activity
19992022
most citedHerschel Survey of Galactic OH+, H2O+, and H3O+: Probing the Molecular Hydrogen Fraction and Cosmic-Ray Ionization Rate

272 citations · 3.4k across the 59 of their papers we have counts for

collaborators

59 papers

astro-ph.SR2022★ 21 cited

Peculiar radioX-ray relationship in active stars

H. K. Vedantham, J. R. Callingham, T. W. Shimwell +5

The empirical relationship between the non-thermal 5GHz radio luminosity and the soft X-ray luminosity of active stellar coronae, canonically called the Güdel-Benz relationship (Gü…

astro-ph.SR2021★ 33 cited

STIX X-ray microflare observations during the Solar Orbiter commissioning phase

Andrea Francesco Battaglia, Jonas Saqri, Paolo Massa +34

The Spectrometer/Telescope for Imaging X-rays (STIX) is the HXR instrument onboard Solar Orbiter designed to observe solar flares over a broad range of flare sizes, between 4-150 k…

astro-ph.SR2021★ 11 cited

ALMA small-scale features in the quiet Sun and active regions

R. Brajsa, I. Skokic, D. Sudar +5

Aims. The main aim of the present analysis is to decipher (i) the small-scale bright features in solar images of the quiet Sun and active regions obtained with the Atacama Large Mi…

astro-ph.GA2021★ 174 cited

Water in star-forming regions (WISH): Physics and chemistry from clouds to disks as probed by Herschel spectroscopy

E. F. van Dishoeck, L. E. Kristensen, the WISH team

(abridged) Data and results from the WISH key program are summarized, designed to provide a legacy data set to address its physics and chemistry. WISH targeted ~80 sources along th…

astro-ph.SR2019

Centre to limb brightness variations from ALMA full disk solar images

Davor Sudar, Roman Brajša, Ivica Skokić +1

Science Verification (SV) data of solar observations with Atacama Large Millimeter-submillimeter Array (ALMA) telescope were released to the scientific community. Understanding the…

astro-ph.SR2018

Observations of the solar chromosphere with ALMA and comparison with theoretical models

R. Brajša, D. Sudar, I. Skokic +9

In this work we use solar observations with the ALMA radio telescope at the wavelength of 1.21 mm. The aim of the analysis is to improve understanding of the solar chromosphere, a…