• A search for successful and choked jets in nearby broad-lined type Ic supernovae 

  O'Dwyer, Tanner; Corsi, Alessandra; Yang, Sheng; Anand, Shreya; Cenko, S. Bradley; Srinivasaragavan, Gokul P; Ho, Anna Y. Q; Sollerman, Jesper; Zhou, Bei; Balasubramanian, Arvind; Chang, Po-Wen; Kamionkowski, Marc; Perley, Daniel A; Laher, Russ R; Murase, Kohta; Masci, Frank J; Kasliwal, Mansi M; Purdum, Josiah; Graham, Matthew J (American Astronomical Society, 2026-05-10)

  The observational link between long gamma-ray bursts (GRBs) and broad-lined stripped-envelope core-collapse supernovae (SNe Ic-BL) is well established. Significant progress has been made in constraining what fraction ...
• Finding the evolutionary link between ULIRGs and radio galaxies 

  Fida, Ayisha; Nandi, Sumana; Mousumi Das; Rubinur, K; Shanbhog, S; Kharb, P; Dev, Barenya (Oxford University Press on behalf of the Royal Astronomical Society, 2026-07)

  Ultraluminous infrared galaxies (ULIRGs) are the remnants of the major mergers of gas-rich galaxies. They are dusty systems and are extremely luminous in the infrared. Both starbursts and active galactic nucleus (AGN) ...
• The CAVITY project: The spatially resolved star formation rate of galaxies in voids 

  Conrado, Ana M; Garcia-Benito, Ruben; González Delgado, R. M; Bidaran, Bahar; Courtois, Helene M; Duarte Puertas, S; Espada, Daniel; Jimenez, Andoni; del Moral-Castro, Ignacio; Perez, Isabel; Ruiz-Lara, Tomas; Sanchez-Menguiano, Laura; Torres-Rios, Gloria; Verley, Simon; Argudo-Fernandez, Maria; De Daniloff, Simon B; Florido, Estrella; Gonzalez-Koda, Yllari K; Lugo-Aranda, Alejandra Z; Roman, Javier; Subramanian, S; Villalba-Gonzalez, Pedro; Alcazar-Laynez, Manuel; Hernandez-Sanchez, Monica; Rodríguez Martínez, Mónica; Vasquez-Bustos, Paulo; Blazek, Martin (EDP Sciences, 2026-05)

  The mass in the Universe is distributed non-uniformly, leading to the large scale structure (LSS), characterised by clusters, filaments, walls, and voids. Galaxies in voids have been found to be bluer, of later type, less ...
• X-Ray and radio campaign of the Z-source GX 340+0. II. the X-Ray polarization in the normal branch 

  Bhargava, Yash; Russell, Thomas D; Ng, Mason; Balasubramanian, Arvind; Zhang, Liang; Ravi, Swati; Jadoliya, Vishal; Bhattacharyya, Sudip; Pahari, Mayukh; Homan, Jeroen; Marshall, H. L; Chakrabarty, Deepto; Carotenuto, Francesco; Kaushik, Aman (American Astronomical Society, 2026-05-20)

  We present the first X-ray polarization measurement of the neutron star low-mass X-ray binary and Z-source, GX 340+0, in the normal branch (NB) using a 200 ks observation with the Imaging X-ray Polarimetric Explorer (IXPE). ...
• The heritage of astronomical manuscripts in Mysore 

  Shubha, B. S; Shylaja, B. S; Subramaniam, A (IOP Publishing, 2026-05)

  The Mysore region, in south India has a rich heritage of astronomical manuscripts, with a significant collection preserved at the Oriental Research Institute (ORI), University of Mysore and numerous private family collections. ...
• Unveiling viśvanātha 's mathematical innovations in astronomy manuscripts 

  Shubha, B. S (IOP Publishing, 2026-05)

  Viśvanātha is a well-known name in north India, who wrote many commentaries on different astronomy texts during 16th century. His work showcases methods for achieving accuracy in predictions of astronomical events. His ...
• Cosmic duets: I. high-spatial resolution spectroscopy of dual and lensed active galactic nuclei with MUSE-NFM 

