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researcher

J. Sanz-Forcada

110 papers hereh-index 262.5k citations102 works total

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

author position
  • first author12
  • middle author79
  • last author8

Across the 99 of 110 papers where every author was matched, so the position is known.

fields
  • astro-ph.EP70
  • astro-ph.SR25
  • astro-ph9
  • astro-ph.GA3
  • astro-ph.HE2
  • astro-ph.IM1
same name
  • J. Sanz-Forcada — 4 papers, h 27

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
19962026
most citedEstimation of the XUV radiation onto close planets and their evaporation

407 citations · 6k across the 109 of their papers we have counts for

collaborators
Showing 2011Show all

4 papers · 1 filter

astro-ph.SR2011★ 48 cited

Herschel discovery of a new class of cold, faint debris discs

C. Eiroa, J. P. Marshall, A. Mora +25

We present Herschel PACS 100 and 160 micron observations of the solar-type stars alpha Men, HD 88230 and HD 210277, which form part of the FGK stars sample of the Herschel Open Tim…

astro-ph.EP2011

Planets and X-rays: a radiation diet

J. Sanz-Forcada, I. Ribas, G. Micela +4

According to theory, high energy emission from the coronae of cool stars can severely erode the atmosphere of orbiting planets. To test the long term effects of the erosion we stud…

astro-ph.EP2011★ 407 cited

Estimation of the XUV radiation onto close planets and their evaporation

J. Sanz-Forcada, G. Micela, I. Ribas +5

Context: The current distribution of planet mass vs. incident stellar X-ray flux supports the idea that photoevaporation of the atmosphere may take place in close-in planets. Integ…

astro-ph.SR2011★ 51 cited

A Herschel resolved far-infrared dust ring around HD 207129

J. P. Marshall, T. Löhne, B. Montesinos +26

Dusty debris discs around main sequence stars are thought to be the result of continuous collisional grinding of planetesimals in the system. The majority of these systems are unre…

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