Further access options are discussed below
For a list of all services and tables belonging to this service's resource, see Information on resource 'DESI photometric redshifts'
This resource contains photometric redshifts from DESI Legacy survey DR8.
20191101 | Update from DR6 and DR7 to DR8 |
20190710 | First publication |
You can access this service using:
This service is published as follows:
local means it is listed on our front page, ivo_managed means it has a record in the VO registry.
The following fields are available to provide input to the service (with some renderers, some of these fields may be unavailable):
Name | Table Head | Description | Unit | UCD |
---|---|---|---|---|
DEC | Delta (ICRS) | Declination (ICRS decimal) | deg | pos.eq.dec |
field | Field | Name of the field in HELP survey | N/A | meta.id;obs.field |
hscs_pos | Position/Name | Coordinates (as h m s, d m s or decimal degrees), or SIMBAD-resolvable object | N/A | N/A |
hscs_sr | Search radius | Search radius in arcminutes | N/A | N/A |
ID | ID | DESI ID = RELEASE*10^12 + BRICKID*10^6 + OBJID | N/A | meta.id;meta.main |
MAXREC | Match limit | Maximum number of records returned. Pass 0 to retrieve service parameters. | N/A | N/A |
MAXREC | Match limit | Maximum number of records returned. Pass 0 to retrieve service parameters. | N/A | N/A |
MAXREC | Match limit | Maximum number of records returned. Pass 0 to retrieve service parameters. | N/A | N/A |
RA | Alpha (ICRS) | Right Ascension (ICRS decimal) | deg | pos.eq.ra |
RESPONSEFORMAT | Output Format | File format requested for output. | N/A | meta.code.mime |
RESPONSEFORMAT | Output Format | File format requested for output. | N/A | meta.code.mime |
RESPONSEFORMAT | Output Format | File format requested for output. | N/A | meta.code.mime |
SR | Search Radius | Search radius | deg | N/A |
VERB | Verbosity | Exhaustiveness of column selection. VERB=1 only returns the most important columns, VERB=2 selects the columns deemed useful to the average user, VERB=3 returns a table with all available columns. | N/A | N/A |
VERB | Verbosity | Exhaustiveness of column selection. VERB=1 only returns the most important columns, VERB=2 selects the columns deemed useful to the average user, VERB=3 returns a table with all available columns. | N/A | N/A |
VERB | Verbosity | Exhaustiveness of column selection. VERB=1 only returns the most important columns, VERB=2 selects the columns deemed useful to the average user, VERB=3 returns a table with all available columns. | N/A | N/A |
The following fields are contained in the output by default. More fields may be available for selection; these would be given below in the VOTable output fields.
Name | Table Head | Description | Unit | UCD |
---|---|---|---|---|
AGE_BEST | AGE_BEST | Best fitted age in yr | yr | N/A |
AGE_INF | AGE_INF | Lower 68% age uncertainty | yr | N/A |
AGE_MED | AGE_MED | Median age | yr | N/A |
AGE_SUP | AGE_SUP | Upper 68% age uncertainty | yr | N/A |
ANYMASK_G | ANYMASK_G | Bitwise mask set if the central pixel from any image satisfies each condition in g | N/A | N/A |
ANYMASK_R | ANYMASK_R | Bitwise mask set if the central pixel from any image satisfies each condition in r | N/A | N/A |
ANYMASK_Z | ANYMASK_Z | Bitwise mask set if the central pixel from any image satisfies each condition in z | N/A | N/A |
CHI_BEST | CHI_BEST | Chi2 of the best fitting | N/A | N/A |
DEC | Dec | Declination (J2000) | deg | pos.eq.dec;meta.main |
EBV_BEST | EBV_BEST | Best fitted intrinsic extinction in E(B-V), three values: 0, 0.5, 1.0 | N/A | N/A |
field | Field | Name of the field in HELP survey | N/A | meta.id;obs.field |
FRACFLUX_G | FRACFLUX_G | Profile-weighted fraction of the flux from other sources in g (typically [0, 1]) | N/A | N/A |
FRACFLUX_R | FRACFLUX_R | Profile-weighted fraction of the flux from other sources in r (typically [0, 1]) | N/A | N/A |
FRACFLUX_W1 | FRACFLUX_W1 | Profile-weighted fraction of the flux from other sources in W1 (typically [0, 1]) | N/A | N/A |
FRACFLUX_W2 | FRACFLUX_W2 | Profile-weighted fraction of the flux from other sources in W2 (typically [0, 1]) | N/A | N/A |
