Possible environmental quenching in an interacting little red dot pair at z ∼ 7

Open Access

Table 2.

Hypotheses for this galaxy group.

Source	z case	`Dense Basis` (Stellar fit)	Bagpipes (Stars + AGN)		`Dense Basis` (Stellar fit)

			Stellar component	AGN	Stellar component
	low-z	Dusty and massive BB galaxy	–	–	–
LRD1	mid-z	Dusty and massive BB galaxy	Low-mass unattenuated SFG	Obscured AGN	Low-mass unattenuated SFG
	high-z	Dusty and massive BB galaxy	Dusty and very massive BB galaxy	Dust-free AGN	Dusty and very massive BB galaxy

LRD2	ALL	Dusty and massive BB galaxy	Dusty and massive BB galaxy	Dust-free AGN	Dusty and massive BB galaxy

	low-z	Massive unattenuated SFG	–	–	–
SAT0	mid-z	Massive unattenuated SFG	–	–	–
	high-z	Massive unattenuated BB galaxy	–	–	–

SAT1	ALL	Low-mass unattenuated SFG	–	–	–

SAT2	ALL	Low-mass unattenuated SFG	–	–	–

Notes. ALL denotes the three redshift intervals, defined in Sect. 4. The low-z interval is the one centered at the photo-z of the galaxy group. BB denotes Balmer break and very massive means M_⋆ > 10¹¹ M_⊙. The values for the stellar masses, attenuations, and SFRs can be found in Table F.1.

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.