Preprints in 2015
PP 015123
The Fe/Ni ratio in ionized nebulae: clues on dust depletion patterns
(1) Instituto de Astronomía, UNAM, (2) Instituto de Astrofísica, Pontificia Universidad Católica de Chile, (3) IAC, (4) ULL, (5) INAOE
PP 015122
On the robustness of the pendulum model for large-amplitude longitudinal oscillations in prominences
Instituto de Astrofísica de Canarias, E-38200 La Laguna, Tenerife, Spain
Universidad de La Laguna, Dept. Astrofísica, E-38206 La Laguna, Tenerife, Spain
Departament de Física, Universitat de les Illes Balears (UIB), E-07122 Palma de Mallorca, Spain
Institute of Applied Computing & Community Code (IAC3), UIB, Spain
PP 015121
The number of tidal dwarf satellite galaxies in dependence of bulge index
(1) IAC, (2) ULL, (3) Helmholtz-Institut für Strahlen- und Kernphysik, Universität Bonn, Germany
PP 015120
Red giant masses and ages derived from carbon and nitrogen abundances
Several institutions from USA and Europe (including IAC and ULL)
PP 015119
Discovery of an eclipsing dwarf nova in the ancient nova shell Te 11
(1) SAAO, (2) SALT, (3) UCT, (4) University of Sheffield, (5) ESO, (6) IAC, (7) ULL, (8) UNAM, (9) OAN, (10) CSIC
PP 015118
Globular Cluster Populations: Results Including S4G Late-Type Galaxies
Arizona, IAC, ULL, otros
PP 015117
Clear evidence for the presence of second-generation asymptotic giant branch stars in metal-poor Galactic globular clusters
(1) IAC-ULL; (2) ELTE; (3) INAF-OAT; (4) DAO; (5) UT-McDonald Obs.; (6) INAF-OAP
PP 015116
Charge exchange in fluid description of partially ionized plasmas
(1) IAC, (2) Chuo University Tokyo
PP 015115
High ionisation absorption in low mass X-ray binaries
(1) Max Planck Institut fu ̈r Extraterrestrische Physik (MPE), (2) Universita Roma Tre, (3) IAC, (4) ULL, (5) Oxford Astrophysics
PP 015114
BlackCAT: A catalogue of stellar-mass black holes in X-ray transients
(1) Pontificia Universidad Católica de Chile (IA-PUC)
(2) IAC
(3) ULL
(4) New York University Abu Dhabi
PP 015113
Modelling the spectral energy distribution of the red giant in RS Ophiuchi: evidence for irradiation
(1) Main Astronomical Observatory of the NASU, (2) Center for Astrophysics Research, University of Hertfordshire, (3) Jeremiah Horrocks Institute for Astrophysics and Supercomputing, University of Central Lancashire, (4) Astronomical Observatory of the Romanian Academy of Sciences, (5) Astrophysics Group, Keele University, (6) Minnesota Institute for Astrophysics, School of Physics and Astronomy, (7) Jodrell Bank Centre for Astrophysics, University of Manchester,(8) Instituto de Astrofísica de Canarias, (9) Universidad de La Laguna
PP 015112
NGC 6778: Strengthening the link between extreme abundance discrepancy factors and central star binarity in planetary nebulae
(1) IAC, (2) ULL, (3) ESO.
PP 015111
The PNe and H II regions in NGC6822 revisited. Hints on AGB nucleosynthesis
(1) IAC, Spain, (2) ULL, Spain, (3) IA-UNAM, Mexico, (4) ICN-UNAM, Mexico
PP 015110
HD144548: A young triply eclipsing system in the Upper Scorpius OB association
IAC, Dpto. Astrofísica, U. Berkeley
PP 015109
Fast-to-Alfvén Mode Conversion Mediated by Hall Current. I. Cold Plasma Model
(1) School of Mathematical Sciences and Monash Centre for Astrophysics,
Monash University, Clayton, Victoria 3800, Australia;
(2) Instituto de Astrofísica de Canarias, 38205 La Laguna, Tenerife, Spain;
(3) Departamento de Astrofísica, Universidad de La Laguna, 38205, La Laguna, Tenerife, Spain
PP 015108
Tracing the reverberation lag in the hard state of black hole X-ray binaries
(1) Max-Planck-Institut fur extraterrestrische Physik (MPE)
(2) IAC
(3) ULL
(4) Oxford Astrophysics
PP 015107
A mid-infrared spectroscopic atlas of local active galactic nuclei on sub-arcsecond resolution using GTC/CanariCam
(1) IFCA, (2) UCM, (3) University of Oxford, (4) IAC, (5) ULL
PP 015106
AGB stars in the SMC: evolution and dust properties based on Spitzer observations
(1) INAF-OAR; (2) Universita Roma "La Sapienza"; (3) IAC-ULL
PP 015105
On the Source of Propagating Slow Magneto-acousticWaves in Sunspots
(1) Astrophysics Research Centre, School of Mathematics and Physics, Queen’s University Belfast, Belfast, BT7 1NN, UK;
(2) Department of Physics and Astronomy, California State University Northridge, Northridge, CA, 91330, U.S.A;
(3) Instituto de Astrofisica de Canarias, 38205 La Laguna, Tenerife, Spain.
