Jeremiah D. Paul

activity

20222026

most citedConnecting Low- and High-Redshift Weak Emission-Line Quasars via HST Spectroscopy of Ly

α

Emission

15 citations · 31 across the 7 of their papers we have counts for

collaborators

Showing 2024Show all

3 papers · 1 filter

astro-ph.HE2024

Do Neutron Star Ultra-Luminous X-Ray Sources Masquerade as Intermediate Mass Black Holes in Radio and X-Ray?

Teresa Panurach, Kristen C. Dage, Ryan Urquhart +8

Ultraluminous X-ray sources (ULXs) were once largely believed to be powered by super-Eddington accretion onto stellar-mass black holes, although in some rare cases, ULXs also serve…

astro-ph.GA2024

Rest-Frame Optical Spectroscopy of Ten z $\sim$ 2 Weak Emission-Line Quasars

Ying Chen, Bin Luo, W. N. Brandt +7

We present near-infrared spectroscopy of ten weak emission-line quasars (WLQs) at redshifts of $z \sim 2$ , obtained with the Palomar 200-inch Hale Telescope. WLQs are an exceptional…

astro-ph.GA2024★ 4 cited

Radio Scrutiny of the X-ray-Weak Tail of Low-Mass Active Galactic Nuclei: A Novel Signature of High-Eddington Accretion?

Jeremiah D. Paul, Richard M. Plotkin, W. N. Brandt +6

The supermassive black holes ( $M_{BH} \sim 1 0^{6}$ $-$ $1 0^{10} M_{⊙}$ ) that power luminous active galactic nuclei (AGNs), i.e., quasars, generally show a correlation between t…

Do Neutron Star Ultra-Luminous X-Ray Sources Masquerade as Intermediate Mass Black Holes in Radio and X-Ray?

Rest-Frame Optical Spectroscopy of Ten z ∼ 2 Weak Emission-Line Quasars

Radio Scrutiny of the X-ray-Weak Tail of Low-Mass Active Galactic Nuclei: A Novel Signature of High-Eddington Accretion?

Rest-Frame Optical Spectroscopy of Ten z $\sim$ 2 Weak Emission-Line Quasars