The JADES Transient Survey II: Volumetric Supernova Rates out to z~5

Kavli Affiliate: Roberto Maiolino | Summary:The JADES Transient Survey (JTS) identified 83 supernova (SN) candidates in the JADES Deep Field, a $sim$25 arcmin$^2$ region with deep ($sim$30 mag) multi-band, multi-epoch JWST/NIRCam coverage. We use this sample to derive the first volumetric core-collapse (CC) SN and Type Ia (SN Ia) rates in the $z$$sim$2-5 range. Many […]


Continue.. The JADES Transient Survey II: Volumetric Supernova Rates out to z~5

The Era of Precision in Computational Models of Gravitational Waves

Kavli Affiliate: Ulrich Sperhake | Summary:Einstein’s equations of general relativity are one of the most complicated set of equations in all of physics and, for all but idealized physical settings, can only be solved by numerical methods on high-performance computing systems. Generating such solutions is a veritable Odyssey in its own right with adventures across […]


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BlackTHUNDER Reveals a Massive Filament around a Compact AGN at $zsimeq5.23$

Kavli Affiliate: Roberto Maiolino | Summary:Despite the growing number of compact active galactic nuclei (AGN) at $z>4$ discovered by JWST, their formation and evolution remain poorly understood. This paper investigates the large-scale environment of GN-77652, a compact AGN at $z=5.229$ observed as part of the JWST NIRSpec IFU Large Program BlackTHUNDER and complemented by deep […]


Continue.. BlackTHUNDER Reveals a Massive Filament around a Compact AGN at $zsimeq5.23$

Globular cluster abundance patterns inherited from giant molecular clouds

Kavli Affiliate: Roberto Maiolino | Summary:Globular clusters exhibit large star-to-star variations and anticorrelations in their light element abundances that are commonly interpreted in terms of in-cluster self-enrichment, in which ejecta from early-forming cluster stars pollute the gas from which later stars form over millions of years. Yet proposed self-enrichment scenarios suffer from a severe mass-budget […]


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Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations

Kavli Affiliate: Debora Sijacki | Summary:The recent detection of a gravitational wave background (GWB) by pulsar timing arrays (PTAs) may represent the first evidence of gravitational waves from merging supermassive black hole binaries, opening a new window on the low-frequency end of the gravitational wave spectrum. These inspiralling binaries are expected to dominate the signal, […]


Continue.. Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations

Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations

Kavli Affiliate: Debora Sijacki | Summary:The recent detection of a gravitational wave background (GWB) by pulsar timing arrays (PTAs) may represent the first evidence of gravitational waves from merging supermassive black hole binaries, opening a new window on the low-frequency end of the gravitational wave spectrum. These inspiralling binaries are expected to dominate the signal, […]


Continue.. Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations

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 […]


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

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 […]


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

Numerical polology: towards next-generation model-building for cosmology

Kavli Affiliate: Anthony Lasenby | Summary:The dark sector need not be restricted to simple field content. Indeed, simple bosonic configurations, such as scalar-tensor or dark photon models, contrast with the much richer picture painted by many ultraviolet scenarios. Polology is the study of propagator poles, which correspond to particle states in any given theory. We […]


Continue.. Numerical polology: towards next-generation model-building for cosmology

Numerical polology: towards next-generation model-building for cosmology

Kavli Affiliate: Anthony Lasenby | Summary:The dark sector need not be restricted to simple field content. Indeed, simple bosonic configurations, such as scalar-tensor or dark photon models, contrast with the much richer picture painted by many ultraviolet scenarios. Polology is the study of propagator poles, which correspond to particle states in any given theory. We […]


Continue.. Numerical polology: towards next-generation model-building for cosmology