IIA Institutional Repository: Recent submissions

  • Kesri, Kartav; Dey, Sahel; Chatterjee, Piyali; Erdelyi, Robertus (The American Astronomical Society, 2024-09-20)
    Solar spicules are plasma jets observed in the interface region between the visible solar surface and the corona. At any given time, there is a forest of spicules originating in the chromosphere of the Sun. While various ...
  • Paswan, Abhishek; Das, Mousumi; Rubinur, K (The American Astronomical Society, 2024-09-10)
    In the last decade, there have been several discoveries of active galactic nuclei (AGN) in dwarf galaxies including an AGN in an ultracompact dwarf galaxy with a black hole mass >106 Me. However, finding a supermassive ...
  • Chatterjee, Debjit; Jana, A; Chang, Hsiang-Kuang (The American Astronomical Society, 2024-09-01)
    Soft X-ray transients (SXTs) are a subclass of the low-mass X-ray binaries that occasionally show a sudden rise in their soft X-ray luminosity; otherwise, they remain in an extremely faint state. We investigate the accretion ...
  • Kumar, Hirdesh; Brajesh Kumar; Mathew, Shibu K; Bayanna, A. Raja; Rajaguru, S. P (The American Astronomical Society, 2024-09-01)
    We report and discuss the phase shift and phase travel time of low-frequency (ν < 5.0 mHz) acoustic waves estimated within the photosphere and photosphere–chromosphere interface regions, utilizing multiheight velocities ...
  • Nayak, Prasanta K; Narang, Mayank; Manoj, P; Gorti, U; Subramaniam, Annapurni; George, Nayana; Mondal, Chayan (The American Astronomical Society, 2024-09-01)
    We present results from simultaneous far-ultraviolet (FUV) and near-ultraviolet (NUV) observations of T Tauri stars (TTSs) in the Taurus molecular cloud with UVIT/AstroSat. This is the very first UVIT study of TTSs. ...
  • Neha, S; Archana Soam; Maheswar, G (EDP Sciences, 2024-09)
    We present an optical polarimetry study of the nearby star-forming region Lambda-Orionis to map the plane-of-the-sky magnetic field geometry to understand the magnetized evolution of the HII region and the associated small ...
  • Aditya, K (EDP Sciences, 2024-09)
    Aims. The discovery of NGC 1052−DF2 and subsequent modeling have shown that NGC 1052−DF2 is deficient in dark matter and is in conflict with the standard stellar-to-halo mass ratio. In this work, we aim to resolve the ...
  • Bhatnagar, Aditi; van der Voort, Luc Rouppe; Joshi, Jayant (EDP Sciences, 2024-09)
    Context. Quiet-Sun Ellerman bombs (QSEBs) are key indicators of small-scale photospheric magnetic reconnection events. Recent high-resolution observations have shown that they are ubiquitous and that large numbers of QSEBs ...
  • Skirvin, S. J; Samanta, T; Van Doorsselaere, T (EDP Sciences, 2024-09)
    Aims. Propagating (intensity) disturbances (PDs) have been extensively reported in observations of coronal loops and polar plumes, along with more recent links to co-temporal spicule activity in the solar atmosphere. ...
  • Kangas, T; Kuncarayakti, H; Nagao, T; Kotak, R; Kankare, E; Fraser, M; Stevance, H; Mattila, S; Maeda, K; Stritzinger, M; Lundqvist, P; Elias-Rosa, N; Ferrari, L; Folatelli, G; Frohmaier, C; Galbany, L; Kawabata, M; Koutsiona, E; Muller-Bravo, T. E; Piscarreta, L; Pursiainen, M; Singh, A; Taguchi, K; Teja, R. S; Valerin, G; Pastorello, A; Benetti, S; Cai, Y. Z; Charalampopoulos, P; Gutierrez, C. P; Kravtsov, T; Reguitti, A (EDP Sciences, 2024-09)
    We present optical and near-infrared photometry and spectroscopy of SN 2023aew and our findings on its remarkable properties. This event, initially resembling a Type IIb supernova (SN), rebrightens dramatically ∼90 d after ...
  • Inkenhaag, Anne; Jonker, Peter G; Levan, A. J; Vásquez, Jonathan Quirola; Bauer, Franz E; Deepak, Eappachen (EDP Sciences, 2024-09)
    Context. Fast X-ray transients (FXTs) are X-ray flares that last from minutes to hours. Multi-wavelength counterparts to these FXTs have proven hard to find. As a result, distance measurements are made through indirect ...
  • Shrivastav, Arpit Kumar; Pant, Vaibhav; Antolin, Patrik (EDP Sciences, 2024-09)
    Decayless kink oscillations are ubiquitously observed in active region coronal loops with an almost constant amplitude for several cycles. Decayless kink oscillations of coronal loops triggered by coronal rain have been ...
