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researcher

J. Henry

6 papers hereh-index 8419 citations16 works total

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

author position
  • first author1
  • middle author3

Across the 4 of 6 papers where every author was matched, so the position is known.

fields
  • astro-ph4
  • astro-ph.CO2
same name
  • J. Henry — 51 papers, h 39
  • J. Henry — 17 papers, h 24
  • J. Henry — 7 papers, h 9
  • J. Henry — 4 papers, h 10
  • J. Henry — 3 papers, h 19
  • J. Henry — 2 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
19992021
most citedThe ROSAT North Ecliptic Pole Survey: The X-ray Catalog

80 citations · 283 across the 6 of their papers we have counts for

collaborators
Showing astro-phShow all

4 papers · 1 filter

astro-ph2008★ 5 cited

The stellar population of the Rosat North Ecliptic Pole survey. II. Spectral analysis

L. Affer, G. Micela, T. Morel

X-ray surveys allow to identify young, main-sequence stars in the solar neighborhood. Young, stellar samples, selected according to their activity, can be used to determine the ste…

astro-ph2005★ 80 cited

The ROSAT North Ecliptic Pole Survey: The X-ray Catalog

J. Patrick Henry, Christopher R. Mullis, Wolfgang Voges +4

The sky around the North Ecliptic Pole (NEP), at α(2000) = 18h00m00s, δ(2000) = +66\degr33\arcmin39\arcsec, has the deepest exposure of the entire {\it ROSAT} All - Sky Su…

astro-ph2004★ 48 cited

Spatial Correlation Function of X-ray Selected AGN

C. R. Mullis, J. P. Henry, I. M. Gioia +4

We present a detailed description of the first direct measurement of the spatial correlation function of X-ray selected AGN. This result is based on an X-ray flux-limited sample of…

astro-ph1999★ 70 cited

RXJ1716.6+6708: a young cluster at z=0.81

I. M. Gioia, J. P. Henry, C. R. Mullis +2

Clusters of galaxies at redshifts nearing one are of special importance since they may be caught at the epoch of formation. At these high redshifts there are very few known cluster…

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