[astro-ph.IM] The orbiter of the Chandrayaan-3 mission of the Indian Space Research Organisation (ISRO) carries an experimental payload called SHAPE (Spectro-polarimetry of HAbitable Planet Earth). This payload makes disc-integrated observations […]
astronomy
![Sensitivity of the adopted contrast curves for the newly validated planets, separated by technique. Each pixel gives the fraction of curves sensitive to a companion of the given magnitude contrast (∆mag) at the given angular separation (∆arcsec), shading from white (all curves sensitive) to black (none sensitive). Speckle observations are confined to their ∼ 1.2 ′′ field of view, while the adaptive-optics curves extend to wider separations. Contrasts are in each observation’s native band and are not directly comparable across instruments (cf. Table 2).-- [astro-ph.EP]](https://i0.wp.com/astrobiology.com/wp-content/uploads/2026/09/Assessing-the.png?resize=1200%2C720&ssl=1)
Posted inExoplanets, -moons, -comets
Assessing the Impact of High-Resolution Imaging on Statistical Validation of TESS Planet Candidates
[astro-ph.EP] High-resolution imaging is widely used to constrain false-positive scenarios in exoplanet validation, but it is a finite follow-up resource that reaches only a subset of candidates, and its population-level […]
Posted inExoplanets, -moons, -comets
Eight New Planets Join The NASA Exoplanet Archive
[NASA Exoplanet Archive]. This week, the archive welcomes eight new planets: CD-35 2722 B b, HD 50554 c & d, KMT-2025-BLG-0975L b, KMT-2025-BLG-1160L b, TOI-3053 b, TOI-3278 b, and TOI-4409 b. We also bid adieu to WASP-126 […]
Posted inAstrochemistry
The Galactic Centre G+0.633-0.0604 Molecular Cloud: A New Astrochemical Gold Mine
[Astronomy and Astrophysics] Context. In the central molecular zone (CMZ) environment, shocks play a key role in both triggering star formation and providing chemical enrichment. The Sgr B2 complex is […]
NASA Planetary Science Early Career Award 2024 Showcase
Join us September 16 from 3-5 PM ET on Webex for the 2024 Planetary Science Early Career Award Showcase, featuring talks from selected investigators from ROSES-2024. Speakers will highlight projects […]
![RMS vs bin-size of the residuals from our TTV fits (see Section 4.1). The four panels show the 2x2 different reduction-likelihood pairings considered in this work. The two jitter treatments find binning behavior worse than that expected from pure Gaussian noise (dashed line), and instead have a slope of ∼ − 1/3, similar to other NIRSpec PRISM results (e.g. Kipping et al. 2025). The inclusion of a GP to absorb time-correlated noise greatly reduces the slopes, as again expected.-- [astro-ph.EP]](https://i0.wp.com/astrobiology.com/wp-content/uploads/2026/09/JWST-Excludes.png?resize=1200%2C720&ssl=1)
Posted inExoplanets, -moons, -comets
JWST Excludes Exomoons Down to 0.1 Earth Radii Around a Rocky, Temperate Exoplanet
[astro-ph.EP] To date, even with JWST, it has not been possible to test for exomoons as small as the Moon. Only two reported searches for exomoons around bound planets have […]
Posted inExoplanets, -moons, -comets
The Metallicity Of Giant Exoplanets Around Low-mass Stars And How Ariel Can Help
[astro-ph.EP] Giant planets orbiting low-mass stars represent a unique population of giant planets that can be studied to constrain planet formation theory. Surveys of transiting giant exoplanets around M-dwarfs (GEMS) […]
![Zoomed-in 12CO J = 3 − 2 channel maps. Contours are 3, 6 and 10σ. The isovelocity contours are calculated with a flat surface. The planet locations are marked with white dots. The beam is given in the bottom right corner while the velocity of the channel is provided in the bottom left corner. Fig. F.5 shows the channel maps over the full extent of the disk.-- [astro-ph.EP]](https://i0.wp.com/astrobiology.com/wp-content/uploads/2026/09/Mapping.png?resize=1200%2C717&ssl=1)
Posted inExoplanets, -moons, -comets
Mapping the WISPIT2 Planet-Hosting Cavity at Sub-Hill-Radius scales
[astro-ph.EP] We present new deep, very high angular resolution observations of the sub-mm continuum (19×13 mas) and 12CO (67×52 mas) emission from the disk surrounding the planet host WISPIT2. Our […]
Posted inSETI & Technosignatures
Identifying Casual SETI Transmissions And Ultra-Faint RFI With Cumulant Imaging
[astro-ph.IM] Techniques for identifying radio beacons transmitted by extra-terrestrial civilizations are well advanced.
Posted inUncategorized
Multi-Wavelength Post-Perihelion Polarimetry of Interstellar Comet 3I/ATLAS
[astro-ph.EP] We present new post-perihelion polarimetric observations of the third discovered interstellar object, 3I/ATLAS (C/2025 N1; hereafter 3I), obtained using FORS2 at the Very Large Telescope, ALFOSC at the Nordic […]