  • Joshi, Arti; Catelan, Marcio; Scaringi, Simone; Schwope, Axel; Anupama, G. C; Rawat, Nikita; Sahu, D. K; Singh, Mridweeka; Dastidar, Raya; Subramanian, Rama Venkata; Rao, Srinivas M (EDP Sciences, 2024-09)
    We present the analysis of optical photometric and spectroscopic observations of two non-magnetic cataclysmic variables, namely CRTS J080846.2+313106 and V416 Dra. We find CRTS J080846.2+313106 to vary with a period of ...
  • Yadav, Jyoti; Jadhav, Vikrant V (EDP Sciences, 2024-09)
    Galaxy interactions in groups can lead to intense starbursts and the activation of active galactic nuclei (AGNs). The stripped gas from the outer disk can lead to star-forming clumps along the tidal tails or sometimes tidal ...
  • Poojary, S. S; Krishna Reddy, B; Ninan, Joe. P; Shah, Harshit; Ojha, D.K; Sharma, Saurabh; Reji, Varghese; Surya, Arun; Udhwani, Purvi; Costa, S. L. D; Naik, M. B; Mookerjea, B; Puravankara, Manoj; Tendulkar, Shriharsh; Jadhav, R. B; Sandimani, P. R; Gharat, S. M; Bhagat, S. B; Jadhav, Krushna (SPIE - Society of Photo-Optical Instrumentation Engineers, 2024-06)
    TA-MOONS is a multi-object Optical to Near Infrared (NIR) spectrometer with the primary science cases to conduct a spectroscopic survey of Young Stellar Objects (YSO’s) at visible as well as at NIR wavebands simultaneously ...
  • Singh, Nitish; Sriram, S; Bharat Kumar, Y; Prasanna, Deshmukh (SPIE - Society of Photo-Optical Instrumentation Engineers, 2024-06)
    In fiber-based spectroscopy within telescopes, a prevailing limitation has been the necessity to align the fiber diameter with the telescope’s seeing conditions, often characterized by the Full Width at Half Maximum of ...
  • Singh, Nitish; Sriram, S; Bharat Kumar, Y; Prasanna, Deshmukh (SPIE - Society of Photo-Optical Instrumentation Engineers, 2024-06)
    The 2.34m Vainu Bappu Telescope (VBT) is a reflecting telescope that operates in two modes, prime focus and cassegrain focus, and is equipped with two instruments. In prime focus mode, the telescope has the F-number ...
  • Wright, Shelley A; Jones, Tucker; Larkin, James; Kupke, Renate; Kassis, Marc; Brown, Aaron; Andersen, David; Armus, Lee; Cale, Bryson; Cosens, Maren; Chu, Devin; Do, Tuan; Fassanacht, Chris; Fisher, Deanne; Fitzgerald, Michael; Ghez, Andrea; Greene, Jenny; Hayashi, Takeru; Hees, Aurelien; Hirtenstein, Jessie; Johnson, Chris; Keane, Jacqueline; Kelly, Patrick; Kirbyo, Evan; Karalidi, Theodora; Konopackya, Quinn; Kress, Evan; Lu, Jessica; Lyke, Jim; Magnone, Kenneth; Maire, Jerome; McGurk, Rosalie; Medling, Anne; Millar-Blanchaer, Maxwell; Minor, Quinn; Nash, Reston; Nierenberg, Anna; Reddy, Naveen; Rich, Michael; Ruffio, Jean-Baptiste; Rundquist, Nils-Erik; Sabhlok, Sanchit; Sand, David; Sanders, Ryan; Sandstrom, Karin; Shapley, Alice; Sohn, Ji-Man; Surya, Arun; Treu, Tommaso; Wang, Eric; Warad, Kanaka; Weber, Robert; Wiley, James; Wizinowich, Peter; Wong, Michael H.; Yeh, Sherry (SPIE - Society of Photo-Optical Instrumentation Engineers, 2024-06)
    Liger is a next-generation near-infrared (0.81 - 2.45 µm) integral field spectrograph (IFS) and imaging camera for the W. M. Keck Observatory (WMKO) adaptive optics (AO) system. The instrument concept originated by ...
  • Radhika, Dharmadhikari; Parihar, P. S (SPIE - Society of Photo-Optical Instrumentation Engineers, 2024-06)
    For a segmented mirror telescope, the desired resolution can only be achieved when all the segments are precisely co-aligned, co-focused and co-phased. The process of minimization of the piston errors is called co-phasing, ...
  • Saraswathi Kalyani, S; Sridharan, R; Prasanna, Deshmukh; Nair, B. G; Mahesh Babu, S (SPIE - Society of Photo-Optical Instrumentation Engineers, 2024-07)
    The Indian Institute of Astrophysics is developing a Multi-Conjugate Adaptive Optics system for the Kodaikanal Tower Telescope. In this context, we measured the daytime turbulence strength profile at the Kodaikanal ...

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