![Left: SCALES optical diagram. Right: Image of the focal plane coronagraph slide mask holder, with flight optics labeled. -- [astro-ph.IM]](https://i0.wp.com/astrobiology.com/wp-content/uploads/2026/09/Pre-shipment.png?resize=1200%2C720&ssl=1)
[astro-ph.IM] The Slicer Combined with an Array of Lenslets for Exoplanet Spectroscopy (SCALES) instrument is a 1-5 micron imager and 2-5 micron integral field spectrograph, currently being commissioned on the […]
astro-ph.IM
Posted inApps - Games
pyEDITH: The Coronagraphic Exposure Time Calculator For The Habitable Worlds Observatory
[astro-ph.IM] To support the development of next-generation missions for the search and characterization of habitable planets, high-fidelity tools for astrophysical and instrumental noise simulations are needed.
![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)
Posted inSETI & Technosignatures
Slysh Haloes: The Waste Heat Of Cold Computing As A Submillimetre Technosignature
[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 […]
![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 […]
![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.
![Early draft of a possible layout for the MPIA to test the Bertin-Alpao 13k DM. Key components are numbered and described in the text. This version makes use of polarization components to simplify the number of optical elements. -- [astro-ph.IM]](https://i0.wp.com/astrobiology.com/wp-content/uploads/2026/08/Development.png?resize=1200%2C712&ssl=1)
Posted inUncategorized
Development Of An Adaptive Optics Testbed At MPIA For The ELT/Planetary Camera And Spectrograph (PCS)
[astro-ph.IM] The Planetary Camera and Spectrograph (PCS) is a proposed second-generation instrument for the Extremely Large Telescope (ELT), dedicated to the direct imaging and characterization of exoplanets.
![LOCO-CV predicted vs DFT binding energies for 13 adsorbate species on ASW12 clusters. Each point represents a single adsorbate–surface configuration, coloured by species identity; asterisks denote radical species. Pooled metrics across all leave-one-cluster-out folds: R2 = 0.896, RMSE = 574 K, MAE = 378 K. -- [astro-ph.GA]](https://i0.wp.com/astrobiology.com/wp-content/uploads/2026/08/AstroBind.png?resize=1200%2C715&ssl=1)
Posted inAstrochemistry
AstroBind: Machine Learning Prediction Of Binding Energy Distributions On Interstellar Water Ice From Geometric Surface Descriptors
[astro-ph.GA] Binding energies on amorphous solid water regulate molecular desorption in molecular clouds and protoplanetary disks, but computing them from first principles across the heterogeneous binding sites of disordered ice […]
![The PM showing the mounted SHAPE instrument (left) along with the zoomed in view (right). Three major sub-systems are also marked. -- [astro-ph.IM]](https://i0.wp.com/astrobiology.com/wp-content/uploads/2026/08/Shaping-SHAPE.png?resize=1200%2C714&ssl=1)
Posted inExoplanets, -moons, -comets
Shaping SHAPE – A Spectro-polarimeter Onboard Chandrayaan-3 To Observe Earth As An Exoplanet
[astro-ph.IM] Spectro-polarimetry of HAbitable Planet Earth (SHAPE) is an experimental instrument onboard the Propulsion Module (Orbiter) of the Chandrayaan-3 mission, designed to perform disc-integrated spectro-polarimetric observations of Earth from lunar […]
Posted inSETI & Technosignatures
The VLA and High-Frequency SETI: Expanding The Search for Life
[astro-ph.IM] The Commensal Open-Source Multimode Interferometer Cluster (COSMIC) runs software that searches for technologies elsewhere in the Universe (“technosignatures”) using the Karl G. Jansky Very Large Array (VLA). Specifically, it […]