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P. Tanga

56 papers hereh-index 3310k citations252 works total

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

author position
  • first author4
  • middle author34
  • last author10

Across the 48 of 56 papers where every author was matched, so the position is known.

fields
  • astro-ph.EP42
  • astro-ph.IM5
  • astro-ph4
  • astro-ph.GA3
  • astro-ph.SR2
same name
  • P. Tanga — 26 papers, h 24
  • P. Tanga — 6 papers
  • P. Tanga — 4 papers, h 1
  • P. Tanga — 3 papers, h 1

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
20042025
most citedGaia Data Release 2: Photometric content and validation

756 citations · 3.2k across the 56 of their papers we have counts for

collaborators
Showing astro-phShow all

4 papers · 1 filter

astro-ph2008★ 114 cited

Thermal inertia of main belt asteroids smaller than 100 km from IRAS data

Marco Delbo, Paolo Tanga

Recent works have shown that the thermal inertia of km-sized near-Earth asteroids (NEAs) is more than two orders of magnitude higher than that of main belt asteroids (MBAs) with si…

astro-ph2008★ 34 cited

Asteroid occultations today and tomorrow: toward the GAIA era

P. Tanga, M. Delbo

Context: Observation of star occultations is a powerful tool to determine shapes and sizes of asteroids. This is key information necessary for studying the evolution of the asteroi…

astro-ph2005★ 6 cited

Asteroids. From Observations to Models

Daniel Hestroffer, Paolo Tanga

We will discuss some specific applications to the rotation state and the shapes of moderately large asteroids, and techniques of observations putting some emphasis on the HST/FGS i…

astro-ph2004★ 34 cited

Gravitational instability and clustering in a disk of planetesimals

P. Tanga, S. J. Weidenschilling, P. Michel +1

For a long time, gravitational instability in the disk of planetesimals has been suspected to be the main engine responsible for the beginning of dust growth, its advantage being t…

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