Amanote Research

Amanote Research

    RegisterSign In

Type 2 Quasars at the Heart of Dust-Obscured Galaxies (DOGs) at High Z

doi 10.1063/1.3475316
Full Text
Open PDF
Abstract

Available in full text

Date

January 1, 2010

Authors
E. PiconcelliG. LanzuisiF. FioreC. FeruglioC. VignaliM. SalvatoC. GruppioniA. ComastriL. AngeliniM. Cappi
Publisher

AIP


Related search

Stellar Populations in the Most Luminous Obscured Quasars at Z > 0.5

Proceedings of the International Astronomical Union
AstrophysicsAstronomyPlanetary ScienceSpace
2012English

The Destruction of Quasars Clustering at Z > 2

Symposium - International Astronomical Union
1989English

Strong Clustering of Lyman Break Galaxies Around Luminous Quasars at Z ∼ 4

Astrophysical Journal
AstrophysicsAstronomyPlanetary ScienceSpace
2017English

Highly Accreting Quasars at Low and High Z.

Astronomical Review
2014English

The Nature of FaintSpitzer‐selected Dust‐obscured Galaxies

Astrophysical Journal
AstrophysicsAstronomyPlanetary ScienceSpace
2008English

Radio Polarisation Studies of Galaxies at Z > 2

Symposium - International Astronomical Union
1996English

Sizes of Passively Evolving Galaxies at Z ~2 in CLASH

Proceedings of the International Astronomical Union
AstrophysicsAstronomyPlanetary ScienceSpace
2012English

ALMA Reveals a Gas-Rich, Maximum Starburst in the Hyperluminous, Dust-Obscured Quasar W0533–3401 at Z ∼ 2.9

Astrophysical Journal
AstrophysicsAstronomyPlanetary ScienceSpace
2019English

The Cosmic Evolution of Quasars at High Redshifts

Symposium - International Astronomical Union
1987English

Amanote Research

Note-taking for researchers

Follow Amanote

© 2026 Amaplex Software S.P.R.L. All rights reserved.

Privacy PolicyRefund Policy