![Waste-heat temperature–luminosity phase space. Existing midinfrared searches occupy the warm band (orange); cold computational radiators fall in the far-infrared/submillimetre band (green) towards the CMB floor. Grey lines show 345-GHz flux-density contours for a source at 100 pc, from equation (10), which is linear in the fractional waste-heat luminosity 𝑓 on the vertical axis; the figure thus covers partial swarms and complete spheres (𝑓 = 1) alike. Markers indicate a complete 1 L⊙ cold sphere, the level of the archival debris-survey limits (Section 6.1), and the domain of warm mid-infrared searches. -- [astro-ph.IM]](https://i0.wp.com/astrobiology.com/wp-content/uploads/2026/09/Slysh.png?resize=1200%2C720&ssl=1)
[astro-ph.IM] Searches for Dysonian waste heat have operated almost exclusively in the mid-infrared and are therefore sensitive primarily to technology radiating at 100-600K. We argue that mature, computation-dominated civilisations may […]
Astronomy & Telescopes
![Best-fit model spectra and residuals for the HWO and LIFE datasets (grey and black data points with error bars). Shaded regions show posterior predictive intervals, and the lower panel shows residuals in units of σ. Bottom: Residual between the data and model as measured by 1-σ uncertainty. -- [astro-ph.EP]](https://i0.wp.com/astrobiology.com/wp-content/uploads/2026/09/on-the.png?resize=1200%2C715&ssl=1)
Posted inBiosignatures & Paleobiology
On The Impact Of Correlated Noise and Spectral Resolution On The Retrieval Analysis Of The Habitable World Observatory
[astro-ph.EP] Finding signs of life elsewhere in the universe is the holy grail of the field of exoplanets. Future space missions such as the Habitable World Observatory (HWO) are under […]
![Schematic diagram of the simulated architecture. It includes the segmented primary mirror, an APLC coronagraph with an apodizer, a focal plane mask and a Lyot stop, two deformable mirrors, and an out-of-band and a low-order Zernike wavefront sensor. -- [astro-ph.IM]](https://i0.wp.com/astrobiology.com/wp-content/uploads/2026/09/JWST-telemetry.png?resize=1200%2C712&ssl=1)
Posted inAstronomy & Telescopes
JWST Telemetry Combined With Active Coronagraphy: Raw Contrast Predictions For Exoplanet Imaging With The Habitable Worlds Observatory
[astro-ph.IM] We provide a quantification of the technological gap between the James Webb Space Telescope (JWST) and the Habitable Worlds Observatory (HWO) for the goal of exo-Earth imaging around Sun-like […]
Posted inAstrobiology (general)
The SETI Institute And ETH Zurich Join Forces To Search For The Origin Of Life
[SETI Institute]. The question of how life originated and whether it exists elsewhere in the universe has fascinated humanity for centuries. Now, ETH Zurich and the SETI Institute in California […]
![Overview of the optical design of the testbed, which features an AO module, a coronagraph module, and ample space for science cameras and visitor experiments. Abbreviations: CDM: Coronagraphic DM, DM: Deformable Mirror, FM: Fold Mirror, (F/L)LOWFS: focal-plane/Lyot-stop low-order wavefront sensor, OAP: Off-Axis Parabola, PSM: PupilSteering Mirror, TS: Turbulence Simulator -[astro-ph.IM]](https://i0.wp.com/astrobiology.com/wp-content/uploads/2026/09/NEXT.png?resize=1200%2C714&ssl=1)
Posted inAstronomy & Telescopes
NEXT: The Netherlands EXoplanet Testbed I. Goals And opto-mechanical Design
[astro-ph.IM] We report on the goals, design, and ongoing development of the Netherlands EXoplanet Testbed (NEXT), a high-contrast imaging testbed under construction in Leiden.
Posted inAstronomy & Telescopes
Roman Space Telescope Leaves Earth
[NASA]. Now on a three-month, million-mile journey to its final orbit, NASA’s Nancy Grace Roman Space Telescope will soon reveal the universe’s darkest secrets. The mission launched at 7:26 a.m. […]
Posted inAtmospheres, Climate, Weather
Atmospheric Retrieval of Combined JWST, HST, and Ground-Based Observations Reveals a Featureless Transmission Spectrum for GJ 1132 b
[astro-ph.EP] We present a panchromatic transmission spectrum of GJ1132b spanning 0.71–5.16 μm, combining published transit observations from Magellan/LDSS3C, HST/WFC3 G141, and JWST/NIRSpec (G395H and G395M).
![[LEFT] The MIRI F2100W observation of the HD 107146 system, shown in logarithmic scaling with the corresponding intensity levels indicated in the colorbar. [RIGHT] Contours from the ALMA observations obtained within the ARKS program (S. Marino et al. 2026), overlaid on the combined F182M and F210M JWST/NIRCam observations for HD 107146. -- [astro-ph.SR]](https://i0.wp.com/astrobiology.com/wp-content/uploads/2026/08/The-JWSTNIRCam.png?resize=1200%2C720&ssl=1)
Posted inAstrogeology
The JWST/NIRCam Scattered Light Disks GTO 2780 program: Panchromatic coronagraphic imaging of the HD 10647, HD 32297, HD 61005, HD 107146, and HD 181327 debris disk systems
[astro-ph.SR]. Debris disks, composed of rocks, boulders, planetesimals, and the dust produced in their collisions, present the most readily observable components of mature planetary systems.
![Three-dimensional layout of the four-aperture SELF optical model implemented in Ansys Zemax OpticStudio (Ansys, Inc. 2024), showing the arrangement of the primary and secondary mirrors, together with the optical path used for focalplane image generation. The inset provides a magnified view of the secondary mirrors. -- [astro-ph.IM]](https://i0.wp.com/astrobiology.com/wp-content/uploads/2026/08/Deep-Learning.png?resize=1200%2C720&ssl=1)
Posted inBiosignatures & Paleobiology
Deep Learning-Based Coarse Alignment and Cophasing of a Distributed-Aperture Telescope. Application to the Small ExoLife Finder (SELF)
[astro-ph.IM] The ExoLife Finder (ELF), a 35–50-meter-class Fizeau interferometric telescope, was designed to detect biosignatures on exoplanets through direct imaging. The Small ExoLife Finder (SELF), a 3.5-meter prototype, serves as […]
![Cumulative oxygen loss for planets at the habitable zone of each sample star over 1 Gyr, assuming constant stellar XUV flux at the HZ and no replenishment of oxygen. The curves are calculated using the energy-limited O2 loss prescription from V. S. Airapetian et al. 2017. Colored lines show individual stars, with solid segments representing the earliest ages (for stars with age ranges) and dashed segments extending beyond the minimum age. The black solid line shows the solar reference. Horizontal lines indicate the present-day Earth atmospheric O2 content (∼0.2 bars; dotted) and the total mass of Earth’s oceans (∼240 bars; dashed), providing reference levels for planetary habitability. -- [astro-ph.SR]](https://i0.wp.com/astrobiology.com/wp-content/uploads/2026/08/Panchromatic.png?resize=1200%2C720&ssl=1)
Posted inHabitable Zones
Panchromatic Spectra of Nearby Low-mass and Sun-like Stars with Directly Imageable Habitable Zones
[astro-ph.SR] Characterizing the high-energy radiation environments of stars plays a critical role in determining which systems’ planets are capable of retaining atmospheres and sustaining habitable conditions.