Man

Denise Elizabeth Riquelme Vásquez

Academica

Universidad de La Serena

La Serena, Chile

Líneas de Investigación


Educación

  •  Astronomia, Instituto de Radioastronomia Milimetrica (grado otorgado por Universidad de Granada). España, 2012
  •  Fisica y Matematicas, UNIVERSIDAD DE GRANADA. España, 2008
  •  Magister en Ciencias, mencion Astronomia, UNIVERSIDAD DE CHILE. Chile, 2007
  •  licenciatura en Ciencias, mencion astronomia, UNIVERSIDAD DE CHILE. Chile, 2005

Experiencia Académica

  •   Academica Full Time

    UNIVERSIDAD DE LA SERENA

    ciencias

    la Serena, Chile

    2023 - A la fecha

  •   posdoct Full Time

    MAX-PLANCK INSTITUT FUR RADIOASTRONOMIE

    Bonn, Alemania

    2012 - 2022

Experiencia Profesional

  •   postdoct Full Time

    MAX-PLANCK INSTITUT FUR RADIOASTRONOMIE

    Bonn, Alemania

    2012 - 2022

Formación de Capital Humano


Laura A. Busch, 2020. Tesis de Magister. Max-Planck Institute for Radioastronomy
Nipesh Dulal. 2023. Co-supervision de tesis de Magister. Max-Planck Institute for Radioastronomy


Difusión y Transferencia


charla en el bootcamp de Ingeniosas. Charla en el liceo Gabriela Mistral, La Serena
charlas y observacion Astronomica para publico general, Cerro Calan, Universidad de Chile



 

Article (25)

Faint absorption of the ground state hyperfine-splitting transitions of hydroxyl at 18 cm in the Galactic disk
SOFIA/upGREAT Imaging Spectroscopy of the [C ii] 158 μm Fine-structure Line toward the Sgr A Region in the Galactic Center
Bright-rimmed clouds in IC 1396 I. Dynamics
Star formation in extreme environments: A 200 pc high velocity gas stream in the Galactic centre
Kinematics of Galactic Centre clouds shaped by shear-seeded solenoidal turbulence
Ionized Carbon around IRC+10216
Living on the edge of the Milky Way's central molecular zone G1.3 is the more likely candidate for gas accretion into the CMZ
Bottlenecks to interstellar sulfur chemistry: Sulfur-bearing hydrides in UV-illuminated gas and grains
Characterizing the Multiphase Origin of [CII] Emission in M101 and NGC 6946 with Velocity-resolved Spectroscopy
Distribution of ionized, atomic, and PDR gas around S 1 in ρ Ophiuchus
The dense warm ionized medium in the inner Galaxy
Interstellar anatomy of the TeV gamma-ray peak in the IC443 supernova remnant
On the Effects of UV Photons/X-Rays on the Chemistry of the Sgr B2 Cloud
Sulphur and carbon isotopes towards Galactic centre clouds
Chemical Evolution along the Circumnuclear Ring of M83
Footpoints of the giant molecular loops in the Galactic center region
Chemical features in the circumnuclear disk of the Galactic center
Lambda=3 mm line survey of nearby active galaxies
Disk-halo interactions: Molecular clouds in the Galactic center
Unbiased line surveys of molecular clouds in the Galactic center region
Kinetic temperatures toward X1/X2 orbit interceptions regions and giant molecular loops in the Galactic center region
Planck early results. XIV. ERCSC validation and extreme radio sources
Planck early results. XV. Spectral energy distributions and radio continuum spectra of northern extragalactic radio sources
A survey of the Galactic center region in HCO+, (HCO+)-C-13, and SiO
Tracing gas accretion in the Galactic center using isotopic ratios

ConferencePaper (2)

Chemical complexity in NGC 1068
Disk-Halo interaction: The molecular clouds in the Galactic center region

Review (1)

A ? =3mm molecular line survey of NGC 1068: Chemical signatures of an AGN environment
6
Leonardo Bronfman

Full Professor

Astronomy

UNIVERSIDAD DE CHILE, FACULTAD DE CIENCIAS FÍSICAS Y MATEMÁTICAS

Santiago, Chile

1
Rodrigo Reeves

Profesor Asociado

Astronomía

Universidad de Concepcion

Concepcion, Chile

1
Walter Max-Moerbeck

Assistant Professor

Astronomy

Universidad de Chile

Las Condes, Chile

28
Denise Riquelme

Academica

Astronomia

Universidad de La Serena

La Serena, Chile

1
Pedro Humire

investigador postdoctoral

Instituto de Astronomia, Geofísica e Ciências Atmosféricas

Universidade de Sao Paulo

Sao Paulo, Brasil