  Scialpi, M; Mannucci, F; D’Amato, Q; Marconcini, C; Cresci, G; Marconi, A; Ulivi, L; Fumagalli, Michele; Rosati, P; Tozzi, G; Zanchettin, M. V; Battistini, L; Bertola, E; Bracci, C; Carniani, S; Cataldi, E; Ceci, M; Chakraborty, Avinanda; Cicone, C; Ciurlo, A; De Rosa, A; Di Rosa, G; Feltre, A; Ginolfi, M; Lamperti, I; Lusso, E; Moreschini, B; Nardini, E; Parvatikar, M; Perna, M; Rubinur, K; Severgnini, P; Singh, Jasbir; Spingola, C; Venturi, G; Vignali, C; Volonteri, M (EDP Sciences, 2026-05)

  We present the first-year results of the MUSE Large Program "Cosmic Duets", whose goal is to obtain adaptive-optics assisted MUSE observations with a typical angular resolution of 0.1″ − 0.2″ in order to provide integral-field ...
• Validating a non-conventional method for expansion of coronal mass ejections (CMEs) and investigating the evolution of a CME substructures using solar orbiter and wind observations 

  Agarwal, Anjali; Mishra, Wageesh; Owens, Mathew J; Amerstorfer, T (Wiley on behalf of American Geophysical Union, 2026-05)

  We present a validation of our recently proposed non‐conventional method, Constant Acceleration Accounted Perspective (CAAP), for estimating the instantaneous expansion speed of coronal mass ejection (CMEs), even when only ...
• LeMMINGs VII: 5-GHz 50-mas e-MERLIN observations of a statistically complete sample of nearby AGNs 

  Williams-Baldwin, D. R. A; Baldi, R. D; Beswick, R. J; McHardy, I. M; Carver, E; Clifford, J; Dullo, B. T; Kill, N; Krishnamoorthi, B; Mutie, I. M; Woodcock, O; Argo, M; Boorman, P; Brinks, E; Fenech, D. M; Knapen, J. H; Mathur, Smita; Moldon, J; Muxlow, T. W. B; Pahari, Mayukh; Wrigley, N. H; Alberdi, A; Baan, W; Beri, Aru; Cheng, X; Green, D. A; Healy, J; Kharb, P; Kording, E; Lucatelli, G; Panessa, F; Puig-Subira, M; Romero-Canizales, C; Saikia, D. J; Saikia, Payaswini; Shankar, F; Sharma, S; Stevens, I. R; Varenius, E (Oxford University Press on behalf of Royal Astronomical Society, 2026-05)

  We present 5 GHz e-MERLIN radio images at 50 mas resolution of the nuclear regions of the Legacy e-MERLIN Multi-band Imaging of Nearby Galaxies survey (LeMMINGs): the deepest statistically complete radio-band survey of the ...
• UVIT magellanic BRidge analysis (UMBRA) – I. Far-UV–Gaia study of seven star clusters 

  Choudhury, Samyaday; Nayak, Prasanta K; Dhanush, S. R; Sahu, S; de Grijs, R (Oxford University Press on behalf of Royal Astronomical Society, 2026-05)

  We present the first high spatial resolution far-ultraviolet (FUV; F148W) images of seven star clusters in the Magellanic Bridge using the UltraViolet Imaging Telescope (UVIT) on the Indian multiwavelength space observatory ...
• The GMRT archive atomic gas survey – IV. consistency of the dark matter halo perturbation parameter from morphological and kinematic lopsidedness of galaxies 

  Biswas, Prerana; Patra, Narendra Nath; Kalinova, Veselina (Oxford University Press on behalf of the Royal Astronomical Society, 2026-05)

  The lopsidedness of galaxies is a commonly observed phenomenon, and through different studies, it has been observed that nearly 30 % of galaxies show this phenomenon. In this work, we study morphological lopsidedness in ...
• Active-region modulation of subsurface meridional flows and magnetic flux transport on the sun 

  Sen, Anisha; Rajaguru, S. P; Chen, Ruizhu; Zhao, Junwei; Kholikov, S (American Astronomical Society, 2026-05-01)

  Using time–distance helioseismology applied to 14 yr of Solar Dynamics Observatory/Helioseismic and Magnetic Imager observations spanning solar cycle 24 and the rising phase of cycle 25, we present evidence that meridional ...
• Cloud fraction estimation using random forest classifier on sky images 