FRACFLUX_Z | FRACFLUX_Z | Profile-weighted fraction of the flux from other sources in z (typically [0, 1]) | N/A | N/A |
FRACIN_G | FRACIN_G | Fraction of a source's flux within the blob in g, near unity for real sources | N/A | N/A |
FRACIN_R | FRACIN_R | Fraction of a source's flux within the blob in r, near unity for real sources | N/A | N/A |
FRACIN_Z | FRACIN_Z | Fraction of a source's flux within the blob in z, near unity for real sources | N/A | N/A |
FRACMASKED_G | FRACMASKED_G | Profile-weighted fraction of pixels masked in g, strictly between [0,1] | N/A | N/A |
FRACMASKED_R | FRACMASKED_R | Profile-weighted fraction of pixels masked in r, strictly between [0,1] | N/A | N/A |
FRACMASKED_Z | FRACMASKED_Z | Profile-weighted fraction of pixels masked in z, strictly between [0,1] | N/A | N/A |
GALDEPTH_G | GALDEPTH_G | galaxy depth in g band | N/A | N/A |
GALDEPTH_R | GALDEPTH_R | galaxy depth in r band | N/A | N/A |
GALDEPTH_Z | GALDEPTH_Z | galaxy depth in z band | N/A | N/A |
ID | ID | DESI ID = RELEASE*10^12 + BRICKID*10^6 + OBJID | N/A | meta.id;meta.main |
LUM_K_BEST | LUM_K_BEST | Best fitting K-band luminosity | N/A | N/A |
LUM_NUV_BEST | LUM_NUV_BEST | Best fitting NUV luminosity in log(L_sun) | N/A | N/A |
LUM_R_BEST | LUM_R_BEST | Best fitting R-band luminosity | N/A | N/A |
MAG_ABS_G | MAG_ABS_G | Absolute magnitude in g band | mag | N/A |
MAG_ABS_R | MAG_ABS_R | Absolute magnitude in r band | mag | N/A |
MAG_ABS_W1 | MAG_ABS_W1 | Absolute magnitude in w1 band | mag | N/A |
MAG_ABS_W2 | MAG_ABS_W2 | Absolute magnitude in w2 band | mag | N/A |
MAG_ABS_Z | MAG_ABS_Z | Absolute magnitude in z band | mag | N/A |
MAG_G | MAG_G | g-band magnitude | mag | N/A |
MAG_R | MAG_R | r-band magnitude | mag | N/A |
MAG_W1 | MAG_W1 | w1-band magnitdue | mag | N/A |
MAG_W2 | MAG_W2 | w2-band magnitude | mag | N/A |
MAG_Z | MAG_Z | z-band mangitude | mag | N/A |
MAGERR_G | MAGERR_G | g-band magnitude error | mag | N/A |
MAGERR_R | MAGERR_R | r-band magnitude error | mag | N/A |
MAGERR_W1 | MAGERR_W1 | w1-band magnitude error | N/A | N/A |
MAGERR_W2 | MAGERR_W2 | w2-band magnitude error | mag | N/A |
MAGERR_Z | MAGERR_Z | z-band magnitude error | mag | N/A |
MASS_BEST | MASS_BEST | Best estimated stellar mass in log(M_sun) | N/A | N/A |
MASS_INF | MASS_INF | Lower 68% mass uncertainty | N/A | N/A |
MASS_MED | MASS_MED | Median mass | N/A | N/A |
MASS_SUP | MASS_SUP | Upper 68% mass uncertainty | N/A | N/A |
mean_dis | mean_dis | mean Ecludean distance in the color space of neighbours | N/A | N/A |
mean_z | mean_z | mean redshift of neigbours | N/A | N/A |
MOD_BEST | MOD_BEST | ID of BC03 model spectra | N/A | N/A |
n_filter | n_filter | number of filters having colors in color cuts | N/A | N/A |
n_neighbour | n_neighbour | number of neighbours | N/A | N/A |
nearest_z | nearest_z | nearest redshift of neighbours | N/A | N/A |
photo_z | photo_z | estimated photo-z value | N/A | N/A |
photo_zerr | photo_zerr | estimated photo-z error | N/A | N/A |
RA | RA | Right Ascension (J2000) | deg | pos.eq.ra;meta.main |
SCALE_BEST | SCALE_BEST | Scale factor between observed SED and model SED | N/A | N/A |
SFR_BEST | SFR_BEST | Best estimated SFR in M_sun/yr | N/A | N/A |
SFR_INF | SFR_INF | Lower 68% SFR uncertainty | N/A | N/A |
SFR_MED | SFR_MED | Median SFR | N/A | N/A |
SFR_SUP | SFR_SUP | Upper 68% SFR uncertainty | N/A | N/A |
spec_z | spec_z | sepctroscopic redshift if available | N/A | N/A |
SSFR_BEST | SSFR_BEST | Best estimated SSFR, in yr^-1 | N/A | N/A |
SSFR_INF | SSFR_INF | Lower 68% SSFR uncertainty | N/A | N/A |
SSFR_MED | SSFR_MED | Median SSFR | N/A | N/A |
SSFR_SUP | SSFR_SUP | Upper 68% SSFR uncertainty | N/A | N/A |
TYPE | TYPE | Tractor Type | N/A | N/A |
The following fields are available in VOTable output. The verbosity level is a number intended to represent the relative importance of the field on a scale of 1 to 30. The services take a VERB argument. A field is included in the output if their verbosity level is less or equal VERB*10.
