Preprints in 2014
PP 014163
3-D Kinematics of the near-IR HH 223 outflow in L723
(1) Departament d’Astronomia i Meteorologia (IEEC-UB), Institut de Ci`encias del Cosmos, U. de Barcelona, Spain
(2) Instituto de Astrof´ısica de Canarias, E-38200 La Laguna, Spain
(3) Departamento de Astrof´ısica, Universidad de La Laguna, E-38205, Tenerife, Spain
(4) GTC Project Office, GRANTECAN S.A. (CALP), E-38712 Bre˜na Baja, La Palma, Spain
PP 014162
Li abundances in F stars: planets, rotation and galactic evolution
(1) Universidade do Porto, (2) IAC and ULL, (3) University of St Andrews
PP 014161
Una hierofanía solar en el santuario ibérico de Castellar (Jaén)
(1) IAC, (2) Universidad de Jaén
PP 014160
Orbital and physical properties of the $σ$ Ori Aa,Ab,B triple system
Several international institutions (including IAC and ULL)
PP 014159
BUBBLY: A method for detecting and characterizing interstellar bubbles using Fabry-Perot spectroscopy
1Instituto de Astrofsica de Canarias, C/Va Lactea s/n, E-38205 La Laguna, Tenerife, Spain
2Department of Astrophysics, University of La Laguna, E-38205 La Laguna, Tenerife, Spain
3CSIC, 2806 Madrid, Spain
4National Observatory of Athens
5Laboratoire d'Astrophysique de Marseille, Aix Marseille Universite, CNRS, F-13388, Marseille, France
PP 014158
The VLT-FLAMES Tarantula Survey XIX. B-type Supergiants - Atmospheric Parameters and Nitrogen Abundances to Investigate the Role of Binarity and the Width of the Main Sequence
Several research institutions in Europe and USA (incl. IAC and ULL)
PP 014157
Chemical abundances of the secondary star in the Neutron star X-ray binary Cygnus X-2
(1) Instituto de Astrofsica de Canarias, E-38205 La Laguna, Tenerife, Spain
(2) Depto. Astrofsica, Universidad de La Laguna (ULL), E-38206 La Laguna, Tenerife, Spain
(3) Consejo Superior de Investigaciones Cientcas, Spain
PP 014156
Discovery of true, likely and possible symbiotic stars in the dwarf spheroidal NGC 205
(1) Observatorio do Valongo (Brazil); (2) Osservatorio di Arcetri (Italia); (3) Instituto de Astrofisica de Canarias (Spain); (4) Universidad de La Laguna (Spain)
PP 014155
A tale of a rich cluster at z∼0.8 as seen by the Star Formation Histories of its ETGs
(1) Subaru Telescope, (2) Universidad Autónoma de Madrid, (3) Instituto de Astrofísica de Canarias, (4) Universidad de La Laguna
PP 014154
A search of diffuse bands in fullerene planetary nebulae: evidence for diffuse circumstellar bands
(1) IAC-ULL; (2) IIA; (3) CSIC; (4) INAF-ACR
PP 014153
Mass spectrometric analysis of selected radiolyzed amino acids in an astrochemical context
C.Cherubini,O. Ursini.-CNR-Istituto di Metodologie Chimiche, Area della Ricerca di
Montelibretti, Via Salaria Km 29.300, 00015 Monterotondo,
RM, Italy
F. Cataldo
Actinium Chemical Research srl, Via Casilina 1626A,
00133 Rome, RM, Italy
S. Iglesias-Groth.-
Instituto de Astrofisica de Canarias, Via Lactea snc, Tenerife,
Canary Islands, Spain
M. E. Crestoni.-Dipartimento di Chimica e Tecnologie del Farmaco, Universita
`
di Roma Sapienza, P. le A. Moro 5, 00185 Rome, RM,Italy
PP 014152
The pillars of the Earth and the Sky: Capital cities, astronomy and landscape
(1)Instituto de Astrofísica de Canarias and Universidad de La Laguna, Tenerife, Spain.
(2)Instituto de Ciencias del Patrimonio, Incipit, CSIC, Santiago de Compostela, Spain.
PP 014151
B fields in OB stars (BOB): on the detection of weak magnetic fields in the two early B-type stars beta CMa and epsilon CMa
(1) AIfA, Univ. Bonn, (2) IAC, (3) ULL among others
PP 014150
A Differential Scanning Calorimetric (DSC) Study on Heavy Ozonized C60 Fullerene
Actinium Chemical Research srl, Via Casilina, Rome, Italy;
Università del la Tuscia, Dipartimento di Scienze Ecologiche e Biologiche, Viterbo, Italy
Instituto de Astrofisica de Canarias, Via Láctea sn, Tenerife, Canary Islands, Spain
Departamento de Astrofısica, Universidad de La Laguna (ULL), La Laguna, Spain
PP 014149
LONG TERM STUDY OF FULLERENE C60+• RADICAL CATION BY ELECTRON SPIN RESONANCE (ESR)
[a] Actinium Chemical Research srl, Via Casilina 1626A, 00133
Rome, Italy
[b] INAF – Osservatorio Astrofisico di Catania, Via S. Sofia 78,
95123 Catania, Italy
[c] Instituto de Astrofisica de Canarias, Via Lactea snc, Tenerife
PP 014148
Dissecting galactic bulges in space and time I: the importance of early formation scenarios vs. secular evolution
1Instituto de Astrofísica de Canarias, E-38200 La Laguna, Tenerife, Spain
2Departamento de Astrofísica, Universidad de La Laguna, E-38205 La Laguna, Tenerife, Spain
3Dpto. de Astrofísica y CC. de la Atmósfera, Universidad Complutense de Madrid, Spain
4Dpto. de Física Teórica y del Cosmos, Universidad de Granada, Facultad de Ciencias (Edificio Mecenas), 18071 Granada, Spain 5Instituto Universitario Carlos I de Física Teórica y Computacional, Universidad de Granada, 18071 Granada, Spain
6Dpto. de Física Teórica, Universidad Autónoma de Madrid, E-28049 Cantoblanco, Spain
7Research School of Astronomy and Astrophysics, Australian National University, Canberra, ACT 2611, Australia 8Max-Planck-Institut für Astronomie, Königstuhl 17, D-69117 Heidelberg, Germany
9European Southern Observatory, Karl-Schwarzschild-Str. 2, 85748 Garching, Germany
PP 014147
Composite Bulges: The Coexistence of Classical Bulges and Disky Pseudobulges in S0 and Spiral Galaxies
(1) Max-Planck-Institut fuer extraterrestrische Physik, Garching, Germany, (2) Stockholm University, Department of Astronomy, Oskar Klein Centre, SE-10691 Stockholm, Sweden, (3) Instituto de Astrofisica de Canarias, C/ Via Lactea s/n, 38200 La Laguna, Tenerife, Spain)(4) Consejo Superior de Investigaciones Científicas, Spain (5) Universidad de La Laguna, Spain.
PP 014146
The Carina Project VII: Towards the breaking of the age-metallicity degeneracy of red giant branch stars using the c_UBI index
(1) Instituto de Astrofísica de Canarias, Calle Via Lactea s/n, 38205 La Laguna, Tenerife, Spain
(2) Departamento de Astrofísica, Universidad de La Laguna, 38200 La Laguna, Tenerife, Spain
(3) Research School of Astronomy and Astrophysics, The Australian National University, Cotter Road, Weston, ACT, 2611,Australia
(4) Istituto Nazionale di Astrofisica-Osservatorio Astronomico Collurania, Via M. Maggini, 64100 Teramo, Italy.
