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researcher

H. Hansen

4 papers hereh-index 359.4k citations100 works total

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

author position
  • middle author3

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

fields
  • astro-ph.HE1
  • astro-ph.IM1
  • astro-ph.SR1
  • gr-qc1
same name
  • H. Hansen — 29 papers, h 10
  • H. Hansen — 13 papers, h 16
  • H. Hansen — 8 papers, h 1
  • H. Hansen — 7 papers
  • H. Hansen — 7 papers, h 7
  • H. Hansen — 5 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
20192026
most citedThe first view of δ Scuti and γ Doradus stars with the TESS mission

125 citations · 134 across the 4 of their papers we have counts for

collaborators

4 papers

astro-ph.IM2026

LIGO A♯: Detector Design and Science Prospects Beyond A+

L. Sun, K. Kuns, B. J. J. Slagmolen +1153

We present the LIGO A♯ detector concept, an upgrade for the LIGO observatories based on room-temperature interferometers beyond the fifth observing run (O5). Building on th…

astro-ph.HE2023★ 1 cited

Impact of O4 future detection on the determination of the dense matter equations of state

J. -F. Coupechoux, R. Chierici, H. Hansen +3

In view of the next LIGO-Virgo-KAGRA Observing period O4 (to start in Spring 2023), we address the question of the ability of the interferometers network to discriminate among diff…

gr-qc2021★ 8 cited

Discriminating same-mass Neutron Stars and Black Holes gravitational wave-forms

J. -F. Coupechoux, A. Arbey, R. Chierici +3

Gravitational wave-forms from coalescences of binary black hole systems and binary neutron star systems with low tidal effects can hardly be distinguished if the two systems have s…

astro-ph.SR2019★ 125 cited

The first view of δ Scuti and γ Doradus stars with the TESS mission

V. Antoci, M. S. Cunha, D. M. Bowman +63

We present the first asteroseismic results for δ Scuti and γ Doradus stars observed in Sectors 1 and 2 of the TESS mission. We utilise the 2-min cadence TESS data for a sample…

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