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J. A. Caballero

4 papers hereh-index 9426 citations19 works total

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

author position
  • sole author1
  • first author1
  • middle author2

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

fields
  • astro-ph4
same name
  • J. A. Caballero — 4 papers
  • J. A. Caballero — 3 papers

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
20032007
most citedThe brightest stars of the sigma Orionis cluster

69 citations · 104 across the 3 of their papers we have counts for

collaborators
Showing astro-phShow all

4 papers · 1 filter

astro-ph2007★ 69 cited

The brightest stars of the sigma Orionis cluster

J. A. Caballero

Context: The very young sigma Orionis cluster (about 3 Ma) is a cornerstone for the understanding of the formation of stars and substellar objects down to planetary masses. However…

astro-ph2006★ 8 cited

GRB 051028: an intrinsically faint GRB at high redshift?

A. J. Castro-Tirado, M. Jelinek, S. B. Pandey +16

We present multiwavelength observations of the gamma-ray burst GRB 051028 detected by HETE-2 in order to derive its afterglow emission parameters and to determine the reason for it…

astro-ph2006★ 27 cited

Are isolated planetary-mass objects really isolated? A brown dwarf-exoplanet system candidate in the sigma Orionis cluster

J. A. Caballero, E. L. Martin, P. D. Dobbie +1

The recent detection by direct imaging of three giant planets at wide separation (50-250 AU) from their primaries has raised the question about the ``true isolation'' of planetary-…

astro-ph2003

Photometric variability of a young, low-mass brown dwarf

M. R. Zapatero Osorio, J. A. Caballero, V. J. S. Bejar +1

We report differential I-band and J-band photometry of S Ori 45, a cool (M8.5), young (1-8 Myr) brown dwarf of the sigma Orionis cluster with a likely mass estimated at around 20 t…

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