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 […]


Continue.. Mechanical Studies of an Additional Light Baffle for the LSST Camera

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 […]


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

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

The Companions to B and A Stars Snapshot (C-BASS) Survey: I. Discovery of a Young Brown Dwarf Companion to HIP 17453

Kavli Affiliate: Bruce Macintosh | Summary:We report the detection of a new brown dwarf companion to HIP 17453 A, a chemically peculiar A0V star located at a distance of 81 pc. HIP 17453 A was observed with high-resolution adaptive optics imaging using the Near-Infrared Camera 2 on the Keck II telescope as part of the […]


Continue.. The Companions to B and A Stars Snapshot (C-BASS) Survey: I. Discovery of a Young Brown Dwarf Companion to HIP 17453

GOATS: The next generation software infrastructure for time-domain astronomy at Gemini/NOIRLab. Application to alerts from Vera C. Rubin Observatory’s Legacy Survey of Space and Time

Kavli Affiliate: Kevin Reil | Summary:Time-domain and multimessenger astronomy (MMA/TDA) targets demand rapid-response follow-up observations. In many cases, it is the only way to make discoveries and advance our understanding of the astrophysical phenomena, for example, kilonovae accompanying gravitational waves from compact object mergers, shock breakout in supernovae, prompt emission from GRBs, etc. Presently the […]


Continue.. GOATS: The next generation software infrastructure for time-domain astronomy at Gemini/NOIRLab. Application to alerts from Vera C. Rubin Observatory’s Legacy Survey of Space and Time

The Multi-phase HI of the Milky Way and Nearby Galaxies

Kavli Affiliate: Susan Clark | Summary:Atomic hydrogen (HI) is the dominant baryonic component of the interstellar medium (ISM) in Milky Way-like galaxies and the reservoir from which molecular clouds and stars ultimately form. The condensation of diffuse HI into cold structures is governed by a complex interplay between radiative cooling, turbulence, magnetic fields, stellar feedback, […]


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Measuring Magnetic Fields Near and Far with the SKA via the Zeeman Effect

Kavli Affiliate: Susan Clark | Summary:Zeeman splitting in spectral lines — both in emission and absorption — provides direct estimates of magnetic field strength and direction in magnetized gas in our own Milky Way and in external galaxies. We discuss the potential for using the Square Kilometre Array (SKA) to measure the Zeeman effect in […]


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Coupled atmospHere Interior modeL Intercomparison (CHILI). I. Evolutionary Modelling — Primordial Magma Oceans of Earth and Venus

Kavli Affiliate: Laura Schaefer | Summary:Earth and Venus represent two evolutionary outcomes arising from initially molten ‘magma ocean’ periods, followed by lifetimes of chemical and geophysical divergence. Their physics is common to all rocky planets and is accessible to simulations that adopt coupled interior-atmosphere modelling approaches. Our understanding of planet histories and interpretation of current […]


Continue.. Coupled atmospHere Interior modeL Intercomparison (CHILI). I. Evolutionary Modelling — Primordial Magma Oceans of Earth and Venus

Discovery of an Exterior Third Planet Orbiting $β$ Pictoris

Kavli Affiliate: Bruce Macintosh | Summary:We report the discovery of $β$ Pictoris d ($β$ Pic d), a third giant planet in the $β$ Pictoris system, which now becomes only the second directly imaged system with more than two confirmed planets. $β$ Pic d was serendipitously detected in JWST/NIRSpec IFU observations. A second epoch of NIRSpec […]


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