emline-SPECTROGRAPH-TILEID-GROUPID.fits¶
- Summary:
This file records simple (Gaussian) emission line fits on the spectra for few major lines.
- Naming Convention:
emline-SPECTROGRAPH-TILEID-GROUPID.fits
, whereSPECTROGRAPH
is the spectrograph ID,TILEID
is the tile number andGROUPID
depends on theGROUPTYPE
of the tile coadd.- Regex:
emline-[0-9]-[0-9]+-([14]xsubset[1-6]|lowspeedsubset[1-6]|exp[0-9]{8}|thru[0-9]{8}|[0-9]{8})\.fits
- File Type:
FITS, 188 KB
Contents¶
Number |
EXTNAME |
Type |
Contents |
---|---|---|---|
IMAGE |
Empty |
||
EMLINEFIT |
BINTABLE |
Emission line fits table |
FITS Header Units¶
HDU0¶
Empty HDU.
HDU1¶
EXTNAME = EMLINEFIT
Table with the emission line fit results for few major lines.
Required Header Keywords¶
Required Header Keywords Table
KEY |
Example Value |
Type |
Comment |
---|---|---|---|
NAXIS1 |
345 |
int |
width of table in bytes |
NAXIS2 |
500 |
int |
number of rows in table |
RRFN |
/global/cfs/cdirs/desi/spectro/redux/fuji/tiles/1x_depth/80608/5/redrock-1-80608-1xsubset5.fits |
str |
full path to the redrock file which contains the redshifts |
COADDFN |
/global/cfs/cdirs/desi/spectro/redux/fuji/tiles/1x_depth/80608/5/coadd-1-80608-1xsubset5.fits |
str |
full path to the coadd file which contains the spectra |
RFHW |
40 |
int |
[Angstrom] rest-frame wavelength width used for fitting on each side of the line |
MINRFHW |
20 |
int |
[Angstrom] minimum requested rest-frame width on each side of the line to consider the fitting |
RFCONTW |
200 |
int |
[Angstrom] rest-frame wavelength extent to fit the continuum |
RV |
3.1 |
float |
value of R_V to convert EBV to magnitudes |
EMNAMES |
OII,HDELTA,HGAMMA,HBETA,OIII,HALPHA |
str |
comma-separated list of emission lines to fit |
RFWAVE00 |
3727.092,3729.874 |
str |
[Angstrom] rest-frame, vacuum, wavelength for the first emission line to fit |
RFWAVE01 |
4102.892 |
str |
[Angstrom] rest-frame, vacuum, wavelength for the second emission line to fit |
RFWAVE02 |
4341.684 |
str |
[Angstrom] rest-frame, vacuum, wavelength for the third emission line to fit |
RFWAVE03 |
4862.683 |
str |
[Angstrom] rest-frame, vacuum, wavelength for the forth emission line to fit |
RFWAVE04 |
4960.295,5008.239 |
str |
[Angstrom] rest-frame, vacuum, wavelength for the fifth emission line to fit |
RFWAVE05 |
6564.613 |
str |
[Angstrom] rest-frame, vacuum, wavelength for the sixth emission line to fit |
Required Data Table Columns¶
Name |
Type |
Units |
Description |
---|---|---|---|
TARGETID |
int64 |
Unique DESI target ID |
|
Z |
float64 |
Redshift measured by Redrock |
|
ZWARN |
int64 |
Redshift warning bitmask from Redrock |
|
SPECTYPE |
char[6] |
Spectral type of Redrock best fit template (e.g. GALAXY, QSO, STAR) |
|
DELTACHI2 |
float64 |
chi2 difference between first- and second-best redrock template fits |
|
TARGET_RA |
float64 |
deg |
Target right ascension |
TARGET_DEC |
float64 |
deg |
Target declination |
OBJTYPE |
char[3] |
Object type: TGT, SKY, NON, BAD |
|
OII_FLUX |
float32 |
10**-17 erg/(s cm2) |
Fitted flux for the [OII] doublet |
OII_FLUX_IVAR |
float32 |
10**+34 (s2 cm4) / erg2 |
Inverse variance of the fitted flux for the [OII] doublet |
OII_SIGMA |
float32 |
Angstrom |
Fitted line width (in the observed frame) for the [OII] doublet |
OII_SIGMA_IVAR |
float32 |
Angstrom^-2 |
Inverse variance of the fitted line width (in the observed frame) for the [OII] doublet |
OII_CONT |
float32 |
10**-17 erg/(s cm2 Angstrom) |
Continuum used for the fitting (fixed value) for the [OII] doublet |
OII_CONT_IVAR |
float32 |
10**+34 (s2 cm4 Angstrom2) / erg2 |
Inverse variance of the continuum for the [OII] doublet |
OII_SHARE |
float32 |
Fitted F1/(F0+F1) for the [OII] doublet, where F0 and F1 are the individual line fluxes |
|
OII_SHARE_IVAR |
float32 |
Inverse variance of the fitted F1/(F0+F1) for the [OII] doublet |
|
OII_EW |
float32 |
Angstrom |
