activity
20202026
most citedML-MOC: Machine Learning (kNN and GMM) based Membership Determination for Open Clusters

69 citations · 280 across the 18 of their papers we have counts for

collaborators

18 papers

astro-ph.GA2026

Examining the stellar-merger origin of the blue main sequence in the open cluster NGC\,3532 with N-body simulations

Khushboo K. Rao, Sambaran Banerjee

Extended main-sequence turnoffs, extended main sequences, and split main sequences observed in the colour-magnitude diagrams of young and intermediate-age star clusters are now wid…

astro-ph.GA2026

Investigating Extended Main-Sequence Turnoffs in Galactic Open Clusters

Khushboo K Rao, Wen-Ping Chen

The extended main sequence (eMS) and extended main sequence turnoff (eMSTO) phenomena have been observed in some young and intermediate-age star clusters in the Milky Way and in th…

astro-ph.SR2026★ 2 cited

A rotation-based census of blue lurker candidates in open clusters

Vikrant V. Jadhav, Khushboo K. Rao, Elisabetta Reggiani

Blue lurkers (BLs) are rejuvenated main-sequence stars hidden among normal main-sequence stars on color-magnitude diagrams of star clusters. In comparison, the blue straggler stars…

astro-ph.GA2026

The Secret Lives of Open Clusters: a Multiwavelength Examination of Three Open Clusters

Kristen C. Dage, Emily L. Hunt, Jasmine Anderson-Baldwin +11

Star clusters are well known for their dynamical interactions, an outcome of their high stellar densities; in this paper we use multiwavelength observations to search for the uniqu…

astro-ph.GA2025

Investigating Unusually Extended Main Sequence Turnoff of the Galactic Open Cluster NGC 3532

Khushboo K Rao, Wen-Ping Chen

Extended main-sequence turnoffs are observed in the color-magnitude diagrams of some young and intermediate-age star clusters. Here we report the case study of NGC 3532. Among the…

astro-ph.SR2024

Characterization of blue and yellow straggler stars of Berkeley 39 using Swift/UVOT

Komal Chand, Khushboo Rao, Kaushar Vaidya +1

We characterize blue straggler stars (BSS) and yellow straggler stars (YSS) of an open cluster (OC) Berkeley 39 using multi-wavelength observations including Swift/UVOT. Our analys…

astro-ph.GA2024

Dynamical Evolution of Four Old Galactic Open Clusters traced by their constituent stars with \textit{Gaia} DR3

Shanmugha Balan, Khushboo K Rao, Kaushar Vaidya +2

We investigate the evolutionary stages of four open clusters, Berkeley 39, Collinder 261, NGC 6819, and NGC 7789, of ages ranging from 1.6 -- 6 Gyr. These clusters have previously…

astro-ph.GA2023

Determination of dynamical ages of open clusters through the A parameter -- II

Khushboo K. Rao, Kaushar Vaidya, Manan Agarwal +2

Blue straggler stars (BSS), one of the most massive members of star clusters, have been used for over a decade to investigate mass segregation and estimate the dynamical ages of gl…

astro-ph.GA2023

Hot Stellar Populations of Berkeley 39 using Swift/UVOT

Komal Chand, Khushboo Kunwar Rao, Kaushar Vaidya +1

Open clusters are excellent tools to probe the history of the Galactic disk and properties of star formation. In this work, we present a study of an old age open cluster Berkley 39…

astro-ph.GA2022★ 13 cited

Discovery of double BSS sequences in the old Galactic open cluster Berkeley 17

Khushboo K Rao, Souradeep Bhattacharya, Kaushar Vaidya +1

Blue straggler stars (BSS) are peculiar objects which normally appear as a single broad sequence along the extension of the main sequence. Only four globular clusters (GCs) have be…

astro-ph.GA2022★ 32 cited

A EDR3 search for tidal tails in disintegrating open clusters

Souradeep Bhattacharya, Khushboo K. Rao, Manan Agarwal +2

We carry out a search for tidal tails in a sample of open clusters with known relatively elongated morphology. We identify the member stars of these clusters from the precise astro…

astro-ph.GA2022★ 22 cited

UOCS-VIII. UV Study of the open cluster NGC 2506 using ASTROSAT

Anju Panthi, Kaushar Vaidya, Vikrant Jadhav +4

We study an intermediate-age open cluster NGC 2506 using the \textit{ASTROSAT}/UVIT data and other archival data. We identified 2175 cluster members using a machine learning-based…

astro-ph.GA2022★ 20 cited

Characterization of hot populations of Melotte 66 open cluster using Swift/UVOT

K. K. Rao, K. Vaidya, M. Agarwal +3

Ultraviolet (UV) wavelength observations have made a significant contribution to our understanding of hot stellar populations of star clusters. Multi-wavelength spectral energy dis…

astro-ph.SR2022★ 31 cited

UOCS VII. Blue Straggler Populations of Open Cluster NGC 7789 with UVIT/AstroSat

Kaushar Vaidya, Anju Panthi, Manan Agarwal +4

NGC 7789 is a 1.6 Gyr old, populous open cluster located at 2000 pc. We characterize the blue straggler stars (BSS) of this cluster using the Ultraviolet (UV) data from…

astro-ph.GA2021★ 33 cited

Tidal tails in the disintegrating open cluster NGC 752

Souradeep Bhattacharya, Manan Agarwal, Khushboo K. Rao +1

We utilize the robust membership determination algorithm, ML-MOC, on the precise astrometric and deep photometric data from Gaia Early Data Release 3 within a region of radius 5$^{…

astro-ph.GA2021★ 20 cited

Determination of dynamical ages of open clusters through the A parameter -- I

Khushboo K. Rao, Kaushar Vaidya, Manan Agarwal +1

The sedimentation level of blue straggler stars (BSS) has been shown to be a great tool to investigate the dynamical states of globular clusters (GCs). The area enclosed between th…

astro-ph.IM2020★ 69 cited

ML-MOC: Machine Learning (kNN and GMM) based Membership Determination for Open Clusters

Manan Agarwal, Khushboo K. Rao, Kaushar Vaidya +1

The existing open cluster membership determination algorithms are either prior dependent on some known parameters of clusters or are not automatable to large samples of clusters. I…

astro-ph.GA2020★ 38 cited

Blue Straggler Populations of Seven Open Clusters with Gaia DR2

Kaushar Vaidya, Khushboo K. Rao, Manan Agarwal +1

Blue straggler stars (BSS) are well studied in globular clusters but their systematic study with secure membership determination is lacking in open clusters. We use Gaia DR2 data t…