Projects
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Poster presented at PLATO Stellar Science Conference
June 26-30, 2023
Corner plot of an Eclipsing Binaries
Dec. 07, 2021
It is shows the uncretainity in our models and fit with the corelation in parameter-space. This is just a sample with a few hundreds of iterations, uncreatainity can be reduce by increasing number of iterations to a few 10's of thousand but it is computationally very expensive.
Forward model of a Heartbeat star using PHOEBE
Oct. 15, 2021
PHysics Of Eclipsing BinariEs (PHOEBE) is an eclipsing binary modeling code written in python with a great documentation.
DSLR photometry of AD CMi, a δ Scuti variable star
Dec. 22, 2017
The δ Scuti stars are population-I pulsating stars, they lies in classical instability strip with mass ranges from 1.5-2.5M⊙. It has a short period of variability, ranges from 18 min to 8 hr. AD CMi is the high amplitude δ Scuti stars (HADS). The below light curve is a result of our team's effort (Akashmitra Mandal) and it shows a period of 2.513 hr.
