Synaptic activity controls local exposure of an ‘eat-me’ signal via ANO3-ITPR1 signaling

Kavli Affiliate: Lily Jan | Authors: Kunal Shroff, Molly C O’Brien, Tyler J Smith, Jialing Fang, Kelly S Yu, Sonia I Lombroso, Shengjie Feng, Chao Chen, Gregory A Mohl, Indigo V L Rose, Nidhi R Lokesh, Mark E Pownall, Lily Y Jan and Martin Kampmann | Summary: Neuronal synapses are eliminated during brain development and […]


Continue.. Synaptic activity controls local exposure of an ‘eat-me’ signal via ANO3-ITPR1 signaling

How can we finally see the first light? Status and perspective in the search for Population III stars

Kavli Affiliate: Roberto Maiolino | Summary:Finding the first (Population III or Pop III) stars is one of the fundamental quests of astronomy, aiming to deliver the missing link in how stars form at early cosmic times. Yet their initial mass function, formation sites and feedback remain highly uncertain, as well as the timing and topology […]


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Rubin M1M3 Dynamic performance : stability and actuation during operations

Kavli Affiliate: Kevin Reil | Summary:The Vera C. Rubin Observatory is preparing to commence the Legacy Survey of Space and Time with the fully integrated Simonyi Survey Telescope. To verify that the primary/tertiary (M1M3) mirror system is ready to meet the demanding survey requirements, dynamic tests of the 8.4 m, 53 ton M1M3 system were […]


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The filter exchange system of the LSSTCam at the Vera C. Rubin Observatory

Kavli Affiliate: Stuart Marshall | Summary:The Filter Exchange System of the LSSTCam at the Vera C. Rubin Observatory is a critical subsystem enabling the Legacy Survey of Space and Time (LSST) by performing rapid, repeatable exchanges among five large-format filters within a highly constrained in-camera volume. Since the start of on-sky operations in April 2025, […]


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An overview of stray light findings and interpretation during on-sky commissioning of LSSTCam

Kavli Affiliate: Aaron Roodman | Summary:Wide-field telescopes are intrinsically difficult to shield from unwanted stray and scattered light, while the search to identify sources of contaminating light is frequently a challenging task. The Vera C.~Rubin Observatory, which achieved its first photon with the LSST Camera (LSSTCam) on April 15, 2025, will initiate a revolutionary era […]


Continue.. An overview of stray light findings and interpretation during on-sky commissioning of LSSTCam

A Suppressed Volumetric Rate of High-Luminosity Mid-Infrared Selected Tidal Disruption Events

Kavli Affiliate: Erin Kara | Summary:Tidal Disruption Events (TDEs) serve as direct probes of the population of supermassive black holes in the center of galaxies and are nowadays regularly detected in optical wide-field time-domain sky surveys. Recent studies have demonstrated that a large fraction of TDEs can be uniquely identified in the infrared (IR) waveband, […]


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Mechanical Studies of an Additional Light Baffle for the LSST Camera

Kavli Affiliate: Aaron Roodman | Summary:Commissioning the NSF-DOE Vera C. Rubin Observatory consisted of engineering operation and on-sky data-taking, initially with the Commissioning Camera followed by the commissioning run of the LSST Camera (LSSTCam). As with other wide-field astronomical projects, the Rubin team anticipated a significant amount of stray light effects which would necessitate investigation […]


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Early Telescope Throughput Results from the Collimated Beam Projector at the Vera C. Rubin Observatory

Kavli Affiliate: Eli Rykoff | Summary:The Vera C. Rubin Observatory LSST requires precise photometric calibration to meet its science goals, particularly for cosmological analyses based on Type Ia supernovae. The Collimated Beam Projector (CBP) has been developed to support this effort by projecting monochromatic point sources of known wavelength and flux directly into the telescope […]


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The On-Sky Performance of the LSST Camera CCD Array

Kavli Affiliate: Steven Kahn | Summary:The focal plane of the LSST Camera contains 189 individual science CCDs, arranged into 21 raft tower modules, along with 4 wavefront and 8 guider CCDs located in 4 additional corner RTMs. Altogether, the LSST Camera CCDs compose the largest focal plane ever constructed. The LSST Camera is the primary […]


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Modeling of the diffuse background produced by the Vera C. Rubin Observatory M2 baffle scattered light

Kavli Affiliate: Aaron Roodman | Summary:The Vera C. Rubin Observatory, with its unprecedented field of view and fast focal ratio, will survey the entire sky every 3.5 nights. This unique capacity requires dealing with off axis light that can produce stray light artefacts on the images. The secondary mirror (M2) baffle restricts the light that […]


Continue.. Modeling of the diffuse background produced by the Vera C. Rubin Observatory M2 baffle scattered light