PP 015104
Evershed flow observed in neutral and singly ionized iron lines
(1) Instituto de Astrofisica de Canarias, 38205 La Laguna, Tenerife, Spain;
(2) Departamento de Astrofisica, ULL, 38205, La Laguna, Tenerife, Spain;
(3) Main Astronomical Observatory, NAS, 03680, Kyiv, Ukraine;
(4) Departament de Fisica, UIB, E-07122 Palma de Mallorca, Spain
PP 015103
Sub-arcsec mid-IR observations of NGC 1614: Nuclear star-formation or an intrinsically X-ray weak AGN?
(1) CAB, (2) IAC, (3) ULL
PP 015102
Bayesian least squares deconvolution
(1) IAC, (2) ULL, (3) Universite de Toulouse, (4) CNRS
PP 015101
Constraints on the missing baryons from the kinetic Sunyaev-Zeldovich effect in Planck data
(1) CEFCA, Teruel
(2) Jodrell Bank, Manchester
(3) AIP, Potsdam
(4) ICC, Durham
(5) IAC, Tenerife
(6) ULL, Tenerife
(7) CNRS, Grenoble
(8) IFCA, Santander
PP 015100
VLT-FORS2 optical imaging and spectroscopy of 9 luminous type 2 AGN at 0.3
VLT-FORS2 optical imaging and spectroscopy of 9 luminous type 2 AGN at 0.3
(1) Universidade do Porto, (2) CAB, (3) IAC, (4) ULL
PP 015099
Evidence for a metal-poor population in the inner Galactic Bulge
Several institutions from USA and Europe (including IAC and ULL)
PP 015098
The little-studied cluster Berkeley 90. II. The foreground ISM
(1) CAB-CSIC/INTA (2) Univ La Serena (3) IAA, (4) IAC/ULL
PP 015097
Mapping atomic and diffuse interstellar band absorption across the Magellanic Clouds and the Milky Way
1. Lennard-Jones Laboratories, Keele University, ST5 5BG, R.Unido; 2. Astrophysics Research Institute, Liverpool John Moores University, IC2, Liverpool Science Park, Liverpool L3 5RF, R. Unido;3. School of Chemistry, University of Nottingham, University Park, Nottingham, NG7 2RD, R. Unido; 4.Instituto de Astrofísica de Canarias, 38205, La Laguna, Tenerife, España,Department of Astrophysics, University of La Laguna, Tenerife, España; CSIC, E-28040, Madrid, España.
PP 015096
Swift J1357.2-0933: a massive black hole in the Galactic thick disc
(1) IAC, (2) Departamento de astrofísica de la Univ. de La Laguna, (3) Instituto de Astrofísica de la Pontificia Universidad Católica de Chile
PP 015095
Interacting galaxies in the nearby Universe: only moderate increase of star formation
IAC, ULL, MPIA
PP 015094
A deep look at the nuclear region of UGC 5101 through high angular resolution mid-IR data with GTC/CanariCam
(1) INAOE, (2) IFCA, (3) IAC, (4) ULL
PP 015093
The Sensitivity of Harassment to Orbit: Mass Loss from Early-Type Dwarfs in Galaxy Clusters
(1) Yonsei Univ., Seoul, Korea
(2) Herzberg Institute of Astrophysics, Canada
(3) IAC
PP 015092
An Infrared Diffuse Circumstellar Band? The Unusual 1.5272 Micron DIB In the Red Square Nebula
(1) Johns Hopkins University; (2) New Mexico State University; (3) Austin College; (4) University of North Carolina at Greensboro; (5) Instituto de Astrofísica de Canarias and Universidad de La Laguna; (6) University of Virginia
PP 015091
Constraints on the evolutionary mechanisms of massive galaxies since z ~ 1 from their velocity dispersions
(1) IAC, (2) ULL, (3) Isaac Newton Group of Telescopes, (4) Universidad Nacional Autónoma de México, (5) Universidad Complutense de Madrid, (6) University of Florida, (7) Universidad Andrés Bello, (8) Universidad Autónoma de Madrid
PP 015090
Open cluster Dolidze 25: Stellar parameters and the metallicity in the Galactic Anticentre
(1) Univ. Alicante, (2) IAC, (3) ULL, (4) Univ. Bonn
PP 015089
The evolution of the disc variability along the hard state of the black hole transient GX 339-4
(1) Max-Planck-Institut fur Extraterrestrische Physik (MPE), (2) IAC, (3) ULL
PP 015088
Model Comparison for the Density Structure Across Solar Coronal Waveguides
(1) IAC, (2) ULL, (3) UIB, (4) Institute of Applied Computing & Community Code, UIB
PP 015087
Transiting exoplanets from the CoRoT space mission XXVIII. CoRoT-33b, an object in the brown dwarf desert with 2:3 commensurability with its host star
(1) Inst. Planetary Research, Berlin (2) IAC, ULL
PP 015086
Damped transverse oscillations of interacting coronal loops
(1) Universitat de les Illes Balears
(2) IAC
(3) ULL
PP 015085
Deconstructing the narrow-line region of the nearest obscured quasar
