B Bihan

Employment

• Tata Institute of Fundamental Research

Education

Education history is unavailable.

Projects & Funding

Projects & funding information is unavailable.

Publications (10)

• Improving accretion diagnostics for young stellar objects with mid-infrared hydrogen lines from JWST/MIRI
  Astronomy & Astrophysics 2026 DOI: 10.1051/0004-6361/202556384
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• Demography of Stellar Radio Population within 500 pc: A VLASS-Gaia DR3 Study
  The Astronomical Journal 2024 DOI: 10.3847/1538-3881/ad84e7
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• uGMRT Survey of EXoplanets Around M-dwarfs (GS-EXAM): Radio Observations of GJ 1151
  The Astronomical Journal 2024 DOI: 10.3847/1538-3881/ad84e4
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• Host-star Properties of Hot, Warm, and Cold Jupiters in the Solar Neighborhood from Gaia Data Release 3: Clues to Formation Pathways
  The Astronomical Journal 2024 DOI: 10.3847/1538-3881/ad429f
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• Identifying the population of T-Tauri stars in Taurus: UV-optical synergy
  Journal of Astrophysics and Astronomy 2023 DOI: 10.1007/s12036-023-09972-6
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• Optical spectroscopy of Gaia detected protostars with DOT: Can we probe protostellar photospheres?
  Journal of Astrophysics and Astronomy 2023 DOI: 10.1007/s12036-023-09982-4
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• Age Distribution of Exoplanet Host Stars: Chemical and Kinematic Age Proxies from GAIA DR3
  The Astronomical Journal 2023 DOI: 10.3847/1538-3881/ace782
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• uGMRT observations of the hot-Saturn WASP-69b: Radio-Loud Exoplanet-Exomoon Survey II (RLEES II)
  Monthly Notices of the Royal Astronomical Society 2023 DOI: 10.1093/mnras/stad1027
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• Galactic Chemical Evolution of Exoplanet Hosting Stars: Are High-mass Planetary Systems Young?
  The Astronomical Journal 2022 DOI: 10.3847/1538-3881/ac756a
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• Galactic chemical evolution of exoplanet host stars: Are high-mass planetary systems young?
  arXiv e-prints 2022
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