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T. Jacobs

34 papers hereh-index 191.4k citations66 works total

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

author position
  • middle author27
  • last author1

Across the 28 of 34 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR20
  • astro-ph.EP14
same name
  • T. Jacobs — 5 papers, h 4
  • T. Jacobs — 3 papers, h 23
  • T. Jacobs — 2 papers, h 10
  • T. Jacobs — 2 papers, h 2
  • T. Jacobs — 1 paper, h 4
  • T. Jacobs — 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
20152026
most citedLikely Transiting Exocomets Detected by Kepler

102 citations · 549 across the 23 of their papers we have counts for

collaborators
Showing 2019Show all

4 papers · 1 filter

astro-ph.SR2019

A 9-Hr CV With One Outburst in 4 Years of Kepler Data

Zhifei Yu, John Thorstensen, Saul Rappaport +11

During a visual search through the Kepler main-field lightcurves, we have discovered a cataclysmic variable (CV) that experienced only a single 4-day long outburst over four years,…

astro-ph.EP2019★ 20 cited

Planetesimals Around Stars with TESS (PAST): I. Transient Dimming of a Binary Solar Analog at the End of the Planet Accretion Era

E. Gaidos, T. Jacobs, D. LaCourse +16

We report detection of quasi-periodic (1.5 day) dimming of HD 240779, the solar-mass primary in a 5" visual binary (also TIC 284730577), by the Transiting Exoplanet Survey Satellit…

astro-ph.EP2019★ 26 cited

The Random Transiter -- EPIC 249706694/HD 139139

S. Rappaport, A. Vanderburg, M. H. Kristiansen +16

We have identified a star, EPIC 249706694 (HD 139139), that was observed during K2 Campaign 15 with the Kepler extended mission that appears to exhibit 28 transit-like events over…

astro-ph.SR2019★ 29 cited

Deep Long Asymmetric Occultation in EPIC 204376071

S. Rappaport, G. Zhou, A. Vanderburg +15

We have discovered a young M star of mass 0.16M⊙​ and radius 0.63R⊙​, likely in the Upper Sco Association, that exhibits only a single 80% deep occultation of 1-…

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