(1) CAB, (2) MPIA, (3) IAC, (4) ULL, (5) University of Sheffield, (6) IAA
PP 015084
Localized starbursts in dwarf galaxies produced by impact of low metallicity cosmic gas clouds
((1) Instituto de Astrofisica de Canarias, La Laguna, Tenerife, Spain, (2) Departamento de Astrofisica, Universidad de La Laguna, (3) IBM Research Division, T.J. Watson Research Center, Yorktown Heights, NY 10598, USA, (4) Department of Physics and Astronomy, Vassar College, Poughkeepsie, NY 12604, USA, (5) Instituto de Astrofisica de Andalucia, CSIC, Granada, Spain, (6) INAF-Osservatorio Astronomico di Roma, Monte Porzio Catone, Italy, (7) SIM/CENTRA, Lisbon, Portugal, (8) Centro de Astrofisica da Universidade do Porto, Porto, Portugal, (9) Instituto de Astrofisica e Ciencias do Espasco, Universidade de Lisboa, Lisboa, Portugal, (10) Universidad Autónoma de Madrid, Madrid, Spain)
PP 015082
The VLT-FLAMES Tarantula Survey. XXIII: two massive double-lined binaries in 30~Doradus
(1) UCL (2) QUB (3) IAC (4) ULL
PP 015081
Chemical Cartography with APOGEE: Metallicity Distribution Functions and the Chemical Structure of the Milky Way Disk
Several institutions from USA and Europe (including IAC and ULL)
PP 015080
High resolution imaging of NGC 2346 with GSAOI/GeMS: disentangling the planetary nebula molecular structure to understand its origin and evolution
(1) IAC-ULL ; (2) NOAO ; (3) UAM ; (4) IA-UNAM
PP 015079
A test for asymptotic giant branch evolution theories: Planetary Nebulae in the Large Magellanic Cloud
(1) INAF-OAR; (2) NOAO ; (3) Universita Roma "La Sapienza"; (4) IAC-ULL
PP 015078
B fields in OB stars (BOB): Detection of a strong magnetic field in the O9.7 V star HD54879
(1) Argelander-Institut für Astronomie der Universität Bonn, (2), IAC, (3) ULL
PP 015077
Observational consequences of turbulent pressure in the envelopes of massive stars
(1) Argelander-Institut fur Astronomie der Universitat Bonn, (2) IAC, (3) ULL
PP 015076
The Magellanic Inter-Cloud Project (MAGIC) II: Slicing up the Bridge
(1) Department of Physics, University of Surrey, (2) Gemini Observatory, (3,4) IAC-ULL, (5) Raytheon Company, (6) MPIA
PP 015075
Fifteen years of XMM-Newton and Chandra monitoring of Sgr A*: Evidence for a recent increase in the bright flaring rate
(1) Max Planck Institute fur Extraterrestriche Physik, 85748, Garching, Germany
(2) Department of Physics & Astronomy, University of Calisfornia, Los Angeles, CA 90095-1547, USA
(3) Instituto de Astrofisica de Canarias, E-38205 La Laguna, Tenerife, Spain
(4) Departamento de astrofisica, Univ. de La Laguna, E-38206 La Laguna, Tenerife, Spain
PP 015074
Constraining the evolution of the CMB temperature with SZ measurements from Planck data
(1) Dept. of Physics, Sapienza, University of Rome
(2) Instituto de Astrofísica de Canarias, C/Vía Láctea s/n, La Laguna, Tenerife, Spain
(3) Departamento de Astrofísica, Universidad de La Laguna
(4) Centro de Astrofísica, Universidade do Porto, Portugal
(5) Instituto de Astrofísica e Ciências do Espaço, CAUP, Rua das Estrelas, Porto, Portugal
PP 015073
Gaia FGK benchmark stars: abundances of alpha and iron-peak elements
(1) IAC and other EU institutions
PP 015072
Constraining the redshift evolution of the Cosmic Microwave Background black-body temperature with PLANCK data
(1) Física Teórica, Universidad de Salamanca, 37008 Salamanca, Spain
(2) Instituto de Astrofísica de Canarias, 38200 La Laguna, Spain
(3) Institute for Astronomy, University of Hawaii, Honolulu
(4) NASA Goddard Space Flight Center and SSAI, Observational Cosmology Lab
(5) Chemistry-Physics Building, University of Kentucky, Lexington, KY 40508 USA
(6) Centro de Astrofísica da Universidade do Porto, Rua das Estrelas
(7) Instituto de Astrofísica e Ciências do Espa¸co, CAUP, Rua das Estrela
PP 015071
Measurements of the Intensity and Polarization of the Anomalous Microwave Emission in the Perseus molecular complex with QUIJOTE
(1) Instituto de Astrofisíca de Canarias
(2) Jodrell Bank Centre for Astrophysics, Alan Turing Building, School of Physics and Astronomy, The University of Manchester
(3) Instituto de Física de Cantabria (CSIC-Universidad de Cantabria)
(4) Astrophysics Group, Cavendish Laboratory, University of Cambridge, J.J.
