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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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 […]


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Unveil the nature of JWST-AGN and Little Red Dots with SKAO continuum surveys

Kavli Affiliate: Roberto Maiolino | Summary:The advent of JWST has revealed a large population of AGN at $z>4$, which are $sim1$ dex more abundant than previously expected, including also the enigmatic population of Little Red Dots (LRDs). Remarkably, the vast majority of JWST-discovered AGN and LRDs are not detected in X-rays, and most of them […]


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No evolution in the number density of little red dots from cosmic dawn to cosmic noon

Kavli Affiliate: Roberto Maiolino | Summary:We present our search for little red dots (LRDs) in the "J1030 field", a region of the sky around the $zsim 6.3$ quasar SDSS J1030+0524, observed by the JWST EIGER program. Over 154 point-like sources selected in a JWST-based photometric catalog, we find five broad line emitters (with $FWHM gtrsim […]


Continue.. No evolution in the number density of little red dots from cosmic dawn to cosmic noon

High-Redshift Signatures from the Cosmic Dawn and the Epoch of Reionization

Kavli Affiliate: George Efstathiou | Summary:In this chapter, we provide a comprehensive overview of the astrophysical and cosmological processes that shape the 21-cm signal during Cosmic Dawn and the Epoch of Reionization. We investigate both standard and exotic signatures potentially observable with SKA-Low. Standard signatures are those expected within the $Λ$CDM framework, including contributions from […]


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SEEDZ: Rapid Galaxy Assembly as a Pathway to Supermassive Stars, Dense Stellar Environments and Massive Black Hole Seeds

Kavli Affiliate: Martin Haehnelt | Summary:We investigate the assembly history of early galaxies in the SEEDZ hydrodynamic simulations, to investigate the high inflow rates believed to be required for the formation of supermassive stars (SMSs), dense stellar clusters and subsequently heavy seed black holes. Using a heavy seed formation criteria of $>$1 M$_odot$ yr$^-1$ flowing […]


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Overview of 21cm Experiments at high redshift with SKAO

Kavli Affiliate: George Efstathiou | Summary:We provide an overview of the eight SKAO Science Book chapters that motivate the Epoch of Reionisation and Cosmic Dawn experiments with SKA-Low. We describe the individual SKA-Low experiments and expected sensitivity – power spectrum, tomography, 21-cm forest, cross-correlations, building on the broad observational plan laid out in the 2015 […]


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Little Red and Blue Dots: AGN-excited narrow lines, Lyman-$α$ emission, and resemblance to standard quasars

Kavli Affiliate: Roberto Maiolino | Summary:We present an analysis of a sample of 36 Little Red and Blue Dots (LRDs and LBDs) at $2.26<z<7.89$, identified by JWST in the GOODS fields. While both categories are selected to have broad Balmer lines, both of them are extremely X-ray weak. Both classes share the same location on […]


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Little Red Dots as Supermassive Analogs of SS 433

Kavli Affiliate: Roberto Maiolino | Summary:High-redshift little red dots (LRDs) are compact sources characterized by V-shaped spectral energy distributions (SEDs), broad emission lines, and often prominent Balmer breaks. Their high number density and apparently large black hole masses suggest that they are essential to the early evolution of galaxies and supermassive black holes (SMBHs); however, […]


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Hawai`i Supernova Flows: Bulk Flow Measurements using SNe Ia in the Optical and NIR

Kavli Affiliate: Kaisey Mandel | Summary:The present day peculiar velocity-field was sourced by primordial density fluctuations and sculpted over the lifespan of the Universe. Cosmological models such as $Λ$CDM make predictions for various statistical properties of peculiar velocities. Bulk flow, the average velocity within a given volume, has an expectation value of $vec0$ due to […]


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