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researcher

J. Isern

4 papers here

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

author position
  • middle author1
  • last author2

Across the 3 of 4 papers where every author was matched, so the position is known.

fields
  • astro-ph3
  • astro-ph.IM1
ORCID 0000-0002-0819-9574
same name
  • J. Isern — 86 papers, h 51
  • J. Isern — 36 papers, h 20
  • J. Isern — 4 papers, h 1
  • J. Isern — 2 papers, h 6
  • J. Isern — 1 paper, h 2

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
19992011
most citedThe Large Observatory for X-ray Timing (LOFT)

214 citations · 236 across the 4 of their papers we have counts for

collaborators

4 papers

astro-ph.IM2011★ 214 cited

The Large Observatory for X-ray Timing (LOFT)

M. Feroci, the LOFT Consortium

High-time-resolution X-ray observations of compact objects provide direct access to strong-field gravity, to the equation of state of ultra-dense matter and to black hole masses an…

astro-ph2005★ 4 cited

The gravitational wave radiation of pulsating white dwarfs revisited: the case of BPM 37093 and PG 1159-035

E. Garcia-Berro, P. Loren-Aguilar, A. H. Corsico +3

We compute the emission of gravitational radiation from pulsating white dwarfs. This is done by using an up-to-date stellar evolutionary code coupled with a state-of-the-art pulsat…

astro-ph2001★ 18 cited

On the White Dwarf distances to Galactic Globular Clusters

M. Salaris, S. Cassisi, E. Garcia-Berro +2

We analyze in detail various possible sources of systematic errors on the distances of globular clusters derived by fitting a local template DA white dwarf sequence to the cluster…

astro-ph1999

The chemical composition of the rare J-type carbon stars

Carlos Abia, Jordi Isern

Abundances of lithium, heavy elements and carbon isotope ratios have been derived in 12 J-type galactic carbon stars. The abundance analysis shows that in these stars the abundance…

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