(5) Departamento de Astrofísica, Universidad de La Laguna (ULL)
(6) Consejo Superior de Investigaciones Científicas
(7) Departamento de Física y Astronomía, Universidad de la Serena, Av. Cisternas 1200, La Serena, Chile
(8) Kavli Institute for Cosmology, Madingley Road, Cambridge
PP 015070
Constraining the Baryon Fraction in the Warm Hot Intergalactic Medium at Low Redshifts with Planck Data
(1) Instituto de Astrofísica de Canarias
(2) Departamento de Astrofísica, Universidad de La Laguna (ULL)
(3) Física Teórica, Universidad de Salamanca, E-37008 Salamanca
(4) Leibniz Institut für Astrophysik, D-14482 Potsdam, Germany
PP 015069
ARE TORNADO-LIKE MAGNETIC STRUCTURES ABLE TO SUPPORT SOLAR PROMINENCE PLASMA?
(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) Mathematics Institute, University of St Andrews St Andrews KY16 9SS, UK
PP 015068
Rotation periods of late-type dwarf stars from time-series high-resolution spectroscopy of chromospheric indicators
(1) IAC, (2) ULL, (3) CSIC
PP 015067
Near-Infrared Polarimetric Adaptive Optics Observations of NGC 1068: A torus created by a hydromagnetic outflow wind
(1) UTSA, (2) IAC, (3)ULL
PP 015066
s-process enrichment in the planetary nebula NGC 3918. Results from deep echelle spectrophotometry
(1) IAC, Spain, (2) U. La Laguna, Spain, (3) U. West Georgia, USA, (4) IA-UNAM, Mexico)
PP 015064
Evidence of amplitude modulation due to Resonant Mode Coupling in the delta Scuti star KIC5892969
(1) IAC, (2) ULL, (3) LESIA, (4) Laboratoire AIM CEA/DSM
PP 015063
Starbursts are preferentially interacting: confirmation from the nearest galaxies
IAC & ULL
PP 015062
Dynamical masses of a nova-like variable on the edge of the period gap
(1) IAC/ULL, (2) IAC/ULL, (3) Warwick, (4) Warwick, (5) Warwick, (6) STScI, (7) IAC/ULL, (8) IAC/ULL, (9) AIP, (10) Valparaíso, (11) SRON, (12) Kiel, (13) Sheffield, (14) Rodeno Obs., (15) Guadarrama Obs.
PP 015061
Ionized gas in the XUV disc of the NGC 1512/1510 system
(1) AAO, Australia
(2) Macquarie University, Australia
(3) ICRAR, Australia
(4) IAC
(5) ULL
(6) CSIRO, Australia
PP 015060
The little-studied cluster Berkeley 90. I. LS III +46 11: a very massive O3.5 If* + O3.5 If* binary
Several, including CAB/CSIC-INTA[1] and IAC/ULL[2]
PP 015059
The VLT-FLAMES Tarantula Survey XXII. Multiplicity properties of the B-type stars
