activity
20152025
most citedThe Nainital-Cape Survey-IV

35 citations · 135 across the 15 of their papers we have counts for

collaborators

15 papers

astro-ph.SR2025★ 1 cited

The impact of stellar rotations and binaries on the shape of upper main sequence near turn off in open cluster NGC\,6067

Jayanand Maurya, Yu Zhang, Sebastian Kamann +7

We present the analysis of the extended Main Sequence Turn-Off (eMSTO) in the open cluster NGC\,6067. We derive the projected rotational velocity, \textit{v}sin\textit{i}, of the s…

astro-ph.SR2025

Exploring Contact Binaries: Observational Analysis of four W Uma Binaries Using Photometry and Spectroscopy

Alaxender Panchal, Yogesh Chandra Joshi, Vishal Joshi +1

We present the multi-band photometric and low-resolution spectroscopic analysis of four W Ursae Majoris eclipsing binaries (EWs) - J080510.1+141528 (hereinafter as J0805a), J080516…

astro-ph.SR2025

Investigating Pulsating Variables and Eclipsing Binaries in NGC 2126 using Ground and Space-based Photometry, Astrometry, Spectroscopy and Modeling

Athul Dileep, Santosh Joshi, Sneh Lata +12

Pulsating variables are prevalent in the classical δ Scuti instability strip of intermediate-age open star clusters. The cluster membership of these stars facilitates a comparative…

astro-ph.EP2024

Low-resolution Transit Spectroscopy of Three Hot Jupiters Using the 2m Himalayan Chandra Telescope

Athira Unni, Thirupathi Sivarani, Jayesh Goyal +3

Here, we present the low-resolution transmission spectroscopy of three giant planets using the Himalayan Faint Object Spectrograph Camera (HFOSC) on the 2m Himalayan Chandra Telesc…

astro-ph.EP2024

Transit Timing Variation of K2-237b: Hints Toward Planet Disk Migration

Fan Yang, Richard J. Long, Eamonn Kerins +8

Hot Jupiters should initially form at considerable distances from host stars and subsequently migrate towards inner regions, supported directly by transit timing variation (TTV). W…

astro-ph.SR2024

Origin of extended Main Sequence Turn Off in open cluster NGC 2355

Jayanand Maurya, M. R. Samal, Louis Amard +5

The presence of extended Main Sequence Turn-Off (eMSTO) in the open clusters has been attributed to various factors, such as spread in rotation rates, binary stars, and dust-like e…