Alejandro Hacker

ORCID: 0009-0009-9452-0181
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About
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Research Areas
  • Geological and Geochemical Analysis
  • Astro and Planetary Science
  • Radioactive element chemistry and processing
  • High-pressure geophysics and materials

Consejo Nacional de Investigaciones Científicas y Técnicas
2024

National University of General San Martín
2024

International Center for Advanced Studies
2024

Abstract In this paper, we present a homogeneous analysis of close-in Neptune planets. To do this, compile sample TESS-observed planets using ranking criterion which takes into account the planet’s period, radius, and visual magnitude its host star. We use archival new HARPS data to ensure every target in has precise radial velocities. This yields total 64 targets, 46 are confirmed 18 show no significant velocity signal. explore mass-radius distribution, planetary density, stellar...

10.1093/mnras/staf670 article EN cc-by Monthly Notices of the Royal Astronomical Society 2025-04-24

ABSTRACT We report the discovery of two transiting planets detected by Transiting Exoplanet Survey Satellite (TESS), TOI-2374 b and TOI-3071 b, orbiting a K5V an F8V star, respectively, with periods 4.31 1.27 d, respectively. confirm characterize these variety ground-based follow-up observations, including photometry, precise radial velocity monitoring high-resolution imaging. The planetary orbital parameters were derived from joint analysis velocities photometric data. found that have...

10.1093/mnras/stae1420 article EN cc-by Monthly Notices of the Royal Astronomical Society 2024-06-08

We report the discovery of two transiting planets detected by Transiting Exoplanet Survey Satellite (TESS), TOI-2374 b and TOI-3071 b, orbiting a K5V an F8V star, respectively, with periods 4.31 1.27 days, respectively. confirm characterize these variety ground-based follow-up observations, including photometry, precise radial velocity monitoring high-resolution imaging. The planetary orbital parameters were derived from joint analysis velocities photometric data. found that have masses $(57...

10.48550/arxiv.2406.12996 preprint EN arXiv (Cornell University) 2024-06-18
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