IIAP Publications

 

Recent Submissions

  • Reshma, M; Stalin, C. S; Mandal, A. K; Kayal, Abhijit; Gudennavar, S. B; Joseph, P (Elsevier B.V., 2026-03)
    Active galactic nuclei are known to exhibit flux variations across the entire electromagnetic spectrum. Among these, correlations between UV/optical and X-ray flux variations serve as a key diagnostics for understanding ...
  • Choraghe, Komal; Mishra, Wageesh; Khuntia, Soumyaranjan (Oxford University Press on behalf of Royal Astronomical Society, 2026-03)
    The solar wind at 1 au is primarily super-Alfvénic, butrare instances occur when the Alfvén speed surpassesthe solar wind speed, resulting in occurrences of sub-Alfvénic intervals. During sub-Alfvénic intervals, the solar ...
  • Dagore, A; Joseph, P; Tandon, S. N; Subramaniam, A; Ghosh, S. K; Stalin, C. S (American Astronomical Society, 2026-03)
    The Ultra-Violet Imaging Telescope (UVIT) is one of the five payloads on board the first Indian multiwavelength astronomical observatory, AstroSat, launched by the Indian Space Research Organisation on 2015 September 28. ...
  • Sarkar, Sougata; Biswas, Prerana; Kalinova, Veselina; Roy, Nirupam; Patra, Narendra Nath; Kurapati, Sushma (Oxford University Press on behalf of Royal Astronomical Society, 2026-03)
    The distribution of dark matter in the inner regions of galaxies poses a key challenge for small-scale Lambda-cold dark matter (Λ-CDM) cosmology. While CDM simulations predict cuspy inner density profiles, observations ...
  • Mukhopadhyay, Swagata; Shantikumar, N. S; Uchiyama, Akihiro; Jorphail, S; Vivek, Chiranjeevi G; Shrungeshwara, T. S; Sreedevi, P; Matsunaga, Tsuneo; Sharma, S; Gupta, Pawan; Angchuk, D; Jade, S (Elsevier B.V., 2026-03-01)
    Sun–sky radiometer (model POM-01) is commonly used for studying aerosol optical and physical properties at selected aerosol-specific channels. Although the instrument is equipped with a precipitable water vapor (PWV) channel ...
  • Chand, Komal; Panthi, Anju; Vaidya, Kaushar (American Astronomical Society, 2026-03)
    Trumpler 5 is a populous, intermediate-age (∼3 Gyr), metal-poor ([Fe/H] ∼ −0.4) open cluster, located at a distance of approximately ∼3050 pc. This is a well-studied cluster for its broadened main-sequence (MS) and blue ...
  • Das, Hrishav; Sahu, D. K; Dutta, Anirban; Singh, Mridweeka; Anupama, G. C; Teja, Rishabh Singh (American Astronomical Society, 2026-03-01)
    We present comprehensive photometric and spectroscopic observations of SN 2022eyw, a luminous member of the Type Iax supernova (SN Iax) subclass. SN 2022eyw reached a peak absolute magnitude of Mg = –17.80 ± 0.15 mag and ...
  • Pradhan, Sunit Sundar; Joshi, Jayant; Samanta, T (American Astronomical Society, 2026-03-10)
    Coronal mass ejections (CMEs) often exhibit a three-part structure consisting of a bright inner core, an outer leading edge, and an intervening dark cavity. While the core has traditionally been attributed to prominence ...
  • Ahanger, Sajad; Shah, Zahir; Sahayanathan, S; Iqbal, Naseer; Malik, Zahoor; Manzoor, Aaqib (American Astronomical Society, 2026-03-10)
    We present a detailed temporal and spectral analysis of the blazar S5 1044+71 using multiwavelength data obtained from the Fermi-LAT and Swift-XRT/UVOT telescopes. Applying the Bayesian block algorithm to the 3-day binned ...
  • Bura, Annu; Nobrega-Siverio, Daniel; Samanta, T; Joshi, Jayant (American Astronomical Society, 2026-03-20)
    Small-scale jet-like eruptions, such as picoflare jets and jetlets, are recognized as potential contributors to coronal heating and solar wind acceleration, yet their physical origin is still not fully established. Using ...
