) DMF-Roma Tre
PP 017023
The JCMT Nearby Galaxies Legacy Survey -- XI. -- Environmental Variations in the Atomic and Molecular Gas Radial Profiles of Nearby Spiral Galaxies
Various
PP 017022
Adapting astronomical source detection software to help detect animals in thermal images obtained by unmanned aerial systems
LJMU, IAC, ULL
PP 017019
The dusty tori of nearby QSOs as constrained by high-resolution mid-IR observations
(1) INAOE, (2) CRyA, (3) CAB, (4) NASA/SOFIA, (5) IAC, (6) ULL
PP 017018
Primeval very low-mass stars and brown dwarfs - II. The most metal-poor substellar object
(1) Instituto de Astrofisica de Canarias, E-38205 La Laguna, Tenerife, Spain;
(2) Universidad de La Laguna, Dept. Astrofisica, E-38206 La Laguna, Tenerife, Spain;
(3) Zentrumfur Astronomie der Universitat Heidelberg, Landessternwarte Konigstuhl 12, D-69117 Heidelberg, Germany;
(4) Centre for Astrophysics Research, Science and Technology Research Institute, University of Hertfordshire, Hatfield AL10 9AB, UK;
(5) Univ Lyon, ENS de Lyon, Univ Lyon 1, CNRS, Centre de Recherche Astrophysique de Lyon UMR5574, F-69007, Lyon, France;
(6) Main Astronomical Observatory, Academy of Sciences of the Ukraine, Golosiiv Woods, 03680 Kyiv-127, Ukraine.
PP 017017
Absence of an X-shaped Structure in the Milky Way Bulge Using Mira Variable Stars
IAC, ULL
PP 017016
Kinematic clues to bar evolution for galaxies in the local universe: why the fastest rotating bars are rotating most slowly
1. IAC 2. Universidad de La Laguna 3. Consejo Superior de Investigaciones Científicas 4.Liverpool John Moores University (UK) 5. University of Oulu (Finland)6.Instituto de Astronomía, UNAM, Ensenada (México), 7. Observatoire de Marseille (France).
PP 017015
EPIC 218916923 b: a low-mass warm Jupiter on a 29-day orbit transiting an active K0 V star
Several institutions from Europe and USA (including IAC and ULL)
PP 017013
Dynamical Study of the Exoplanet Host Binary System HD 106515
(1) Astronomical Federation of Extremadura, C/José Martínez Ruíz Azorín, 14, 4° D, Mérida E-06800, Spain
(2) IAC
(3) ULL
(4) Grupo de Observadores Astronómicos de Tenerife (GOAT), SPAIN
(5) La Palma Astronomical Society, Breña Baja E-38712, Spain
PP 017011
Laboratory and telescope demonstration of the TP3-WFS for the adaptive optics segment of AOLI
(1) Departamento de Electrónica y Tecnología de Computadoras, Universidad Politécnica de Cartagena, (2) Instituto de Astrofísica de Canarias, (3) Departamento de Astrofísica, Universidad de La Laguna, (4) Departamento de Ingenieria Industrial, Universidad de La Laguna, (5) Wooptix S.L., (6) Consejo Superior de Investigaciones Científicas, (7) W. M. Keck Observatory, (8) Institute of Astronomy, University of Cambridge, (9) I. Physikalisches nstitut, Universität zu Köln, (10) Departamento de Física Aplicada, Universidad Politécnica de Cartagena, (11) Centro de Investigaciones Biomédicas de Canarias.
PP 017010
Uncertainties in the solar photospheric oxygen abundance
(1) Instituto de Astrofísica de Canarias (IAC), Avda Vía Láctea S/N, 38200 La Laguna, Tenerife, Spain
(2) Departamento de Astrofísica, Universidad de La Laguna, 38205 La Laguna, Tenerife, Spain
PP 017009
Evidence for a White-light Flare on 10 September 1886
(1) Departamento de Física, Universidad de Extremadura, Mérida, Spain, (2) Instituto Universitario de Investigación del Agua, Cambio Climático y Sostenibilidad (IACYS), Universidad de Extremadura, Badajoz, Spain, (3) IAC, (4) Dept. Astrofisica, ULL, Spain
PP 017008
The VLT-FLAMES Tarantula Survey XXIV. Stellar properties of the O-type giants and supergiants in 30 Doradus
(1) Astronomical Institute Anton Pannekoek, Amsterdam University
(2) Argelander-Institut fur Astronomie, Universitat Bonn
(3) UK Astronomy Technology Centre, Royal Observatory Edinburg
(3) Instituto de Astrofisica de Canarias
(4) Universidad de La Laguna
PP 017007
Orientaciones astronómicas en el oppidum oretano del Cerro de las Cabezas (Valdepeñas, Ciudad Real)
(1) IAC, (2) Universidad Autónoma de Madrid
PP 017006
Suzaku spectroscopy of the neutron star transient 4U 1608-52 during its outburst decay.
(1) IAC, (2) ULL, (3) Kyoto University, (4) MAXI Team RIKEN
PP 017005
The deep OB star population in Carina from the VST Photometric H$α$ Survey (VPHAS+)
(1) University of Hertfordsh, (2) IAC, (3) ULL
PP 017004
B field in OB stars (BOB): The outstandingly strong magnetic field in the evolved He-strong star CPD-62 2124
(1) University of Michigan, (2) Argelander-Institut für Astronomie der Universität Bonn, (3), IAC, (4), ULL
PP 017003
A study of the effect of rotational mixing on massive stars evolution: surface abundances of Galactic O7-8 giant stars
(1) LUPM, CNRS and Montpellier University, (2) IAC and La Laguna University, (3) La Serena University, (4) CONICET--UNLP, (5) Geneva Observatory
PP 017002
The puzzling case of the accreting millisecond X-ray pulsar IGR J00291+5934: flaring optical emission during quiescence
(1) INAF-Brera, (2) INAF-Roma, (3) Cagliari University, (4) Palermo University, (5) IAC, (6) CSIC-IEEC Barcelona
PP 017001
Inference of the chromospheric magnetic field orientation in the Ca II 8542 A line fibrils
(1) IAC
(2) ULL
(3) University of Stockholm