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1. BARBIE. Bayesian Analysis for Remote Biosignature Identification on exoEarths. III. Introducing the KEN

2. The Pale Blue Dot: Using the Planetary Spectrum Generator to Simulate Signals from Hyperrealistic Exo-Earths

3. Investigating Possible Binarity for GJ 229B

4. Grid-based Atmospheric Retrievals for Reflected-light Spectra of Exoplanets Using PSGnest

5. Bayesian Analysis for Remote Biosignature Identification on exoEarths (BARBIE). I. Using Grid-based Nested Sampling in Coronagraphy Observation Simulations for H2O

6. Bayesian Analysis for Remote Biosignature Identification on exoEarths (BARBIE). II. Using Grid-based Nested Sampling in Coronagraphy Observation Simulations for O2 and O3

8. GJ 229B: Solving the Puzzle of the First Known T Dwarf with the APOLLO Retrieval Code

9. Utilizing a Database of Simulated Geometric Albedo Spectra for Photometric Characterization of Rocky Exoplanet Atmospheres

10. The First Habitable-zone Earth-sized Planet from TESS. I. Validation of the TOI-700 System

11. The First Habitable-zone Earth-sized Planet from TESS. III. Climate States and Characterization Prospects for TOI-700 d

12. Validation of 13 Hot and Potentially Terrestrial TESS Planets

13. Dim Prospects for Transmission Spectra of Ocean Earths Around M Stars

14. Optical design of the Extreme Coronagraph for Living Planetary Systems instrument for the LUVOIR mission study

15. Was the Sun a Slow Rotator? Sodium and Potassium Constraints from the Lunar Regolith

17. The Exoplanet Modeling and Analysis Center at NASA Goddard

18. GJ 229B: Solving the Puzzle of the First Known T-Dwarf with the APOLLO Retrieval Code

19. HyDRo: Atmospheric Retrieval of Rocky Exoplanets in Thermal Emission

20. The Transiting Exoplanet Community Early Release Science Program for JWST

25. A Comparison of Simulated JWST Observations Derived from Equilibrium and Non-equilibrium Chemistry Models of Giant Exoplanets.

27. Transiting Exoplanet Studies and Community Targets for JWST's Early Release Science Program.

28. SPECTROSCOPIC EVIDENCE FOR A TEMPERATURE INVERSION IN THE DAYSIDE ATMOSPHERE OF HOT JUPITER WASP-33b.

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