(5) Dipartimento di Fisica, Universitá di Roma Tor Vergata, Via della Ricerca Scientifica 1, 00133 Rome, Italy
(6) Dominion Astrophysical Observatory, NRC-Herzberg, 5071 West Saanich Road, Victoria, BC V9E 2E7, Canada
(7) Cerro Tololo Inter-American Observatory, National Optical Astronomy Observatory, Casilla 603, La Serena, Chile.
(8) Istituto Nazionale di Astrofisica-Osservatorio Astronomico di Trieste, Via G.B. Tiepolo 11, 40131 Trieste, Italy.
(9) INAF- Osservatorio Astronomico di Capodimonte, Salita Moiariello 16, I - 80131 Napoli, Italy.
(10) Istituto Nazionale di Astrofisica-Osservatorio Astronomico di Roma, Via Frascati 33, Monte Porzio Catone, Rome, Italy.
(11) Université de Nice Sophia-antipolis, CNRS, Observatoire de la Cóte d'Azur, Laboratoire Lagrange, BP 4229,06304 Nice, France.
PP 014145
Planck 2013 results. XXXI. Consistency of the Planck data
1 School of Physics and Astronomy, Cardiff University, Queens Buildings, The Parade, Cardiff, CF24 3AA, UK
2 IAC
3 ULL
PP 014144
Planck 2013 results. XXX. Cosmic infrared background measurements and implications for star formation
1 School of Physics and Astronomy, Cardiff University, Queens Buildings, The Parade, Cardiff, CF24 3AA, UK
2 IAC
3 ULL
4 CSIC
PP 014143
Planck 2013 results. XXIX. The Planck catalogue of Sunyaev-Zeldovich sources⋆
1 School of Physics and Astronomy, Cardiff University, Queens Buildings, The Parade, Cardiff, CF24 3AA, UK
2 IAC
3 ULL
4 CSIC
PP 014142
Planck 2013 results. XXVIII. The Planck Catalogue of Compact Sources
1 School of Physics and Astronomy, Cardiff University, Queens Buildings, The Parade, Cardiff, CF24 3AA, UK
2 IAC
3 ULL
4 CSIC
PP 014141
Planck 2013 results. XXVII. Doppler boosting of the CMB: Eppur si muove⋆
1 Institut d’Astrophysique Spatiale, CNRS, Université Paris-Sud 11, Orsay, France
2 IAC
3 ULL
PP 014140
Planck 2013 results. XXVI. Background geometry and topology of the Universe
1 School of Physics and Astronomy, Cardiff University, Queens Buildings, The Parade, Cardiff, CF24 3AA, UK
2 IAC
3 ULL
4 CSIC
PP 014139
Planck 2013 results. XXV. Searches for cosmic strings and other topological defects
1 School of Physics and Astronomy, Cardiff University, Queens Buildings, The Parade, Cardiff, CF24 3AA, UK
2 IAC
3 ULL
4 CSIC
PP 014138
Planck 2013 results. XXIV. Constraints on primordial non-Gaussianity
1 School of Physics and Astronomy, Cardiff University, Queens Buildings, The Parade, Cardiff, CF24 3AA, UK
2 IAC
3 ULL
4 CSIC
PP 014137
Planck 2013 results. XXIII. Isotropy and statistics of the CMB
1 School of Physics and Astronomy, Cardiff University, Queens Buildings, The Parade, Cardiff, CF24 3AA, UK
2 IAC
3 ULL
4 CSIC
PP 014136
Planck 2013 results. XXII. Constraints on inflation
1 School of Physics and Astronomy, Cardiff University, Queens Buildings, The Parade, Cardiff, CF24 3AA, UK
2 IAC
3 ULL
4 CSIC
PP 014135
Planck 2013 results. XXI. Power spectrum and high-order statistics of the Planck all-sky Compton parameter map
1 School of Physics and Astronomy, Cardiff University, Queens Buildings, The Parade, Cardiff, CF24 3AA, UK
2 IAC
3 ULL
4 CSIC
PP 014134
Planck 2013 results. XX. Cosmology from Sunyaev–Zeldovich cluster counts
1 School of Physics and Astronomy, Cardiff University, Queens Buildings, The Parade, Cardiff, CF24 3AA, UK
2 IAC
3 ULL
4 CSIC
PP 014133
Planck 2013 results. XIX. The integrated Sachs-Wolfe effect
1 School of Physics and Astronomy, Cardiff University, Queens Buildings, The Parade, Cardiff, CF24 3AA, UK
2 IAC
3 ULL
4 CSIC
PP 014132
Planck 2013 results. XVIII. The gravitational lensing-infrared background correlation
1 School of Physics and Astronomy, Cardiff University, Queens Buildings, The Parade, Cardiff, CF24 3AA, UK
2 IAC
3 ULL
4 CSIC
PP 014131
Planck 2013 results. XVII. Gravitational lensing by large-scale structure
1 School of Physics and Astronomy, Cardiff University, Queens Buildings, The Parade, Cardiff, CF24 3AA, UK
2 IAC
3 ULL
4 CSIC
PP 014130
Planck 2013 results. XVI. Cosmological parameters
1 School of Physics and Astronomy, Cardiff University, Queens Buildings, The Parade, Cardiff, CF24 3AA, UK
2 IAC
3 ULL
4 CSIC
PP 014129
Planck 2013 results. XV. CMB power spectra and likelihood
1 School of Physics and Astronomy, Cardiff University, Queens Buildings, The Parade, Cardiff, CF24 3AA, UK
2 IAC
3 ULL
4 CSIC
PP 014128
Planck 2013 results. XIV. Zodiacal emission
1 School of Physics and Astronomy, Cardiff University, Queens Buildings, The Parade, Cardiff, CF24 3AA, UK
2 IAC
3 ULL
4 CSIC
PP 014127
Planck 2013 results. XIII. Galactic CO emission
1 School of Physics and Astronomy, Cardiff University, Queens Buildings, The Parade, Cardiff, CF24 3AA, UK
2 IAC
3 ULL
4 CSIC
PP 014126
Planck 2013 results. XII. Diffuse component separation
1 School of Physics and Astronomy, Cardiff University, Queens Buildings, The Parade, Cardiff, CF24 3AA, UK
2 IAC
3 ULL
4 CSIC
PP 014125
Planck 2013 results. XI. All-sky model of thermal dust emission
1 Institut d’Astrophysique Spatiale, CNRS,Université Paris-Sud 11, Orsay, France
2 IAC
3 ULL
4 CSIC
PP 014124
Planck 2013 results. VI. High Frequency Instrument data processing
1 School of Physics and Astronomy, Cardiff University, Queens Buildings, The Parade, Cardiff, CF24 3AA, UK
2 IAC
3 ULL
4 CSIC
PP 014123
Planck 2013 results. V. LFI calibration
1 Institut d’Astrophysique Spatiale, CNRS (UMR 8617) Université Paris-Sud 11, Orsay, France
2 IAC
3 ULL
4 CSIC
PP 014122
Planck 2013 results. IV. Low Frequency Instrument beams and window functions
1 Institut d’Astrophysique Spatiale, CNRS,Université Paris-Sud 11, Orsay, France
2 IAC
3 ULL
4 CSIC
PP 014121
Planck 2013 results. III. LFI systematic uncertainties
1 Institut d’Astrophysique Spatiale, CNRS (UMR 8617) Université Paris-Sud 11, Bâtiment 121, Orsay, France
2 IAC
3 ULL
4 CSIC
PP 014120
Planck 2013 results. II. Low Frequency Instrument data processing
1 Institut d’Astrophysique Spatiale, CNRS (UMR 8617) Université Paris-Sud 11, Bâtiment 121, 91405 Orsay, France
2 IAC
3 ULL
4 CSIC
PP 014119
Planck 2013 results. I. Overview of products and scientific results
1 School of Physics and Astronomy, Cardiff University, UK
2 IAC
3 ULL
4 CSIC
PP 014118
MID-IR SPECTRA OF TYPE IA SN 2014J IN M82 SPANNING THE FIRST FOUR MONTHS
1 University of Florida, Department of Astronomy, Gainesville, Florida, 32611, USA, telesco@astro.ufl.edu
2 Instituto de Astrofísica de Canarias, C/ Vía Láctea, s/n E38205 La Laguna (Tenerife), Spain
PP 014117
The old, metal-poor, anticentre open cluster Trumpler 5
(1)INAF-Osservatorio Astronomico di Bologna, Italy, (2) Dipartamento di Fisica e Astronomia, Universita di Bologna, Italy, (3) ASI Science Data Center, Italy, (4) Dipartamento di Fisica e Astronomia, Universita di Padova, Italy, (5) INAF-Osservatorio Astronomico di Padova, Italy, (6) IAC, (7) ULL
PP 014116
Optical study of the hyper-luminous X-ray source 2XMM J011942.7+032421
1. Instituto de Astrofísica de Canarias, E-38205 La Laguna, Tenerife, SPAIN
2. Dep. de Astrof\'\i sica, Universidad de la Laguna, E-38206 Tenerife, SPAIN
3. Department of Astronomy and Astrophysics, University of Toronto, Toronto, ON M5S 3H4, Canada
PP 014115
Internal Proper Motions in the Eskimo Nebula
(1)Departamento de Astronomía, UNAM, Ensenada, México. (2) IAC. (3) CSIC (4) ULL
PP 014114
Differences between CO- and calcium triplet-derived velocity dispersions in spiral galaxies: evidence for central star formation?
