Issue |
A&A
Volume 649, May 2021
|
|
---|---|---|
Article Number | C5 | |
Number of page(s) | 1 | |
Section | Numerical methods and codes | |
DOI | https://doi.org/10.1051/0004-6361/201629507e | |
Published online | 10 May 2021 |
LSDCat: Detection and cataloguing of emission-line sources in integral-field spectroscopy datacubes (Corrigendum)
1
European Southern Observatory, Av. Alonso de Córdova 3107, 763 0355 Vitacura, Santiago, Chile
e-mail: eherenz@eso.org
2
Leibniz-Institut für Astrophysik Potsdam (AIP), An der Sternware 16, 14482 Potsdam, Germany
Key words: methods: data analysis / techniques: imaging spectroscopy / errata, addenda
We correct an error in Eq. (34) of Herenz & Wisotzki (2017), where we provided an estimate for the signal-to-noise ratio for an emission line that matches the 3D Gaussian filter template of LSDCat. The correct equation reads
that is, σG is not under the square root as presented in the paper. All previous steps that lead to this equation, that is, Eqs. (29)–(33), were correct.
As a consequence of this correction, the numerical value of the limiting flux in the MUSE HDF-S data at 7000 Å, given in Eq. (35) of our paper, was also incorrect. Inserting the given values (σG = 1.84 px, σz = 1.46, erg s−1 cm−2 Å−1, Δλ = 1.2 Å, and S/Ndet ≈ 8) into Eq. (1) delivers
Therefore Fig. 3, where the theoretical limiting flux was compared with the results of a source insertion and recovery experiment, also needs to be corrected. The corrected version of Fig. 3 is shown here in Fig. 1. The match between the experiment and theoretical expectation in Fig. 1 is closer in comparison to what was originally presented, so parts of the discussion in the final paragraph of Sect. 3.2 are thus obsolete.
![]() |
Fig. 1. Completeness curve fC(log F [erg s−1 cm−2 Å−1]) from a fake source insertion and recovery experiment on the MUSE HDF-S datacube at 5000 Å. The dotted vertical line shows the 50% completeness limit at log F [erg s−1 cm−2]= − 17.75 and the dashed vertical line shows the analytically approximated minimum line flux given in Eq. (2) as log Fline [erg s−1 cm−2] ≈ − 17.69 at which LSDCat is expected to detect emission line sources in this experiment. |
References
- Herenz, E. C., & Wisotzki, L. 2017, A&A, 602, A111 [NASA ADS] [CrossRef] [EDP Sciences] [Google Scholar]
© ESO 2021
All Figures
![]() |
Fig. 1. Completeness curve fC(log F [erg s−1 cm−2 Å−1]) from a fake source insertion and recovery experiment on the MUSE HDF-S datacube at 5000 Å. The dotted vertical line shows the 50% completeness limit at log F [erg s−1 cm−2]= − 17.75 and the dashed vertical line shows the analytically approximated minimum line flux given in Eq. (2) as log Fline [erg s−1 cm−2] ≈ − 17.69 at which LSDCat is expected to detect emission line sources in this experiment. |
In the text |
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