The High-Speed FPGA Readout System for the Advanced X-ray Imaging Satellite (AXIS)

Kavli Affiliate: Marshall Bautz | Summary:The Advanced X-ray Imaging Satellite (AXIS) is a Probe-class mission concept designed to deliver arcsecond spatial resolution, high-sensitivity spectral imaging across the 0.3-10 keV band. The X-ray Astronomy and Observational Cosmology (XOC) Group at Stanford, in collaboration with the MIT Kavli Institute (MKI) and MIT Lincoln Laboratory (MIT-LL), is developing […]


Continue.. The High-Speed FPGA Readout System for the Advanced X-ray Imaging Satellite (AXIS)

Fast, low-noise CCD systems for future strategic X-ray missions

Kavli Affiliate: Marshall Bautz | Summary:Future strategic X-ray missions, such as those targeted by the Great Observatories Maturation Program (GOMaP), require fast, low-noise X-ray imaging spectrometers. To achieve the speed and noise capabilities required by such programs, our Stanford team, in collaboration with the MIT Kavli Institute (MKI) and MIT Lincoln Laboratory (MIT-LL), is developing […]


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RNDR noise modeling in first-generation Single electron Sensitive Readout (SiSeRO) devices

Kavli Affiliate: Marshall Bautz | Summary:Flagship observatories require single-photon detectors with ultra-fast readout, sub-electron noise performance, and scalable large-format architectures. The X-ray Astronomy and Observational Cosmology group at Stanford, in collaboration with the MIT Kavli Institute and MIT Lincoln Laboratory, is developing readout technologies for next-generation detectors. Prototypes employing Single-electron Sensitive Readout (SiSeRO) amplifiers demonstrate […]


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The GOLIATH Survey: OVI Absorption Reveals CGM Evolution through the Starburst-to-Quiescent Transition in Massive Galaxies

Kavli Affiliate: Robert Simcoe | Summary:We present the GOLIATH survey (Galaxies, Outflows, and the Lifecycle of Immense, Active, Transforming Halos), a study of the multiphase circumgalactic medium (CGM) of massive ($langlelog M_star/M_odotrangle approx 11$), blue ($u-r < 1.65$) starburst and post-starburst galaxies at $langle zrangle approx$ 0.43. This work characterizes the warm-hot CGM through OVI […]


Continue.. The GOLIATH Survey: OVI Absorption Reveals CGM Evolution through the Starburst-to-Quiescent Transition in Massive Galaxies

First results for second generation SiSeRO CCD devices

Kavli Affiliate: Marshall Bautz | Summary:The Astro2020 Decadal recommended the development of a suite of next generation astronomical observatories spanning the X-ray to near-IR spectrum. These programs require fast, extremely low noise detectors to fulfill their science goals. To address this technology gap, Stanford X-ray Astronomy and Observational Cosmology (XOC) group, MIT Lincoln Laboratory (MIT-LL), […]


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Star formation, stellar evolution, and planets in high-resolution X-ray imaging

Kavli Affiliate: Moritz Guenther | Summary:Stars set the conditions for planet formation, planet evolution, and habitability — all major topics in astronomy today. Stars are also important in their own right as the most visible component of galaxies. In cool stars, X-ray emission is powered by magnetic fields, and so far our Sun is the […]


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The Lightspeed project: high-speed, ultra-low read noise imaging and polarimetry for the Magellan telescopes

Kavli Affiliate: Gabor Furesz | Summary:Lightspeed will be an ultra-fast (> kHz), ultra-low read noise, multicolor (ugriz + IR) imager for the 6.5 meter Magellan Clay telescope. In a single-channel configuration, Lightspeed will also enable single-shot linear polarimetry, narrowband imaging, or white-light imaging. Lightspeed is designed around groundbreaking single-photon-resolving detector technologies: deep sub-electron read noise […]


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Stellar Multiplicity of M Dwarfs with Short-period Giant Planets, and the Characterization of TOI-5628Ab

Kavli Affiliate: Avi Shporer | Summary:Binary stars are ubiquitous, yet it remains unclear how wide-orbit stellar companions influence the formation of hot Jupiters, particularly around M dwarfs. Here, we first report the discovery of TOI-5628Ab, a giant planet transiting a mid-type M dwarf ($M_ast=0.36pm0.02 M_odot$) every 4.34 days, accompanied by an associated white dwarf TOI-5628B […]


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Overview of the Canadian Hydrogen Observatory and Radio Transient Detector (CHORD) Project

Kavli Affiliate: Kiyoshi Masui | Summary:The Canadian Hydrogen Observatory and Radio-transient Detector (CHORD) is a next-generation wideband radio interferometer currently being constructed and commissioned at the Dominion Radio Astrophysical Observatory in British Columbia, Canada. CHORD is designed for precision 21,cm cosmology, fast radio transient discovery, spectral line galaxy surveys, and pulsar science using a highly […]


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The Thesan-Zoom project: bursty star formation is incompatible with prolonged dust survival

Kavli Affiliate: Mark Vogelsberger | Summary:Cosmic dust is a key regulator of galaxy evolution, but its build-up and survival in the first billion years remain poorly constrained. We present a systematic analysis of dust in the thesan-zoom suite of radiation-hydrodynamical zoom-in simulations, which self-consistently model dust formation, growth, destruction, and its coupling to radiative transfer […]


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