(1) Universidade Federal de Santa Maria, Brazil; (2) IAC; (3) ULL
PP 014113
Mapping the Interstellar Medium with Near-Infrared Diffuse Interstellar Bands
(1) Johns Hopkins University; (2) New Mexico State University; (3) IAC-ULL; (4) University of Virginia; (5) The Ohio State University; (6) Apache Point Observatory; (7) University of Michigan; (8) The University of Texas at Austin
PP 014112
Chemo-Archaeological Downsizing in a Hierarchical Universe: Impact of a Top Heavy IGIMF
(1) Instituto de Astrofisica de La Plata, (2) Universidad Nacional de La Plata, (3) Consejo Nacional de Investigaciones Cientificas y Tecnicas, (4) PUC Chile, (5) Centro de Astro-Ingenieria PUC Chile, (6) CCT Cordoba, (7) Observatorio Astronomico de Cordoba, (8) IAC, (9) ULL, (10) UNAM
PP 014111
Mass accretion rates from multi-band photometry in the Carina Nebula: the case of Trumpler 14
(1) ESO-Santiago, (2) ESA-Noordwijk, (3) Space Telescope Science Institute, (4) INAF-NA, (5) Supernova Ltd, (6) ESO-Garching, (7) PUC Chile, (8) Millennium Institute of Astrophysics, (9) IAC, (10) ULL
PP 014110
Three-dimensional decomposition of galaxies with bulge and long bar
Instituto de Astrofísica de Canarias (IAC) - Departamento de Astrofísica, Universidad de La Laguna (ULL)
PP 014109
Tracking Advanced Planetary Systems with HARPS-N (TAPAS). I. A multiple planetary system around the red giant star TYC 1422-614-1
(1) Torun Centre for Astronomy; (2) UAM; (3) Pennsylvania State University (4) IAC-ULL
PP 014108
Constraining the shaping mechanism of the Red Rectangle through spectro-polarimetry of its central star
(1) IAC-ULL, (2) Catania University
PP 014107
Hierarchical analysis of the quiet Sun magnetism
Instituto de Astrofísica de Canarias
Departamento de Astrofísica, Universidad de La Laguna
PP 014106
MY Camelopardalis, a very massive merger progenitor
Universidad de Alicante
CSIC/CAB
IAC
ULL
PP 014105
The spectroscopic Hertzsprung-Russell diagram of Galactic massive stars
(1) Argelander-Institut für Astronomie der Universität Bonn
(2) Instituto de Astrofisica de Canarias
(3) Universidad de La Laguna
PP 014104
Spectroscopic confirmation of KOI-1299b: A massive warm Jupiter in a 52-day eccentric orbit transiting a giant star
(1) Heidelberg Univ., (2) IAC/ULL
PP 014103
On the use of the index N2 to derive the metallicity in metal-poor galaxies
(1) Instituto de Astrofisica de Canarias, La Laguna, Tenerife, Spain, (2) Departamento de Astrofisica, Universidad de La Laguna, Tenerife, Spain, (3) Instituto de Astrofisica de Andalucia - CSIC, Granada, Spain
PP 014102
KOI-183b: a half-Jupiter mass planet transiting a very old solar-like star
(1) Heidelberg U. (2) INAF Catania, (3) IAC/ULL
PP 014101
The Spitzer Survey of Stellar Structure in Galaxies (S4G). The Pipeline 5: High-precision stellar masses at 3.6 micron
(1) Max-Planck-Institut fu ̈r Astronomie, Ko ̈nigstuhl 17, D-69117 Heidelberg, Germany
(2) Instituto de Astrof ́ısica de Canarias, Spain
(3) Departamento de Astrof ́ısica, Universidad de La Laguna, Spain
PP 014100
The Cocoon Nebula and its ionizing star: do stellar and nebular abundances agree?
(1) IAC, Tenerife, Spain, (2) Dep. Astrofísica, ULL, tenerife, Spain
PP 014099
Vertical velocities from proper motions of red clump giants
(1) IAC, ULL; (2) Dept. d'Astronomia i Meteorologia, Institut de Ciències del Cosmos, Universitat de Barcelona
PP 014098
The IACOB project: II. On the scatter of O-dwarf spectral type -- effective temperature calibrations
IAC, ULL, ULS, CAB, USM, ROE
PP 014097
Ionized gas kinematics of galaxies in the CALIFA survey. I. Velocity fields, kinematic parameters of the dominant component, and presence of kinematically distinct gaseous systems
(1) Instituto de Astrofísica de Canarias, C/Via Lactea S/N, 38200-La Laguna, Tenerife, Spain
(2) Dept. Astrofísica, Universidad de La Laguna, C/ Astrofísico Francisco Sánchez, E-38205-La Laguna, Tenerife, Spain
(3) Instituto de Astrofísica de Andalucía (CSIC), Glorieta de la Astronomía S/N, 18008 Granada, Spain
(4) European Southern Observatory, Karl-Schwarzschild-Str. 2, D-85748 Garching b. Muenchen, Germany
(5) Leibniz-Institut für Astrophysik Potsdam (AIP), An der Sternwarte 16, 14482, Potsdam, Germany
(6) Max Planck Institute for Astronomy, Königstuhl 17, 69117 Heidelberg, Germany
(7) Instituto de Astronomía, Universidad Nacional Autónoma de Mexico, A.P.70-264,04510, Máxico, D.F.
