[astro-ph.IM]. A wavefront-sensor (WFS) prediction can select the photon measurement before detection or condition its likelihood afterward.
astronomy
![Grad-CAM autopsy at an amplitude of 4.0. (a) Q2_bright_hit: D1-3 S-shaped, detected. (b) Q2c_bright_mis: D1-1 extreme drift, missed. Columns: input, Grad-CAM map, and CAM difference (injected minus clean). Inputs are shown as the detector sees them: the three ON panels side by side, with frequency running vertically; white lines mark panel boundaries and the green line the injection’s starting channel. -- [astro-ph.IM]](https://i0.wp.com/astrobiology.com/wp-content/uploads/2026/10/Missed-Detections.png?resize=1200%2C720&ssl=1)
Posted inSETI & Technosignatures
Missed Detections and False Alarms in a CNN Technosignature Detector on Breakthrough Listen Data
[astro-ph.IM] Radio technosignature searches rely on machine learning detectors to shrink the candidate pool before a human looks at it.
Posted inExoplanets, -moons, -comets
Trailblazing Technique Uncovers The Real Shape Of Scorching-hot Exoplanet Atmospheres
[University of Bristol] Until now the alien white-hot worlds of exoplanets have been depicted as circular, but new research has revealed the true shape of their atmospheres to be a […]
Posted inExoplanets, -moons, -comets
Ultraviolet Reflected-Light Spectroscopy of Modern Earth Analogs with Starshade Observations
[astro-ph.EP] Characterizing rocky, habitable zone planets in reflected light is a key science objective for future direct imaging missions, and the ultraviolet (UV) is uniquely suited for supporting the characterization […]
![Time evolution of the vertical gradient of AH across different height layers is shown. The black line overlaid indicates the corresponding PWV in mm.-- [astro-ph.IM]](https://i0.wp.com/astrobiology.com/wp-content/uploads/2026/10/MidIR.png?resize=1200%2C715&ssl=1)
Posted inExoplanets, -moons, -comets
Mid-IR Water-Vapor Seeing: Implications for ELT/METIS High-Contrast Imaging from VLTI Data
[astro-ph.IM] Direct imaging and characterization of rocky exoplanets remains one of the central challenges in exoplanetary science. The mid-infrared (mid-IR) offers a favorable high-contrast imaging (HCI) regime, as the planet-star […]
Posted inAstronomy & Telescopes
Call For White Papers On Multi-Cycle Treasury Concepts With JWST
[ESA Hubble] STScI has issued a call for White Papers for compelling scientific ideas for Multi-Cycle Treasury (MCT) programmes that require large allocations of JWST time to complete.
![[Left]: A concept raytrace showing the IFS, with just the FUV channels shown. The NUV channels take the zero-order from each FUV grating and reflect it towards the IFS fold mirror (on either side) into a similar format NUV IFS (see Haughton et al., 2026 for a depiction of the INFUSE design that this IFS is based on13). The IFS assembly is forward (out of the page) from the MOS at the focal plane, with the IFS fold mirror canted slightly to move the slicer, gratings, and detectors over 0.7 meters from the MOS optical path. [Right]: The slicer-based IFS operates by reflecting portions of the image plane to different gratings, which then focus a spectrogram to a unique portion of the detector. In essence, each reflective slice operates like a long-slit spectrograph, with the slicer geometry separating the multi-slit spectrograph to avoid spectral confusion.-- astro-ph.IM](https://i0.wp.com/astrobiology.com/wp-content/uploads/2026/10/An-Ultraviolet.png?resize=1200%2C563&ssl=1)
Posted inAstronomy & Telescopes
An Ultraviolet Instrument On The Habitable Worlds Observatory: Considerations and Capability Trades On The Multi-Object, Integral-field, and High-resolution Modes Of A Potential UVI
[astro-ph.IM] The Habitable Worlds Observatory (HWO) is NASA’s next-generation astrophysics platform, delivering transformative capability in the search for life and study of the origins of the universe.
![Planet mass as a function of host mass for systems included in the NASA Exoplanet Archive (Christiansen et al. 2025) queried on 4 March 2026. Only systems with a host mass M < 0.2 M⊙ and available system distance are shown. PALTA-1 b is indicated with a diamond and the symbol colour indicates the system’s distance from the Sun.-- [astro-ph.EP]](https://i0.wp.com/astrobiology.com/wp-content/uploads/2026/10/Astrometric-planet.png?resize=1200%2C721&ssl=1)
Posted inExoplanets, -moons, -comets
Astrometric Planet Search Around Southern Ultracool Dwarfs: V. Discovery Of The Exoplanet Candidate PALTA-1 b
[astro-ph.EP] We report the discovery of PALTA-1 b, a sub-Jupiter mass exoplanet candidate orbiting the nearby early-L dwarf DENIS-P J1253108-570924 (DE1253-57) located at a distance of ~17 pc.
![(Top row:) Composite images on three dates (Table 1) shown with a common display range from -0.01 to 0.02 adu pixel−1 . (Bottom row:) Same images from the top row contoured from 0.0004 adu pixel−1 in steps of 0.002 adu pixel−1 . Contours are smoothed over 8×8 pixel boxes. Yellow arrows show the projected antisolar direction while white arrows show the projected negative heliocentric velocity vector, from Table 1. The two directions are overlapping in the 2023 data. A 1′′ scale is common to all panels.-- [astro-ph.EP]](https://i0.wp.com/astrobiology.com/wp-content/uploads/2026/10/Hubble-Space-.png?resize=1200%2C725&ssl=1)
Posted inComets and Asteroids
Hubble Space Telescope Observations of Active Asteroid (101955) Bennu
[astro-ph.EP] Measurements from NASA’s OSIRIS-REx spacecraft revealed (101955) Bennu as a member of the active asteroid class.
Posted inExoplanets, -moons, -comets
SOPHIE And TESS Characterization Of Fourteen TESS Objects Of Interest: Nine Planetary Systems And Five Low-mass Stellar Companions
[astro-ph.EP] We present fourteen TESS Objects of Interest (TOIs) from the SOPHIE-TESS follow-up program. Combining TESS photometry, SOPHIE radial velocities (RVs), ground-based photometry, and high-resolution imaging, we establish the nature […]