Table 1.
Radio detections of DES0141−54 found in radio archives.
| νobs | Sν | Reference survey | Years of observation |
|---|---|---|---|
| (GHz) | (mJy) | ||
| (1) | (2) | (3) | (4) |
| 20 | 43.0 ± 2.0 | AT20G | 2004–2008 |
| 8.6 | 70.0 ± 4.0 | AT20Gfollow-up | 2004–2008 |
| 8.6 | 63.0 ± 10.0 | ATPMN | 1992–1994 |
| 8.4 | 59.5 ± 3.0 | CRATES | 2005 |
| 4.85 | 100.0 ± 9.0 | PMN | 1990 |
| 4.8 | 90.0 ± 5.0 | AT20Gfollow-up | 2004–2008 |
| 4.8 | 82 ± 7.0 | ATPMN | 1992–1994 |
| 0.843 | 178.3 ± 5.5 | SUMSS | 2002 |
| 0.076–0.231 | 392.5 ± 69.8–241.9 ± 12.3 | GLEAM | 2013–2014 |
Notes. Column (1): observed frequency in GHz; Col. (2): flux density in mJy; Col. (3) reference survey: AT20G = Australia Telescope 20 GHz Survey (Murphy et al. 2010), AT20Gfollow-up = the AT20G high-resolution follow-up (Chhetri et al. 2013), ATPMN = Australia Telescope-PMN survey (McConnell et al. 2012), CRATES = Combined Radio All-sky Targeted Eight GHz Survey (Healey et al. 2007), PMN = 4.85 GHz PARKES-MIT-NRAO survey (Wright et al. 1994), SUMSS = Sidney University Molonglo Survey (Mauch et al. 2003), GLEAM = GaLactic and Extragalactic All-sky MWA Survey (Wayth et al. 2015; Hurley-Walker et al. 2017); Col. (4): years of the observation. In the last line we report the range of the GLEAM detections, from 76 to 231 MHz. All the GLEAM fluxes can be found in Table A.1.
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