(8) Centro Astronómico Hispano Alemán de Calar Alto (CSIC-MPG), C/ Jesús Durbán Remón 2-2, 4004 Almería, Spain
(9) School of Physics and Astronomy, University of St Andrews, North Haugh, St Andrews, KY16 9SS, UK
(10) Department of Physics, Royal Military College of Canada, PO Box 17000, Station Forces, Kingston, Ontario, K7K 7B4, Canada
(11) GEPI Observatoire de Paris, CNRS, Université Paris Diderot, Place Jules Janssen, 92190 Meudon, France
(12) University of Vienna, Department of Astrophysics, Türkenschanzstr. 17, 1180 Vienna, Austria
(13) Sydney Institute for Astronomy, School of Physics A28, University of Sydney, NSW 2006, Australia
(14) Departamento de Física Teórica, Universidad Autónoma de Madrid, 28049 Madrid, Spain
(15) Centro de Astrofísica and Faculdade de Ciências, Universidade do Porto, Rua das Estrelas, 4150-762 Porto, Portugal
(16) CEI Campus Moncloa, UCM-UPM, Departamento de Astrofísica y CC. de la Atmósfera, Facultad de CC. Físicas, Universidad
Complutense de Madrid, Avda. Complutense s/n, 28040 Madrid, Spain
(17) Australian Astronomical Observatory, PO Box 915, North Ryde, NSW 1670, Australia
(18) Department of Physics and Astronomy, Macquarie University , NSW 2109, Australia
(19) Astronomical Institute of the Ruhr-University Bochum Universitaetsstr. 150, 44801 Bochum, Germany
PP 014096
An Open Source, Massively Parallel Code for Non-LTE Synthesis and Inversion of Spectral Lines and Zeeman-induced Stokes Profiles
(1) Instituto de Astrofísica de Canarias, (2), Departamento de Astrofísica, Universidad de La Laguna, (3)Institute for Solar Physics, Dept. of Astronomy, Stockholm University, (4)Consejo Superior de Investigaciones Científicas
PP 014095
Chemical tagging of the Ursa Major moving group: A northern selection of FGK stars
(1) UCM, (2) IAC, (3) ULL, (4) TLS, (5) MPS
PP 014093
Two physical regimes for the Giant HII Regions and Giant Molecular Clouds in the Antennae Galaxies
(1) IAC, (2) ULL, (3) CSIC, (4) UNAM
PP 014092
Gaia-ESO Survey: The analysis of high-resolution UVES spectra of FGK-type stars
(1) IAC, (2) ULL, and other European Institutions
PP 014090
A mid-infrared view of the inner parsecs of the Seyfert galaxy Mrk 1066 using CanariCam/GTC
(1) IAC, (2) ULL, (3) GTC
PP 014089
IRAC Near-Infrared Features in the Outer Parts of S4G Galaxies
Spitzer Science Center, IAC & ULL, et al.
PP 014087
SPIDER X - Environmental effects in central and satellite early-type galaxies through the stellar fossil record
INAF - Osservatorio Astronomico di Capodimonte, Italy; Universitat Heidelberg, Zentrum fur Astronomie, Germany; Mullard Space Science Laboratory, UK; INAF-Osservatorio Astrofisico di Arcetri, Italy; Dark Cosmology Center, University of Copenhagen, Denmark; Instituto Nacional de Pesquisas Espaciais, Brazil; Instituto de Astrofisica de Canarias, Spain
PP 014086
Planetary nebulae: the universal mass-metallicity relation for Local Group dwarf galaxies and the chemistry of NGC 205
Observatorio do Valongo, UFRJ, Brazil
Instituto de Astrofisica de Canarias, Spain
Osservatorio Astrofisico di Arcetri, Italy
Institute for Astronomy, Hawaii, USA
PP 014085
Physical conditions derived from OII recombination lines in planetary nebulae and their implications
(1) Instituto Astronomia, UNAM, México, (2) IAC, (3) ULL
PP 014084
The Ratio of Pattern Speeds in Double-Barred Galaxies
1. Instituto de Astrofísica de Canarias, 2.Departamento de Astrofísica de la Universidad de La Laguna 3. CSIC, 4. Department of Astronomy, Stockholm University, 5. Oskar Klein Centre for Cosmoparticle Physics 6. Laboratoire d'Astrophysique, Université d'Aix-Marseille 7. CNRS
PP 014083
The dust masses of powerful radio galaxies: clues to the triggering of their activity
(1)Univ of Sheffield, (2)CEA-Saclay, (3)ASTRON, (4)IAS, (5)IAC, (6)ULL
PP 014082
Rossiter-McLaughlin Observations of 55 Cnc e
CfA-Harvard, MIT, varios (incluye IAC, Dpto Astrofísica ULL)
PP 014081
CoRoT-22 b: a validated 4.9 RE exoplanet in 10-day orbit
LAM, varios (incluye IAC, Dpto Astrofísica ULL)
PP 014080
Revisiting the transits of CoRoT-7b at a lower activity level
LAM, Varios (incluye IAC, Dpto Astrofísica)
PP 014078
Polarized Mid-Infrared Synchrotron Emission in the Core of Cygnus A
(1) UTSA, (2) IAC, (3) ULL, (4) GTC
PP 014077
On the use of the Fourier Transform to determine the projected rotational velocity of line-profile variable B stars
(1) IvS, KULeuven
(2) IMAPP
(3) IAC
(4) ULL
PP 014076
Extended Warm Gas in the ULIRG Mrk273: Galactic Outflows and Tidal Debris
(1) IAC, (2) ULL
PP 014075
Neutron bombardment of single wall carbon nanohorn (SWCNH): DSC determination of the stored Wigner-Szilard energy
F. Cataldo
Istituto Nazionale di Astrofisica – Osservatorio Astrofisica di
Catania, Via S. Sofia 78, 95123 Catania, Italy
&
Actinium Chemical Research, Via Casilina 1626/A,
00133 Rome, Italy;
S. Iglesias-Groth
Instituto de Astrofisica de Canarias, Via Lactea s/n, 38200 La
Laguna, Tenerife, Spain;
Y. Hafez
National Center for Astronomy, KACST, P.O. Box
6086, Riyadh 11442, Saudi Arabia;
G. Angelini
Istituto di Metodologie Chimiche, CNR, Via Salaria Km 29,300,
00016 Monterotondo Stazione, Rome, Italy
PP 014074
Mass spectrometric analysis of selected radiolyzed amino acids in an astrochemical context
C. Cherubini & O. Ursini (CNR-Istituto di Metodologie Chimiche, Area della Ricerca di
Montelibretti, Via Salaria Km 29.300, 00015 Monterotondo,
RM, Italy)
F. Cataldo (Actinium Chemical Research srl, Via Casilina 1626A,
00133 Rome, RM, Italy)
S. Iglesias-Groth
(Instituto de Astrofisica de Canarias, Via Lactea snc, Tenerife,
Canary Islands, Spain)
M. E. Crestoni
(Dipartimento di Chimica e Tecnologie del Farmaco, Universita di Roma Sapienza, P. le A. Moro 5, 00185 Rome, RM, Italy)
PP 014073
Formation of S0 galaxies through mergers
1 Departamento de Astrofísica y CC. de la Atmósfera, Universidad Complutense de Madrid, E-28040 Madrid, Spain
e-mail: asborlaff@ucm.es
2 Max-Planck-Institut für Astronomie, Königstuhl, 17, 69117 Heidelberg, Germany
3 Instituto de Astronomía, Universidad Nacional Autónoma de México, Apdo. 106, Ensenada BC 22800, Mexico
4 Instituto de Astrofísica de Canarias, C/ Vía Láctea, E-38200 La Laguna, Tenerife, Spain
5 Facultad de Física, Universidad de La Laguna, Avda. Astrofísico Fco. Sánchez s/n, 38200, La Laguna, Tenerife, Spain
6 Consejo Superior de Investigaciones Científicas, Spain
PP 014072
The VLT-FLAMES Tarantula Survey XVII. Physical and wind properties of massive stars at the top of the main sequence
Several institutions in Europe and America, including IAC (1) and ULL(2)
PP 014071
Deep spectroscopic luminosity function of Abell 85: no evidence for a steep upturn of the faint-end slope
(1) Instituto de Astrofisica de Canarias, C/ Via Lactea s/n, 38200 La Laguna, Tenerife, Spain,
(2) Departamento de Astrofisica, Universidad de La Laguna, E-38205 La Laguna, Tenerife, Spain,
(3) NRC Herzberg Institute of Astrophysics, 5071 West Saanich Road, Victoria, V9E2E7, Canada
(4) Dipartimento di Fisica, Universit\`a di Torino, Via P. Giuria 1, I-10125, Torino, Italy\\
(5) Istituto Nazionale di Fisica Nucleare (INFN), sezione di Torino, Via P. Giuria 1, I-10125, Torino, Italy\\
(6) Istituto Nazionale di Astrofisica (INAF), Osservatorio Astronomico di Torino, Strada Osservatorio 20, I-10025 Pino Torinese, Torino, Italy\\
(7) School of Physics \& Astronomy, University of St Andrews, St Andrews KY16 9AJ, Fife, Scotland, UK}
PP 014070
The effect of the environment on the stellar mass - size relation of present-day galaxies
(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
PP 014069
Masgomas-04: Physical characterization of a double-core obscured cluster with a massive and very young population
(1) The Millennium Institute of Astrophysics (MAS), Santiago, Chile.
