Man

Kseniia Telikova

Adjunct researcher

Universidad Diego Portales

Santiago, Chile

Líneas de Investigación


cosmology – early universe – early galaxies – quasars – interstellar medium – circum-galactic medium – intergalactic medium – absorption lines

Educación

  •  Physics, Peter the Great St. Petersburg Polytechnic University. Rusia, 2016
  •  Physics, Peter the Great St. Petersburg Polytechnic University. Rusia, 2018
  •  Space physics, astronomy, Ioffe Institute. Chile, 2023

Experiencia Académica

  •   Research Assistant Part Time

    Ioffe Institute

    Saint Petersburg, Rusia

    2016 - 2018

  •   Junior Research Scientist Part Time

    Ioffe Institute

    Saint Petersburg, Rusia

    2018 - 2023

  •   Adjunct researcher Full Time

    UNIVERSIDAD DIEGO PORTALES

    Santiago, Chile

    2023 - A la fecha

  •   Student Other

    EUROPEAN SOUTHERN OBSERVATORY

    Santiago, Chile

    2022 - 2023

Experiencia Profesional

  •   Postdoctoral Researcher Other

    Universidad Diego Portales

    Santiago, Chile

    2023 - A la fecha

  •   Research Assistant Part Time

    Ioffe Institute

    Saint Petersburg, Rusia

    2016 - 2018

  •   Junior Research Scientist Part Time

    Ioffe Institute

    Saint Petersburg, Chile

    2018 - 2023


 

Article (17)

A hidden active galactic nucleus powering bright [O III] nebulae in a protocluster at z = 4.5 revealed by JWST
The ALMA-CRISTAL Survey: Spatial extent of [C II] line emission in star-forming galaxies at <i>z</i>=4-6
The ALMA-CRISTAL survey. Discovery of a 15 kpc-long gas plume in a z=4.54 Lyman-alpha blob
The ALMA-CRISTAL survey: Dust temperature and physical conditions of the interstellar medium in a typical galaxy at <i>z</i>=5.66
Low-ionization iron-rich broad absorption-line quasar SDSS J 1652+2650: physical conditions in the ejected gas from excited FeII and metastable HeI
CII*/CII ratio in high-redshift DLAs: ISM phase separation drives the observed bimodality of [CII] cooling rates
Extremely strong DLAs at high redshift: gas cooling and H2 formation
Multi-phase gas properties of extremely strong intervening DLAs towards quasars
Constraints on the temperature-density relation of the intergalactic medium with non-negligible absorber spatial structure
Sharpening quasar absorption lines with ESPRESSO. Temperature of warm gas at z~2, constraints on the Mg isotopic ratio, and structure of cold gas at z~0.5
Extremely strong damped Ly-alpha systems at high redshifts
Jeans smoothing of the Ly-alpha forest absorption lines
Thermal state of the intergalactic medium at z~2-4
Equation of state of the intergalactic medium in the early Universe
Estimation of the temperature-density relation in the intergalactic medium at z~2-4 via Ly-alpha forest
Stellar and dark matter density in the Local Universe
The primordial deuterium abundance: sub-DLA system at zabs=2.437 towards the QSO J1444+2919
2
Manuel Aravena

Full Professor

Facultad de Ingeniería y Ciencias

Universidad Diego Portales

Santiago, Chile

1
Roberto Assef

Profesor Titular

Núcleo de Astronomía de la Facultad de Ingeniería y Ciencias

Universidad Diego Portales

Santiago, Chile

2
Jorge González

Profesor asistente

Facultad de Física

Pontificia Universidad Católica de Chile

Santiago, Chile

17
Kseniia Telikova

Adjunct researcher

Universidad Diego Portales

Santiago, Chile