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N. Hara

10 papers hereh-index 443 citations15 works total

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

author position
  • middle author9

Across the 9 of 10 papers where every author was matched, so the position is known.

fields
  • astro-ph.EP9
  • astro-ph.SR1
same name
  • N. Hara — 42 papers, h 24
  • N. Hara — 6 papers, h 17
  • N. Hara — 4 papers, h 5
  • N. Hara — 4 papers, h 2
  • N. Hara — 1 paper
  • N. Hara — 1 paper, h 0

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
20162026
most citedRadial-Velocity Fitting Challenge. II. First results of the analysis of the data set

115 citations · 166 across the 10 of their papers we have counts for

collaborators
Showing 2024Show all

3 papers · 1 filter

astro-ph.SR2024

Stellar surface information from the Ca II H&K lines -- II. Defining better activity proxies

M. Cretignier, N. C. Hara, A. G. M. Pietrow +6

In our former paper I, we showed on the Sun that different active regions possess unique intensity profiles on the Ca II H & K lines. We now extend the analysis by showing how thos…

astro-ph.EP2024★ 4 cited

A low-mass sub-Neptune planet transiting the bright active star HD 73344

S. Sulis, I. J. M. Crossfield, A. Santerne +33

Context. Planets with radii of between 2-4 RE closely orbiting solar-type stars are of significant importance for studying the transition from rocky to giant planets. Aims. Our goa…

astro-ph.EP2024★ 2 cited

An improved correction of radial-velocity systematic for the SOPHIE spectrograph

S. Grouffal, A. Santerne, N. C. Hara +4

High precision spectrographs might exhibit temporal variations of their reference velocity or nightly zero point (NZP). One way to monitor the NZP is to measure bright stars, which…

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