X-ray detected active galactic nuclei in dwarf galaxies at 0 < z < 1
We present a sample of accreting supermassive black holes (SMBHs) in dwarf galaxies at z<1. We identify dwarf galaxies in the NEWFIRM Medium Band Survey with stellar masses of M{sub ⋆}<3×10{sup 9} M{sub ⊙} that have spectroscopic redshifts from the DEEP2 survey and lie within the region covered by deep (flux limit of ∼5×10{sup −17}--6×10{sup −16} erg cm{sup −2} s{sup −1}) archival Chandra X-ray data. From our sample of 605 dwarf galaxies, 10 exhibit X-ray emission consistent with that arising from active galactic nucleus (AGN) activity. If black-hole mass scales roughly with stellar mass, then we expect that these AGNs are powered by SMBHs with masses of ∼10{sup 5}--10{sup 6} M{sub ⊙} and typical Eddington ratios of ∼5%. Furthermore, we find an AGN fraction consistent with extrapolations of other searches of ∼0.6%--3% for 10{sup 9} M{sub ⊙}⩽M{sub ⋆}⩽3×10{sup 9} M{sub ⊙} and 0.1<z<0.6. Our AGN fraction is in good agreement with a semi-analytic model, suggesting that, as we search larger volumes, we may use comparisons between observed AGN fractions and models to understand seeding mechanisms in the early universe.