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Prasanta Kumar Nayak

CATA postdoctoral fellow

Pontificia Universidad Católica de Chile

Santiagp, Chile

Líneas de Investigación


Educación

  •  Physics (Astronomy & Astrophysics), Pondicherry University. India, 2019
  •  Physics, IIT Kharagpur, India. India, 2013
  •  Physics, University of Calcutta . Chile, 2011

Experiencia Académica

  •   CATA postdoctoral fellow Part Time

    Pontificia Universidad Católica de Chile

    Santiago, Chile

    2022 - A la fecha

  •   Postdoctoral Visiting Fellow Part Time

    Tata Institute of Fundamental Research

    Mumbai, India

    2019 - 2022

Experiencia Profesional

  •   CATA postdoctoral fellow Part Time

    Instituto de Astrofísica, Pontificia Universidad Catolica de Chile

    Santiago, Chile

    2022 - A la fecha

Premios y Distinciones

  •   CATA postdoctoral fellowship

    PONTIFICIA UNIVERSIDAD CATOLICA DE CHILE

    Chile, 2022

    I have been selected for the CATA postdoctoral fellowship to perform research in Chile.


 

Article (21)

Beyond the main sequence: Binary evolution pathways to blue stragglers in the Gaia era: I. Galactic open and globular clusters
Relighting the fire in Hickson Compact Group (HCG) 15: Magnetised fossil plasma revealed by the SKA Pathfinders and Precursors
A chemodynamical analysis of bright metal-poor stars from the HESP-GOMPA survey - indications of a non-prevailing site for light r-process elements
A uGMRT search for radio emission from planets around evolved stars
Demography of Stellar Radio Population within 500 pc: A VLASS-Gaia DR3 Study
Host-star Properties of Hot, Warm, and Cold Jupiters in the Solar Neighborhood from Gaia Data Release 3: Clues to Formation Pathways
Hunting down white dwarf-main sequence binaries using multiwavelength observations
Simultaneous Far-ultraviolet and Near-ultraviolet Observations of T Tauri Stars with UVIT/AstroSat: Probing the Accretion Process in Young Stars
Spatiotemporal map of star clusters in the Magellanic Clouds using Gaia: synchronized peaks and radial shrinkage of cluster formation
uGMRT Survey of EXoplanets Around M-dwarfs (GS-EXAM): Radio Observations of GJ 1151
UVIT Study of the MAgellanic Clouds (U-SMAC). II. A Far-UV Catalog of the Small Magellanic Cloud: Morphology and Kinematics of Young Stellar Population
Identifying the population of T-Tauri stars in Taurus: UV-optical synergy
Optical spectroscopy of Gaia detected protostars with DOT: Can we probe protostellar photospheres?
uGMRT observations of the hot-Saturn WASP-69b: Radio-Loud Exoplanet-Exomoon Survey II (RLEES II)
UV Spectral Characterization of Low-mass Stars with AstroSat UVIT for Exoplanet Applications: The Case Study of HIP 23309
White Dwarfs Revealed in Gaia's Candidate Compact Object Binaries
Li Distribution, Kinematics, and Detailed Abundance Analysis among Very Metal-poor Stars in the Galactic Halo from the HESP-GOMPA Survey
UOCS - III. UVIT catalogue of open clusters with machine learning-based membership using <i>Gaia</i> EDR3 astrometry
UVIT-<i>HST</i>-<i>Gaia</i>-VISTA study of Kron 3 in the Small Magellanic Cloud: a cluster with an extended red clump in ultraviolet
Star clusters in the Magellanic Clouds. II. Age-dating, classification, and spatio-temporal distribution of the SMC clusters
Star clusters in the Magellanic Clouds - I. Parametrization and classification of 1072 clusters in the LMC

Review (1)

Stars and stellar populations in Milky Way and the nearby galaxies
22
Prasanta Kumar Nayak

CATA postdoctoral fellow

Instituto de Astrofisica

Pontificia Universidad Católica de Chile

Santiagp, Chile