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author D'Amato, Quirino
Mannucci, Filippo
Sonnenfeld, Alessandro
Scialpi, Martina
Nightingale, James W.
Spingola, Cristiana
Zibetti, Stefano
Marconi, Alessandro
Rosati, Piero
Marconcini, Cosimo
Agapito, Guido
Gallazzi, Anna
Di Teodoro, Enrico
Andreuzzi, Gloria
Belfiore, Francesco
Bertola, Elena
Bracci, Caterina
Carniani, Stefano
Cataldi, Elisa
Chakraborty, Avinanda
Ceci, Matteo
Cicone, Claudia
Ciurlo, Anna
Cresci, Giovanni
De Rosa, Alessandra
Di Carlo, Elisa
Feltre, Anna
Ginolfi, Michele
Lamperti, Isabella
Moreschini, Bianca
Nardini, Emanuele
Perna, Michele
Portaluri, Elisa
Rubinur, Khatun
Saracco, Paolo
Severgnini, Paola
Testa, Vincenzo
Tozzi, Giulia
Venturi, Giacomo
Ulivi, Lorenzo
Vignali, Cristian
Zanchettin, Maria Vittoria
Pepe, Antonio
author_facet D'Amato, Quirino
Mannucci, Filippo
Sonnenfeld, Alessandro
Scialpi, Martina
Nightingale, James W.
Spingola, Cristiana
Zibetti, Stefano
Marconi, Alessandro
Rosati, Piero
Marconcini, Cosimo
Agapito, Guido
Gallazzi, Anna
Di Teodoro, Enrico
Andreuzzi, Gloria
Belfiore, Francesco
Bertola, Elena
Bracci, Caterina
Carniani, Stefano
Cataldi, Elisa
Chakraborty, Avinanda
Ceci, Matteo
Cicone, Claudia
Ciurlo, Anna
Cresci, Giovanni
De Rosa, Alessandra
Di Carlo, Elisa
Feltre, Anna
Ginolfi, Michele
Lamperti, Isabella
Moreschini, Bianca
Nardini, Emanuele
Perna, Michele
Portaluri, Elisa
Rubinur, Khatun
Saracco, Paolo
Severgnini, Paola
Testa, Vincenzo
Tozzi, Giulia
Venturi, Giacomo
Ulivi, Lorenzo
Vignali, Cristian
Zanchettin, Maria Vittoria
Pepe, Antonio
contents The assembly of stellar-dominated cores in elliptical galaxies is key to understanding how cosmic structures evolved. Gravitational lensing offers unique insights into the nature of their stars. We report the discovery of the smallest known quadruply lensed quasar (radius ~0.2"), whose lensing galaxy at redshift 1.055 (5.5 billion years after the Big Bang) features a lensing mass of only ~2x10^10 M_sun. A Bayesian analysis, based on the system's exceptional properties and standard scaling relations, allowed us to sample the central galactic initial mass function with unmatched accuracy and in a previously uncharted regime in terms of mass and redshift. We found it consistent with the Milky Way one, while excluding bottom-heavy functions. This suggests that the core either grew slowly or underwent early disruptive events altering its stellar build-up, in contrast with the classical view that bulges form rapidly and remain unchanged by later interactions.
format Preprint
id arxiv_https___arxiv_org_abs_2604_01828
institution arXiv
publishDate 2026
record_format arxiv
spellingShingle Milky-Way-like stars in a galaxy core 8 billion years ago revealed by gravitational lensing
D'Amato, Quirino
Mannucci, Filippo
Sonnenfeld, Alessandro
Scialpi, Martina
Nightingale, James W.
Spingola, Cristiana
Zibetti, Stefano
Marconi, Alessandro
Rosati, Piero
Marconcini, Cosimo
Agapito, Guido
Gallazzi, Anna
Di Teodoro, Enrico
Andreuzzi, Gloria
Belfiore, Francesco
Bertola, Elena
Bracci, Caterina
Carniani, Stefano
Cataldi, Elisa
Chakraborty, Avinanda
Ceci, Matteo
Cicone, Claudia
Ciurlo, Anna
Cresci, Giovanni
De Rosa, Alessandra
Di Carlo, Elisa
Feltre, Anna
Ginolfi, Michele
Lamperti, Isabella
Moreschini, Bianca
Nardini, Emanuele
Perna, Michele
Portaluri, Elisa
Rubinur, Khatun
Saracco, Paolo
Severgnini, Paola
Testa, Vincenzo
Tozzi, Giulia
Venturi, Giacomo
Ulivi, Lorenzo
Vignali, Cristian
Zanchettin, Maria Vittoria
Pepe, Antonio
Astrophysics of Galaxies
The assembly of stellar-dominated cores in elliptical galaxies is key to understanding how cosmic structures evolved. Gravitational lensing offers unique insights into the nature of their stars. We report the discovery of the smallest known quadruply lensed quasar (radius ~0.2"), whose lensing galaxy at redshift 1.055 (5.5 billion years after the Big Bang) features a lensing mass of only ~2x10^10 M_sun. A Bayesian analysis, based on the system's exceptional properties and standard scaling relations, allowed us to sample the central galactic initial mass function with unmatched accuracy and in a previously uncharted regime in terms of mass and redshift. We found it consistent with the Milky Way one, while excluding bottom-heavy functions. This suggests that the core either grew slowly or underwent early disruptive events altering its stellar build-up, in contrast with the classical view that bulges form rapidly and remain unchanged by later interactions.
title Milky-Way-like stars in a galaxy core 8 billion years ago revealed by gravitational lensing
topic Astrophysics of Galaxies
url https://arxiv.org/abs/2604.01828