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researcher

L. Malavolta

5 papers here

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

author position
  • middle author5

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

fields
  • astro-ph.EP3
  • astro-ph.SR2
ORCID 0000-0002-6492-2085
same name
  • L. Malavolta — 175 papers, h 34
  • L. Malavolta — 3 papers, h 2
  • L. Malavolta — 1 paper, h 1
  • L. Malavolta — 1 paper, h 2

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
20122023
most citedCold Jupiters and improved masses in 38 Kepler and K2 small planet systems from 3661 HARPS-N radial velocities. No excess of cold Jupiters in small planet systems

118 citations · 166 across the 5 of their papers we have counts for

collaborators
Showing 2023Show all

3 papers · 1 filter

astro-ph.EP2023★ 2 cited

The GAPS programme at TNG XLIX. TOI-5398, the youngest compact multi-planet system composed of an inner sub-Neptune and an outer warm Saturn

G. Mantovan, L. Malavolta, S. Desidera +68

Short-period giant planets are frequently found to be solitary compared to other classes of exoplanets. Small inner companions to giant planets with P≲ 15 days are known…

astro-ph.SR2023★ 5 cited

The GAPS programme at TNG XLIII. A massive brown dwarf orbiting the active M dwarf TOI-5375

J. Maldonado, A. Petralia, G. Mantovan +23

Context. Massive substellar companions orbiting active low-mass stars are rare. They, however, offer an excellent opportunity to study the main mechanisms involved in the formation…

astro-ph.EP2023★ 118 cited

Cold Jupiters and improved masses in 38 Kepler and K2 small planet systems from 3661 HARPS-N radial velocities. No excess of cold Jupiters in small planet systems

A. S. Bonomo, X. Dumusque, A. Massa +31

The exoplanet population characterized by relatively short orbital periods (P<100 d) around solar-type stars is dominated by super-Earths and sub-Neptunes. However, these planets…

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