Results 91 to 100 of about 6,459 (144)

Fully fluorinated non-carbon compounds NF3 and SF6 as ideal technosignature gases. [PDF]

open access: yesSci Rep, 2023
Seager S   +5 more
europepmc   +1 more source

Lessons from Hubble and Spitzer: 1D Self-consistent Model Grids for 19 Hot Jupiter Emission Spectra

open access: yesThe Astrophysical Journal
We present a population-level analysis of the dayside thermal emission spectra of 19 planets observed with Hubble WFC3 and Spitzer IRAC 3.6 and 4.5 μ m, spanning equilibrium temperatures 1200–2700 K and 0.7–10.5 Jupiter masses.
Lindsey S. Wiser   +6 more
doaj   +1 more source

Earth as an Exoplanet. III. Using Empirical Thermal Emission Spectra as an Input for Atmospheric Retrieval of an Earth-twin Exoplanet

open access: yesThe Astrophysical Journal
In this study, we treat Earth as an exoplanet and investigate our home planet by means of a potential future mid-infrared space mission called the Large Interferometer For Exoplanets (LIFE).
Jean-Noël Mettler   +3 more
doaj   +1 more source

X-Ray and UV Observations of the Young Sun HIP 67522: Evidence of Lyα Absorption within the Planetary System

open access: yesThe Astronomical Journal
We present ultraviolet (UV) spectroscopy of the 17 Myr, G0V star HIP 67522. The UV spectrum is characterized by strong chromospheric and transition region emission lines.
Cynthia S. Froning   +9 more
doaj   +1 more source

Characterizing the Time Variability of 2M1207 A + b with JWST NIRSpec/PRISM

open access: yesThe Astronomical Journal
We present JWST NIRSpec/PRISM integral field unit time-resolved observations of 2M1207 A and b (TWA 27), an ∼10 Myr binary system consisting of an ∼2500 K substellar primary hosting an ∼1300 K companion.
Arthur D. Adams   +15 more
doaj   +1 more source

Lyα Emission from K and M Dwarfs: Intrinsic Profiles, Variability, and Flux in the Habitable Zone

open access: yesThe Astrophysical Journal
Lyman-alpha (Ly α ) is the most prominent ultraviolet (UV) emission line in low-mass stars, playing a crucial role in exoplanet atmospheric photochemistry, heating, and escape.
Sarah Peacock   +6 more
doaj   +1 more source

Photochemically produced SO<sub>2</sub> in the atmosphere of WASP-39b. [PDF]

open access: yesNature, 2023
Tsai SM   +84 more
europepmc   +1 more source

No thick carbon dioxide atmosphere on the rocky exoplanet TRAPPIST-1 c. [PDF]

open access: yesNature, 2023
Zieba S   +18 more
europepmc   +1 more source

Home - About - Disclaimer - Privacy