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Issue DateTitleAuthor(s)
2024-10-01Casting light on degeneracies: A comprehensive study of lightcurve variations in microlensing events OGLE-2017-BLG-0103 and OGLE-2017-BLG-0192Shah, Sarang
2024-10Full non-LTE spectral line formation III. The case of a two-level atom with broadened upper levelSampoorna, M; Paletou, F; Bommier, V; Lagache, T
2023-12-20Correlation between Supergranular Lane Widths and Sunspot Number; A Simple Way to Predict the Amplitude of Sunspot CycleRaju, K. P; Singh, J; Ravindra, B; Priyal, M
2024-10-01Redshifted sodium transient near exoplanet transitOza, Apurva V; Seidel, Julia V; Hoeijmakers, H. Jens; Unni, Athira; Kesseli, Aurora Y; Schmid, Carl A; Sivarani, T; Bello-Arufe, Aaron; Gebek, Andrea; Moritz Meyer zu, Westram; Sousa, S. G; Lopes, Rosaly M. C; Hu, Renyu; Kleer, Katherine de; Fisher, Chloe; Charnoz, Sebastien; Baker, Ashley D; Halverson, Sam; Schneider, Nick M; Psaridi, Angelica; Wyttenbach, Aurelien; Torres, Santiago; Bhatnagar, Ishita; Johnson, Robert E
2024-11-10Exploring the dynamic rotational profile of the hotter solar atmosphere: A multiwavelength approach using SDO/AIA dataRouth, Srinjana; Jha, Bibhuti K; Mishra, Dibya Kirti; Doorsselaere, Tom Van; Pant, V; Chatterjee, Subhamoy; Banerjee, D
2024-10Investigative study of five low mass ratio semi-detached binariesVinay Kumar, G; Devarapalli, Shanti Priya; Parthasarathy, M; Jagirdar, Rukmini; Stassun, K. G
2024-11Non-conventional approach for deriving the radial sizes of coronal mass ejections at different instances: discrepancies in the estimates between remote and in situ observationsAgarwal, Anjali; Mishra, Wageesh
2024-10Long term CCD photometry of the distant cluster NGC2419: The CMD revisitedArellano Ferro, A; Muneer, S; Giridhar, S; Bustos Fierro, I; Yepez, M. A; Garcia Perez, G. A; Rios Segura, G
2024-10-20Helium Abundance of the Sun: A Spectroscopic AnalysisMoharana, Satyajeet; Hema, B. P; Pandey, Gajendra
2021-10Planetary nebulae with UVIT: A progress reportKameswara Rao, N; Sutaria, F. K; Murthy, J; Ray, A; Pandey, G

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