◍wovepaper
SearchResearchersInstitutions
Sign in
researcher

N. Santos

6 papers hereh-index 27 citations6 works total

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

author position
  • middle author5

Across the 5 of 6 papers where every author was matched, so the position is known.

fields
  • astro-ph.EP3
  • astro-ph.SR1
  • cs.DL1
  • physics.gen-ph1
same name
  • N. Santos — 270 papers, h 81
  • N. Santos — 86 papers, h 19
  • N. Santos — 64 papers, h 29
  • N. Santos — 58 papers, h 32
  • N. Santos — 40 papers, h 7
  • N. Santos — 20 papers, h 9

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
20142026
most citedSOAP 2.0: A tool to estimate the photometric and radial velocity variations induced by stellar spots and plages

268 citations · 284 across the 6 of their papers we have counts for

collaborators
Showing astro-ph.EPShow all

3 papers · 1 filter

astro-ph.EP2025

The NCORES Program: Precise planetary masses, null results, and insight into the planet mass distribution near the radius gap

David J. Armstrong, Ares Osborn, Remo Burn +39

NCORES was a large observing program on the ESO HARPS spectrograph, dedicated to measuring the masses of Neptune-like and smaller transiting planets discovered by the TESS satellit…

astro-ph.EP2025★ 6 cited

KOBE-1: The first planetary system from the KOBE survey. Two planets likely residing in the sub-Neptune mass regime around a late K-dwarf

O. Balsalobre-Ruza, J. Lillo-Box, A. M. Silva +35

K-dwarf stars are promising targets in the exploration of potentially habitable planets. Their properties, falling between G and M dwarfs, provide an optimal trade-off between the…

astro-ph.EP2020★ 10 cited

Constraining the oblateness of transiting planets with photometry and spectroscopy

B. Akinsanmi, S. C. C. Barros, N. C. Santos +2

Rapid planetary rotation can cause the equilibrium shape of a planet to be oblate. While planetary oblateness has mostly been probed by examining the subtle ingress and egress feat…

◍wovepaper

Papers, researchers and institutions, woven together.

Explore
  • Search
  • Researchers
  • Institutions
Account
  • Library
  • Chat
Data
  • arXiv.org
  • Semantic Scholar
  • OpenAlex
  • Latest RSS
AboutContactPrivacyDevelopersllms.txtopenapi.json
Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.