Hidden Monsters with SPHEREx I: A goldmine for heavily reddened quasars at cosmic noon

TL;DR

This study expands the sample of heavily reddened quasars at cosmic noon using SPHEREx data, revealing their properties, evolutionary stage, and dust characteristics, and suggesting they are in a feedback-driven blow-out phase.

Contribution

It significantly increases the known population of HRQs at z > 1.5 and provides detailed spectral energy distribution analysis linking them to galaxy evolution.

Findings

Confirmed 77 new HRQs with redshifts 1.5 < z < 3.9.

Detected UV excess in 76% of HRQs, indicating scattered emission.

Found HRQs are hot-dust poor and have fainter 6um luminosities compared to blue quasars.

Abstract

Heavily reddened quasars (HRQs) are luminous, dust-obscured broad-line quasars thought to represent a short-lived phase of intense black hole growth and feedback. Previous studies have been limited by small sample sizes, restricting robust statistical analysis. We expand the sample of the most luminous HRQs to enable population-level studies, connecting their spectral energy distributions (SEDs) to other quasar populations and placing them within an evolutionary sequence of massive galaxy and black hole formation. We assemble multiwavelength broadband photometry for the brightest HRQ candidates (K$_{AB}$ < 18 mag) and select AGN with red near-infrared colours (J-K)$_{AB}$ > 1.6. Using SPHEREx spectrophotometry, we confirm HRQs and determine redshifts. Detailed SED fitting allows comparison with other luminous quasars, including a control sample of hyper-luminous, unobscured Quaia quasars and luminous Hot Dust-Obscured Galaxies (Hot DOGs). We confirm 77 new HRQs with redshifts 1.5 < z < 3.9, dust-corrected optical continuum luminosities log$_{10}(\lambda L_\lambda (3000A)$ [erg/s])>47.0, and line-of-sight extinctions 0.4 < E(B-V) < 1.6 (A$_V$ mag). This more than doubles the known HRQs at z > 1.5, including the first seven at z > 3. A UV excess consistent with scattered quasar emission is detected in 76% of HRQs. We show that HRQs are hot-dust poor compared to blue quasars of similar luminosity and redshift. Their 6um continuum luminosities are systematically fainter at fixed 3000A continuum luminosity relative to blue Quaia quasars, indicating deficiency in both hot and warm dust. These results support a scenario in which HRQs represent a blow-out phase, where strong feedback begins clearing obscuring material from central regions.