The formation and cosmic evolution of dust in the early Universe. I. Dust sources

Kavli Affiliate: Roberto Maiolino | First 5 Authors: Raffaella Schneider, Roberto Maiolino, , , | Summary: Dust-obscured star formation has dominated the cosmic history of star formation since z = 4. However, the recent finding of significant amount of dust in galaxies out to z = 8 has opened the new frontier of investigating the […]


Continue.. The formation and cosmic evolution of dust in the early Universe. I. Dust sources

The formation and cosmic evolution of dust in the early Universe. I. Dust sources

Kavli Affiliate: Roberto Maiolino | First 5 Authors: Raffaella Schneider, Roberto Maiolino, , , | Summary: Dust-obscured star formation has dominated the cosmic history of star formation since z = 4. However, the recent finding of significant amount of dust in galaxies out to z = 8 has opened the new frontier of investigating the […]


Continue.. The formation and cosmic evolution of dust in the early Universe. I. Dust sources

Manifestly covariant variational principle for gauge theories of gravity

Kavli Affiliate: Anthony Lasenby | First 5 Authors: Michael Hobson, Anthony Lasenby, Will Barker, , | Summary: A variational principle for gauge theories of gravity is presented, which maintains manifest covariance under the symmetries to which the action is invariant, throughout the calculation of the equations of motion and conservation laws. This is performed by […]


Continue.. Manifestly covariant variational principle for gauge theories of gravity

GA-NIFS: Early-stage feedback in a heavily obscured AGN at $z=4.76$

Kavli Affiliate: Roberto Maiolino | First 5 Authors: Eleonora Parlanti, Stefano Carniani, Hannah Übler, Giacomo Venturi, Francesco D’Eugenio | Summary: Dust-obscured galaxies are thought to represent an early evolutionary phase of massive galaxies in which the active galactic nucleus (AGN) is still deeply buried in significant amounts of dusty material and its emission is strongly […]


Continue.. GA-NIFS: Early-stage feedback in a heavily obscured AGN at $z=4.76$

GA-NIFS: Early-stage feedback in a heavily obscured AGN at $z=4.76$

Kavli Affiliate: Roberto Maiolino | First 5 Authors: Eleonora Parlanti, Stefano Carniani, Hannah Übler, Giacomo Venturi, Chiara Circosta | Summary: Dust-obscured galaxies are thought to represent an early evolutionary phase of massive galaxies in which the active galactic nucleus (AGN) is still deeply buried in significant amounts of dusty material and its emission is strongly […]


Continue.. GA-NIFS: Early-stage feedback in a heavily obscured AGN at $z=4.76$

JADES: Resolving the Stellar Component and Filamentary Overdense Environment of HST-Dark Submillimeter Galaxy HDF850.1 at $z=5.18$

Kavli Affiliate: Roberto Maiolino | First 5 Authors: Fengwu Sun, Jakob M. Helton, Eiichi Egami, Kevin N. Hainline, George H. Rieke | Summary: HDF850.1 is the brightest submillimeter galaxy (SMG) in the Hubble Deep Field. It is known as a heavily dust-obscured star-forming galaxy embedded in an overdense environment at $z = 5.18$. With nine-band […]


Continue.. JADES: Resolving the Stellar Component and Filamentary Overdense Environment of HST-Dark Submillimeter Galaxy HDF850.1 at $z=5.18$

JADES: Resolving the Stellar Component and Filamentary Overdense Environment of HST-Dark Submillimeter Galaxy HDF850.1 at $z=5.18$

Kavli Affiliate: Roberto Maiolino | First 5 Authors: Fengwu Sun, Jakob M. Helton, Eiichi Egami, Kevin N. Hainline, George H. Rieke | Summary: HDF850.1 is the brightest submillimeter galaxy (SMG) in the Hubble Deep Field. It is known as a heavily dust-obscured star-forming galaxy embedded in an overdense environment at $z = 5.18$. With nine-band […]


Continue.. JADES: Resolving the Stellar Component and Filamentary Overdense Environment of HST-Dark Submillimeter Galaxy HDF850.1 at $z=5.18$

The black hole mass metallicity relation and insights into galaxy quenching

Kavli Affiliate: Roberto Maiolino | First 5 Authors: William M. Baker, Roberto Maiolino, Asa F. L. Bluck, Francesco Belfiore, Mirko Curti | Summary: One of the most important questions in astrophysics is what causes galaxies to stop forming stars. Previous studies have shown a tight link between quiescence and black hole mass. Other studies have […]


Continue.. The black hole mass metallicity relation and insights into galaxy quenching

JWST CEERS & JADES Active Galaxies at z = 4-7 Violate the Local $M_bullet-M_star$ Relation at $>3σ$: Implications for Low-Mass Black Holes and Seeding Models

Kavli Affiliate: Roberto Maiolino | First 5 Authors: Fabio Pacucci, Bao Nguyen, Stefano Carniani, Roberto Maiolino, Xiaohui Fan | Summary: JWST is revolutionizing our understanding of the high-z Universe by expanding the black hole horizon, looking farther and to smaller masses, and revealing the stellar light of their hosts. New detections of high-z systems offer […]


Continue.. JWST CEERS & JADES Active Galaxies at z = 4-7 Violate the Local $M_bullet-M_star$ Relation at $>3σ$: Implications for Low-Mass Black Holes and Seeding Models