Little red dots as obscured little blue dots: relative abundances, luminosities, and black-hole masses

Kavli Affiliate: Roberto Maiolino | Summary:We test whether "little red dots” (LRDs) are the dust-reddened, high-inclination counterparts of bluer compact broad-line active galactic nuclei, here referred to as "little blue dots” (LBDs), by modeling their relative number densities and luminosities. Using the observed UV luminosity function (LF) of broad-line active galactic nuclei (BLAGNs) at z>4 […]


Continue.. Little red dots as obscured little blue dots: relative abundances, luminosities, and black-hole masses

New constraints on primordial non-Gaussianity from large-scale cross-correlations of CMB lensing and the cosmic infrared background

Kavli Affiliate: Blake Sherwin | Summary:We present new constraints on the local-type primordial non-Gaussianity parameter, $f_mathrmNL^mathrmlocal$, through analysis of the scale-dependent bias effect on the cosmic infrared background (CIB). To avoid biases from galactic dust contamination on large scales, we use cross-correlations between the CIB and Planck cosmic microwave background (CMB) lensing maps to constrain […]


Continue.. New constraints on primordial non-Gaussianity from large-scale cross-correlations of CMB lensing and the cosmic infrared background

Dust enrichment from core-collapse supernovae and extinction curves in the high-redshift universe

Kavli Affiliate: Roberto Maiolino | Summary:Recent JWST observations have revealed that some galaxies at $z gtrsim 7$ generally exhibit relatively flat ultraviolet (UV) attenuation curves and a weak UV bump. These features suggest that the first dust grains formed rapidly, possibly originating from core-collapse supernovae (SNe). We investigate the time evolution of grain size distributions […]


Continue.. Dust enrichment from core-collapse supernovae and extinction curves in the high-redshift universe

Lessons from binary dynamics of inspiralling equal-mass boson-star mergers

Kavli Affiliate: Ulrich Sperhake | Summary:We explore the gravitational-wave phenomenology of equal-mass inspiralling boson-star binaries using numerical relativity simulations. In particular, we characterise the waveform differences between binary boson-star and black-hole systems across (i) the early inspiral, by matching our waveforms to post-Newtonian expressions, (ii) merger, and (iii) late ringdown, by extracting the quasi-normal mode […]


Continue.. Lessons from binary dynamics of inspiralling equal-mass boson-star mergers

Intense and extended CIII] emission suggests a strong outflow in JADES-GS-z14-0

Kavli Affiliate: Roberto Maiolino | Summary:JWST has revealed an overabundance of very bright, blue galaxies at z>10, raising fundamental questions about how star formation and feedback operate at Cosmic Dawn. We present new JWST/NIRSpec MSA PRISM/CLEAR spectroscopy of JADES-GS-z14-0 (z=14.18) obtained with the JADES and OASIS programmes. While the rest-frame UV continuum flux level and […]


Continue.. Intense and extended CIII] emission suggests a strong outflow in JADES-GS-z14-0

Impact of Stochastic Pop~III X-ray Binaries on the Cosmological 21-cm Signal

Kavli Affiliate: George Efstathiou | Summary:High-mass X-ray binaries are one of the primary drivers of the 21-cm signal from Cosmic Dawn and Reionization, playing a leading role in the thermal history of the intergalactic medium. In traditional semi-numerical simulations, a deterministic scaling relation between the total X-ray luminosity of high-mass X-ray binaries, $L_rm X$, and […]


Continue.. Impact of Stochastic Pop~III X-ray Binaries on the Cosmological 21-cm Signal

Impact of Stochastic Pop~III X-ray Binaries on the Cosmological 21-cm Signal

Kavli Affiliate: George Efstathiou | Summary:High-mass X-ray binaries are one of the primary drivers of the 21-cm signal from Cosmic Dawn and Reionization, playing a leading role in the thermal history of the intergalactic medium. In traditional semi-numerical simulations, a deterministic scaling relation between the total X-ray luminosity of high-mass X-ray binaries, $L_rm X$, and […]


Continue.. Impact of Stochastic Pop~III X-ray Binaries on the Cosmological 21-cm Signal

The Cliff: A Metal-Poor Little Red Dot Hosting an Overmassive Black Hole at $z = 3.55$

Kavli Affiliate: Roberto Maiolino | Summary:JWST has revealed a large population of massive black holes (BHs) in the early Universe with unusual properties which mark them as distinct from low-redshift active galactic nuclei. Such findings have prompted the development of new models of BH formation and growth, and of their co-evolution with host galaxies. Linking […]


Continue.. The Cliff: A Metal-Poor Little Red Dot Hosting an Overmassive Black Hole at $z = 3.55$

The Way We Tally Becomes the Tale: the Impact of Selection Strategies on the Inferred Evolution of Little Red Dots Across Cosmic Time

Kavli Affiliate: Roberto Maiolino | Summary:Little Red Dots (LRDs) have emerged as a key population linked to early black hole growth, yet photometric selections have predominantly targeted only the most extreme red systems, thereby shaping our current understanding of this new population of objects. In this work, we deliberately explore a broad range of optical […]


Continue.. The Way We Tally Becomes the Tale: the Impact of Selection Strategies on the Inferred Evolution of Little Red Dots Across Cosmic Time

Metal Mayhem at $rm z sim 7-10$: Diversity and Evolution of Gas-Phase Metallicity Gradients

Kavli Affiliate: Roberto Maiolino | Summary:We present a JWST/NIRSpec-IFU study of metallicity gradients in seven low-metallicity systems at $z=7.2-9.5$. The main sample spans stellar masses of $rm log(M_*/M_odot) sim 7.8-9.5$, star formation rates (SFRs) of $rm log(textSFR / M_odot textyr^-1) sim 0.5-2.5$, and gas-phase metallicities of $4%-15 %~Z_odot$. Within our sample, we also identify three […]


Continue.. Metal Mayhem at $rm z sim 7-10$: Diversity and Evolution of Gas-Phase Metallicity Gradients