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Table B.1.
XSL keyword dictionary (primary header).
General topic | Data reduction step | Keyword | Description | Default value |
---|---|---|---|---|
General information | OBJECT | Machine-readable name of the star | ||
HNAME | Human-readable name of the star | |||
XSL_ID | X-shooter Spectral Library unique identifier | |||
PROVi | Originating raw science file(s) | |||
Data reduction | 1D extraction | EXT_AVG | Two 1D-spectra averaged | F |
Response curve | CAL_STAR | Spectro-photometric standard star target | ||
CAL_RAWi | Originating raw flux-standard file(s) | |||
First flux calibration | FLUX_COR | First flux calibration applied | F | |
Flux-loss correction | LOSS_COR | Correction for slit-losses applied in DR2 | F | |
SPL_COR | Correction for slit-losses with a spline function applied in DR3 | F | ||
STA_RAWi | Originating raw wide-slit file(s) | |||
Characterization and quality assurance | Rest-frame correction | REST_COR | Correction to rest-frame applied | T |
REST_UVB | UVB cz values(1) [in km s−1] | |||
REST_VIS | VIS cz values(1) [in km s−1] | |||
REST_NIR | NIR cz values(1) [in km s−1] | |||
Barycor values | BARY_COR | Barycentric radial velocity correction value | ||
Merging UVB, VIS, NIR spectra | S_U_VAL | UVB scaling factor value | ||
S_U_ORI | UVB scaling factor reference | |||
S_N_VAL | NIR scaling factor value | |||
S_N_ORI | NIR scaling factor origin reference | |||
ARM_ZERO | DR2 arm spectrum missing (zeros) | F | ||
Galactic dust extinction | AV_VAL | Total extinction in V | ||
AV_ORI | AV origin reference (interp.;interp/spline;reference) | |||
Quality flags | SNR | Median signal-to-noise ratio | ||
WAVY_UVB | Wavy spectrum between 460 and 520 nm | F | ||
(suspected residuals of the blaze function) | ||||
HAIR_VIS | Some narrow spikes in the VIS spectrum | F | ||
NOIS_VIS | Noisy VIS spectrum | F | ||
WAVY_VIS | Wavy in some part of the VIS spectrum | F | ||
HAIR_NIR | Some narrow spikes in the NIR spectrum | F | ||
WAVY_NIR | Wavy in some part of the NIR spectrum | F |
Notes to Table B.1. (1) The cz values are barycentric.
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