activity
20152025
most citedThe 60 pc Environment of FRB 20180916B

94 citations · 130 across the 9 of their papers we have counts for

collaborators

9 papers

astro-ph.GA2025

MEGADES: MEGARA galaxy disc evolution survey. Ionised gas diagnosis

M. Chamorro-Cazorla, A. Gil de Paz, A. Castillo-Morales +13

We present the ionised gas properties and metallicity gradients of 43 galaxies observed by the MEGADES survey. Using the MEGARA (Multi-Espectrografo en GTC de Alta Resolucion para…

astro-ph.HE2025★ 8 cited

A Hyperactive FRB Pinpointed in an SMC-Like Satellite Host Galaxy

M. Bhardwaj, M. P. Snelders, J. W. T. Hessels +24

Precise localizations of fast radio bursts (FRBs) are essential for uncovering their host galaxies and immediate environments. We present the milliarcsecond-precision European VLBI…

astro-ph.HE2024

A Repeating Fast Radio Burst Source in a Low-Luminosity Dwarf Galaxy

Danté M. Hewitt, Mohit Bhardwaj, Alexa C. Gordon +48

We present the localization and host galaxy of FRB 20190208A, a repeating source of fast radio bursts (FRBs) discovered using CHIME/FRB. As part of the PRECISE repeater localizatio…

astro-ph.GA2024

Compact and High Excitation Molecular Clumps in the Extended Ultraviolet Disk of M83

Jin Koda, Francoise Combes, Monica Rubio +9

The extended ultraviolet (XUV) disks of nearby galaxies show ongoing massive star formation, but their parental molecular clouds remain mostly undetected despite searches in CO(1-0…

astro-ph.SR2020★ 5 cited

MEGARA-GTC Stellar Spectral Library (II). MEGASTAR First Release

E. Carrasco, M. Mollá, M. L. García-Vargas +4

MEGARA is an optical integral field and multiobject fibre based spectrograph for the 10.4m Gran Telescopio CANARIAS that offers medium to high spectral resolutions (FWHM) of R $\si…

astro-ph.HE2020★ 94 cited

The 60 pc Environment of FRB 20180916B

Shriharsh P. Tendulkar, Armando Gil de Paz, Aida Yu. Kirichenko +18

Fast Radio Burst FRB 20180916B in its host galaxy SDSS J015800.28+654253.0 at 149 Mpc is by far the closest-known FRB with a robust host galaxy association. The source also exhibit…