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researcher

J. Schmitt

81 papers hereh-index 509.3k citations452 works total

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

author position
  • middle author30
  • last author43

Across the 73 of 81 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR31
  • astro-ph27
  • astro-ph.EP16
  • astro-ph.IM3
  • astro-ph.HE2
  • astro-ph.CO1
same name
  • J. Schmitt — 43 papers, h 27
  • J. Schmitt — 36 papers, h 11
  • J. Schmitt — 33 papers, h 16
  • J. Schmitt — 15 papers, h 5
  • J. Schmitt — 11 papers, h 10
  • J. Schmitt — 9 papers, h 6

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
19992022
most citedSimulating the escaping atmospheres of hot gas planets in the solar neighborhood

177 citations · 3.1k across the 81 of their papers we have counts for

collaborators
Showing 2006Show all

4 papers · 1 filter

astro-ph2006★ 13 cited

A deep XMM-Newton X-ray observation of the Chamaeleon I dark cloud

J. Robrade, J. H. M. M. Schmitt

Methods. The northern-eastern fringe of the Chameleon I dark cloud was observed with XMM-Newton, revisiting a region observed with ROSAT 15 years ago. Centered on the extended X-ra…

astro-ph2006★ 70 cited

Simultaneous optical and X-ray observations of a giant flare on the ultracool dwarf LP412-31

B. Stelzer, J. H. M. M. Schmitt, G. Micela +1

Cool stars are known to produce flares probably as a result of magnetic reconnection in their outer atmospheres. We present simultaneous XMM-Newton optical V band and X-ray observa…

astro-ph2006★ 16 cited

The coronal Ne/O abundance of alpha Centauri

C. Liefke, J. H. M. M. Schmitt

Recent improvements in the modeling of solar convection and line formation led to downward revisions of the solar photospheric abundances of the lighter elements, which in turn led…

astro-ph2006★ 66 cited

XMM-Newton X-ray spectroscopy of classical T Tauri stars

J. Robrade, J. H. M. M. Schmitt

We present results from a comparative study of XMM-Newton observations of four classical T Tauri stars (CTTS), namely BP Tau, CR Cha, SU Aur and TW Hya. In these objects coronal, i…

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