activity
20142024
most citedApex determination and detection of stellar clumps in the open cluster M 67

19 citations · 51 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.EP2024

Probing the Possible Causes of the Transit Timing Variation for TrES-2b in TESS Era

Shraddha Biswas, D. Bisht, Ing-Guey Jiang +2

Nowadays, transit timing variations (TTVs) are proving to be a very valuable tool in exoplanetary science to detect exoplanets by observing variations in transit times. To study th…

astro-ph.EP20243 cited

Constraining Planetary Formation Models Using Conditional Occurrences of Various Planet Types

Sridhar Gajendran, Ing-Guey Jiang, Li-Chin Yeh +1

We report the conditional occurrences between three planetary types: super-Earths (m sin i 10 M, P 100 days), warm Jupiters (m sin i 95 , 10 P $<…

astro-ph.GA20236 cited

Investigating kinematics and dynamics of three open clusters towards Galactic anti-center

Geeta Rangwal, R. K. S. Yadav, D. Bisht +2

We present the intra-cluster kinematics and dynamics of three open clusters: NGC 1193, NGC 2355, and King 12 by incorporating kinematical and photometric data from Gaia DR3, as wel…

astro-ph.EP202110 cited

The Transit Timing and Atmosphere of Hot Jupiter HAT-P-37b

Napaporn A-thano, Ing-Guey Jiang, Supachai Awiphan +13

The transit timing variation (TTV) and transmission spectroscopy analyses of the planet HAT-P-37b, which is a hot Jupiter orbiting an G-type star, were performed. Nine new transit…

astro-ph.SR201713 cited

A proper motions study of the globular cluster NGC 3201

Devesh P. Sariya, Ing-Guey Jiang, R. K. S. Yadav

With a high value of heliocentric radial velocity, a retrograde orbit, and being suspected to have an extragalactic origin, NGC 3201 is an interesting globular cluster for kinemati…

astro-ph.GA201419 cited

Apex determination and detection of stellar clumps in the open cluster M 67

S. V. Vereshchagin, N. V. Chupina, Devesh P. Sariya +2

We determined the cluster apex coordinates, studied the substructures and performed membership analysis in the central part (34'X33') of the open cluster M 67. We used the individu…