S
Saurabh
Stellar Universe, Max Planck Institute for Radio Astronomy, Charotar University of Science and Technology, Dyal Singh College
Research areas: Physics and Astronomy · Astronomy and Astrophysics · Astrophysical Phenomena and Observations · Pulsars and Gravitational Waves Research · Black Holes and Theoretical Physics
0000-0001-7156-4848
Employment
-
Stellar Universe Founder2017 - Present
Education
- 2023 - Present
-
Charotar University of Science and Technology MSc. Physics (Astrophysics and Cosmology)2021 - 2023
-
Dyal Singh College BSc. Physics (Hons.)2017 - 2020
Projects & Funding
Projects & funding information is unavailable.
Publications (30)
- Broadband multiwavelength properties of the archetypal blazar $^{3}$C 279 during the 2017 Event Horizon Telescope campaign Save
- Dynamics and geometry of the inner sub-parsec-scale jet in $^{3}$C 279 observed with the Event Horizon Telescope Save
- Locating the missing large-scale emission in the jet of M87* with short EHT baselines Save
- Full-polarization millimeter wavelength variability of Sagittarius A* during the 2018 EHT campaign Save
- Ring Asymmetry and Spin in M87* Save
- Novel Polarimetric Analysis of Near-horizon Flaring Episodes in M87* in Millimeter Wavelength Save
- Probing jet base emission of M87* with the 2021 Event Horizon Telescope observations Save
- Spatially resolved polarization swings in the supermassive binary black hole candidate OJ 287 with first Event Horizon Telescope observations Save
- Horizon-scale variability of M87* from 2017–2021 EHT observations Save
- Author Correction: Fundamental physics opportunities with the next-generation Event Horizon Telescope Save
- Time delay of pulsar signals in astrophysical black hole spacetimes Save
- Shadow Formation Conditions Beyond the Kerr Black Hole Paradigm Save
- Semi-analytic studies of accretion disk and magnetic field geometry in M87* Save
- First polarization study of the M87 jet and active galactic nuclei at submillimeter wavelengths with ALMA Save
- Origin of the ring ellipticity in the black hole images of M87* Save
- Fundamental physics opportunities with future ground-based mm/sub-mm VLBI arrays Save
- Imaging ultracompact objects with radiatively inefficient accretion flows Save
- GALLIFRAY—A Geometric Modeling and Parameter Estimation Framework for Black Hole Images Using Bayesian Techniques Save
- Constraining wormhole geometries using the orbit of S2 star and the Event Horizon Telescope Save
- Thin accretion disk in the Simpson-Visser black-bounce and wormhole spacetimes Save