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David J. Wilner

18 papers hereh-index 00 citations0 works total

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

author position
  • first author2
  • middle author9
  • last author6

Across the 17 of 18 papers where every author was matched, so the position is known.

fields
  • astro-ph5
  • astro-ph.SR5
  • astro-ph.GA4
  • astro-ph.EP3
  • astro-ph.HE1
same name
  • David J. Wilner — 7 papers, h 2
  • David J. Wilner — 5 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 citedEvidence for dust clearing through resolved submillimeter imaging

215 citations · 930 across the 18 of their papers we have counts for

collaborators
Showing 2009Show all

4 papers · 1 filter

astro-ph.EP2009★ 6 cited

Exoplanet Characterization and the Search for Life

J. Kasting, W. Traub, A. Roberge +119

Over 300 extrasolar planets (exoplanets) have been detected orbiting nearby stars. We now hope to conduct a census of all planets around nearby stars and to characterize their atmo…

astro-ph.SR2009★ 15 cited

183 GHz H2​O maser emission around the low-mass protostar Serpens SMM1

T. A. van Kempen, D. Wilner, M. Gurwell

We report the first interferomteric detection of 183 GHz water emission in the low-mass protostar Serpens SMM1 using the Submillimeter Array with a resolution of 3" and rms of $\…

astro-ph.SR2009★ 215 cited

Evidence for dust clearing through resolved submillimeter imaging

J. M. Brown, G. A. Blake, C. Qi +3

Mid-infrared spectrophotometric observations have revealed a small sub-class of circumstellar disks with spectral energy distributions (SEDs) suggestive of large inner gaps with lo…

astro-ph.GA2009★ 23 cited

Resolving the molecular environment of Super Star Clusters in Henize 2-10

G. Santangelo, L. Testi, L. Gregorini +4

The rate of star formation both in the Galaxy and in external galaxies should be related to the physical properties of the molecular clouds from which stars form. This is expected…

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