(2) Instituto de Astrofísica, Universidad de Valparaíso, Valparaíso, Chile
(3) Centro de Estudios de F ́ısica del Cosmos de Arago ́n (CEFCA), E-44001, Teruel, Spain.
(4) Instituto de Astrof ́ısica de Canarias, 38205 La Laguna, Tenerife, Spain.
(5) Departamento de Astrof ́ısica, Universidad de La Laguna, E-38205 La Laguna, Tenerife, Spain.
PP 014068
Nuclear 11.3 micron PAH emission in local active galactic nuclei
(1) IFCA, (2) IAC, (3) ULL, (4) CAB
PP 014067
Accurate Atmospheric Parameters at Moderate Resolution Using Spectral Indices: Preliminary Application to the MARVELS Survey
Several institutions in Europe and America, including IAC (1) and ULL(2)
PP 014066
Tracing a high redshift cosmic web with quasar systems
(1)Tartu Observatory, 61602 Tõravere, Estonia,
(2)Instituto de Astrofísica de Canarias, E-38205 La Laguna, Tenerife, Spain,
(3)Universidad de La Laguna, Dept. Astrofísica, E-38206 La Laguna, Tenerife, Spain,
(4)School of Physics, Korea Institute for Advanced Study, 85 Hoegiro, Dong-Dae-Mun-Gu, Seoul 130-722, Korea,
(5)Tuorla Observatory, University of Turku, Väisäläntie 20, Piikkiö, Finland,
(6)Estonian Academy of Sciences, EE-10130 Tallinn, Estonia,
(7)Institute of Physics, Tartu University, Tähe 4, 51010 Tartu, Estonia,
(8)ICRANet, Piazza della Repubblica 10, 65122 Pescara, Italy
PP 014065
Near- to Mid-infrared Imaging and Spectroscopy of Two Buried AGNs of the Nearby Merging Galaxy NGC 6240 with Subaru/IRCS+AO and GTC/CanariCam
(1) The University of Tokyo, (2) Subaru Telescope, (3) IFCA, (4) UTSA, (5) IAC, (6) ULL, (7) Universidad Andrés Bello
PP 014064
SOPHIE velocimetry of $\textit{Kepler}$ transit candidates XII. KOI-1257 b: a highly-eccentric 3-month period transiting exoplanet
CAUP, LAM, IAP, ... (incluye IAC y Dtpo. Astrofísica)
PP 014063
Transiting exoplanets from the CoRoT space mission: XXVI. CoRoT-24: A transiting multi-planet system
IAC, Dpto Astrofísica, Obs. Genève, LAM, ... (+23 institutions)
PP 014062
Recent activity of the Be/X-ray binary system SAXJ2103.5+4545
(1) IEEC-CSIC, Spain, (2) IAC, Spain, (3) ULL, Spain, (4) VIU, Spain, (5) IAA-CSIC, Spain (6) Middle East Technical University, Turkey, (7) Obs. Astron. U. Valencia, Spain, (8) NOT, Spain, (9) Stockholm University, Sweden, (10) Süleyman Demirel University, Turkey, (11) Czech Technical University, Czech Republic
PP 014061
Carbon and oxygen abundances from recombination lines in low-metallicity star-forming galaxies. Implications for chemical evolution
(1) IAC, (2) Depto. Astrofísica ULL, (3) Instituto de Astronomía UNAM , (4) IfA U. Hawaii, (5) AAT, (6) Instituto de Astrofísica PUC
PP 014060
The Gaia-ESO Survey: metallicity of the Chamaeleon I star forming region
Several institutions in Europe, including IAC (1) and ULL(2)
PP 014059
SACRED ARCHITECTURE ORIENTATION ACROSS THE MEDITERRANEAN: A COMPARATIVE STATISTICAL ANALYSIS
(1) Heritage Sciences Institute, Incipit, Spanish National Research Council –CSIC, Rúa San Roque 2, Santiago, SPAIN
(2) Instituto de Astrofísica de Canarias and Astrophysics Department, University of La laguna, Calle Vía Láctea s/n, La Laguna, Tenerife, SPAIN
PP 014058
Flare in the Galactic stellar outer disc detected in SDSS-SEGUE data
(1) IAC, ULL; (2) GRANTECAN
PP 014057
Molecular line emission in NGC1068 imaged with ALMA. I An AGN-driven outflow in the dense molecular gas
(1) OAN, (2) IAC, (3) ULL
PP 014056
Characterizing the Purple Earth: Modeling the Globally Integrated Spectral Variability of the Archean Earth
AA(Instituto de Astrofísica de Canarias (IAC), Vía Láctea s/n E-38200, La Laguna, Spain ; Departamento de Astrofísica, Universidad de La Laguna, E-38206 La Laguna, Spain; mesr@iac.es), AB(Instituto de Astrofísica de Canarias (IAC), Vía Láctea s/n E-38200, La Laguna, Spain ; Departamento de Astrofísica, Universidad de La Laguna, E-38206 La Laguna, Spain), AC(NASA Ames Research Center, Exobiology Branch, Mountain View, CA 94035, USA ; SETI Institute, Mountain View, CA 94035, USA), AD(NASA Goddard Institute for Space Studies, New York, NY 10025, USA), AE(Department of Microbiology, Faculty of Biology, University of La Laguna, ES-38206 La Laguna, Spain), AF(Instituto de Astrofísica de Canarias (IAC), Vía Láctea s/n E-38200, La Laguna, Spain ; Departamento de Astrofísica, Universidad de La Laguna, E-38206 La Laguna, Spain), AG(Instituto de Astrofísica de Canarias (IAC), Vía Láctea s/n E-38200, La Laguna, Spain ; Departamento de Astrofísica, Universidad de La Laguna, E-38206 La Laguna, Spain)
PP 014055
Simultaneous optical and near-infrared linear spectropolarimetry of the earthshine
AA(Instituto de Astrofísica de Canarias, 38205, La Laguna, Spain pamp@iac.es; Departamento de Astrofísica, Universidad de La Laguna, Av. Astrofísico Francisco Sánchez, s/n, 38206, La Laguna, Spain), AB(Instituto de Astrofísica de Canarias, 38205, La Laguna, Spain epalle@iac.es; Departamento de Astrofísica, Universidad de La Laguna, Av. Astrofísico Francisco Sánchez, s/n, 38206, La Laguna, Spain), AC(Centro de Astrobiología (CSIC-INTA), Carretera de Ajalvir km 4, 28850 Torrejón de Ardoz, Madrid, Spain mosorio@cab.inta-csic.es)
PP 014054
The GTC exoplanet transit spectroscopy survey I: OSIRIS transmission spectroscopy of the short period planet WASP-43b
Instituto de Astrofísica de Canarias (IAC), E-38205 La Laguna, Tenerife, Spain
e-mail: murgas_ext@iac.es
2 Departamento de Astrofísica, Universidad de La Laguna (ULL), E-38206 La Laguna, Tenerife, Spain
3 Centro de Astrobiología (CSIC-INTA), E-28850 Torrejón de Ardoz, Madrid, Spain
4
Institut für Astrophysik, Georg-August-Universität, Friederich-Hund-Platz 1, D-37077 Göttingen, Germany
PP 014053
WTS-2 b: a hot Jupiter orbiting near its tidal destruction radius around a K dwarf