Several, including [1] QUB and [2] IAC/ULL
PP 015058
Central star formation and metallicity in CALIFA interacting galaxies
1 Instituto de Astrofísica de Canarias (IAC), E-38205 La Laguna, Tenerife, Spain
2 Depto. Astrofísica, Universidad de La Laguna (ULL), E-38206 La Laguna, Tenerife, Spain
3 Instituto de Astronomía,Universidad Nacional Autonóma de Mexico, A.P. 70-264, 04510, México,D.F.
4 Instituto de Cosmologia, Relatividade e Astrofísica – ICRA, Centro Brasileiro de Pesquisas Físicas, Rua
Dr.Xavier Sigaud 150, CEP 22290-180, Rio de Janeiro, RJ, Brazil
5 Instituto de Astrofísica de Andalucía (CSIC), Glorieta de la Astronomía s/n, Aptdo. 3004, E18080-
Granada, Spain
6 European Southern Observatory (ESO), Karl-Schwarzschild-Str. 2, D-85748 Garching b. Muenchen,
Germany
7 Max-Planck-Institut für Astronomie, Heidelberg, Germany.
8 Estación Experimental de Zonas Aridas (CSIC), Ctra. de Sacramento s/n, La Cañada, Almería, Spain
9 Instituto Nacional de Astrofísica, Óptica y Electrónica, Luis E. Erro 1, 72840 Tonantzintla, Puebla, Mexico
10 Centro de Estudios de la Física del Cosmos de Aragón, E-44001 Teruel, Spain
11 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.
12 Millennium Institute of Astrophysics, Universidad de Chile, Santiago, Chile
13 Departamento de Astronomía, Universidad de Chile, Casilla 36-D, Santiago, Chile
14 Australian Astronomical Observatory, PO Box 915, North Ryde, NSW 1670, Australia
15 Department of Physics and Astronomy, Macquarie University , NSW 2109, Australia
16 Leibniz-Institut für Astrophysik Potsdam (AIP), An der Sternwarte 16, D-14482 Potsdam, Germany
PP 015057
An equatorial ultra iron-poor star identified in BOSS
(1)IAC; (2)Chungnam National University; (3)University of Notre Dame; (4)University of California; (5)University of Florida
PP 015056
Photometric scaling relations of antitruncated stellar discsin S0-Scd galaxies
(1) Departamento de Astrofísica y CC. de la Atmósfera, Universidad Complutense de Madrid, E-28040 Madrid,(2) IAC (3)Dept. Astrofísica, ULL (5) UNAM,
Ensenada,México
PP 015055
The balance of power: accretion and feedback in stellar mass black holes
(1) Oxford
(2) IAC
(3) ULL
PP 015054
Stellar population synthesis models between 2.5 and 5 μm based on the empirical IRTF stellar library
IAC, ULL, Univ. Groningen
PP 015053
The Spitzer Survey of Stellar Structure in Galaxies (S4G): Stellar Masses, Sizes and Radial Profiles for 2352 Nearby Galaxies
ESO, ..., IAC, ULL, ...
PP 015052
The trace of a substantial assembly of massive E-S0 galaxies at 0.8
The trace of a substantial assembly of massive E-S0 galaxies at 0.8
Instituto de Astrofisica de Canarias, Universidad de La Laguna, Universidad Complutense de Madrid, Spain)
PP 015051
A SLUGGS and Gemini/GMOS combined study of the elliptical galaxy M60: wide-field photometry and kinematics of the globular cluster system
1 University of California Observatories, Santa Cruz
2 Department of Physics, Queen’s University, Canada
3 Department of Physics and Astronomy, Michigan State University
4 Department of Physics and Astronomy, San Jose State University
5 (CONICET) Argentina
6 Instituto de Astrof´ısica de La Plata
7 Centre for Astrophysics & Supercomputing, Swinburne University, Australia
8 Australian Astronomical Observatory
9 Macquarie University, Sydney Australia
10 Harvard-Smithsonian Center for Astrophysic
11 Max Planck Institut f¨ur Astronomie, Heidelberg, Germany
13 IAC
14 Astronomy Department, University of Texas, Austin
15 Department of Physics, University of Durham, UK
PP 015050
Evolutionary stellar population synthesis with MILES - II. Scaled-solar and α-enhanced models
(1,5,8) IAC, (2) Inst. Astronomia, Sao Paulo, (3,9) INAF, Teramo, (4) U. Valencia, (5) U. Autonoma, Madrid, (7)
