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G. Wahlgren

23 papers hereh-index 272.7k citations212 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • sole author1
  • first author1
  • middle author11
  • last author6

Across the 19 of 23 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR13
  • astro-ph4
  • astro-ph.IM4
  • astro-ph.GA1
  • physics.atom-ph1
same name
  • G. Wahlgren — 2 papers

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

activity
19982026
most citedIn-orbit Performance of the Near-Infrared Spectrograph NIRSpec on the James Webb Space Telescope

183 citations · 452 across the 21 of their papers we have counts for

collaborators
Showing 2010Show all

3 papers · 1 filter

astro-ph.SR2010★ 53 cited

The spectroscopic evolution of the symbiotic-like recurrent nova V407 Cygni during its 2010 outburst. I. The shock and its evolution

S. N. Shore, G. M. Wahlgren, T. Augusteijn +7

On 2010 Mar 10, V407 Cyg was discovered in outburst, eventually reaching V< 8 and detected by Fermi. Using medium and high resolution ground-based optical spectra, visual and Swift…

astro-ph.SR2010★ 10 cited

The O I] 1641A line as a probe of symbiotic star winds

S. N. Shore, G. M. Wahlgren

The neutral oxygen resonance 1302A line can, if the optical depth is sufficiently high, de-excite by an intercombination transition at 1641A to a metastable state. This has been no…

astro-ph.SR2010★ 28 cited

HD 65949: Rosetta Stone or Red Herring

C. R. Cowley, S. Hubrig, P. Palmeri +5

HD 65949 is a late B star with exceptionally strong Hg II at 3984[A], but it is not a typical HgMn star. The Re II spectrum is of extraordinary strength. Abundances, or upper limit…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.