Name | Table Head | Description | Unit | UCD | Verb. Level |
---|---|---|---|---|---|
field | Field | Name of the field in HELP survey | N/A | meta.id;obs.field | 1 |
ID | ID | DESI ID = RELEASE*10^12 + BRICKID*10^6 + OBJID | N/A | meta.id;meta.main | 1 |
RA | RA | Right Ascension (J2000) | deg | pos.eq.ra;meta.main | 1 |
DEC | Dec | Declination (J2000) | deg | pos.eq.dec;meta.main | 1 |
MAG_G | MAG_G | g-band magnitude | mag | N/A | 1 |
MAG_R | MAG_R | r-band magnitude | mag | N/A | 1 |
MAG_Z | MAG_Z | z-band mangitude | mag | N/A | 1 |
MAG_W1 | MAG_W1 | w1-band magnitdue | mag | N/A | 1 |
MAG_W2 | MAG_W2 | w2-band magnitude | mag | N/A | 1 |
MAGERR_G | MAGERR_G | g-band magnitude error | mag | N/A | 1 |
MAGERR_R | MAGERR_R | r-band magnitude error | mag | N/A | 1 |
MAGERR_Z | MAGERR_Z | z-band magnitude error | mag | N/A | 1 |
MAGERR_W1 | MAGERR_W1 | w1-band magnitude error | N/A | N/A | 1 |
MAGERR_W2 | MAGERR_W2 | w2-band magnitude error | mag | N/A | 1 |
GALDEPTH_G | GALDEPTH_G | galaxy depth in g band | N/A | N/A | 1 |
GALDEPTH_R | GALDEPTH_R | galaxy depth in r band | N/A | N/A | 1 |
GALDEPTH_Z | GALDEPTH_Z | galaxy depth in z band | N/A | N/A | 1 |
TYPE | TYPE | Tractor Type | N/A | N/A | 1 |
FRACFLUX_G | FRACFLUX_G | Profile-weighted fraction of the flux from other sources in g (typically [0, 1]) | N/A | N/A | 1 |
FRACFLUX_R | FRACFLUX_R | Profile-weighted fraction of the flux from other sources in r (typically [0, 1]) | N/A | N/A | 1 |
FRACFLUX_Z | FRACFLUX_Z | Profile-weighted fraction of the flux from other sources in z (typically [0, 1]) | N/A | N/A | 1 |
FRACFLUX_W1 | FRACFLUX_W1 | Profile-weighted fraction of the flux from other sources in W1 (typically [0, 1]) | N/A | N/A | 1 |
FRACFLUX_W2 | FRACFLUX_W2 | Profile-weighted fraction of the flux from other sources in W2 (typically [0, 1]) | N/A | N/A | 1 |
FRACMASKED_G | FRACMASKED_G | Profile-weighted fraction of pixels masked in g, strictly between [0,1] | N/A | N/A | 1 |
FRACMASKED_R | FRACMASKED_R | Profile-weighted fraction of pixels masked in r, strictly between [0,1] | N/A | N/A | 1 |
FRACMASKED_Z | FRACMASKED_Z | Profile-weighted fraction of pixels masked in z, strictly between [0,1] | N/A | N/A | 1 |
FRACIN_G | FRACIN_G | Fraction of a source's flux within the blob in g, near unity for real sources | N/A | N/A | 1 |
FRACIN_R | FRACIN_R | Fraction of a source's flux within the blob in r, near unity for real sources | N/A | N/A | 1 |
FRACIN_Z | FRACIN_Z | Fraction of a source's flux within the blob in z, near unity for real sources | N/A | N/A | 1 |
ANYMASK_G | ANYMASK_G | Bitwise mask set if the central pixel from any image satisfies each condition in g | N/A | N/A | 1 |
ANYMASK_R | ANYMASK_R | Bitwise mask set if the central pixel from any image satisfies each condition in r | N/A | N/A | 1 |
