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19922026
most citedNeutrino Masses and Leptogenesis with Heavy Higgs Triplets

518 citations

Showing 2026Show all

17 papers · 1 filter

astro-ph.SR2026

Aditya-L1 and SDO Observations of a Confined X-Class Flare with an EUV Late Phase: Thermal and Nonthermal Emission, Magnetic Topology, and Flux Rope Confinement

Vishwa Vijay Singh, Bhuwan Joshi, N. P. S. Mithun

We study a long-duration, confined X2.0-class solar flare exhibiting three distinct episodes of HXR emission, along with an accompanying EUV late phase. A key highlight of this wor…

astro-ph.GA2026

Magnetic Fields in Massive Star-forming Regions (MagMaR). IX. Radiative Torque Alignment and Disruption in NGC6334I

Vineet Rawat, Thiem Hoang, Patricio Sanhueza +18

Intense radiation from high-mass stars is expected to significantly affect dust grain alignment and evolution through RAdiative Torques (RATs). We investigate this effect in a mass…

astro-ph.SR2026

Multi-Wavelength Diagnostics of Pre-Flare Evolution with Aditya-L1: From the Solar Chromosphere to the Corona

Adithya H. N., Sreejith Padinhatteeri, Soumya Roy +13

The pre-flare phase of solar flares provides important insight into the processes that drive active regions toward instability. We investigate chromospheric pre-flare activity usin…

astro-ph.SR2026

A Quiet Host in an Active Planet-Forming Disk: Optical Spectroscopy of WISPIT 2

C. Swastik, M. Bestha, L. S. Sonith +11

WISPIT 2 is a young pre-main-sequence star hosting a multi-ringed transition disk and two directly imaged protoplanets, including the accreting WISPIT 2b, making it the closest kno…

astro-ph.HE2026

Can We Find the Emission Mechanism Behind the Extremely Bright GRB 230812B?

Utkarsh Pathak, Sameer K. Patil, Hitesh Tanenia +23

GRB 230812B is a bright long-duration GRB with a luminous, long-lived afterglow and an AstroSat/CZTI polarization measurement during the prompt phase, enabling a joint study of its…

astro-ph.EP2026

Understanding eccentric temperate giants: an in-depth study of the architecture and stellar obliquity of the TOI-2134 system

Federica Rescigno, Manu Stalport, Ancy Anna John +28

We revisit the TOI-2134 planetary system with three new high-cadence TESS sectors and 98 more spectra. This new analysis confirms the two orbiting planets by simultaneously modelli…

astro-ph.EP2026

TOI-6884b: A low-mass brown dwarf transiting a slightly evolved star

Akanksha Khandelwal, Shubhendra Nath Das, Rishikesh Sharma +42

We report the discovery of a low-mass transiting brown dwarf orbiting TOI-6884 (TIC~156514476, ) from NASA's \textit{Transiting Exoplanet Survey Satellite} (\text…

astro-ph.IM2026

Instruments for Focal Plane X-Ray Polarimetry in the Next Decade

Fabio Muleri, Stefano Cesare, Enrico Costa +18

The successful detection of X-ray polarization from many celestial sources belonging to different classes by the IXPE mission has opened a new window in X-ray astronomy. While an i…

astro-ph.SR2026

Source Surface Height Optimisation for Improved Solar Wind Velocity Forecasting Across Solar Cycles 23, 24 and 25

Sandeep Kumar, Nandita Srivastava, Dana-Camelia Talpeanu

The potential field source surface (PFSS) model is a cornerstone of many state-of-the-art space weather forecasting frameworks. It includes a single physical free parameter, the so…

astro-ph.IM2026

Design and development of Fabry-Perot based wavelength calibration system for PARAS-2 spectrograph

Shubhendra Nath Das, Kapil Kumar Bharadwaj, Abhijit Chakraborty +5

Precise wavelength calibration is essential for high-precision radial velocity (RV) spectrographs, necessitating a stable calibrator that provides a dense grid of uniformly spaced…

astro-ph.IM2026★ 1 cited

Design and Development of Cassegrain Module for PARAS-2 Spectrograph (CAMPAS)

Kevikumar A. Lad, Neelam J. S. S. V. Prasad, Kapil Bharadwaj +5

We present here the design and development of the CAMPAS, the Cassegrain Module for the PARAS-2 spectrograph. PARAS-2 is a high-resolution fiber-fed echelle spectrograph developed…

astro-ph.IM2026

Development of a one-dimensional position sensitive detector for Compton X-ray polarimeters

Abhay Kumar, Santosh V. Vadawale, N. P. S. Mithun +4

The scientific potential of X-ray polarimetry has long been recognized, but the challenges in measuring polarization have left it largely unexplored, particularly in the hard X-ray…

astro-ph.SR2026

Near-infrared spectroscopy of RS Ophiuchi in 2021: the calm, the storm, and the abatement

C. E. Woodward, A. Evans, D. P. K. Banerjee +4

We present near-infrared (NIR) observations of the 2021 eruption of the recurrent nova RS Ophiuchi. The dataset provides both pre- and post-eruption perspectives on the eruption, a…

astro-ph.HE2026

Episode-wise spectro-polarimetry of GRB 220107A: Testing the hypothesis of evolving radiation mechanisms

Rahul Gupta, Rushikesh Sonawane, Shabnam Iyyani +17

We investigate the spectro-polarimetric properties of the long-duration GRB~220107A, which exhibited two distinct emission episodes separated by a 40 s quiescent gap, to test wheth…

astro-ph.GA2026

A multi-wavelength study of nearby starburst galaxy M 82

Nilkanth Vagshette, Satish S. Sonkamble, Madhav Patil +2

We present a multi-wavelength study of the nearby starburst galaxy M 82 by combining high-resolution Far-ultraviolet (FUV) imaging from the Ultra-Violet Imaging Telescope (UVIT) on…

astro-ph.HE2026

Discovery of burst oscillations in the newly discovered millisecond X-ray pulsar SRGA J144459.2604207

Manoj Mandal, Sachindra Naik

Burst oscillations during thermonuclear X-ray bursts are powered by thermonuclear energy on the neutron star (NS) surface and typically occur close to the spin frequency of the NS.…

astro-ph.SR2026

Evidence for the merger hypothesis in V4332 Sgr: a low C/C ratio and multiple outbursts

D. P. K. Banerjee, A. Evans, Watson P. Varricatt +1

Following the detections of the first extragalactic ``Luminous Red Nova'' (LRN) M31 RV in 1989, and its first Galactic counterpart V4332~Sgr in 1994, there have been many discoveri…