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20242026
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8 papers · 1 filter

astro-ph.CO2026

Cosmography with DESI-DR1 Cosmic Chronometers: Direct H(z) measurements from Luminous Red Galaxy ages

Carlos A. Álvarez, Marcos M. Cueli, Balakrishna S. Haridasu +6

Providing robust redshift estimates for almost 3 million luminous red galaxies (LRGs), the Dark Energy Spectroscopic Instrument (DESI) offers a unique opportunity to test the expan…

astro-ph.CO2025

Semi-empirical Framework of Supermassive Black Hole Evolution: Highlighting a possible tension between Demographics and Gravitational Wave Background

Andrea Lapi, Francesco Shankar, Michele Bosi +4

The evolution of the supermassive Black Hole (BH) population across cosmic times remains a central unresolved issue in modern astrophysics, due to the many noticeable uncertainties…

astro-ph.CO2025

Cosmic magnification on high-redshift submillimeter galaxies

Marcos M. Cueli, Joaquín González-Nuevo, Laura Bonavera +1

Weak lensing magnification probes the correlation between galaxies and the underlying matter field in a similar fashion to galaxy-galaxy lensing shear. Although it has long been si…

astro-ph.CO2025

Cosmography via stellar archaeology of low-redshift early-type galaxies from SDSS

Carlos A. Álvarez, Marcos M. Cueli, Alessandro Bressan +5

Cosmic chronometers offer a model-independent way to trace the expansion history of the Universe via the dating of passively evolving objects. This enables testing the validity of…

astro-ph.CO2025

Outer regions of galaxy clusters as a new probe to test modifications to gravity

Minahil Adil Butt, Sandeep Haridasu, Antonaldo Diaferio +4

We apply the caustic technique to samples of galaxy clusters stacked in redshift space to estimate the gravitational potential in the cluster's outer region and test modifications…

astro-ph.CO2025

Little ado about everything II: an `emergent' dark energy from structure formation to rule cosmic tensions

Andrea Lapi, Balakrishna S. Haridasu, Lumen Boco +3

[abridged] The CDM framework is a new cosmological model aimed to cure some drawbacks of the standard CDM scenario, such as the origin of the accelerated expansion at late…