[O iv]- and [Ne v]-weak Active Galactic Nuclei Hidden by Compton-thick Material in Late Mergers

MLA

Satoshi Yamada, et al. “[O Iv]- and [Ne v]-Weak Active Galactic Nuclei Hidden by Compton-Thick Material in Late Mergers.” The Astrophysical Journal, vol. 965, no. 2, Jan. 2024, p. 153. EBSCOhost, https://doi.org/10.3847/1538-4357/ad2936.

APA

Satoshi Yamada, Yoshihiro Ueda, Taiki Kawamuro, Claudio Ricci, Yoshiki Toba, Masatoshi Imanishi, Takamitsu Miyaji, Atsushi Tanimoto, Kohei Ichikawa, Martín Herrera-Endoqui, Shoji Ogawa, Ryosuke Uematsu, & Keiichi Wada. (2024). [O iv]- and [Ne v]-weak Active Galactic Nuclei Hidden by Compton-thick Material in Late Mergers. The Astrophysical Journal, 965(2), 153. https://doi.org/10.3847/1538-4357/ad2936

Chicago

Satoshi Yamada, Yoshihiro Ueda, Taiki Kawamuro, Claudio Ricci, Yoshiki Toba, Masatoshi Imanishi, Takamitsu Miyaji, et al. 2024. “[O Iv]- and [Ne v]-Weak Active Galactic Nuclei Hidden by Compton-Thick Material in Late Mergers.” The Astrophysical Journal 965 (2): 153. doi:10.3847/1538-4357/ad2936.