DTI | Doctorado en Tecnologías de Información

Dr. Eduardo De La Fuente Acosta

Dirección: Av Vallarta #2602, Col. Arcos Vallarta Guadalajara, Jalisco, México 44130.

Teléfono: +52 (33) 36164937

Correo electrónico:

Contribuciones:

CVU Dr. Eduardo De La Fuente Acosta

Brief Biography

Estudio la licenciatura de Física en la Universidad de Guadalajara en 1993-1997, la maestría en ciencias en Astronomía en la UNAM (1998-2003) y el doctorado en ciencias en Física por la Universidad de Guadalajara con una estancia predoctoral de 3 años en el Centro de Radioastronomía y Astrofísica de la UNAM, en Morelia (2004-2008). Realizo una estancia postdoctoral en el Instituto Nacional de Astrofísica, Óptica y Electrónica en el periodo 2008-2009.

Actualmente es Profesor Investigador Titular A del Departamento de Física del CUCEI, miembro de la planta académica del doctorado en Tecnologías de la Información del CUCEA, miembro del Sistema Nacional de Investigadores en el nivel I desde 2008, tiene perfil PROMEP, y ha impartido cátedras en distintas escuelas internacionales de Física y Astronomía en el mundo, en la carrera de Física del CUCEI, y en el doctorado en Tecnologías de la Información en CUCEA.

Hasta 2013 cuenta con 52 artículos se investigación de los cuales 20 han sido publicados en revistas indizadas de alto impacto, y 32 en memorias de congresos internacionales en extenso, con 234 citas. Ha publicado un libro especializado de Astrofísica, y es autor principal en un capitulo de otro sobre formación de estrellas.

Participa activamente en el proyecto binacional México-Estados Unidos "High Altitude Water Cherenkov (HAWC)", representando a la Universidad de Guadalajara en este proyecto, desempeñándose como el Jefe Nacional de la red de cables en el mismo, y presentador del proyecto a través de ponencias invitadas en el mundo representando a la colaboración HAWC. Cabe destacar que HAWC es el observatorio de rayos gamma mas poderoso del mundo en su tipo, y desde 2009, el proyecto mas importante del país en el área de Física de Altas Energías.

Ha dirigido varias tesis de licenciatura, actualmente esta dirigiendo 2 tesis de postgrado, asesorando una de doctorado, y ha impartido varias platicas divulgativas de Astrofísica en el país.

Publications

Chapters

Deep Optical Imaging of ESO 383–45: A Galaxy Undergoing Ram-pressure Stripping, or a Tidal Merger Remnant? (2nd).DOI: 10.1007/978-3-540-71173-5_23 .(2007)

BVRI photometric analysis for the galaxy group NGC 4410 (4th).DOI: 10.1007/978-3-540-71173-5_20 .(2007)

HAWC @ Mexico (17th).SN.(2007)

Articles

Observation of the Crab Nebula with the HAWC Gamma-Ray Observatory (25th).SN.(2017)

Search for TeV Gamma-Ray Emission from Point-like Sources in the Inner Galactic Plane with a Partial Configuration of the HAWC Observatory (24th).DOI: 10.3847/0004-637X/817/1/3.(2015)

HAWC Contributions to the 34th International Cosmic Ray Conference (ICRC2015) (26).SN.(2015)

Search for gamma-rays from the unusually bright GRB 130427A with the HAWC Gamma-ray Observatory (18th).DOI: 10.1088/0004-637X/800/2/78.(2014)

Observation of Small-scale Anisotropy in the Arrival Direction Distribution of TeV Cosmic Rays with HAWC (21st).DOI: 10.1088/0004-637X/796/2/108.(2014)

VAMOS: A pathfinder for the HAWC gamma-ray observatory (30th).DOI: 10.1016/j.astropartphys.2014.08.004 .(2014)

Milagro Limits and HAWC Sensitivity for the Rate-Density of Evaporating Primordial Black Holes (28th).DOI: 10.1016/j.astropartphys.2014.10.007 ·.(2014)

The Sensitivity of HAWC to High-Mass Dark Matter Annihilations (23rd).DOI: 10.1103/PhysRevD.90.122002.(2014)

