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Joint Survey Processing: Compact Oddballs in the COSMOS Field — Low-Luminosity Quasars at z > 6?

Presentation #230.07 in the session AGN and Quasars IV.

Published onJun 29, 2022
Joint Survey Processing: Compact Oddballs in the COSMOS Field — Low-Luminosity Quasars at z > 6?

The faint-end slope of the quasar luminosity function at z ~ 6 and its implication on the role of quasars in reionizing the intergalactic medium at early times has been an outstanding problem for some time. The identification of faint high-redshift quasars with luminosities of <1044.5 erg/s is challenging. They are rare (few per square degree) and the separation of these unresolved quasars from late-type stars and compact star-forming galaxies is difficult from ground-based observations alone. In addition, source confusion becomes significant at >25 mag, with ~30% of sources having their flux contaminated by foreground objects when the seeing resolution is 0.7”. We mitigate these issues by performing a pixel-level joint processing of ground and space-based data from Subaru/HSC and HST/ACS. We create a deconfused catalog over the 1.64deg2 of the COSMOS field, after accounting for spatial varying PSFs and astrometric differences between the two datasets. We identify twelve low-luminosity (MUV ~ -21 mag) z > 6 quasar candidates through (i) their red color measured between ACS/F814W and HSC/i-band and (ii) their compactness in the space-based data. Non-detections of our candidates in Hubble DASH data argues strongly against late-type stars, which are the dominant contaminants of the above selection. Our constraints on the faint end of the quasar luminosity function at z ~ 6 suggests a negligibly small contribution to reionization compared to the star-forming galaxy population. The confirmation of our candidates and the evolution of number density with redshift could provide better insights into how supermassive galaxies grew in the first billion years of cosmic time.

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