Paper

{
  "raw_xml": "<entry>\n    <id>http://arxiv.org/abs/2602.18276v1</id>\n    <title>Chromaticity-Optimized Antenna Design and Bayesian Foreground Validation for the CANTAR Global 21 cm Experiment</title>\n    <updated>2026-02-20T15:01:53Z</updated>\n    <link href='https://arxiv.org/abs/2602.18276v1' rel='alternate' type='text/html'/>\n    <link href='https://arxiv.org/pdf/2602.18276v1' rel='related' title='pdf' type='application/pdf'/>\n    <summary>Detecting the global 21 cm signal from the epoch of reionization remains a major observational challenge due to bright foregrounds and instrumental systematics. As part of the Colombian Antarctic Telescopes for 21 cm Absorption during Reionization (CANTAR) initiative, we present a simulation and analysis framework to evaluate antenna chromaticity, optimize instrument design, and assess site suitability for global 21 cm experiments. Using frequency-dependent beam models and Haslam-based sky maps, we compute dynamic spectra for the EDGES blade dipole and a set of dipole and novel monopole antennas optimized via particle swarm optimization. The optimized designs exhibit improved spectral smoothness compared to EDGES, particularly in the 70-120 MHz range. We also evaluate latitude-dependent sky brightness and identify mid-latitude sites (-40° to +5°) as optimal for foreground suppression. We apply Bayesian inference together with posterior predictive model validation to the publicly released EDGES data, assessing statistical consistency rather than hypothesis testing or model comparison. We find that physically motivated foreground and ionospheric models are statistically consistent with the data only when a 21 cm absorption feature is excluded. From the validated posterior, we generate a statistically validated ensemble of foreground corrections for use in beam-sky simulations. These results support a two-phase strategy for CANTAR: Antarctic deployments for calibration and testing, and future science operations at mid-latitude sites. Our framework provides a validated path toward robust foreground modeling, antenna design, and systematics control for global 21 cm signal detection.</summary>\n    <category scheme='http://arxiv.org/schemas/atom' term='astro-ph.IM'/>\n    <published>2026-02-20T15:01:53Z</published>\n    <arxiv:comment>Accepted to ApJ, part of the CANTAR collaboration</arxiv:comment>\n    <arxiv:primary_category term='astro-ph.IM'/>\n    <author>\n      <name>Michelle Mora</name>\n    </author>\n    <author>\n      <name>German Chaparro</name>\n    </author>\n    <author>\n      <name>Juan D. Guerrero</name>\n    </author>\n    <author>\n      <name>Catalina Alzate</name>\n    </author>\n    <author>\n      <name>Juan P. Urrego</name>\n    </author>\n    <author>\n      <name>Jimena Giraldo</name>\n    </author>\n    <author>\n      <name>Pablo Cuartas-Restrepo</name>\n    </author>\n    <author>\n      <name>Julian Rodriguez-Ferreira</name>\n    </author>\n    <author>\n      <name>Oscar Restrepo</name>\n    </author>\n  </entry>"
}