The-to-UV luminosity ratio () is often used to probe bursty star formation histories (SFHs) of
star-forming galaxies and it is important to validate it against other proxies for burstiness. To …

Global, radial, and local photometric measurements of several nearby low-mass galaxies
are presented. Multiwavelength observations are used to trace the distributions of old and …

With the aim to study the extended H i environment around dwarf galaxies in the local
universe, we performed a high-sensitivity H i observation of the DDO 168 and DDO 167 pair …

We present a far-ultraviolet (FUV) study of 16 star-forming dwarf galaxies (SFDGs) using the
Ultra Violet Imaging Telescope. Morphologically, SFDGs are classified as dwarf spirals …

NGC 7793, NGC 300, M 33, and NGC 2403 are four nearby undisturbed and bulgeless low-
mass spiral galaxies whose morphology and stellar mass are similar. They are ideal …

This multiwavelength study of the star formation and star formation history (SFH) trends in
the nearby universe looks at nine nearby late-type spirals. Spectral energy distributions fitted …

It has long been uncertain how effective the dust-corrected H $\alpha $-to-UV luminosity
ratio ($ L (\rm H\alpha)/L (\rm UV) $) is in probing bursty SFHs for high-redshift galaxies. To …

It has long been uncertain how effective the dust-corrected H𝛼-to-UV luminosity ratio (𝐿
(H𝛼)/𝐿 (UV)) is in probing bursty star-formation histories (SFHs) for high-redshift galaxies …

I analyze resolved near-ultraviolet (NUV) stellar photometry of star-forming galaxy NGC
6946 (The Fireworks Galaxy) taken with the Hubble Space Telescope's (HST) Wide Field …

Dust attenuation refers to the absorption and scattering of light by interstellar dust particles
within a galaxy. This effect, which depends on wavelength, is also known as dust reddening …