Table B.7
Photometric data of the gas.
| Bin Number | ... | fHβ | dfHβ | f[OIII] | df[OIII] | f[NI] | df[NI] | fHβ,2 | dfHβ,2 | f[OIII],2 | df[OIII],2 | f[NI],2 | df[NI],2 |
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| Flux units: 10−15 [erg s−1 cm−2] | |||||||||||||
| 0 | ... | – | – | – | – | – | – | 2.3 | 0.4 | 2.8 | 0.4 | 1.1 | 0.3 |
| 1 | ... | 2.7 | 0.4 | 5.3 | 0.7 | 7.4 | 0.2 | 0.1 | 0.1 | 0.5 | 0.3 | 0.0 | 0.0 |
| 2 | ... | 3.2 | 0.2 | 7.1 | 0.3 | 1.4 | 0.2 | – | – | – | – | – | – |
| 3 | ... | 1.5 | 0.2 | 3.8 | 0.3 | 6.6 | 0.2 | 1.1 | 0.2 | 1.8 | 0.3 | 0.3 | 0.2 |
| 4 | ... | 5.4 | 0.2 | 1.1 | 0.3 | 0.3 | 0.2 | 1.8 | 0.2 | 4.4 | 0.3 | 0.7 | 0.2 |
| ... | |||||||||||||
Notes. Flux values are given with respect to the aperture of a single VIRUS-W fiber. The projected fiber diameter on sky is 3.2′′ . Hence to convert flux to per arcsec2 quantities, the values have to be divided by the corresponding on-sky fiber aperture area of 8.04 arcsec2. Where multiple fibers are binned together, average flux values are reportedsuch that the same normalisation holds true. To obtain the integrated flux for a specific bin, the values in this table must be multiplied by the number of respective fibers that are listed for that bin in Table B.4.
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.