activity
20142026
most citedThe ESO Diffuse Interstellar Bands Large Exploration Survey: EDIBLES I. Project description, survey sample and quality assessment

62 citations · 266 across the 18 of their papers we have counts for

collaborators

18 papers

astro-ph.SR2026

Unveiling Complex Chemistry in Planet-forming Disks with the SKAO

Linda Podio, Lisa Giani, Catherine Walsh +38

The chemical composition of planets is inherited from that of the natal protoplanetary disk at the time of planet formation. In recent years, we have made huge progress in characte…

astro-ph.GA2025★ 1 cited

The EDIBLES survey. X. The 6196 Å diffuse interstellar band: Identification of side DIBs as an indication of a small carrier molecule

A. Ebenbichler, M. Ončák, N. Przybilla +11

Context: Numerous studies of diffuse interstellar band (DIB) profiles have detected substructures, which in turn suggests that large molecules are acting as their carriers. However…

astro-ph.SR2024★ 36 cited

A magnetic massive star has experienced a stellar merger

A. J. Frost, H. Sana, L. Mahy +13

Massive stars (those larger than 8 solar masses at formation) have radiative envelopes that cannot sustain a dynamo, the mechanism that produces magnetic fields in lower-mass stars…

astro-ph.GA2024

The EDIBLES Survey. VIII. Band profile alignment of diffuse interstellar bands

A. Ebenbichler, J. V. Smoker, R. Lallement +9

Context: There have been many attempts to identify families of diffuse interstellar bands (DIBs) with perfectly correlating band strengths. Although major efforts have been made to…

astro-ph.GA2023★ 10 cited

The EDIBLES Survey. VII. A survey of C2 and C3 in interstellar clouds

Haoyu Fan, Carlos M. R. Rocha, Martin Cordiner +14

We carried out a sensitive survey of C and C using the EDIBLES data set. We also expanded our searches to C, C, and CC isotopologue in the most molecu…

astro-ph.GA2023★ 2 cited

The EDIBLES survey VI. Searching for time variations of interstellar absorption features

Amin Farhang, Jonathan Smoker, Nick L. J. Cox +10

Interstellar lines observed toward stellar targets change slowly over long timescales, mainly due to the proper motion of the background target relative to the intervening clouds.…