  Sarangi, Sougat Kumar; Sarangi, Chandan; Patel, Niravkumar; Madhavan, B. L; Shantikumar, N. S; Ravindra, B; Ratnam, Madineni Venkat (Copernicus Publications on behalf of the European Geosciences Union, 2025-10)

  Cloud fraction (CF) is an integral aspect of weather and radiation forecasting, but real time monitoring of CF is still inaccurate, expensive and exclusive to commercial sky imagers. Traditional cloud segmentation methods, ...
• Morphological complexity of NGC 628—a multiwavelength multiscale analysis using the ordinal pattern framework 

  Chanu, Athokpam Langlen; Amrutha, S; Pravabati, C; Park, C (American Astronomical Society, 2026-05-20)

  As statistical systems, galaxies exhibit a rich interplay between organized structure and stochastic fluctuations across a broad range of spatial scales. This duality motivates the need for quantitative frameworks capable ...
• Temporal variation in the coronal radius parameter in a jetted tidal disruption event: Swift J1644+57 

  Chatterjee, Arka; Hayasaki, Kimitake; Nandi, Prantik; Neeraj, Kumari; Heiland, Skye R; Jana, Arghajit; Naik, Sachindra; Safi-Harb, Samar (American Astronomical Society, 2026-05-01)

  Tidal disruption events are exotic astrophysical phenomena where matter from a star or the interstellar medium is captured by a supermassive black hole. The process liberates enormous energy, within a few months to a year ...
• An FUV-optical approach for studying hierarchical star formation in nearby galaxies with UVIT 

  Ananthu, Sanal; Shashank, Gairola; Subramanian, S; Jayanth, Rao C; Menon, Shyam H; Mondal, Chayan; Muraleedharan, Sreedevi (American Astronomical Society, 2026-05-10)

  Young star-forming clumps (SFCs) emit strongly in the ultraviolet (UV), making UV imaging ideal for detecting them. The Ultraviolet Imaging Telescope (UVIT) on board AstroSat, with 1.5 resolution, has enabled the ...
• Investigating the circumgalactic medium through Mg II absorption coincidence 

  Sharma, Paryag; Srianand, R; Chand, H; Guha, Labanya Kumar (Oxford University Press on behalf of the Royal Astronomical Society, 2026-05)

  We present a statistical measurement of the transverse coherence of Mg ii λλ2796, 2803 absorption using a large sample of 9204 absorber-centric quasar sightline pairs from the Sloan Digital Sky Survey. We quantify the ...
• Galactic-scale evolution of classical and complex radio galaxies: Impact of ambient morphology and jet geometry 

  Giri, Gourab; Ghosh, Prajnadipt; Joshi, Ravi; Caproni, Anderson; Rossi, Paola; Bodo, Gianluigi; Kundu, Sayan; Thorat, K; Chatterjee, Swarna; Borgogno, Dario; Vittorini, Valerio; Tavani, Marco (EDP Sciences, 2026-05)

  Context. Extragalactic jets, following their launching, exhibit a wide range of propagation orientations relative to the host galaxy’s principal axis. This initial (mis)alignment has been shown to exert a substantial ...
• Stationary stars are axisymmetric in higher curvature gravity 

  Dubey, Nitesh K; Kolekar, Sanved; Sarkar, Sudipta (American Physical Society, 2026-05-15)

  The final equilibrium stage of stellar evolution can result in either a black hole or a compact object, such as a white dwarf or neutron star. In general relativity, both stationary black holes and stationary stellar c ...
• Baryonic ecosystem IN galaxies (BEINGMgII) III. Cool gas reservoirs at 0.3≤z ≤1.6 in the dark energy survey 

  Chaudhary, Reena; Joshi, Ravi; Das, Sarbeswar; Fumagalli, Michele; Kacprzak, Glenn G; Fossati, Matteo; Peroux, Celine; Ho, Luis C (EDP Sciences, 2026-05)

  We investigate the origin of intervening cool Mg ii absorption detected in the spectra of background quasars and the nature of associated galaxies across a broad redshift range of 0.3 ≤ z ≤ 1.6, and a largely unexplored ...

View more