Wings of little dots: Exponential broad lines from a stratified BLR

Kavli Affiliate: Roberto Maiolino | Summary:We investigate the origin of the broad exponential wings observed in a significant fraction of the Halpha profiles of JWST-discovered little red dots (LRDs) and little blue dots (LBDs). Recent studies have shown that exponential broad-line profiles are not a prerogative of LRDs, are often also present in LBDs, and […]


Continue.. Wings of little dots: Exponential broad lines from a stratified BLR

Holes in the BH$^star$? AGN signatures in the FUV spectrum of a black-hole dominated Little Red Dot at $z=7.04$

Kavli Affiliate: Roberto Maiolino | Summary:It has been suggested that "Little Red Dots" (LRDs) might be accreting black holes enshrouded by dense gas in a nearly closed geometry, which completely covers the central black hole, leading to an atmosphere-like structure known as the "black-hole star" ($rm BH^star$). We test this scenario by analysing new JWST […]


Continue.. Holes in the BH$^star$? AGN signatures in the FUV spectrum of a black-hole dominated Little Red Dot at $z=7.04$

Supernova 2025wny: High-angular resolution Keck/NIRC2 observations and preliminary lens modeling

Kavli Affiliate: Kaisey Mandel | Summary:Multiply imaged, gravitationally lensed supernovae are rare but powerful tools for providing independent measurements on cosmological parameters. Supernova (SN) 2025wny ("SN Winny") is the first gravitationally-lensed Type I superluminous supernova and the first lensed supernova in a galaxy-scale system that is suitable for time-delay cosmography studies. In this work, we […]


Continue.. Supernova 2025wny: High-angular resolution Keck/NIRC2 observations and preliminary lens modeling

Optimisation of calibration sources for global 21-cm experiments: the REACH case

Kavli Affiliate: George Efstathiou | Summary:The spin-flip 21-cm signal from the Cosmic Dawn and the Epoch of Reionization is an essential probe of the conditions that led to the formation of the first luminous objects in the early Universe. However, its detection remains a major challenge owing to its low strength compared to the bright […]


Continue.. Optimisation of calibration sources for global 21-cm experiments: the REACH case

Constraints on the host galaxy and AGN properties of three z > 6 JWST AGN from NOEMA observations

Kavli Affiliate: Roberto Maiolino | Summary:We targeted with deep NOEMA observations the [CII]158$μ$m emission of three JWST-discovered AGN at z>6. Two of them have the typical features of Little Red Dots (LRDs), while the third one is a blue, extended, Type I AGN. We do not significantly detect [CII] emission or dust continuum in any […]


Continue.. Constraints on the host galaxy and AGN properties of three z > 6 JWST AGN from NOEMA observations

Estimation and mitigation of foregrounds in projected kSZ velocity reconstruction

Kavli Affiliate: Anthony Challinor | Summary:The kSZ effect has recently emerged as a powerful probe for precision cosmology through its ability to reconstruct the large-scale velocity field. In particular, the kSZ-reconstructed velocity-galaxy cross-correlation is sensitive to signatures of primordial non-Gaussianity through its imprint on the galaxy bias. The kSZ velocity reconstruction is performed using small-scale […]


Continue.. Estimation and mitigation of foregrounds in projected kSZ velocity reconstruction

Catching the Nebular Needle in a Polluted Haystack: Line-emission Signatures from Population III-forming Pockets around Massive Galaxies at the End of Reionization

Kavli Affiliate: Roberto Maiolino | Summary:Finding the first generation of (Population III or Pop III) stars is one of the most ambitious and exciting challenges of astrophysics. JWST opened concrete prospects for their detection during the Epoch of Reionization (EoR), where increasing evidence suggests that residual Pop III formation may persist, even within pristine pockets […]


Continue.. Catching the Nebular Needle in a Polluted Haystack: Line-emission Signatures from Population III-forming Pockets around Massive Galaxies at the End of Reionization

The Impact of Fuzzy Dark Matter Dynamics on the Accumulation and Fragmentation of Primordial Gas

Kavli Affiliate: George Efstathiou | Summary:Fuzzy Dark Matter (FDM), composed of ultra-light axions ($m_a sim 1 times 10^-22$ eV), exhibits wave-like properties that can significantly impact early-universe star formation. Using the arepo code with the axirepo module, we simulate the assembly of haloes across a range of axion masses ($1 times 10^-22$ eV $le m_a […]


Continue.. The Impact of Fuzzy Dark Matter Dynamics on the Accumulation and Fragmentation of Primordial Gas

The Impact of Fuzzy Dark Matter Dynamics on the Accumulation and Fragmentation of Primordial Gas

Kavli Affiliate: George Efstathiou | Summary:Fuzzy Dark Matter (FDM), particularly in the $10^-22$ eV mass regime is frequently used to characterize wave-like interference effects. It exhibits macroscopic wave properties, which drive distinct baryonic dynamics within collapsed haloes. Using the hydrodynamical code AREPO with the AxiREPO module and primordial chemistry, we simulate the assembly of haloes […]


Continue.. The Impact of Fuzzy Dark Matter Dynamics on the Accumulation and Fragmentation of Primordial Gas

The Pristine HeII Emitter near GN-z11: Constraining the Mass Distribution of the First Stars

Kavli Affiliate: Roberto Maiolino | Summary:The properties of the first metal-free stars remain largely unknown, and so far, the only data-driven constraints on their mass distribution (IMF) come from near-field cosmology. Here, we interpret new observations of the C1 and C2 components of Hebe, the HeII emitter near the galaxy GN-z11. Using a locally calibrated […]


Continue.. The Pristine HeII Emitter near GN-z11: Constraining the Mass Distribution of the First Stars