_version_ 1866909894586662912
author Ding, Xuheng
Onoue, Masafusa
Silverman, John D.
Matsuoka, Yoshiki
Izumi, Takuma
Strauss, Michael A.
Yang, Lilan
Jahnke, Knud
Phillips, Camryn L.
Treu, Tommaso
Andika, Irham T.
Aoki, Kentaro
Arita, Junya
Baba, Shunsuke
Bosman, Sarah E. I.
Eilers, Anna-Christina
Fujimoto, Seiji
Haiman, Zoltan
Imanishi, Masatoshi
Inayoshi, Kohei
Iwasawa, Kazushi
Kartaltepe, Jeyhan
Kashikawa, Nobunari
Kawaguchi, Toshihiro
Li, Junyao
Lee, Chien-Hsiu
Lupi, Alessandro
Schindler, Jan-Torge
Schramm, Malte
Shimasaku, Kazuhiro
Shuntov, Marko
Tanaka, Takumi S.
Toba, Yoshiki
Trakhtenbrot, Benny
Umehata, Hideki
Vestergaard, Marianne
Wang, Feige
Yang, Jinyi
author_facet Ding, Xuheng
Onoue, Masafusa
Silverman, John D.
Matsuoka, Yoshiki
Izumi, Takuma
Strauss, Michael A.
Yang, Lilan
Jahnke, Knud
Phillips, Camryn L.
Treu, Tommaso
Andika, Irham T.
Aoki, Kentaro
Arita, Junya
Baba, Shunsuke
Bosman, Sarah E. I.
Eilers, Anna-Christina
Fujimoto, Seiji
Haiman, Zoltan
Imanishi, Masatoshi
Inayoshi, Kohei
Iwasawa, Kazushi
Kartaltepe, Jeyhan
Kashikawa, Nobunari
Kawaguchi, Toshihiro
Li, Junyao
Lee, Chien-Hsiu
Lupi, Alessandro
Schindler, Jan-Torge
Schramm, Malte
Shimasaku, Kazuhiro
Shuntov, Marko
Tanaka, Takumi S.
Toba, Yoshiki
Trakhtenbrot, Benny
Umehata, Hideki
Vestergaard, Marianne
Wang, Feige
Yang, Jinyi
contents The advent of JWST has opened new horizons in the study of quasar host galaxies during the reionization epoch (z>6). Building upon our previous initial measurements of stellar light from two quasar host galaxies at these redshifts, we now report the detection of the stellar light from the full Cycle 1 sample of 12 distant moderate-luminosity quasar (M1450>-24 mag) host galaxies at z>6 from the Hyper Suprime-Cam Subaru Strategic Program (HSC-SSP). Using JWST/NIRCam observations at 1.5 and 3.6 um combined with 2D image decomposition analysis, we successfully detect the host galaxies in 11 of the 12 targets, underscoring the high detection rates achievable with moderate-luminosity quasars. Based on two-band photometry and SED fitting, we find that our host galaxies are massive, with logM*/M_sun = 9.5-11.0. The effective radii range from 0.6 to 3.2 kpc, comparable to the sizes of inactive galaxies with similar masses at z~6 as measured with imaging from COSMOS-Web.Intriguingly, the two quasar hosts with post-starburst features, which reside at the high-mass end of our sample and exhibit relatively compact morphologies, have similar size and stellar mass surface densities to quiescent galaxies at z~4-5. These findings suggest that the so-called galaxy compaction scenario is already in place at the reionization epoch, in which gas inflows during starburst phases drive centrally concentrated star formation followed by rapid quenching, bridging the structural transition of massive galaxies from relatively extended star-forming disks to compact quiescent systems.
format Preprint
id arxiv_https___arxiv_org_abs_2505_03876
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle SHELLQs-JWST Unveils the Host Galaxies of 12 Quasars at z>6
Ding, Xuheng
Onoue, Masafusa
Silverman, John D.
Matsuoka, Yoshiki
Izumi, Takuma
Strauss, Michael A.
Yang, Lilan
Jahnke, Knud
Phillips, Camryn L.
Treu, Tommaso
Andika, Irham T.
Aoki, Kentaro
Arita, Junya
Baba, Shunsuke
Bosman, Sarah E. I.
Eilers, Anna-Christina
Fujimoto, Seiji
Haiman, Zoltan
Imanishi, Masatoshi
Inayoshi, Kohei
Iwasawa, Kazushi
Kartaltepe, Jeyhan
Kashikawa, Nobunari
Kawaguchi, Toshihiro
Li, Junyao
Lee, Chien-Hsiu
Lupi, Alessandro
Schindler, Jan-Torge
Schramm, Malte
Shimasaku, Kazuhiro
Shuntov, Marko
Tanaka, Takumi S.
Toba, Yoshiki
Trakhtenbrot, Benny
Umehata, Hideki
Vestergaard, Marianne
Wang, Feige
Yang, Jinyi
Astrophysics of Galaxies
The advent of JWST has opened new horizons in the study of quasar host galaxies during the reionization epoch (z>6). Building upon our previous initial measurements of stellar light from two quasar host galaxies at these redshifts, we now report the detection of the stellar light from the full Cycle 1 sample of 12 distant moderate-luminosity quasar (M1450>-24 mag) host galaxies at z>6 from the Hyper Suprime-Cam Subaru Strategic Program (HSC-SSP). Using JWST/NIRCam observations at 1.5 and 3.6 um combined with 2D image decomposition analysis, we successfully detect the host galaxies in 11 of the 12 targets, underscoring the high detection rates achievable with moderate-luminosity quasars. Based on two-band photometry and SED fitting, we find that our host galaxies are massive, with logM*/M_sun = 9.5-11.0. The effective radii range from 0.6 to 3.2 kpc, comparable to the sizes of inactive galaxies with similar masses at z~6 as measured with imaging from COSMOS-Web.Intriguingly, the two quasar hosts with post-starburst features, which reside at the high-mass end of our sample and exhibit relatively compact morphologies, have similar size and stellar mass surface densities to quiescent galaxies at z~4-5. These findings suggest that the so-called galaxy compaction scenario is already in place at the reionization epoch, in which gas inflows during starburst phases drive centrally concentrated star formation followed by rapid quenching, bridging the structural transition of massive galaxies from relatively extended star-forming disks to compact quiescent systems.
title SHELLQs-JWST Unveils the Host Galaxies of 12 Quasars at z>6
topic Astrophysics of Galaxies
url https://arxiv.org/abs/2505.03876