Savita Mathur

TL;DR: The Earth 2.0 (ET) mission as mentioned in this paper is designed to measure, for the first time, the occurrence rate and the orbital distributions of Earth-sized planets, and consists of seven 30cm telescopes, to be launched to the Earth-Sun's L2 point.

TL;DR: In this paper, the evolution of rotation and magnetic activity in solar-type stars appears to be strongly coupled during the first half of main-sequence lifetimes, and the authors aim to characterize this mid-life transition by combining archival stellar activity data from the Mount Wilson Observatory with asteroseismology from the Transiting Exoplanet Survey Satellite (TESS).

TL;DR: In this paper, the authors presented the first indirect detection of solar oscillations in intensity measurements using a global asteroseismic approach, which consists of measuring the oscillation frequency at maximum amplitude max velocity and the mean frequency separation between mode overtones delta velocity.

TL;DR: Mathur et al. as mentioned in this paper proposed a detection run for exoplanets and proposed a method to detect the existence of worlds in the solar system using the ApJS detection run.

TL;DR: In this article, the authors characterize the acoustic modes over the entire p-mode range in both, Doppler velocity and luminosity, with a special care for the low-frequency modes taking advantage of the stability and the high duty cycle of space observations.