AA(Leiden Observatory, Leiden University, Niels Bohrweg 2, NL-2333 CA Leiden, the Netherlands birkby@strw.leidenuniv.nl), AB(Max-Planck-Institut für extraterrestrische Physik, Giessenbachstrasse, D-85741 Garching, Germany), AC(Depto. Astrofísica, Centro de Astrobiología (INTA-CSIC), ESAC Campus, PO Box 78, E-28691 Villanueva de la Cañada, Spain), AD(Max-Planck-Institut für extraterrestrische Physik, Giessenbachstrasse, D-85741 Garching, Germany; Universitatssternwarte, Scheinerstrasse 1, D-81679 Munchen, Germany), AE(Main Astronomical Observatory of Ukrainian Academy of Sciences, Golosiiv Woods, Kyiv-127, UA-03680, Ukraine), AF(Departamento de Física Teórica, Facultad de Ciencias, Universidad Autónoma de Madrid, Cantoblanco, E-28049 Madrid, Spain; Lund Observatory, Department of Astronomy and Theoretical Physics, Lund University, Box 43, SE-221 00 Lund, Sweden), AG(Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge CB3 0HA, UK), AH(Centre for Astrophysics Research, University of Hertfordshire, College Lane, Hatfield, Hertfordshire AL10 9AB, UK), AI(Centre for Astrophysics Research, University of Hertfordshire, College Lane, Hatfield, Hertfordshire AL10 9AB, UK), AJ(Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge CB3 0HA, UK), AK(Max-Planck-Institut für extraterrestrische Physik, Giessenbachstrasse, D-85741 Garching, Germany; Universitatssternwarte, Scheinerstrasse 1, D-81679 Munchen, Germany), AL(Main Astronomical Observatory of Ukrainian Academy of Sciences, Golosiiv Woods, Kyiv-127, UA-03680, Ukraine; Centre for Astrophysics Research, University of Hertfordshire, College Lane, Hatfield, Hertfordshire AL10 9AB, UK), AM(Depto. Astrofísica, Centro de Astrobiología (INTA-CSIC), ESAC Campus, PO Box 78, E-28691 Villanueva de la Cañada, Spain), AN(European Southern Observatory, Alonso de Córdova 3107, Vitacura, Santiago, Chile; Max Planck Institut für Astronomie, Königstuhl 17, D-69117 Heidelberg, Germany), AO(Centre for Astrophysics Research, University of Hertfordshire, College Lane, Hatfield, Hertfordshire AL10 9AB, UK), AP(Centre for Astrophysics Research, University of Hertfordshire, College Lane, Hatfield, Hertfordshire AL10 9AB, UK; Department of Physics, University of Warwick, Gibbet Hill Rd, Coventry CV4 7AL, UK), AQ(Department of Physical Sciences, The Open University, Walton Hall, Milton Keynes MK7 6AA, UK), AR(Centro de Astrobiología (CSIC-INTA). Crta, Ajalvir km 4, E-28850 Torrejón de Ardoz, Madrid, Spain), AS(Leiden Observatory, Leiden University, Niels Bohrweg 2, NL-2333 CA Leiden, the Netherlands), AT(Depto. Astrofísica, Centro de Astrobiología (INTA-CSIC), ESAC Campus, PO Box 78, E-28691 Villanueva de la Cañada, Spain), AU(Centro de Astrobiología (CSIC-INTA). Crta, Ajalvir km 4, E-28850 Torrejón de Ardoz, Madrid, Spain), AV(Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge CB3 0HA, UK), AW(Department of Astronomy and Astrophysics, University of Toronto, 50 St. George Street, Toronto, ON M5S 3H4, Canada), AX(Leiden Observatory, Leiden University, Niels Bohrweg 2, NL-2333 CA Leiden, the Netherlands), AY(Leiden Observatory, Leiden University, Niels Bohrweg 2, NL-2333 CA Leiden, the Netherlands), AZ(Depto. Astrofísica, Centro de Astrobiología (INTA-CSIC), ESAC Campus, PO Box 78, E-28691 Villanueva de la Cañada, Spain), BA(Max-Planck-Institut für extraterrestrische Physik, Giessenbachstrasse, D-85741 Garching, Germany), BB(Instituto Nacional de Astrofísica, Óptica y Electrónica, Luis Enrique Erro 1, Sta. Ma. Tonantzintla, Puebla, Mexico), BC(Centre for Astrophysics Research, University of Hertfordshire, College Lane, Hatfield, Hertfordshire AL10 9AB, UK), BD(Centre for Astrophysics Research, University of Hertfordshire, College Lane, Hatfield, Hertfordshire AL10 9AB, UK), BE(Department of Physical Sciences, The Open University, Walton Hall, Milton Keynes MK7 6AA, UK), BF(Main Astronomical Observatory of Ukrainian Academy of Sciences, Golosiiv Woods, Kyiv-127, UA-03680, Ukraine; Instituto Nacional de Astrofísica, Óptica y Electrónica, Luis Enrique Erro 1, Sta. Ma. Tonantzintla, Puebla, Mexico), BG(Instituto de Astrofísica de Canarias, Calle Vía Láctea s/n, E-38200 La Laguna, Tenerife, Spain; Departamento de Astrofísica, Universidad de La Laguna (ULL), E-38205 La Laguna, Tenerife, Spain), BH(Instituto de Astrofísica de Canarias, Calle Vía Láctea s/n, E-38200 La Laguna, Tenerife, Spain), BI(Instituto de Astrofísica de Canarias, Calle Vía Láctea s/n, E-38200 La Laguna, Tenerife, Spain; Departamento de Astrofísica, Universidad de La Laguna (ULL), E-38205 La Laguna, Tenerife, Spain), BJ(Depto. Astrofísica, Centro de Astrobiología (INTA-CSIC), ESAC Campus, PO Box 78, E-28691 Villanueva de la Cañada, Spain; Spanish Virtual Observatory Thematic Network, Spain), BK(Max-Planck-Institut für extraterrestrische Physik, Giessenbachstrasse, D-85741 Garching, Germany), BL(Instituto de Astrofísica de Canarias, Calle Vía Láctea s/n, E-38200 La Laguna, Tenerife, Spain; Departamento de Astrofísica, Universidad de La Laguna (ULL), E-38205 La Laguna, Tenerife, Spain)
PP 014052
The Gaia-ESO Survey: the first abundance determination of the pre-main-sequence cluster Gamma Velorum
Several institutions in Europe, including IAC (1) and ULL(2)
PP 014051
Confirmation of an exoplanet using the transit color signature: Kepler-418b, a blended giant planet in a multiplanet system
(1) Aarhus Univ., (2) IAC, (3) ULL, (4) INAF, (5) Univ. Heidelberg, (6) DLR
PP 014050
Kinematic study of planetary nebulae in NGC6822
(1) IA-UNAM, Mexico, (2) IAC, Spain, (3) ULL, Spain, (4) U. Chile (Chile)
PP 014049
The structure of Abell 1351: a bimodal galaxy cluster with peculiar diffuse radio emission
(1) IAC
(2) DA, ULL
(3) Physics Department (Astronomy Section). Trieste Univ, via Tiepolo 11, I-34143, Trieste, Italy
