A Challenge to the Standard Cosmological Model

ArXiv 2206.05624 (2022)


Nathan Secrest, Sebastian von Hausegger, Mohamed Rameez, Roya Mohayaee, Subir Sarkar

Hybrid photometric redshifts for sources in the COSMOS and XMM-LSS fields

ArXiv 2206.00748 (2022)


PW Hatfield, MJ Jarvis, N Adams, RAA Bowler, B Häußler, KJ Duncan

The star-formation rates of QSOs

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) (2022)


M Symeonidis, N Maddox, MJ Jarvis, MJ Michałowski, P Andreani, DL Clements, G De Zotti, S Duivenvoorden, J Gonzalez-Nuevo, E Ibar, RJ Ivison, L Leeuw, MJ Page, R Shirley, MWL Smith, M Vaccari


Abstract We examine the far-IR properties of a sample of 5391 optically selected QSOs in the 0.5 < z < 2.65 redshift range down to log [νLν, 2500(erg/s)] > 44.7, using SPIRE data from Herschel-ATLAS. We split the sample in a grid of 74 luminosity-redshift bins and compute the average optical–infrared spectral energy distribution (SED) in each bin. By normalising an intrinsic AGN template to the AGN optical power (at 5100Å) we decompose the total infrared emission (LIR; 8—1000μm) into an AGN (LIR, AGN) and star-forming component (LIR, SF). We find that the AGN contribution to LIR increases as a function of AGN power which manifests as a reduction of the ‘far-IR bump’ in the average QSO SEDs. We note that LIR, SF does not correlate with AGN power; the mean star formation rates (SFRs) of AGN host galaxies are a function of redshift only and they range from ∼6 M⊙/yr at z ∼ 0 to a plateau of ≲ 200 M⊙/yr at z ∼ 2.6. Our results indicate that the accuracy of far-IR emission as a proxy for SFR decreases with increasing AGN luminosity. We show that, at any given redshift, observed trends between infrared luminosity (whether monochromatic or total) and AGN power (in the optical or X-rays) can be explained by a simple model which is the sum of two components: (A) the infrared emission from star-formation, uncorrelated with AGN power and (B) the infrared emission from AGN, directly proportional to AGN power in the optical or X-rays.

Joint constraints on cosmology and the impact of baryon feedback: Combining KiDS-1000 lensing with the thermal Sunyaev-Zeldovich effect from Planck and ACT

Astronomy and Astrophysics EDP Sciences 660 (2022) A27


T Tröster, Aj Mead, C Heymans, Z Yan, D Alonso, M Asgari, M Bilicki, A Dvornik, H Hildebrandt, B Joachimi, A Kannawadi, K Kuijken, P Schneider, Hy Shan, L van Waerbeke, Ah Wright


We conduct a pseudo-C analysis of the tomographic cross-correlation between 1000 deg2 of weak-lensing data from the Kilo-Degree Survey (KiDS-1000) and the thermal Sunyaev–Zeldovich (tSZ) effect measured by Planck and the Atacama Cosmology Telescope (ACT). Using HMX, a halo-model-based approach that consistently models the gas, star, and dark matter components, we are able to derive constraints on both cosmology and baryon feedback for the first time from these data, marginalising over redshift uncertainties, intrinsic alignment of galaxies, and contamination by the cosmic infrared background (CIB). We find our results to be insensitive to the CIB, while intrinsic alignment provides a small but significant contribution to the lensing–tSZ cross-correlation. The cosmological constraints are consistent with those of other low-redshift probes and prefer strong baryon feedback. The inferred amplitude of the lensing–tSZ cross-correlation signal, which scales as σ8m/0.3)0.2, is low by ∼2 σ compared to the primary cosmic microwave background constraints by Planck. The lensing–tSZ measurements are then combined with pseudo-C measurements of KiDS-1000 cosmic shear into a novel joint analysis, accounting for the full cross-covariance between the probes, providing tight cosmological constraints by breaking parameter degeneracies inherent to both probes. The joint analysis gives an improvement of 40% on the constraint of S8 = σ8Ωm/0.3 over cosmic shear alone, while providing constraints on baryon feedback consistent with hydrodynamical simulations, demonstrating the potential of such joint analyses with baryonic tracers such as the tSZ effect. We discuss remaining modelling challenges that need to be addressed if these baryonic probes are to be included in future precision-cosmology analyses.

MIGHTEE - H I. The relation between the H I gas in galaxies and the cosmic web



Madalina N Tudorache, MJ Jarvis, I Heywood, AA Ponomareva, N Maddox, BS Frank, NJ Adams, RAA Bowler, IH Whittam, M Baes, H Pan, SHA Rajohnson, F Sinigaglia, K Spekkens