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Record W4417437252 · doi:10.1088/1538-3873/ae215a

Are We There Yet? Challenges in Quantifying the Frequency of Earth Analogs in the Habitable Zone

2025· article· W4417437252 on OpenAlexafffund
Rachel B. Fernandes, Samson A. Johnson, Galen J. Bergsten, Sakhee Bhure, Kiersten M. Boley, Alan P. Boss, Steve Bryson, William DeRocco, Jeremy Dietrich, Alison Duck, Steven Giacalone, Arvind F. Gupta, Matthias Y. He, Michelle Kunimoto, Kristo Ment, Sheila Sagear, Michele L. Silverstein, Kendall Sullivan, Eliot Halley Vrijmoet, Kevin Wagner, Robert F. Wilson, L. Brefka, Ruslan Belikov, Aritra Chakrabarty, Jessie L. Christiansen, David R. Ciardi, Anne Dattilo, Evan Fitzmaurice, Eric B. Ford, Andrew Hotnisky, Sinclaire Jones, Aman Kar, Ravi Kopparapu, Nataliea Lowson, Eric E. Mamajek, Bertrand Mennesson, Michael R. Meyer, Sarah Millholland, Gijs D. Mulders, Susan E. Mullally, Arjun Murlidhar, Ilaria Pascucci, Darin Ragozzine, Paul Robertson, Karl R. Stapelfeldt, Jason T. Wright

Bibliographic record

VenuePublications of the Astronomical Society of the Pacific · 2025
Typearticle
Language
FieldPhysics and Astronomy
TopicStellar, planetary, and galactic studies
Canadian institutionsUniversity of British Columbia
FundersNatural Sciences and Engineering Research Council of CanadaJet Propulsion LaboratorySpace Telescope Science InstituteOffice of Naval ResearchNational Academies of Sciences, Engineering, and MedicineAmes Research CenterPennsylvania State UniversityU.S. Naval Research LaboratoryAgencia Nacional de Investigación y DesarrolloUniversity of PennsylvaniaNational Aeronautics and Space AdministrationCalifornia Institute of TechnologyOak Ridge Associated UniversitiesNational Science Foundation
KeywordsExoplanetCircumstellar habitable zonePlanetPlanetary habitabilityContext (archaeology)ObservatorySolar System

Abstract

fetched live from OpenAlex

Abstract Searching for life elsewhere in the universe is one of the most highly prioritized pursuits in astronomy today. However, the ability to observe evidence of Earth-like life through biosignatures is limited by the number of planets in the solar neighborhood with conditions similar to Earth. The occurrence rate of Earth-like planets in the habitable zones of Sun-like stars, η ⊕ , is therefore crucial for addressing the apparent lack of consensus on its value in the literature. Here we present a review of the current understanding of η ⊕ . We first provide definitions for parameters that contribute to η ⊕ . Then, we discuss the previous and current estimated parameter values and the context of the limitations on the analyses that produced these estimates. We compile an extensive list of the factors that go into any calculation of η ⊕ , and how detection techniques and surveys differ in their sensitivity and ability to accurately constrain η ⊕ . Understanding and refining the value of η ⊕ is crucial for upcoming missions and telescopes, such as the planned Habitable Worlds Observatory and the Large Interferometer for Exoplanets, which aim to search for biosignatures on exoplanets in the solar neighborhood.

Fetched live from OpenAlex and de-inverted. Abstracts are not stored in this database: the inverted indexes are 8.6 GB of the frame’s 9.3 GB of text, and the host has 13 GB free.

How this classification was reachedexpand

Full frame machine prediction

Teacher imitation

Not calibrated prevalence, not ground truth. Human validation pending. The Gemma side is a direct model label for every work in the frame, read from the title-only record. The Codex side is a classifier learned from the 10,348 direct Codex labels and calibrated to design-weighted sample rates; fields without enough sample support carry no Codex call. Candidate is the union of the two sides; consensus is their intersection. These outputs are machine_predicted_unvalidated and are not human labels.

metaresearch head score (Codex)0.019
metaresearch head score (Gemma)0.100
Version: metacan-v3-hybrid-931329e0061cValidation status: machine_predicted_unvalidated
Candidate categoriesnone
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Simulation or modeling · Consensus signal: none
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.019
Threshold uncertainty score0.099

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0190.100
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0010.001
Bibliometrics0.0040.005
Science and technology studies0.0010.003
Scholarly communication0.0050.010
Open science0.0020.003
Research integrity0.0010.003
Insufficient payload (model declined to judge)0.0040.001

Machine scores (provisional)

The two teacher heads of the student model, read on this work. A score orders the frame for review; it never asserts a category, and the validation status ships verbatim with every row.

Baseline scores from an immature model (maturity gate not passed, 7 training rounds). Scores rank; they never assert a category.

Opus teacher head0.054
GPT teacher head0.263
Teacher spread0.209 · how far apart the two teachers sit on this one work
Validation statusscore_only:v0-immature-baseline · verbatim from the scoring run: score_only means the number may rank works, and no category label ships from it

Classification

machine, unvalidated

Machine predicted; a candidate call from one source (direct Gemma or distilled Codex), not a consensus.

The models applied no category: nothing in the taxonomy fit this work.
Study designSimulation or modeling
Domainnot available
GenreEmpirical

How this classification was reached, model by model and score by score, is at the end of the page under "How this classification was reached".

Quick stats

Citations2
Published2025
Admission routes2
Has abstractyes

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