Table 4
Best available redshifts for the 30 brightest JCMT/AzTEC-detected SMGs.
| Source | Redshift | Comment and | |
| reference | |||
|
|
|||
| AzTEC1 | 4.3415 | spec-z; Yun et al. (2012) | |
| AzTEC2a | 1.125 | spec-z; Baloković et al. (in prep.) | |
| (4.28 ± 0.82) | radio/submm-z; this work | ||
( ) |
radio/submm-z; | ||
| Koprowski et al. (2014) | |||
| AzTEC3 | 5.298 | spec-z; Riechers et al. (2010); | |
| Capak et al. (2011) | |||
| AzTEC4 |
|
photo-z; Smolčić et al. (2012b) | |
| AzTEC5 |
|
photo-z; Smolčić et al. (2012b) | |
| (1.85 ± 0.23) | radio/submm-z; this work | ||
| AzTEC6a | > 3.52 | radio/submm-z; this work | |
( ) |
radio/submm-z; | ||
| Koprowski et al. (2014) | |||
| AzTEC7 | 2.30 ± 0.10 | photo-z; Smolčić et al. (2012b) | |
| AzTEC8 | 3.179 | spec-z; Riechers et al. (in prep.) | |
| AzTEC9a |
|
photo-z; Smolčić et al. (2012b) | |
| (1.357) | spec-z; Salvato et al. (in prep.) | ||
| (2.82 ± 0.76) | radio/submm-z; this work | ||
( ) |
photo-z; | ||
| Koprowski et al. (2014) | |||
| AzTEC10a |
|
photo-z; Smolčić et al. (2012b) | |
( ) |
photo-z; | ||
| Koprowski et al. (2014) | |||
| AzTEC11b | 1.599 | spec-z; Salvato et al. (in prep.) | |
| AzTEC12 |
|
photo-z; Smolčić et al. (2012b) | |
| AzTEC13 | > 4.07 | radio/submm-z; this work | |
( ) |
radio/submm-z; | ||
| Koprowski et al. (2014) | |||
| AzTEC14-Ec | > 2.95 | radio/submm-z; this work | |
( ) |
radio/submm-z; | ||
| Koprowski et al. (2014) | |||
| AzTEC14-Wc |
|
photo-z; Smolčić et al. (2012b) | |
| AzTEC15 |
|
photo-z; Smolčić et al. (2012b) | |
|
|
|||
| AzTEC16 | > 2.42 | radio/submm-z; this work | |
| AzTEC17a | 0.834 | spec-z; Salvato et al. (in prep.) | |
( ) |
photo-z; this work | ||
| (2.29 ± 0.42) | radio/submm-z; this work | ||
| AzTEC17b |
|
photo-z; this work | |
| (> 2.49) | radio/submm-z; this work | ||
| AzTEC18 |
|
photo-z; this work | |
| (> 2.20) | radio/submm-z; this work | ||
| AzTEC19a |
|
photo-z; this work | |
| (4.22 ± 0.91) | radio/submm-z; this work | ||
| AzTEC19b | 1.11 ± 0.10 | photo-z; this work | |
| (> 6.57) | radio/submm-z; this work | ||
| AzTEC20 | > 2.35 | radio/submm-z; this work | |
| AzTEC21a |
|
photo-z; this work | |
| (> 3.45) | radio/submm-z; this work | ||
| AzTEC21b |
|
photo-z; this work | |
| (> 2.47) | radio/submm-z; this work | ||
| AzTEC21c | > 1.93 | radio/submm-z; this work | |
| AzTEC22 | > 3.00 | radio/submm-z; this work | |
| AzTEC23 |
|
photo-z; this work | |
| (> 2.06) | radio/submm-z; this work | ||
| AzTEC24a | > 2.35 | radio/submm-z; this work | |
| AzTEC24b | > 2.28 | radio/submm-z; this work | |
| AzTEC24c | > 3.17 | radio/submm-z; this work | |
| AzTEC26a |
|
photo-z; this work | |
| (> 1.87) | radio/submm-z; this work | ||
| AzTEC26b | > 1.79 | radio/submm-z; this work | |
| AzTEC27 | > 4.17 | radio/submm-z; this work | |
| AzTEC28 | > 3.11 | radio/submm-z; this work | |
| AzTEC29a | > 2.96 | radio/submm-z; this work | |
| AzTEC29b |
|
photo-z; this work | |
| (> 7.25) | radio/submm-z; this work | ||
| AzTEC30 | > 2.51 | radio/submm-z; this work | |
Notes. When multiple values are given for the redshift, the one not enclosed in parentheses has been adopted in the present study. Among AzTEC16-30 the source names highlighted in bold-face indicate detections with S/N1.3 mm ≥ 5.5.
See text for details about the difference between our redshifts and those from Koprowski et al. (2014).
AzTEC11 was resolved into two 890 μm sources (N and S) by Younger et al. (2009). Here, for the redshift analysis, we treat it as a single source because the two components are probably physically related (Koprowski et al. 2014).
AzTEC14 was resolved into two 890 μm sources (E and W) by Younger et al. (2009). The eastern component appears to lie at a higher redshift than the western one (Smolčić et al. 2012b).
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.