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L. Vican

20 papers hereh-index 16869 citations43 works total

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

author position
  • sole author1
  • first author2
  • middle author12
  • last author2

Across the 17 of 20 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR11
  • astro-ph.EP5
  • astro-ph.GA4
same name
  • L. Vican — 1 paper

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
20102024
most citedResolved Debris Discs Around A Stars in the Herschel DEBRIS Survey

154 citations · 1k across the 20 of their papers we have counts for

collaborators
Showing 2013Show all

4 papers · 1 filter

astro-ph.SR2013★ 24 cited

The Evolution of Dusty Debris Disks Around Solar Type Stars

Laura Vican, Adam Schneider

We used chromospheric activity to determine the ages of 2,820 field stars.. We searched these stars for excess emission at 22 um with the Wide-Field Infrared Survey Explorer. Such…

astro-ph.SR2013★ 62 cited

Alignment in star-debris disc systems seen by Herschel

J. S. Greaves, G. M. Kennedy, N. Thureau +28

Many nearby main-sequence stars have been searched for debris using the far-infrared Herschel satellite, within the DEBRIS, DUNES and Guaranteed-Time Key Projects. We discuss here…

astro-ph.SR2013★ 60 cited

Young Stars Near Earth: The Octans-Near Association and Castor Moving Group

Ben Zuckerman, Laura Vican, Inseok Song +1

All cataloged stellar moving groups and associations with ages <100 Myr and within 100 pc of Earth have Galactic space motions (UVW) situated in a "good box" with dimensions ~20 km…

astro-ph.SR2013★ 92 cited

The GALEX Nearby Young-Star Survey

David R. Rodriguez, B. Zuckerman, Joel H. Kastner +3

We describe a method that exploits data from the GALEX ultraviolet and WISE and 2MASS infrared source catalogs, combined with proper motions and empirical pre-main sequence isochro…

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