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The Nuclear Near-Infrared Spectral Properties of Nearby Galaxies
(2015-03)
, Porto Alegre 91501-970, RS, Brazil
5 Instituto de Astrofísica de Canarias, Calle Vía Láctea, s/n, E-38205, La Laguna, Tenerife, Spain
6 Departamento de Astrofísica, Universidad de La Laguna, E-38205, La Laguna, Tenerife, Spain
7 Kavli Institute...
of Physics, 3601 Pacific Avenue, Stockton, CA 95211, USA 11 Instituto de Física de Cantabria, CSIC-UC, E-39005 Santander, Spain 12 Departamento de Astronomía, Universidad de Chile, Casilla 36-D, Santiago, Chile 13 Department of Physics and Astronomy...
of Physics, 3601 Pacific Avenue, Stockton, CA 95211, USA 11 Instituto de Física de Cantabria, CSIC-UC, E-39005 Santander, Spain 12 Departamento de Astronomía, Universidad de Chile, Casilla 36-D, Santiago, Chile 13 Department of Physics and Astronomy...
Two-year Cosmology Large Angular Scale Surveyor (CLASS) Observations: 40 GHz Telescope Pointing, Beam Profile, Window Function, and Polarization Performance
(IOP, 2020)
´ıa, Universidad Cato´lica de la Sant´ısima Concepcio´n, Alonso de Ribera 2850, Concepcio´n, Chile
8Department of Physics, Villanova University, 800 Lancaster Avenue, Villanova, PA 19085, USA
9Goddard Space Flight Center, 8800 Greenbelt Road, Greenbelt, MD 20771...
A meta-process for defining adaptable software processes
(Universidad de Chile, 2012)
a las particularidades del proyecto en el que será usado. Típicamente, un ingeniero de procesos define un proceso específico para cada proyecto en forma ad-hoc, lo cual resulta costoso, irrepetible y propenso al error. Por otro lado, la...
Sloan digital sky survey IV: mapping the milky way, nearby galaxies, and the distant universe
(IOP Publishing Ltd., 2017)
,56, Luiz da Costa50,51,
Marie-Claude Cousinou58, Kevin Covey59, Jeffrey D. Crane24, Rupert A. C. Croft60, Irene Cruz-Gonzalez14,
Daniel Garrido Cuadra8, Katia Cunha28,51, Guillermo J. Damke8,61, Jeremy Darling62, Roger Davies46, Kyle Dawson23,
Axel de la...
, Benjamin A. Thompson19, Jeremy L. Tinker1, Patricia Tissera90, Rita Tojeiro21, Hector Hernandez Toledo14, Sylvain de la Torre34, Christy Tremonti2, Nicholas W. Troup61, Octavio Valenzuela14, Inma Martinez Valpuesta6,7, Jaime Vargas-González8, Mariana Vargas...
, Benjamin A. Thompson19, Jeremy L. Tinker1, Patricia Tissera90, Rita Tojeiro21, Hector Hernandez Toledo14, Sylvain de la Torre34, Christy Tremonti2, Nicholas W. Troup61, Octavio Valenzuela14, Inma Martinez Valpuesta6,7, Jaime Vargas-González8, Mariana Vargas...
New planetary systems from the Calan-Hertfordshire Extrasolar planet search
(Oxford University, 2017)
-127, UA-03680, Ukraine
7Department of Physical Sciences, The Open University, Walton Hall, Milton Keynes MK7 6AA, UK
8Instituto de Astrofı´sica de Canarias, Via Lactea, E-38205 La Laguna, Tenerife, Spain
9Center of Astro-Engineering UC, Pontificia...
instrument at La Silla Chile, with the goal of finding more gas giant planets orbiting supermetal-rich stars to increase the statistics, whilst also following up any discoveries to search for transit events. The first results from this work and the target...
instrument at La Silla Chile, with the goal of finding more gas giant planets orbiting supermetal-rich stars to increase the statistics, whilst also following up any discoveries to search for transit events. The first results from this work and the target...
Alkaloids from the Genus Duguetia
(Elsevier, 2010)
CAMPOS: A context-aware model for positioning in outdoor environments that supports loosely coupled mobile activities
(Universidad de Chile, 2017)
En escenarios ubicuos, conocer la posición de un dispositivo es imperativo para proveer al usuario de servicios personalizados basados en location awareness, un aspecto de diseño clave en la mayoría de las aplicaciones ubicuas que dependiente de las...