PP 015049
Evidence for temporal evolution in the M33 disc as traced by its star clusters
(1,3,5) IAC, (2) CEFCA, (4) U. Florida
PP 015047
The Large Magellanic Cloud as a laboratory for hot bottom burning in massive asymptotic giant branch stars
(1) INAF-OAR; (2) RSAA-ANU ; (3) Universita Roma "La Sapienza"; (4) OCL-NASA ; (5) IAC-ULL
PP 015046
Asymptotic giant branch stars in the Large Magellanic Cloud: evolution of dust in circumstellar envelopes
(1) INAF-OAR; (2) Universita Roma "La Sapienza"; (3) IAC-ULL
PP 015045
Young alpha-enriched giant stars in the solar neighbourhood
Several institutions from USA and Europe (including IAC and ULL)
PP 015044
New H-band stellar spectral libraries for the SDSS-III/APOGEE survey
Several institutions from USA and Europe (including IAC and ULL)
PP 015043
Rapid rotation of low-mass red giants using APOKASC: a measure of interaction rates on the post-main-sequence
Several institutions from USA and Europe (including IAC and ULL)
PP 015042
Model comparison for the density structure along solar prominence threads
(1) Instituto de Astrofísica de Canarias, E-38205 La Laguna, Tenerife, Spain
(2) Departamento de Astrofísica, Universidad de La Laguna, E-38206 La Laguna, Tenerife, Spain
(3) Departament de Física, Universitat de les Illes Balears, E-07122 Palma de Mallorca, Spain
PP 015041
On the nature of transverse coronal waves revealed by wavefront dislocations
(1) THEMIS - CNRS UPS 853. C/ Vía Láctea s/n. 38200. La Laguna, Spain
(2) IRAP - CNRS UMR 5277. 14, Av. E. Belin. 31400 Toulouse, France
(3) Instituto de Astrofísica de Canarias. C/ Vía Láctea s/n. 38200 La Laguna, Spain
(4) Departamento de Astrofísica, Universidad de La Laguna, 38205 La Laguna, Tenerife, Spain
PP 015040
Comparative internal kinematics of the HII regions in interacting and isolated galaxies: implications for massive star formation modes
1. Instituto de Astrofísica de Canarias 2. Dept. Astrofísica, U. La Laguna
3. CSIC, 4. Observatorio de Estocolmo, Dto. Astronomía U. Estocolmo, 5. Instituto de Investigación en Astrofísica, U. Liverpool John Moores-
PP 015039
DISCOVERY OF A YOUNG PLANETARY MASS COMPANION TO THE NEARBY M DWARF VHS J125601.92-125723.9
(1) Instituto de Astrofísica de Canarias (IAC)
(2) Departamento de Astrofísica, Universidad de La Laguna (ULL)
(3) Dpto. Física Aplicada, Universidad Politécnica de Cartagena,
(4) Centro de Astrobiología (CSIC-INTA)
(5) Consejo Superior de Investigaciones Cientcas, CSIC
PP 015038
The BaLROG project - I. Quantifying the influence of bars on the kinematics of nearby galaxies
(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) Astronomy and Space Physics, P.O. Box 3000, FI-90014 University of Oulu, Finland, (4) Finnish Center for Astronomy with ESO (FINCA), University of Turku, Finland
PP 015037
H-alpha kinematics of S4G spiral galaxies-II. Data description and non-circular motions
(1) Instituto de Astrofisica de Canarias
(2) Departamento de Astrofisica, Universidad de La Laguna
(3) Max-Planck-Institut für Astronomie / Königstuhl 17 D-69117 Heidelberg, Germany
(4) Consejo Superior de Investigaciones Científicas, Spain.
PP 015035
The Stellar Spectral Features of Nearby Galaxies in the Near-Infrared: Tracers of Thermally-Pulsing Asymptotic Giant Branch Stars?
(1)Universidade Federal do Rio Grande do Sul (2)IAC, (3)ULL
PP 015034
Radial velocities and metallicities from infrared Ca II triplet spectroscopy of open clusters II. Berkeley 23, King 1, NGC 559, NGC 6603 and NGC 7245
(1) Instituto de Astrofísica de Canarias, La Laguna, Tenerife, Spain, (2) Departamento de Astrofísica, Universidad de La Laguna, Tenerife, Spain, (3) Departament d'Astronomia i Meteorologia, Universitat de Barcelona, ICC/IEEC, Barcelona, Spain, (4) Institut de Ciéncies de l'Espai (CSIC-IEEC), Campus UAB, Bellaterra, Spain
