activity
20132026
most citedSEDIGISM: Structure, excitation, and dynamics of the inner Galactic interstellar medium

128 citations · 433 across the 15 of their papers we have counts for

collaborators

17 papers

astro-ph.GA2026

Self Calibrated Galaxy Groups from the DESI DR1 Bright Galaxy Survey

I. Williams, J. Tinker, K. Wang +45

We present a galaxy group catalog built from Data Release 1 of the Dark Energy Spectroscopic Instrument (DESI) Bright Galaxy Survey, using the Self Calibrated Group Finder. The alg…

astro-ph.SR2026

The Stellar Observations Network Group (SONG) -- A Legacy Archive of Stellar Time-Domain Spectroscopy

M. N. Lund, F. Grundahl, M. S. Fredslund +41

The Stellar Observations Network Group (SONG) network has operated for more than a decade, providing long-baseline, high-cadence spectroscopic observations of bright stars and the…

astro-ph.GA2023★ 17 cited

Large-scale Velocity-coherent Filaments in the SEDIGISM Survey: Association with Spiral Arms and Fraction of Dense Gas

Y. Ge, K. Wang, A. Duarte-Cabral +15

Context. Filamentary structures in the interstellar medium are closely related to star formation. Dense gas mass fraction (DGMF) or clump formation efficiency in large-scale filame…

astro-ph.GA2023★ 9 cited

Infall and Outflow Towards High-mass Starless Clump Candidates

T. G. S. Pillai, J. S. Urquhart, S. Leurini +6

The evolutionary sequence for high-mass star formation starts with massive starless clumps that go on to form protostellar, young stellar objects and then compact HII regions. Whil…

astro-ph.GA2021

Singly- and doubly-deuterated formaldehyde in massive star-forming regions

S. Zahorecz, I. Jimenez-Serra, L. Testi +5

Deuterated molecules are good tracers of the evolutionary stage of star-forming cores. During the star formation process, deuterated molecules are expected to be enhanced in cold,…

astro-ph.GA2021★ 38 cited

ALMA-IRDC: Dense gas mass distribution from cloud to core scales

A. T. Barnes, J. D. Henshaw, F. Fontani +15

Infrared dark clouds (IRDCs) are potential hosts of the elusive early phases of high-mass star formation (HMSF). Here we conduct an in-depth analysis of the fragmentation propertie…