Table 1.
ARCTOMO data.
Field | G1 emission properties (a) |
Absorption properties |
|||||||||
---|---|---|---|---|---|---|---|---|---|---|---|
z | ![]() |
log(M*/M⊙) | SFR | # sp. | # det. | EW | R | Scale | Refs. | ||
(M⊙ yr−1) | (Å) | (kpc) | (kpc) | ||||||||
(1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) | (10) | ||
PSZ1 G311.65−18.48 | 0.73379 | 0.14 ± 0.03 | 9.7 ± 0.3 | 1.1 ± 0.3 | 148 | 29 | 0.2–3.7 | 0–43 | 2.8 | L20 | |
RCS2 032727−132623 | 0.98238 | 0.11 ± 0.01 | 9.8 ± 0.2 | 0.4 ± 0.1 | 103 | 26 | 0.3–1.9 | 17–52 | 2.9 | L18 | |
SGAS J1226+2152 | 0.77138 | 0.27 ± 0.02 | 10.1 ± 0.1 | 0.6 ± 0.2 | 90 | 36 | 0.6–4.2 | 1–21 | 2.6 | T21 |
Notes. (1) Redshift; (2) B-band luminosity; (3) stellar mass; (4) star-formation rate; (5) number of 0.6″ × 0.6″ binned spaxels with S/N > 2; (6) number of Mg II detections (significance > 2 in both doublet lines); (7) range in Mg IIλ2796 rest-frame EW; (8) range in impact parameters(b) in the absorber plane (only detections); (9) median linear scale of the binned spaxels (only detections) in the absorber plane; (10) references: L20 Lopez et al. (2020)(a); L18 Lopez et al. (2018); T21 Tejos et al. (2021).
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