pith. sign in

H. Brunner (5)

Identifiers

  • name variant H. Brunner (5) 0.60 · backfill

Papers (1)

  1. High Excitation Emission Line Nebula associated with an Ultra Luminous X-ray Source at $z=$ 0.027 in the \textit{AKARI} North Ecliptic Pole Deep Field astro-ph.GA · 2017 · author #6

Mentions

  • 1706.01986 #6 · arxiv_oai · confidence 0.70 H. Brunner (5)

Frequent Coauthors