Searching for distant RR Lyrae in the galactic halo using the high cadence transient survey
(Universidad de Chile, 2017)
Utilizando datos del High cadence Transient Survey (HiTS), inspeccionamos el halo de la Vía Láctea en busca de estrellas variables RR Lyrae distantes (dH >100 kpc). Los datos del proyecto HiTS, diseñado principalmente para encontrar explosiones de...
Using data from the High cadence Transient Survey (HiTS), we inspected the halo of the Milky Way looking for distant RR Lyrae variable stars (dH >100 kpc). The HiTS project, which was originally designed to find supernovae explosions in real time, consists of images taken with the Dark Energy Camera mounted at the Blanco telescope (4 m) at the Cerro Tololo Inter-American Observatory during three different campaigns, covering 200 sq. degrees of the Galactic halo. We identified a total of 332 RR Lyrae stars (173 with data from HiTS 2014, and 159 with HiTS 2015), covering a range in distance from ~ 9 to ~ 260 kpc. According to this study, within our sample of RR Lyrae stars at least 18 are beyond 90 kpc from the Sun (and 16 beyond 100 kpc). The analysis of the catalog allowed us to study the spatial distribution of RR Lyrae stars and to associate three ovendensities with known dwarf spheroidal galaxies (Sextans, Leo~IV y Leo~V). We used this as a proof-of-concept for ideas about the role of RR Lyrae in the discovery of ultra-faint dwarf galaxies that might be difficult to find by other methods. Using the spatial distribution of RR Lyrae from HiTS 2014, we built and analyzed number density profiles of the Milky Way, of the form rho(r) ~ r^{-n}. Following a Markov chain Monte Carlo methodology, we found that the best fit for the data is a simple power law with n=-4.18^{+0.18}_{-0.19}. However, fitting a broken profile is also valid, with a break at R_b=19.34^{+10.66}_{-3.16} kpc, and inner/outer slope of n_1=-3.47^{+2.26}_{-1.32}/n_2=-4.23^{+0.33}_{-0.25}....
Using data from the High cadence Transient Survey (HiTS), we inspected the halo of the Milky Way looking for distant RR Lyrae variable stars (dH >100 kpc). The HiTS project, which was originally designed to find supernovae explosions in real time, consists of images taken with the Dark Energy Camera mounted at the Blanco telescope (4 m) at the Cerro Tololo Inter-American Observatory during three different campaigns, covering 200 sq. degrees of the Galactic halo. We identified a total of 332 RR Lyrae stars (173 with data from HiTS 2014, and 159 with HiTS 2015), covering a range in distance from ~ 9 to ~ 260 kpc. According to this study, within our sample of RR Lyrae stars at least 18 are beyond 90 kpc from the Sun (and 16 beyond 100 kpc). The analysis of the catalog allowed us to study the spatial distribution of RR Lyrae stars and to associate three ovendensities with known dwarf spheroidal galaxies (Sextans, Leo~IV y Leo~V). We used this as a proof-of-concept for ideas about the role of RR Lyrae in the discovery of ultra-faint dwarf galaxies that might be difficult to find by other methods. Using the spatial distribution of RR Lyrae from HiTS 2014, we built and analyzed number density profiles of the Milky Way, of the form rho(r) ~ r^{-n}. Following a Markov chain Monte Carlo methodology, we found that the best fit for the data is a simple power law with n=-4.18^{+0.18}_{-0.19}. However, fitting a broken profile is also valid, with a break at R_b=19.34^{+10.66}_{-3.16} kpc, and inner/outer slope of n_1=-3.47^{+2.26}_{-1.32}/n_2=-4.23^{+0.33}_{-0.25}....
First language lexical activation during second language sentence comprehension in highly proficient bilinguals
(Universidad de Chile, 2013)
the ongoing reading provides throughout
sentence reading and that this information is accrued to make predictions of
forthcoming words in advance.
However, Schwanenflugel and LaCount (1988) found that a facilitation effect
appeared for unexpected (but...
Variations on the double-multiple streamtube model for Darrieus straight-bladed vertical-axis wind turbines to improve predictions of performance and flow expansion
(Universidad de Chile, 2014)
El propósito del presente trabajo es formular una herramienta computacional de bajo costo que determine la potencia y la expansión de flujo de turbinas eólicas de eje vertical (VAWTs) tipo Darrieus. Esta herramienta puede ser útil para predecir el...