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E. Gillen

85 papers hereh-index 222.1k citations106 works total

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

author position
  • first author6
  • middle author72

Across the 78 of 85 papers where every author was matched, so the position is known.

fields
  • astro-ph.EP52
  • astro-ph.SR31
  • astro-ph.IM2
same name
  • E. Gillen — 1 paper, h 0
  • E. Gillen — 1 paper, h 1

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
20132026
most citedCSI 2264: Simultaneous optical and infrared light curves of young disk-bearing stars in NGC 2264 with CoRoT and Spitzer-- evidence for multiple origins of variability

411 citations · 3.2k across the 81 of their papers we have counts for

collaborators
Showing 2015Show all

3 papers · 1 filter

astro-ph.SR2015

HII 2407: A Low-Mass Eclipsing Binary Revealed by K2 Observations of the Pleiades

Trevor J. David, John Stauffer, Lynne A. Hillenbrand +16

The star HII 2407 is a member of the relatively young Pleiades star cluster and was previously discovered to be a single-lined spectroscopic binary. It is newly identified here wit…

astro-ph.SR2015★ 20 cited

The doubly eclipsing quintuple low-mass star system 1SWASP J093010.78+533859.5

M. E. Lohr, A. J. Norton, E. Gillen +6

Our discovery of 1SWASP J093010.78+533859.5 as a probable doubly eclipsing quadruple system containing a contact binary with P~0.23 d and a detached binary with P~1.31 d was announ…

astro-ph.SR2015★ 98 cited

CSI 2264: Characterizing Young Stars in NGC 2264 with Short-Duration, Periodic Flux Dips in their Light Curves

John Stauffer, Ann Marie Cody, Pauline McGinnis +27

We identify nine young stellar objects (YSOs) in the NGC 2264 star-forming region with optical {\em CoRoT} light curves exhibiting short-duration, shallow, periodic flux dips. All…

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