(4) INAF - Osservatorio Astronomico di Trieste, via Tiepolo 11, I-34143 Trieste, Italy
(5) Fundacion Galileo Galilei - INAF (Telescopio Nazionale Galileo), Rambla J. A. Fernandez Perez 7, E-38712 Brena Baja (La Palma), Spain
(6) INAF, Osservatorio Astronomico di Brera, via E. Bianchi 46, 23807, Merate (LC), Italy
(7) Physics Dep. Milan Univ, via Celoria 16, I-20133, Milan, Italy
(8) IASF-Milano, INAF, via Bassini 15, Milan 20133, Italy
PP 014048
The central parsecs of active galactic nuclei: challenges to the torus
(1) Instituto de Astrofísica de Canarias (IAC), E-38200 La Laguna, Tenerife, Spain
(2) Universidad de La Laguna, Dept. Astrofísica, E-38206 La Laguna, Tenerife, Spain
(3) Max-Planck-Institut für Radioastronomie (MPIfR), Auf dem Hügel 69, D-53121 Bonn, Germany
(4) Max-Planck-Institut für Extraterrestrische Physik, Giessenbachstrasse, D-85748 Garching, Germany
(5) Universitäts-Sternwarte München, Scheinerstrasse 1, D-81679 München, Germany
PP 014047
Star formation sustained by gas accretion
(1) Instituto de Astrofisica de Canarias, Spain, (2) Departamento de Astrofisica, Universidad de La Laguna, (3) IBM Research Division, T.J. Watson Research Center, USA, (4) Department of Physics and Astronomy, Vassar College,USA
PP 014046
An early clear sky record from Eastern Spain: 1837–1879
1. Instítuto de Astrofísica de Canarias
2. Universidad de Extremadura
PP 014045
Sher 25: pulsating but apparently alone
(1) UK Astronomy Technology Centre, Royal Observatory Edinburg
(2) IAC
(3) ULL
PP 014044
Spitzer Mid-IR Spectroscopy of Powerful 2Jy and 3CRR Radio Galaxies. II. AGN Power Indicators and Unification
(1)CEA-Saclay, (2)University of Sheffield, (3)ASTRON, (4)Rochester Institute of Technology, (5)Indian Institute of Astrophysics, (6)IAC, (7)ULL
PP 014043
Satellite galaxies around present-day massive ellipticals
(1) Departamento de Astrofisica, Universidad de La Laguna, E-38205, La
Laguna, Tenerife, Spain
(2) IAC
(3) Institute for Astronomy, University of Edinburgh, Royal Observatory, Edinburgh, EH9 3HJ
PP 014042
A Candidate Massive Black Hole in the Low-metallicity Dwarf Galaxy Pair Mrk 709
(1) National Radio Astronomy Observatory, Charlottesville, VA 22903, USA
(2) Department of Astronomy, University of Michigan, 500 Church Street, Ann Arbor, MI 48109, USA
(3) International Centre for Radio Astronomy Research, Curtin University, GPO Box U1987, Perth, WA 6845, Australia
(4) Instituto de Astrofsica de Canarias (IAC), E-38200 La Laguna, Tenerife, and
Universidad de La Laguna, Dept. Astrofsica, E-38206 La Laguna, Tenerife, Spain
(5) National Radio Astronomy Observatory, Charlottesville, VA 22903, USA
(6) Department of Physics, University of Alberta, CCIS 4-181, Edmonton AB T6G 2E1, Canada
(7) Department of Astronomy, University of Virginia, P.O. Box 400325, Charlottesville, VA 22904-4325, USA
PP 014041
Chemical abundances in Galactic Planetary Nebulae with Spitzer spectra
(1) IAC-ULL; (2) N. Copernicus Astronomical Center
PP 014040
On the origin of stars with and without planets. Tc trends and clues to Galactic evolution
(1) Centro de Astrofísica, Universidade do Porto, Rua das Estrelas, 4150-762 Porto, Portugal
(2) Departamento de Física e Astronomia, Faculdade de Cîencias, Universidade do Porto, Portugal
(3) Instituto de Astrofísica de Canarias, 38200 La Laguna, Tenerife, Spain
(4) Departamento de Astrofísica, Universidad de La Laguna, 38206 La Laguna, Tenerife, Spain
PP 014039
Astrophysical parameters and orbital solution of the peculiar X-ray transient IGR J00370+6122
(1) Departamento de Física, Ingeniería de Sistemas y Teoría de la Señal. Universidad de Alicante
(2) Argelander Institut für Astronomie, Bonn
(3) Instituto de Astrofisica de Canarias
(4) Universidad de La Laguna
(5) Institut d’Estudis Espacials de Catalunya
PP 014038
A fast version of the k-means classification algorithm for astronomical applications
(1) Instituto de Fisica de Cantabria, Santander, Spain, (2) Departamento de Astrofisica, ULL, Spain, (3) IAC
PP 014037
Upper limits to the magnetic field in central stars of planetary nebulae
(1) Instituto de Astrofísica de Canarias
(2) Universidad de La Laguna
(3) Universitá di Catania
PP 014036
Sampling methods for stellar masses and the mmax-Mecl relation in the starburst dwarf galaxy NGC 4214
(1) IAC, (2) ULL, (3) HISKP Bonn, Germany
PP 014035
On the inversion of the scattering polarization and the Hanle effect signals in the hydrogen Lyman-α line
(1) NAOJ, (2) IAC, (3) IRSOL, (4) KIS, (5) AIAS, (6) NIFS, (7) JAXA
PP 014034
Chemical abundances of stars with brown-dwarf companions
(1) Instituto de Astrofísica de Canarias, 38200 La Laguna, Tenerife, Spain
(2) Departamento de Astrofísica, Universidad de La Laguna, 38206 La Laguna, Tenerife, Spain
(3) Centro de Astrofísica, Universidade do Porto, Rua das Estrelas, 4150-762 Porto, Portugal
(4) Departamento de Física e Astronomia, Faculdade de Cîencias, Universidade do Porto, Portugal
(5) Observatoire Astronomique de l?Université de Genève, 51 Ch. des Maillettes, CH-1290 Sauverny, Versoix, Switzerland
(6) European Space Agency, European Space Astronomy Centre, P.O. Box 78, Villanueva de la Cañada, 28691 Madrid, Spain
PP 014033
On the alumina dust production in the winds of O-rich Asymptotic Giant Branch stars
(1) INAF-OAR; (2) Universita Roma "La Sapienza"; (3) IAC-ULL
PP 014032
Determination of the cross-field density structuring in coronal waveguides using the damping of transverse waves
(1) IAC, (2) ULL
PP 014031
Dissecting the Spitzer color-magnitude diagrams of extreme LMC AGB stars
(1) INAF-OAR; (2) Universita Roma "La Sapienza"; (2) IAC-ULL
PP 014030
The GAPS Programme with HARPS-N at TNG. III: The retrograde orbit of HAT-P-18b.