Framework for Estimating Travel Time, Distance, Speed, and Street Segment Level of Service (LOS), based on GPS Data (3rd).DOI: 10.1016/j.protcy.2013.04.008.(2013)

The HAWC Gamma-Ray Observatory: Design, Calibration, and Operation (23rd).SN.(2013)

The HAWC Gamma-Ray Observatory: Dark Matter, Cosmology, and Fundamental Physics (23rd).SN.(2013)

The HAWC Gamma-Ray Observatory: Observations of Cosmic Rays (23rd).SN.(2013)

The HAWC Gamma-Ray Observatory: Sensitivity to Steady and Transient Sources of Gamma Rays (23rd).SN.(2013)

Sensitivity of the High Altitude Water Cherenkov Detector to Sources of Multi-TeV Gamma Rays (21st).DOI: 10.1016/j.astropartphys.2013.08.002.(2013)

PMS and ZAMS stars associated with the dark cloud LDN 1655 (4th).DOI: 10.1016/j.newast.2012.06.002.(2013)

The High Altitude Water Čerenkov (HAWC) TeV Gamma Ray Observatory (1st).DOI: 10.1007/978-3-642-35410-6_32.(2013)

Optics and the mechanical system of the 62-cm telescope at the Severo Díaz Galindo Observatory in Guadalajara, Jalisco, México (1st).DOI: 10.1117/12.926509.(2012)

Spectral Optical Monitoring of the Narrow Line Seyfert 1 galaxy Ark 564 (17th).DOI: 10.1088/0067-0049/202/1/10 .(2012)

On the sensitivity of the HAWC observatory to gamma-ray bursts (33rd).SN.(2012)

About pulsars dynamical evolution (3rd).SN.(2011)

On the sensitivity of the HAWC observatory to gamma-ray bursts (34th).DOI: 10.1016/j.astropartphys.2012.02.001 .(2011)

Numerical models for the 19th century outbursts of eta Carinae (7th).SN.(2011)

Insights Into the High-Energy Gamma-ray Emission of Markarian 501 from Extensive Multifrequency Observations in the Fermi Era (92nd).DOI: 10.17877/DE290R-4295 .(2010)

The Hot Molecular Core of G12.21-0.10: NH3(4, 4) Observations (1st).DOI: 10.1017/S1743921310003030.(2010)

Spectral optical monitoring of 3C 390.3 in 1995–2007 (14th).DOI: 10.1051/0004-6361/201016317.(2010)

Spectral optical monitoring of 3C390.3 in 1995-2007: I. Light curves and flux variation of the continuum and broad lines.DOI: 10.1051/0004-6361/201014118.(2010)

Revisiting 2D Numerical Models for the 19th century outbursts of $\eta$ Carinae (8th).DOI: 10.1111/j.1365-2966.2009.15950.x .(2009)

Optical characterization of the 62-cm telescope at the Severo Diaz Galindo Observatory in Guadalajara (2nd).DOI: 10.1117/12.849194.(2009)

The unusual interacting pair of galaxies IC 3481 and IC 3481A: An optical-NIR photometric and spectroscopic analysis (3rd).DOI: 10.1016/j.newast.2009.02.004.(2009)

Spitzer--IRAC Imagery and Photometry of Ultracompact HII Regions With Extended Emission (1st).SN.(2009)

A CCD Photometric and Morphological Study of the Extended Halo and Filaments of ESO 383-45: A Galaxy Undergoing Ram Pressure Stripping, or a Tidal Merger Remnant? (2nd).DOI: 10.1086/429269.(2008)

Lenticular galaxies in the process of evolution (4th).DOI: 10.1017/S1743921308017481.(2008)

The inner galactic structure traced by molecular clouds associated with ultra-compact hii regions (3rd).SN.(2008)

U Geminorum: A Test Case for Orbital Parameter Determination (2nd).DOI: 10.1086/518562 .(2007)

The Extended Emission of Ultracompact HII Regions: An Overview and New Observations (1st).DOI: 10.1007/978-0-387-87621-4_26 .(2007)