ANYMASK_Z | ANYMASK_Z | Bitwise mask set if the central pixel from any image satisfies each condition in z | N/A | N/A | 1 |
n_neighbour | n_neighbour | number of neighbours | N/A | N/A | 1 |
n_filter | n_filter | number of filters having colors in color cuts | N/A | N/A | 1 |
photo_z | photo_z | estimated photo-z value | N/A | N/A | 1 |
photo_zerr | photo_zerr | estimated photo-z error | N/A | N/A | 1 |
spec_z | spec_z | sepctroscopic redshift if available | N/A | N/A | 1 |
mean_z | mean_z | mean redshift of neigbours | N/A | N/A | 1 |
nearest_z | nearest_z | nearest redshift of neighbours | N/A | N/A | 1 |
mean_dis | mean_dis | mean Ecludean distance in the color space of neighbours | N/A | N/A | 1 |
CHI_BEST | CHI_BEST | Chi2 of the best fitting | N/A | N/A | 1 |
MOD_BEST | MOD_BEST | ID of BC03 model spectra | N/A | N/A | 1 |
EBV_BEST | EBV_BEST | Best fitted intrinsic extinction in E(B-V), three values: 0, 0.5, 1.0 | N/A | N/A | 1 |
SCALE_BEST | SCALE_BEST | Scale factor between observed SED and model SED | N/A | N/A | 1 |
MAG_ABS_G | MAG_ABS_G | Absolute magnitude in g band | mag | N/A | 1 |
MAG_ABS_R | MAG_ABS_R | Absolute magnitude in r band | mag | N/A | 1 |
MAG_ABS_Z | MAG_ABS_Z | Absolute magnitude in z band | mag | N/A | 1 |
MAG_ABS_W1 | MAG_ABS_W1 | Absolute magnitude in w1 band | mag | N/A | 1 |
MAG_ABS_W2 | MAG_ABS_W2 | Absolute magnitude in w2 band | mag | N/A | 1 |
AGE_BEST | AGE_BEST | Best fitted age in yr | yr | N/A | 1 |
AGE_INF | AGE_INF | Lower 68% age uncertainty | yr | N/A | 1 |
AGE_MED | AGE_MED | Median age | yr | N/A | 1 |
AGE_SUP | AGE_SUP | Upper 68% age uncertainty | yr | N/A | 1 |
MASS_BEST | MASS_BEST | Best estimated stellar mass in log(M_sun) | N/A | N/A | 1 |
MASS_INF | MASS_INF | Lower 68% mass uncertainty | N/A | N/A | 1 |
MASS_MED | MASS_MED | Median mass | N/A | N/A | 1 |
MASS_SUP | MASS_SUP | Upper 68% mass uncertainty | N/A | N/A | 1 |
SFR_BEST | SFR_BEST | Best estimated SFR in M_sun/yr | N/A | N/A | 1 |
SFR_INF | SFR_INF | Lower 68% SFR uncertainty | N/A | N/A | 1 |
SFR_MED | SFR_MED | Median SFR | N/A | N/A | 1 |
SFR_SUP | SFR_SUP | Upper 68% SFR uncertainty | N/A | N/A | 1 |
SSFR_BEST | SSFR_BEST | Best estimated SSFR, in yr^-1 | N/A | N/A | 1 |
SSFR_INF | SSFR_INF | Lower 68% SSFR uncertainty | N/A | N/A | 1 |
SSFR_MED | SSFR_MED | Median SSFR | N/A | N/A | 1 |
SSFR_SUP | SSFR_SUP | Upper 68% SSFR uncertainty | N/A | N/A | 1 |
LUM_NUV_BEST | LUM_NUV_BEST | Best fitting NUV luminosity in log(L_sun) | N/A | N/A | 1 |
LUM_R_BEST | LUM_R_BEST | Best fitting R-band luminosity | N/A | N/A | 1 |
LUM_K_BEST | LUM_K_BEST | Best fitting K-band luminosity | N/A | N/A | 1 |
hp_idx | HP_Idx | HEALPix index of the source position at order 13 using the nested scheme. | N/A | pos.healpix | 30 |
VOResource XML (that's something exclusively for VO nerds)