(1) Instituto de Astrof\'isica de Canarias, C/ V\'ia L\'actea, s/n, E38205 - La Laguna (Tenerife), Spain;
(2) Dep. de Astrof\'isica, Universidad de La Laguna, Avda. Astrof\'isico Francisco S\'anchez, s/n 38206 La Laguna, Tenerife, Spain;
(3) INAF -- Osservatorio Astronomico di Capodimonte, via Moiariello, 16, 80131 Naples, Italy;
(4) Max-Planck-Institut f\"ur Astronomie, K\"onigstuhl 17, D-69117 Heidelberg, Germany;
(5) Fundaci\'on Galileo Galilei - INAF, Rambla Jos\'e Ana Fernandez P\'erez, 7 38712 Bre\~na Baja, TF - Spain;
(6) Astrophysics Group, Keele University, Staffordshire,ST5 5BG, UK;
(7) INAF -- Osservatorio Astrofisico di Catania, via S. Sofia 78, 95123 Catania, Italy;
(8) Dipartimento di Fisica e Astronomia Galileo Galilei, Universit\`a di Padova, Vicolo dell'Osservatorio 2, I-35122, Padova, Italy;
(9) INAF -- Osservatorio Astrofisico di Torino, Via Osservatorio 20, I-10025, Pino Torinese, Italy;
(10) INAF -- Osservatorio Astronomico di Brera, Via E. Bianchi 46, 23807, Merate (LC), Italy;
(11) INAF -- Osservatorio Astronomico di Padova, Vicolo dell'Osservatorio 5, 35122 Padova, Italy;
(12) INAF -- Osservatorio Astronomico di Palermo, Piazza del Parlamento, Italy 1, I-90134, Palermo, Italy;
(13) INAF -- IASF Milano, via Bassini 15, I-20133 Milano, Italy;
(14) INAF -- Osservatorio Astronomico di Trieste, Via Tiepolo 11, 34143 Trieste Italy
PP 014029
Evidence of parsec-scale jets in Low-luminosity Active Galactic Nuclei
(1) Instituto de Astrofísica de Canarias
PP 014028
Rayleigh-Taylor instability in partially ionized compressible plasmas; one fluid approach
IAC
PP 014027
Rayleigh-Taylor instability in prominences from numerical simulations including partial ionization effects
IAC
PP 014026
Observations and Implications of Large-Amplitude Longitudinal Oscillations in a Solar Filament
(1) IAC, (2) ULL, (3) The Johns Hopkins University, (4) NASA, (5) ARTEP, (6) CUA
PP 014025
The transfer of resonance line polarization with partial frequency redistribution and J-state interference
IAC
PP 014024
A Key Physical Mechanism for Understanding the Enigmatic Linear Polarization of the Solar Ba II and Na I D1 Lines
IAC
PP 014023
PORTA: A three-dimensional multilevel radiative transfer code for modeling the intensity and polarization of spectral lines with massively parallel computers
ASCR and IAC
PP 014021
Circumstellar effects on the Rb abundances in O-rich AGB stars
(1): IAC-ULL; (2): LUPM; (3): CSIC
PP 014020
Photometric decomposition of mergers in disk galaxies
(1) Instituto de Astrofísica de Canarias (IAC), E-38200 La Laguna, Tenerife, Spain; (2) Universidad de La Laguna, Dept. Astrofísica, E-38206 La Laguna, Tenerife, Spain; (3) Max Planck Institute for Radio Astronomy, Auf dem Hügel 69, D-53121 Bonn, Germany; (4) Institut für Experimentalphysik, Universität Hamburg, Luruper Chausse 149, D-22761 Hamburg, Germany; (5) Center for the Exploration of the Origin of the Universe, Seoul National University, Seoul 151-742, Korea
PP 014019
Revealing the nature of the ULX and X-ray population of the spiral galaxy NGC 4088
(1) IAC, (2) Universidad de La Laguna, (3) Harvard-Smithsonian Center for Astrophysics, (4)Department of Physics, University of Alberta, Canada, (5) Sydney Institute for Astronomy, The University of Sydney, Australia, (6) International Centre for Radio Astronomy Research, Curtin University, Australia
PP 014018
The VLT-FLAMES Tarantula Survey XIV. The O-Type Stellar Content of 30 Doradus
(1) STSci, (2) IAC, (3) ULL
PP 014017
The Trace of the CNO Cycle in the Ring Nebula NGC6888
(1) Instituto de Astrofísica, Pontificia Univ. Católica de Chile, (2) IAC, (3) Depto. de Astrofísica, ULL, (4) Instituto de Astronomía, UNAM, (5) Institute for Astronomy, Univ. of Hawaii
PP 014016
Does the diurnal temperature range respond to changes in the cosmic ray flux?
(1) IAC, (2) Hvar Observatory
PP 014015
Satellite-detected Carbon Monoxide pollution during 2000--2012: Examining global trends and also regional anthropogenic periods over China, the EU and the USA, Climate
(1) IAC
PP 014012
The VLT-FLAMES Tarantula Survey XVI. The optical+NIR extinction laws in 30 Doradus and the photometric determination of the effective temperatures of OB stars
IAA-CSIC + various institutions in Europe, USA and Chile, including IAC and ULL
PP 014011
Composite analysis with Monte Carlo methods: an example with cosmic rays and clouds
IAC, Hvar Observatory
PP 014009
La rotación y el transporte de momento en plasmas astrofísicos y de laboratorio
(1)CIEMAT-Laboratorio Nacional de Fusión, avda. Complutense 40, 28040 Madrid,
(2) IAC
PP 014008
Investigating the sensitivity of observed spectral energy distributions to clumpy torus properties in Seyfert galaxies
(1) IAC, (2) ULL, (3) IFCA, (4) Gemini Observatory, (5) UTSA, (6) INAOE
PP 014007
Clear evidence for the early triggering of a luminous quasar-like AGN in a major, gas rich merger
(1) University of Sheffield, (2) IAC, (3) ULL, (4) CAB
PP 014006
The spotty donor star in the X-ray transient Cen X-4
(1,2) IAC, University of La Laguna, Spain, (3) Queens University Belfast, UK (4) University of Sheffield, UK
PP 014005
A search for magnetic fields on central stars in planetary nebulae
(1) Università di Catania, Dipartimento di Fisica e Astronomia
(2) Instituto de Astrofísica de Canarias
(3) Departamento de Astrofísica, Universidad de La Laguna
PP 014004
Improved Hubble Space Telescope Proper Motions for Tycho-G and Other Stars in the Remnant of Tycho's Supernova 1572
(1) INAF, (2) UB-IEEC, (3) IAC, (4) University of California, (5) ING
PP 014003
Transiting exoplanets from the CoRoT space mission XXV. CoRoT-27b: a massive and dense planet on a short-period orbit
(1)IAC/ULL, (2) U. Oxford, (3) ESA/ESTEC, (4) LAM Marseilla
PP 014002
SDSS superclusters: morphology and galaxy content
(1) Tartu Observatory, 61602 Tõravere, Estonia,
(2) Instituto de Astrofísica de Canarias, E-38200 La Laguna, Tenerife, Spain,
(3) Universidad de La Laguna, Dept. Astrofísica, E-38206 La Laguna, Tenerife, Spain,
(4) National Institute of Chemical Physics and Biophysics, Rävala pst 10, Tallinn 10143, Estonia,
(5) Institute of Physics, Tartu University, Tähe 4, 51010 Tartu, Estonia,
(6) Estonian Academy of Sciences, EE-10130 Tallinn, Estonia,
(7) ICRANet, Piazza della Repubblica 10, 65122 Pescara, Italy
PP 014001
Metallicity inhomogeneities in local star-forming galaxies as sign of recent metal-poor gas accretion
((1)
Instituto de Astrofisica de Canarias, La Laguna, Tenerife, Spain, (2)
Departamento de Astrofisica, Universidad de La Laguna, Tenerife, Spain, (3)
Department of Physics and Astronomy, Vassar College, NY, USA, (4) IBM
Research Division, T.J. Watson Research Center, NY, USA, (5) School of
Physics and Astronomy, University of St Andrews, UK)