  • Ni, Lei; Lin, Jun; Samanta, T; Cheng, Guanchong; Wang, Yifu; Erdelyi, Robertus (American Astronomical Society, 2026-03-20)
    How the solar atmosphere is heated from a temperature of about 5000 to 6000 K in the lower atmosphere to about 1–2 MK in the corona has challenged the astrophysical community for nearly 80 yr. The same puzzle exists for ...
  • Gupta, A. C; Volvach, A. E; Kishore, Shubham; Volvach, L. N; Wiita, P. J; Cui, Lang; Valtonen, Mauri J; Mondal, Sandeep K; Gaur, H (EDP Sciences, 2026-03)
    Context. Blazars are a subclass of radio-loud active galactic nuclei (AGN) that display strong multi-wavelength variability on diverse timescales ranging from years down to minutes. In the last 1.5 decades, there have been ...
  • Sharma, Vipin Kumar; Chaudhary, Himanshu; Kolekar, Sanved (Elsevier B.V., 2026-03)
    As an update on the initial findings of DESI, the new results provide the first hint of potential deviations from a cosmological constant (𝜔 = −1), which, if confirmed with significance > (2 − 4)𝜎, would challenge the ...
  • Kishore, Shubham; Gupta, A. C; Wiita, P. J (American Astronomical Society, 2026-02-20)
    Using an unprecedented cadence of 30 minutes provided by the Transiting Exoplanet Survey Satellite, we have examined the optical light curves (LCs) of the blazar S5 0716+714 obtained from its Sectors 40, 47, and 53 over ...
  • Nagdeo, Ameya Uday; Sur, Sharanya; Vaidya, Bhargav (American Astronomical Society, 2026-02-20)
    Fluctuation dynamos provide a robust mechanism for amplifying weak seed magnetic fields in turbulent astrophysical plasmas. However, their behaviour in the highly compressible regimes characteristic of the interstellar ...
  • Chand, Tarak; Sharma, Saurabh; Singh, Koshvendra; Ninan, J. P; Ghosh, Arpan; Ojha, D. K; Baug, Tapas; Sahu, D. K; Bhatt, B. C; Pramod Kumar, S; Yadav, R. K; Panwar, Neelam; Verma, Aayushi; Kaur, Harmeen; Mamta; Chakraborty, Manojit; Gokhe, Kartik; Singh, Ajay Kumar (American Astronomical Society, 2026-02-20)
    We present a detailed analysis of the long-term photometric and spectroscopic evolution of V1180 Cas over a decade, aiming to identify the dominant mechanisms behind its variability. We combine multiband light curves from ...
  • Rahul, Sharma; Beri, Aru; Paul, B; Sanna, Andrea; Maitra, Chandreyee; Yang, Haonan (EDP Sciences, 2026-02)
    Context. After nearly a decade of quiescence, the transient Be/X-ray binary pulsar RX J0520.5–6932 underwent an outburst in 2024. Weperformed X-ray monitoring of the source with NICER and AstroSat near the peak of the ...
  • Kapoor, R. C (National Astronomical Research Institute of Thailand, 2025-09)
    In this paper we provide information on some of the telescopes to which one of the most prominent names in the history of astronomy is attached: Frederick William Herschel. He built telescopes of different apertures and ...
  • Kapoor, R. C (National Astronomical Research Institute of Thailand, 2025-09)
    Planets passing across the disk of the Sun are among the most uncommon and fascinating phenomena in the Solar System. From the Earth, the transits of only Mercury and Venus can be seen. Early on, the transits of Venus were ...
  • Shubham Jankiram, Ghatul; Mohan, Rekhesh; Murthy, J; Safonova, M; Kumar, P; Gopinathan, Maheswar; Jain, Shubhangi; Mahesh Babu, S (Frontiers, 2025-12)
    The Near Ultraviolet Transient Explorer (NUTEx) is a CubeSat-based nearultraviolet (NUV) imaging payload designed for transient sky surveys and is currently under development. CubeSats are compact and cost-effective satellite ...

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