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Anwesha Sahu

I am a first year PhD researcher working with the white dwarfs and transients research group. My supervisors are Deanne Coppejans, and Danny Steeghs. I study AM CVn stars (a sub-class of binary white dwarf stars) in the radio spectrum using data from the VLA.

Fundamental questions remain about the accretion and outflow physics of cataclysmic variable stars, and their compact binary counterparts, AM CVn systems. Using observations from the Karl J. Jansky Very Large Array (VLA), I have obtained the deepest radio constraints to date, for two such AM CVn systems: AM CVn and HP Lib. By cross-matching with other large scale surveys such as LOFAR and VLASS, the radio emission properties and mechanisms of AM CVn and CV populations can be better characterised. A key question this study aims to contribute to is whether the emissions observed in CVs are due to flares in the atmosphere of the donor star, as compared to transient jets originating from the accretion disk. Understanding outflows from accreting white dwarfs such as these can propel our undestanding of the Type Ia supernovae progenitors. (Paper in prep)

I completed my MSci at the University of Birmingham with my final year dissertation on machine learning applications for radio astronomy, with a focus on classification of radio objects from MeerKAT. I also work with the GOTO and ePESSTO+ collaborations for follow-up and data analysis on transients.

Research/Publications

First author:

Co-author:

Past Research

  • Using the MeerKAT Galactic Plane Survey and the VLA FIRST survey, I constructed a deep learning model to identify and classify radio objects within the MeerKAT GPS using a GAN (generative adversarial network). This project was performed as a preparatory study for an automated classification algorithm to identify radio objects with the Square Kilometre Array (SKA) 
  • Due to inaccurate weather outputs from on-site weather stations at the SPECULOOS South Observatory, Paranal, Chile, resulting in a reduction in observation time, I constructed an algorithm which analyses the sky conditions in real-time from an on-site All-Sky camera. This provided accurate sky conditions with accuracies of over 90% which would result in an increase in observation time, thus aiding the detection of transits with longer durations.
  • During my third year of my BSc/MSci, I calculated habitable exoplanet occurrence rates around K dwarf stars, using a simulated set of stars from TRILEGAL, and performed asteroseismology investigations, in preparation for the upcoming ESA PLATO mission.

Meetings & Conferences

Outreach/Engagement

  • Astronomy & Astrophysics Representative at the Postgrad Student Staff Liaison Committee, Department of Physics, University of Warwick.
  • Speaker for talks at local schools and astronomical societies
  • Organiser for Machine Learning for Transient Science, Warwick 2023
  • Chair and Outreach Officer, University of Birmingham's Astronomical Society from 2020 - 2023.
  • Find out more about my public outreach engagements and watch talks I have delivered on my website, Sitara Tales.
  • You can check my LinkedIn for other current/past engagements.

Awards/Scholarships

Teaching

  • Year 1 electronics lab sessions demonstrator
  • Year 1 physics undergraduate math support sessions

 

Write to:

Anwesha Sahu,
Department of Physics,
University of Warwick,
Coventry CV4 7AL
UK
 

Contact details:

E-Mail: anwesha.sahu@warwick.ac.uk