K. J. Nikitha
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View article: A Swarm of WASP Planets: Nine Giant Planets Identified by the WASP Survey
A Swarm of WASP Planets: Nine Giant Planets Identified by the WASP Survey Open
The Wide Angle Search for Planets (WASP) survey provided some of the first transiting hot Jupiter candidates. With the addition of the Transiting Exoplanet Survey Satellite (TESS), many WASP planet candidates have now been revisited and gi…
View article: A Swarm of WASP Planets: Nine giant planets identified by the WASP survey
A Swarm of WASP Planets: Nine giant planets identified by the WASP survey Open
The Wide Angle Search for Planets (WASP) survey provided some of the first transiting hot Jupiter candidates. With the addition of the Transiting Exoplanet Survey Satellite (TESS), many WASP planet candidates have now been revisited and gi…
View article: TOI-6038 A b: A Dense Sub-Saturn in the Transition Regime between the Neptunian Ridge and Savanna
TOI-6038 A b: A Dense Sub-Saturn in the Transition Regime between the Neptunian Ridge and Savanna Open
We present the discovery and characterization of a sub-Saturn exoplanet, TOI-6038 A b, using the PARAS-2 spectrograph. The planet orbits a bright ( m V = 9.9), metal-rich late F-type star, TOI-6038 A, with T eff = 6110 ± 100 K, …
View article: TOI-6038 A b: A dense sub-Saturn in the transition regime between the Neptunian ridge and savanna
TOI-6038 A b: A dense sub-Saturn in the transition regime between the Neptunian ridge and savanna Open
We present the discovery and characterization of a sub-Saturn exoplanet, TOI-6038~A~b, using the PARAS-2 spectrograph. The planet orbits a bright ($m_V=9.9$), metal-rich late F-type star, TOI-6038~A, with $T_{\rm{eff}}=6110\pm100~\mathrm{K…
View article: Discovery and characterization of a dense sub-Saturn TOI-6651b
Discovery and characterization of a dense sub-Saturn TOI-6651b Open
We report the discovery and characterization of a transiting sub-Saturn exoplanet TOI-6651b using PARAS-2 spectroscopic observations. The host, TOI-6651 ( m V ≈ 10.2), is a sub-giant, metal-rich G-type star with [Fe / H] = 0.225 −0.045 0.0…
View article: Stellar populations of the globular cluster NGC 5053 investigated using <i>AstroSat</i>-Ultra Violet Imaging Telescope
Stellar populations of the globular cluster NGC 5053 investigated using <i>AstroSat</i>-Ultra Violet Imaging Telescope Open
Globular clusters (GCs), being old and densely packed, serve as ideal laboratories to test stellar evolution theories. Although there is enormous literature on GCs in optical bands, studies in the ultraviolet (UV) regime are sparse. In thi…