Page 5: Research news on Optical astronomy

Optical astronomy is the research area focused on observing and analyzing electromagnetic radiation in the optical band, typically encompassing near-ultraviolet, visible, and near-infrared wavelengths accessible to ground- and space-based telescopes using optical elements and detectors. It employs instruments such as imaging cameras, spectrographs, and polarimeters on refracting or reflecting telescopes to study the photometric, spectroscopic, and polarimetric properties of astronomical sources. The field addresses topics including stellar and galactic structure, interstellar medium characterization, planetary systems, and cosmological parameters, and it relies on advanced techniques in adaptive optics, precision calibration, and data reduction to mitigate atmospheric and instrumental effects.

Observations explore a rare type Iax supernova

An international team of astronomers has conducted detailed multicolor photometric and spectroscopic observations of SN 2022xlp—a type Iax supernova. Results of the observational campaign, published September 9 on the arXiv ...

Astronomers discover dozens of new luminous quasars

Astronomers from Seoul National University, South Korea and elsewhere report the detection of 62 new luminous quasars as part of the All-sky BRIght, Complete Quasar Survey (AllBRICQS). The discovery was detailed in a research ...

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