The composite form of the supernova remnant 3C 400.2: Two interacting supernova remnants or a single supernova remnant with a blow-out? (2nd).SN.(2006)

Simulated X‐ray emission from a single‐explosion model for a supernova remnant 3C 400.2 (2nd).DOI: 10.1111/j.1365-2966.2006.10652.x.(2006)

H alpha Fabry-Perot Study in the Orion Nebula (M 42): Protoplanetary Disks (1st).SN.(2003)

Revista Mexicana de Astronoma y Astrofsica, 39, 127--137 (2003) (1).SN.(2003)

The Radial Velocity Profiles of some Proplyds in the Orion Nebula (4th).SN.(2003)

The Supernova Remnant 3C 400.2: Kinematics of its Ionized Gas and Theoretical Results (4th).SN.(2003)

Protoplanetary Disks in the Orion Nebula: An H$\alpha$ Fabry-Perot study and Astrobiological Aspects (1st).SN.(2002)

RevMexAA (Serie de Conferencias), 12, 93--93 (2002) (1st).SN.(2002)

Laser laboratory experiments, observations and numerical simulations of strong explosions (4th).SN.(2002)

An Halpha Radial Velocity Report of Five LV Proplyds in the Orion Nebula (1st).SN.(2002)

Is the supernova remnant 3c400.2 The result of a single supernova explosion? (1st).SN.(2002)

Optically thick giant H II regions with decreasing density gradients in three barred galaxies (2nd).SN.(2002)

Hα Fabry-Perot Study in the Orion Nebula (M 42): Protoplanetary Disks.SN.(2002)

Fabry-Perot kinematics of HH 202-204 in the orion nebula: Are they part of a big bipolar outflow? (3rd).SN.(2002)

RevMexAA (Serie de Conferencias), 10, 45--48 (2001) (6th).SN.(2002)

A single explosion model for the supernova remnant 3C 400.2 (1st).DOI: 10.1051/0004-6361:20011116.(2001)

Fabry-Perot Kinematics of HH 202, 203-204 in the Orion Nebula: Are they part of a Big Bipolar Outflow? (2nd).SN.(2001)

Kinematics of Herbig-Haro Objects and Jets in the Orion Nebula (2nd).DOI: 10.1086/323303 .(2001)

Pressure and density gradients in H II Regions (5th).DOI: 10.1023/A:1012779627430.(2001)

Decreasing density gradients in circumnuclear HII regions of barred galaxies NGC 1022, NGC 1326, and NGC 4314 (3rd).DOI: 10.1086/317189 .(2000)

Optically Thick HII Regions With Density Gradients in Barred Galaxies (1st).SN.(2000)

A New Deep North-West CCD Halpha Mosaic Images Of The Supernova Remnant 3C400.2 (1st).SN.(2000)

RevMexAA (Serie de Conferencias), 9, 177--180 (2000) (6th).SN.(2000)

Dusty UCH II Regions: cloud pressures and density distributions (6th).SN.(2000)

The effects of dust and density distributions in uc H II regions (3rd).SN.(2000)

A New Faint, Giant Halo in the Planetary Nebula NGC 7009 (2nd).SN.(1998)

Más información de Artículos publicados

Ligas de interés:

http://www.hawc-observatory.org/

http://www.inaoep.mx/~hawc/

http://www.nature.com/news/mexican-observatory-pushes-the-limits-of-γ-ray-astronomy-1.14056

http://www.lanl.gov/science-innovation/science-features/hawc-observatory-captures-image.php

http://www.udg.mx/noticias/udeg-lidera-y-coordina-un-trabajo-del-observatorio-hawc

http://www.cucei.udg.mx/noticia/colabora-udeg-en-investigacion-de-detectores-de-rayos-gamma

http://www.cucei.udg.mx/noticia/se-inaugura-el-cicyta-2013-0

http://www.lajornadajalisco.com.mx/2013/11/21/cientifico-jalisciense-participa-en-programa-hawc-pide-mayor-proyeccion-para-la-ciencia-en-los-estados/

http://www.youtube.com/watch?v=uSRONMZXxOg

Correo electrónico:

edfuente@gmail.com

Titulo Educativo:

Dr.