Fitted rest-frame equivalent width for the [OII] doublet |
OII_EW_IVAR |
float32 |
Angstrom^-2 |
Inverse variance of the fitted rest-frame equivalent width for the [OII] doublet |
OII_CHI2 |
float32 |
Reduced chi2 of the fit for the [OII] doublet |
|
OII_NDOF |
int32 |
Number of degrees of freedom of the fit for the [OII] doublet |
|
HDELTA_FLUX |
float32 |
10**-17 erg/(s cm2) |
Fitted flux for the HDELTA line |
HDELTA_FLUX_IVAR |
float32 |
10**+34 (s2 cm4) / erg2 |
Inverse variance of the fitted flux for the HDELTA line |
HDELTA_SIGMA |
float32 |
Angstrom |
Fitted line width (in the observed frame) for the HDELTA line |
HDELTA_SIGMA_IVAR |
float32 |
Angstrom^-2 |
Inverse variance of the fitted line width (in the observed frame) for the HDELTA line |
HDELTA_CONT |
float32 |
10**-17 erg/(s cm2 Angstrom) |
Continuum used for the fitting (fixed value) for the HDELTA line |
HDELTA_CONT_IVAR |
float32 |
10**+34 (s2 cm4 Angstrom2) / erg2 |
Inverse variance of the continuum for the HDELTA line |
HDELTA_SHARE |
float32 |
NaN (SHARE not relevant for HDELTA line) |
|
HDELTA_SHARE_IVAR |
float32 |
NaN (SHARE not relevant for HDELTA line) |
|
HDELTA_EW |
float32 |
Angstrom |
Fitted rest-frame equivalent width for the HDELTA line |
HDELTA_EW_IVAR |
float32 |
Angstrom^-2 |
Inverse variance of the fitted rest-frame equivalent width for the HDELTA line |
HDELTA_CHI2 |
float32 |
Reduced chi2 of the fit for the HDELTA line |
|
HDELTA_NDOF |
int32 |
Number of degrees of freedom of the fit for the HDELTA line |
|
HGAMMA_FLUX |
float32 |
10**-17 erg/(s cm2) |
Fitted flux for the HGAMMA line |
HGAMMA_FLUX_IVAR |
float32 |
10**+34 (s2 cm4) / erg2 |
Inverse variance of the fitted flux for the HGAMMA line |
HGAMMA_SIGMA |
float32 |
Angstrom |
Fitted line width (in the observed frame) for the HGAMMA line |
HGAMMA_SIGMA_IVAR |
float32 |
Angstrom^-2 |
Inverse variance of the fitted line width (in the observed frame) for the HGAMMA line |
HGAMMA_CONT |
float32 |
10**-17 erg/(s cm2 Angstrom) |
Continuum used for the fitting (fixed value) for the HGAMMA line |
HGAMMA_CONT_IVAR |
float32 |
10**+34 (s2 cm4 Angstrom2) / erg2 |
Inverse variance of the continuum for the HGAMMA line |
HGAMMA_SHARE |
float32 |
NaN (SHARE not relevant for HGAMMA line) |
|
HGAMMA_SHARE_IVAR |
float32 |
NaN (SHARE not relevant for HGAMMA line) |
|
HGAMMA_EW |
float32 |
Angstrom |
Fitted rest-frame equivalent width for the HGAMMA line |
HGAMMA_EW_IVAR |
float32 |
Angstrom^-2 |
Inverse variance of the fitted rest-frame equivalent width for the HGAMMA line |
HGAMMA_CHI2 |
float32 |
Reduced chi2 of the fit for the HGAMMA line |
|
HGAMMA_NDOF |
int32 |
Number of degrees of freedom of the fit for the HGAMMA line |
|
HBETA_FLUX |
float32 |
10**-17 erg/(s cm2) |
Fitted flux for the HBETA line |
HBETA_FLUX_IVAR |
float32 |
10**+34 (s2 cm4) / erg2 |
Inverse variance of the fitted flux for the HBETA line |
HBETA_SIGMA |
float32 |
Angstrom |
Fitted line width (in the observed frame) for the HBETA line |
HBETA_SIGMA_IVAR |
float32 |
Angstrom^-2 |
Inverse variance of the fitted line width (in the observed frame) for the HBETA line |
HBETA_CONT |
float32 |
10**-17 erg/(s cm2 Angstrom) |
Continuum used for the fitting (fixed value) for the HBETA line |
HBETA_CONT_IVAR |
float32 |
10**+34 (s2 cm4 Angstrom2) / erg2 |
Inverse variance of the continuum for the HBETA line |
HBETA_SHARE |
float32 |
NaN (SHARE not relevant for HBETA line) |
|
HBETA_SHARE_IVAR |
float32 |
NaN (SHARE not relevant for HBETA line) |
|
HBETA_EW |
float32 |
Angstrom |
Fitted rest-frame equivalent width for the HBETA line |
HBETA_EW_IVAR |
float32 |
Angstrom^-2 |
Inverse variance of the fitted rest-frame equivalent width for the HBETA line |
HBETA_CHI2 |
float32 |
Reduced chi2 of the fit for the HBETA line |
|
HBETA_NDOF |
int32 |
Number of degrees of freedom of the fit for the HBETA line |
|
OIII_FLUX |
float32 |
10**-17 erg/(s cm2) |