PP 015033
Estimating the magnetic field strength from magnetograms
Instituto de Astrofísica de Canarias
Departamento de Astrofísica, Universidad de La Laguna
PP 015032
Sparse inversion of Stokes profiles. I. Two-dimensional Milne-Eddington inversions
(1) Instituto de Astrofísica de Canarias
(2) Departamento de Astrofísica, Universidad de La Laguna
(3) Institute for Solar Physics, Dept. of Astronomy, Stockholm University
PP 015031
ASTRONOMY, ARCHITECTURE AND SYMBOLISM: THE GLOBAL PROJECT OF SNEFERU AT DAHSHUR
(1) Instituto de Astrofísica de Canarias & Universidad de Laguna
82) Politecnico di Milano
PP 015029
Period, epoch and prediction errors of ephemeris from continuous sets of timing measurements
IAC, ULL
PP 015028
Solar Space Density of the Red Clump Stars and the Scale-length of the Thin Disc
(1) Istanbul University, Faculty of Science, Department of Astronomy and Space Sciences, 34119, Beyazıt, Istanbul, Turkey
(2) Istanbul University, Graduate School of Science and Engineering, Department of Astronomy and Space Sciences, 34116, Beyazıt, Istanbul, Turkey
(3) Mithatpa ̧sa cd. 16/4, 35320, Narlıdere, Izmir, Turkey
(4) IAC
(5) ULL
PP 015027
The Nuclear Near-Infrared Spectral Properties of Nearby Galaxies
(1) Gemini Observatory, (2) IAC, (3) ULL
PP 015026
On the Origin of the Angular Momentum of Galaxies: Cosmological Tidal Torques supplemented by the Coriolis Force Force
1.Instituto de Astrofísica de Canarias, La Laguna, Tenerife, Spain
2. Departamento de Astrofísica, Universidad de La Laguna, La Laguna, Tenerife,Spain
3. Consejo Superior de Investigaciones Científicas, Spain
PP 015025
Testing the chemical tagging technique with open clusters
(1)IAC, (2)ULL, and other European institutions
PP 015024
Stellar parameters of early M dwarfs from ratios of spectral features at optical wavelengths
(1) IAC, (2) ULL and other spanish and italian institutions
PP 015023
Resolving the AGN and host emission in the mid-infrared using a model-independent spectral decomposition
(1) IFCA, (2) ESO, (3) Cornell University, (4) IAC, (5) ULL
PP 015022
Binarity and the abundance discrepancy problem in planetary nebulae
(1) Instituto de Astrofísica de Canarias, Spain, (2) Dept. Astrofísica. Universidad de La Laguna, Spain
PP 015021
The nuclear and extended infrared emission of the Seyfert galaxy NGC 2992 and the interacting system Arp 245
(1) IAC, (2) ULL, (3) IFCA, (4) ESAC
PP 015020
Three-dimensional radiative transfer simulations of the scattering polarization of the hydrogen Ly-alpha line in a MHD model of the chromosphere-corona transition region
1) Astronomical Institute, Czech Republic
2) Instituto de Astrofisica de Canarias, Spain
3) Universidad de Estocolmo
4) Universidad de Oslo
PP 015019
Large SDSS quasar groups and their statistical significance
(1) School of Physics, Korea Institute for Advanced Study, Heogiro 85, Seoul 130-722, Korea, (2) Tartu Observatory, 61602 Toravere, Estonia, (3) Instituto de Astrof ́ısica de Canarias, E-38205 La Laguna, Tenerife, Spain, (4) Universidad de La Laguna, Dept. Astrof ́ısica, E-38206 La Laguna, Tenerife, Spain, (5) Tuorla Observatory, University of Turku, Va ̈isa ̈la ̈ntie 20, Piikkio ̈, Finland
PP 015018
VIMOS integral field spectroscopy of blue compact galaxies. I. Morphological properties, diagnostic emission-line ratios, and kinematics.
1) Institut für Astrophysik, Georg-August-Universität, Göttingen. 2) Instituto de Astrofísica de Canarias. 3) Departamento de Astrofísica, Universidad de la Laguna. 4) Leibniz-Institut für Astrophysik Potsdam (AIP).
