Emission line catalog (musewide_dr1.mw_44fields_main_table)
Description
This table contains the main table from Herenz et al. 2017.
Attribution
If you have used MUSE-Wide data in your research, please use the following acknowledgement:
This work is based on observations taken by the MUSE-Wide Survey as part of the MUSE Consortium.
and cite the following paper: Urrutia et al. 2019, A&A, 624, A141
Columns
| Name | Type | UCD | Unit | Description |
|---|---|---|---|---|
| unique_id | long |
meta.id meta.ref |
Unique MUSE-Wide object ID |
|
| field_name | char |
meta.id meta.ref |
Name of the field |
|
| ra | double | pos.eq.ra | deg |
Right Ascension (J2000) in degrees |
| dec | double | pos.eq.dec | deg |
Declination (J2000) in degrees |
| z | double | src.redshift |
Redshift of the source |
|
| z_err | double |
stat.error src.redshift |
Error on the determined redshift |
|
| lead_line | char |
Highest S/N detected line |
||
| sn | double |
S/N of the lead line (abbreviations according to Table 5 in Herenz et al., 2017) |
||
| quality | char |
Quality flag (see Sect. 3.2 of Herenz et al., 2017) |
||
| confidence | short |
Confidence value (see Sect. 3.2 of Herenz et al., 2017) |
||
| other_lines | char |
Other detected lines in that source |
||
| guo_id | long |
meta.id meta.ref |
Associated source in the Guo et al. (2013) photometric catalogue |
|
| guo_sep | double | pos.angDistance |
Angular separation (in arcsec) to the Guo et al. (2013) source |
|
| skelton_id | long | meta.id |
Associated source in the Skelton et al. (2014) photometric catalogue |
|
| skelton_sep | double | pos.angDistance |
Angular separation (in arcsec) to the Skelton et al. (2014) source |
|
| stellar_mass | double |
Log stellar mass in solar masses of the galaxy associated to the emission line |