Fitted flux for the [OIII] doublet |
OIII_FLUX_IVAR |
float32 |
10**+34 (s2 cm4) / erg2 |
Inverse variance of the fitted flux for the [OIII] doublet |
OIII_SIGMA |
float32 |
Angstrom |
Fitted line width (in the observed frame) for the [OIII] doublet |
OIII_SIGMA_IVAR |
float32 |
Angstrom^-2 |
Inverse variance of the fitted line width (in the observed frame) for the [OIII] doublet |
OIII_CONT |
float32 |
10**-17 erg/(s cm2 Angstrom) |
Continuum used for the fitting (fixed value) for the [OIII] doublet |
OIII_CONT_IVAR |
float32 |
10**+34 (s2 cm4 Angstrom2) / erg2 |
Inverse variance of the continuum for the [OIII] doublet |
OIII_SHARE |
float32 |
F1/(F0+F1) for the [OIII] doublet, where F0 and F1 are the individual line fluxes (SHARE value fixed during the fit) |
|
OIII_SHARE_IVAR |
float32 |
Infinite value, as SHARE is fixed during the fit |
|
OIII_EW |
float32 |
Angstrom |
Fitted rest-frame equivalent width for the [OIII] doublet |
OIII_EW_IVAR |
float32 |
Angstrom^-2 |
Inverse variance of the fitted rest-frame equivalent width for the [OIII] doublet |
OIII_CHI2 |
float32 |
Reduced chi2 of the fit for the [OIII] doublet |
|
OIII_NDOF |
int32 |
Number of degrees of freedom of the fit for the [OIII] doublet |
|
HALPHA_FLUX |
float32 |
10**-17 erg/(s cm2) |
Fitted flux for the HALPHA line |
HALPHA_FLUX_IVAR |
float32 |
10**+34 (s2 cm4) / erg2 |
Inverse variance of the fitted flux for the HALPHA line |
HALPHA_SIGMA |
float32 |
Angstrom |
Fitted line width (in the observed frame) for the HALPHA line |
HALPHA_SIGMA_IVAR |
float32 |
Angstrom^-2 |
Inverse variance of the fitted line width (in the observed frame) for the HALPHA line |
HALPHA_CONT |
float32 |
10**-17 erg/(s cm2 Angstrom) |
Continuum used for the fitting (fixed value) for the HALPHA line |
HALPHA_CONT_IVAR |
float32 |
10**+34 (s2 cm4 Angstrom2) / erg2 |
Inverse variance of the continuum for the HALPHA line |
HALPHA_SHARE |
float32 |
NaN (SHARE not relevant for HALPHA line) |
|
HALPHA_SHARE_IVAR |
float32 |
NaN (SHARE not relevant for HALPHA line) |
|
HALPHA_EW |
float32 |
Angstrom |
Fitted rest-frame equivalent width for the HALPHA line |
HALPHA_EW_IVAR |
float32 |
Angstrom^-2 |
Inverse variance of the fitted rest-frame equivalent width for the HALPHA line |
HALPHA_CHI2 |
float32 |
Reduced chi2 of the fit for the HALPHA line |
|
HALPHA_NDOF |
int32 |
Number of degrees of freedom of the fit for the HALPHA line |
Notes and Examples¶
The fit is done with the desispec.scripts.emline script.
[OII] is fit as a doublet (3927 and 3929), with the line ratio left free during the fit.
[OIII] is fit as a doublet (4960 and 5007), with the line ratio fixed during the fit.
The SHARE is fitted only for the [OII] doublet; for the [OIII] doublet, its value is fixed (hence the infinite OIII_SHARE_IVAR); for the other lines, the SHARE is not used, and NaN are reported.
If there are not enough pixels to fit or if the fit fails, NaN values are reported.
The default settings are designed for the ELGs (e.g. max_sigma); values to be interpreted with caution for the other targets.
The fitted flux is not forced to be positive, so negative values can happen.
The Z,ZWARN,SPECTYPE,DELTACHI2 (TARGET_RA,TARGET_DEC,OBJTYPE, respectively) columns come from the REDSHIFTS (FIBERMAP, respectively) extension of the input redrock file (see redrock-SPECTROGRAPH-TILEID-GROUPID).
For the SURVEY=cmx m33 tile (TILEID=80615) tile and all the SURVEY=sv1 tiles (except TILEID=80971-80976, the dc3r2 ones), proper-motion correction was applied at the fiberassign design step; thus the following columns can have different values than in the desitarget products:
TARGET_RA
,TARGET_DEC
,REF_EPOCH
,PLATE_RA
,PLATE_DEC
, andPLATE_REF_EPOCH
.For the fuji (EDR) and guadalupe productions, the equivalent widths are wrong (overestimated) by a factor (1+Z) ** 2; the code bug has been corrected for subsequent productions (e.g. iron).