We review the properties of the established Scaling Relations (SRs) of galaxies and active
galactic nuclei (AGN), focusing on their origin and expected evolution back in time, providing …

The primordial matter power spectrum quantifies fluctuations in the distribution of dark matter
immediately following inflation. Over cosmic time, overdense regions of the primordial …

Recent studies have suggested that red quasars are a phase in quasar evolution when
feedback from black hole accretion evacuates obscuring gas from the nucleus of the host …

Characterizing the physical conditions (density, temperature, ionization state, metallicity, etc)
of the interstellar medium is critical to improving our understanding of the formation and …

Dark matter could comprise, at least in part, primordial black holes (PBHs). To test this
hypothesis, we present an approach to constrain the PBH mass (M PBH) and mass fraction …

Understanding the nature of high-redshift dusty galaxies requires a comprehensive view of
their interstellar medium (ISM) and molecular complexity. However, the molecular ISM at …

We present a panchromatic study of 11 (sub-) millimetre selected DSFGs with
spectroscopically confirmed redshift (1.5< z spec< 3) in the GOODS-S field, with the aim of …

We present the average rest-frame spectrum of the final catalog of dusty star-forming
galaxies (DSFGs) selected from the South Pole Telescope's SPT-SZ survey and measured …

Context. The low-ionization nuclear emission-line region (LINER) galaxy TXS 2226− 184 is
known to host a very luminous 22 GHz water maser, called a gigamaser at the time of its …

Aims. In this paper we present the detection of H 2 O and OH+ emission in z> 3 hot dust-
obscured galaxies (Hot DOGs). Methods. Using ALMA Band-6 observations of two Hot …