PP 015017
The discrepancy between dynamical and stellar masses in massive compact galaxies traces non-homology
(1) IAC, (2) ULL, (3) Isaac Newton Group of Telescopes
PP 015016
Exploring Anticorrelations and Light Element Variations in Northern Globular Clusters Observed by the APOGEE Survey
Several institutions from USA and Europe (including IAC and ULL)
PP 015015
Extremely Metal-Poor Galaxies: The Environment
(1) Tri-continental Atlantic Campus, ULPG ULL, (2) IAC, (3) Departamento Astrofisica, ULL, (4) Centro de Astrofisica Universidade do Porto, (5) Instituto de Astrofisica e Ciencias do Espacio, Universidade do Lisboa, (6) Leibniz-Institute fur Astrophysik, Postdam
PP 015014
Spectro-polarimetric imaging reveals helical magnetic fields in solar prominence feet
(1,2) IAC, ULL (3) National Solar Observatory (4) Stockholm University (5) Universitat de les Illes Balears
PP 015013
On the difference of torus geometry between hidden and non-hidden broad line active galactic nuclei
(1) Kyoto University, (2) UTSA, (3) IAC, (4) ULL
PP 015012
The GALEX/S4G UV-IR color-color diagram: Catching spiral galaxies away from the Blue Sequence
(1) Universidad Complutense de Madrid, (2) LAM Laboratoire d'Astrophysique de Marseille, (3) I.N.A.F. Osservatorio Astronomico di Bologna, (4) European Southern Observatory, (5) NRAO National Radio Astronomy Observatory, (6) University of Arizona, (7) University of Oulu, (8) Kapteyn Astronomical Institute, (9) Instituto de Astrofísica de Canarias, (10) Universidad de La Laguna
PP 015010
New radio observations of anomalous microwave emission in the HII region RCW175
(1) Department of Physics, Sapienza University of Rome, Piazzale Aldo Moro 5, 00185 Rome, Italy
(2) CSIRO Astronomy and Space Science, PO Box 76, Epping, NSW 1710, Australia
(3) Instituto de Astrofísica de Canarias, C/ Va Lactea, s/n, E38205 - La Laguna (Tenerife), Spain
(4) Departamento de Astrofísica, Universidad de La Laguna (ULL), 38206 La Laguna, Tenerife, Spain
(5) Infrared Processing Analysis Center, California Institute of Technology, Pasadena, CA 91125, USA
(6) Scientific Support Office, Directorate of Science and Robotic Exploration, European Space Research and Technology Centre (ESA/ESTEC), Keplerlaan 1, 2201 AZ Noordwijk, The Netherlands
(7) IAS, CNRS (UMR 8617), Universit ́e Paris-Sud 11, bˆatiment 121, 91400 Orsay, France
PP 015009
The powerful jet of an off-nuclear intermediate-mass black hole in the spiral galaxy NGC 2276
(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) Department of Physics, University of Durham, South Road, Durham DH1 3LE, UK
(4) Max Planck Institute for Radio Astronomy, Auf dem Hügel 69, D-53121 Bonn, Germany
PP 015008
Gaia-ESO Survey: The analysis of pre-main sequence stellar spectra
IAC and other European institutions
PP 015007
On the LINER nuclear obscuration, Compton-thickness and the existence of the dusty torus; Clues from Spitzer/IRS spectra
(1) CRyA-UNAM, (2) IAA, (3) IAC, (4) ULL
PP 015006
The VLT-FLAMES Tarantula Survey. XVIII. Classifications and radial velocities of the B-type stars
Several institutions from Europe and USA (including IAC and ULL)
PP 015005
Globular Cluster Populations: First Results from S4G Early-Type Galaxies
1 Steward Observatory, University of Arizona, 933 North Cherry Avenue, Tucson, AZ 85721, USA; den- nis.zaritsky@gmail.com
2 Nu ́cleo de Astronom ́ıa, Facultad de Ingenier ́ıa, Universidad Diego Portales, Av. Ej ́ercito 441, Santiago, Chile
3 Instituto de Astrof ́ısica de Canarias, V ́ıa L ́acteas 38205 La Laguna, Spain
4 Departamento de Astrof ́ısica, Universidad de La Laguna, 38206, La Laguna, Spain
PP 015004
The Mass Profile and Shape of Bars in the Spitzer Survey of Stellar Structure in Galaxies (S4G): Search for an Age Indicator for Bars
1 Astronomy Program, Department of Physics and As- tronomy, Seoul National University, Seoul 151-742, Korea Email: thkim@astro.snu.ac.kr
2 National Radio Astronomy Observatory/NAASC, 520 Edgemont Road, Charlottesville, VA 22903, USA
3 European Southern Observatory, Casilla 19001, Santiago 19, Chile
4 Instituto de Astrofísica de Canarias, E-38200 La Laguna, Tenerife, Spain
5 Departamento de Astrofísica, Universidad de La Laguna, E-38205 La Laguna, Tenerife, Spain
PP 015002
Mass constraints to Sco X-1 from Bowen flourescence and deep near-infrared spectroscopy
(1) Instituto de Astrofísica de Canarias, 38205 La Laguna, Tenerife, Spain.
(2)Departamento de astrofísica, Univ. de La Laguna, E-38206 La Laguna, Tenerife, Spain.
(3)Department of Physics, Astrophysics, University of Oxford, Keble Road, Oxford, OX1 3RH, United Kingdom.
(4)Department of Physics, University of Warwick, Coventry CV4 7AL, UK.
PP 015001
A Classical Morphological Analysis of Galaxies in the Spitzer Survey of Stellar Structure in Galaxies (S4G)
1. Department of Physics & Astronomy, University of Alabama, Box 870324, Tuscaloosa, AL 35487-0324
2. National Radio Astronomy Observatory / NAASC, 520 Edgemont Road, Charlottesville, VA 22903
3. Instituto de Astrofisica de Canarias. Via Lactea sn. 38205. La Laguna. Spain
4. Departamento de Astrofisica, Universidad de La Laguna, 38206 La Laguna, Spain