Using observations of the solar corona in the 5303 Å (Fe XIV) emission line with the Visible Emission Line Coronagraph (VELC) on board Aditya-L1, we estimated the electron density (…
We present the results of low-resolution spectroscopic and densely sampled multiband photometric follow-up of supernova (SN) 2024aecx. The SN was discovered in the spiral galaxy …
Morbidity and mortality data constitute an important component of a health information system and their coding enables uniform data collation and analysis as well as meaningful …
… Since there is a substantial gap in our data between 150 and 300 days, we cannot comment on the behavior of the colors during that interval. In addition, the final two measurements …
… For each orientation, we took longer (300 s) exposure frames to get the weaker lines with good signal-to-noise ratio. Since the stronger emission lines were saturated by the long …
The Indian National Science Academy was established in January 1935 with the object of promoting science in India and harnessing scientific knowledge for the cause of humanity and …
… We discuss the development and selection of different components in Section 4. The four mechanisms in SUIT are discussed in Section 5. We discuss the SUIT electronics package in …
Globally, of many toxic heavy metals, lead is the most widely used for various purposes, resulting in a variety of health hazards due to environmental contamination. Lead in the …
The origin of γ-ray flares observed from blazars is one of the major mysteries in jet physics. We have attempted to address this problem following a novel spectral energy distribution (…
… (2005), we infer that the cocoon shock velocity is of order ∼300 km s −1 . If the direction of jet propagation is almost in the plane of the sky, then the way in which the radial velocity falls …