Stellar Cartography

COUNTESS I: A Uniformly Vetted Catalog of Known and New Transiting Exoplanets in the TESS Northern Continuous Viewing Zone

By Keith Cowing
Status Report
astro-ph.EP
June 15, 2026
Filed under , , , , , , , , , , , , , ,
COUNTESS I: A Uniformly Vetted Catalog of Known and New Transiting Exoplanets in the TESS Northern Continuous Viewing Zone
The distribution of planetary radius and orbital period of TOIs and new false positives and planet candidates. COUNTESS discovered 38 new planetary signals, with 28 of them being FPs through triceratops validation and LEOVetter pixel-vetting. Note that the square symbols indicate TOI FPs that were successfully recovered as FPs through COUNTESS. — astro-ph.EP

The Transiting Exoplanet Survey Satellite (TESS) has transformed the study of nearby exoplanetary systems; however, its nominal observing strategy limits sensitivity to planets with orbital periods shorter than ∼10 days for most parts of the sky.

The two TESS Continuous Viewing Zones (CVZs) provide extended temporal baselines that help overcome this limitation, enabling the detection of longer-period (>10 days) transiting planets around nearby stars.

Here, we present COUNTESS, a transit-search pipeline optimized for long-baseline TESS observations that combines multi-sector light curves with heterogeneous cadences, and implements fast-folding BLS period detection, vetting, and statistical validation. As a first application of the pipeline, we conducted a search on the primary and first extended mission photometry in the TESS northern CVZ.

For this analysis, we used Gaia DR3 and 2MASS photometry to homogeneously derive a stellar catalog of FGKM stars for the TESS northern CVZ, resulting in a sample of 391,059 stars. We used COUNTESS to search for transiting planets around 26,114 of these stars with TESS-SPOC light curves and assessed its performance, recovering 115 out of 159 known TESS Objects of Interest (TOIs; 0.85 days<P<124.72 days; 1.03 R<Rp<16.35 R).

Additionally, we identified 10 new exoplanet candidates (1.20 days<P<34.62 days; 1.73 R<Rp<4.19 R) that passed vetting tests, including two new statistically validated sub-Neptunes, TIC 219893931b and TIC 237254473b. COUNTESS enables extended-baseline TESS analyses and identification of longer-period planets, establishing a foundation for future exoplanet demographic studies, including comparisons with Kepler and K2.

Andrew Hotnisky, Rachel B. Fernandes, Kevin K. Hardegree-Ullman, Steven Giacalone, Kiersten M. Boley, Kristo Ment, Michelle Kunimoto, Galen J. Bergsten, Sakhee Bhure, Jessie L. Christiansen, Brandon Radzom, Suvrath Mahadevan

Comments: 26 pages, 10 figures, 6 tables; resubmitted to AAS Journals after addressing referee comments
Subjects: Earth and Planetary Astrophysics (astro-ph.EP); Instrumentation and Methods for Astrophysics (astro-ph.IM); Solar and Stellar Astrophysics (astro-ph.SR)
Cite as: arXiv:2606.13789 [astro-ph.EP] (or arXiv:2606.13789v1 [astro-ph.EP] for this version)
https://doi.org/10.48550/arXiv.2606.13789
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Submission history
From: Andrew Hotnisky
[v1] Thu, 11 Jun 2026 18:01:13 UTC (14,312 KB)
https://arxiv.org/abs/2606.13789
Astrobiology, Astronomy, Exoplanet,

Biologist, Explorers Club Fellow, ex-NASA Space Biologist and Payload integrator, Editor of NASAWatch.com and Astrobiology.com, Lapsed climber, Explorer, Synaesthete, Former Challenger Center board member 🖖🏻