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Saul A. Rappaport

4 papers hereh-index 25 citations4 works total

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

author position
  • middle author1
  • last author3

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

fields
  • astro-ph.SR4
same name
  • Saul A. Rappaport — 5 papers, h 3

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

collaborators

4 papers

astro-ph.SR2026

A Few Years Later: Revisiting Period Variations of Eclipsing Binaries in the Northern Continuous Viewing Zone of TESS

T. Borkovits, T. Mitnyan, D. R. Czavalinga +1

In our previous analysis of the eclipse timing variation patterns of eclipsing binaries located in and near the Northern Continuous Viewing Zone (NCVZ) of the TESS space telescope,…

astro-ph.SR2026

A Binary-Based Reassessment of the Age and Stellar Properties of NGC 7789 Using Twelve Binary Components

Kadri Yakut, Belinda Kalomeni, Saul Rappaport

We present a binary-based reassessment of the age of the intermediate-age open cluster NGC 7789, together with well-constrained stellar parameters for twelve components in six SB2…

astro-ph.SR2025

A Deep Look into the Intermediate-Age Open Cluster NGC 2506: What Binary Systems Reveal About Cluster Distance and Age

K. Yakut, B. Kalomeni, S. Rappaport +1

Using high-precision observations from the space-based \textit{Gaia} and \textit{TESS} missions, complemented by ground-based spectroscopic data and multi-band photometric surveys,…

astro-ph.SR2025

A novel approach to determining the age of stellar clusters: application to NGC 188

K. Yakut, B. Kalomeni, S. Rappaport

We present a new independent determination for the age of one of the oldest open clusters, NGC 188: 6.41±0.33 Gyr. We utilize a novel approach where we jointly fit the radial…

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