TY - JOUR
T1 - Uncovering a Massive z∼7.7 Galaxy Hosting a Heavily Obscured Radio-loud Active Galactic Nucleus Candidate in COSMOS-Web
AU - Lambrides, Erini
AU - Chiaberge, Marco
AU - Long, Arianna S.
AU - Liu, Daizhong
AU - Akins, Hollis B.
AU - Ptak, Andrew F.
AU - Andika, Irham Taufik
AU - Capetti, Alessandro
AU - Casey, Caitlin M.
AU - Champagne, Jaclyn B.
AU - Chworowsky, Katherine
AU - Clarke, Tracy E.
AU - Cooper, Olivia R.
AU - Ding, Xuheng
AU - Dong, Dillon Z.
AU - Faisst, Andreas L.
AU - Forman, Jordan Y.
AU - Franco, Maximilien
AU - Gillman, Steven
AU - Gozaliasl, Ghassem
AU - Hall, Kirsten R.
AU - Harish, Santosh
AU - Hayward, Christopher C.
AU - Hirschmann, Michaela
AU - Hutchison, Taylor A.
AU - Jahnke, Knud
AU - Jin, Shuowen
AU - Kartaltepe, Jeyhan S.
AU - Kleiner, Emma T.
AU - Koekemoer, Anton M.
AU - Kokorev, Vasily
AU - Manning, Sinclaire M.
AU - Martin, Crystal L.
AU - McKinney, Jed
AU - Norman, Colin
AU - Nyland, Kristina
AU - Onoue, Masafusa
AU - Robertson, Brant E.
AU - Shuntov, Marko
AU - Silverman, John D.
AU - Stiavelli, Massimo
AU - Trakhtenbrot, Benny
AU - Vardoulaki, Eleni
AU - Zavala, Jorge A.
AU - Allen, Natalie
AU - Ilbert, Olivier
AU - McCracken, Henry Joy
AU - Paquereau, Louise
AU - Rhodes, Jason
AU - Toft, Sune
N1 - Funding Information:
We thank the anonymous referees for their thoughtful insight and important contributions to this work. E.L.L. and T.A.H. are supported by appointment to the NASA Postdoctoral Program (NPP) at NASA Goddard Space Flight Center, administered by Oak Ridge Associated Universities under contract with NASA. The National Radio Astronomy Observatory is a facility of the National Science Foundation operated under cooperative agreement by Associated Universities, Inc. Basic research in radio astronomy at the U. S. Naval Research Laboratory is supported by 6.1 Base funding. Construction and installation of VLITE was supported by the NRL Sustainment Restoration and Maintenance fund. ALMA is a partnership of ESO (representing its member states), NSF (USA) and NINS (Japan), together with NRC (Canada), MOST and ASIAA (Taiwan), and KASI (Republic of Korea), in cooperation with the Republic of Chile. The Joint ALMA Observatory is operated by ESO, AUI/NRAO and NAOJ. Support for this work was provided by NASA through grant JWST-GO-01727 and HST-AR-15802 awarded by the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS 5-26555. Some of the data presented in this paper were obtained from the Mikulski Archive for Space Telescopes (MAST) at the Space Telescope Science Institute. The specific observations analyzed can be accessed via doi: 10.17909/ym93-d513 .
PY - 2024/1/1
Y1 - 2024/1/1
N2 - In this Letter, we report the discovery of the highest redshift, heavily obscured, radio-loud (RL) active galactic nucleus (AGN) candidate selected using JWST NIRCam/MIRI, mid-IR, submillimeter, and radio imaging in the COSMOS-Web field. Using multifrequency radio observations and mid-IR photometry, we identify a powerful, RL, growing supermassive black hole with significant spectral steepening of the radio spectral energy distribution (f1.28 GHz ∼ 2 mJy, q24 μm = −1.1, α1.28−3 GHz = − 1.2, Δα = − 0.4). In conjunction with ALMA, deep ground-based observations, ancillary space-based data, and the unprecedented resolution and sensitivity of JWST, we find no evidence of AGN contribution to the UV/optical/near-infrared (NIR) data and thus infer heavy amounts of obscuration (NH > 1023 cm−2). Using the wealth of deep UV to submillimeter photometric data, we report a singular solution photo-z of zphot = 7.7-+0.30.4 and estimate an extremely massive host galaxy (log M* = 11.92 0.5M) hosting a powerful, growing supermassive black hole (LBol = 4−12x × 1046 erg s−1). This source represents the farthest known obscured RL AGN candidate, and its level of obscuration aligns with the most representative but observationally scarce population of AGN at these epochs.
AB - In this Letter, we report the discovery of the highest redshift, heavily obscured, radio-loud (RL) active galactic nucleus (AGN) candidate selected using JWST NIRCam/MIRI, mid-IR, submillimeter, and radio imaging in the COSMOS-Web field. Using multifrequency radio observations and mid-IR photometry, we identify a powerful, RL, growing supermassive black hole with significant spectral steepening of the radio spectral energy distribution (f1.28 GHz ∼ 2 mJy, q24 μm = −1.1, α1.28−3 GHz = − 1.2, Δα = − 0.4). In conjunction with ALMA, deep ground-based observations, ancillary space-based data, and the unprecedented resolution and sensitivity of JWST, we find no evidence of AGN contribution to the UV/optical/near-infrared (NIR) data and thus infer heavy amounts of obscuration (NH > 1023 cm−2). Using the wealth of deep UV to submillimeter photometric data, we report a singular solution photo-z of zphot = 7.7-+0.30.4 and estimate an extremely massive host galaxy (log M* = 11.92 0.5M) hosting a powerful, growing supermassive black hole (LBol = 4−12x × 1046 erg s−1). This source represents the farthest known obscured RL AGN candidate, and its level of obscuration aligns with the most representative but observationally scarce population of AGN at these epochs.
KW - Active galactic nuclei (16)
KW - High-redshift galaxies (734)
KW - Radio loud quasars (1349)
KW - Reionization (1383)
KW - Supermassive black holes (1663)
KW - Unified Astronomy Thesaurus concepts: Quasars (1319)
UR - http://www.scopus.com/inward/record.url?scp=85184272274&partnerID=8YFLogxK
U2 - 10.3847/2041-8213/ad11ee
DO - 10.3847/2041-8213/ad11ee
M3 - Article
AN - SCOPUS:85184272274
SN - 2041-8205
VL - 961
SP - 1
EP - 9
JO - Astrophysical Journal Letters
JF - Astrophysical Journal Letters
IS - 1
M1 - L25
ER -