Further access options are discussed below
For a list of all services and tables belonging to this service's resource, see Information on resource 'WISE High Synchroton Peak blazar candidates catalog'
We assembled a sample including 992 sources, which is currently the largest existing list of confirmed and candidates HSP blazars. All objects are expected to radiate up to the highest gamma-ray photon energies. In fact, 299 of these are confirmed emitters of GeV gamma-ray photons (based on Fermi-LAT catalogues), and 36 have already been detected in the TeV band. The majority of sources in the sample are within reach of the upcoming Cherenkov Telescope Array (CTA), and many may be detectable even by the current generation of Cherenkov telescopes during flaring episodes. The sample includes 425 previously known blazars, 151 new identifications, and 416 HSP candidates (mostly faint sources) for which no optical spectra is available yet. The sample was defined starting from a primary list of infrared colour-colour selected sources from the ALLWISE all sky survey database, and applying further restrictions on IR-radio and IR-X-ray flux ratios. Using a polynomial fit to the multi-frequency data (radio to X-ray) we estimated synchrotron peak frequencies and fluxes of each object.
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, gavo means it is within GAVO's service 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 |
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 |
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 |
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 |
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 |
---|---|---|---|---|
asdc_link | asdc sed tool | N/A | N/A | N/A |
blazar_type | Blazar type | Blazar extended information flag Note blazar_type | N/A | meta.code |
BZcat_name | BZcat name | BZcat designation if any | N/A | meta.id.cross |
decj2000 | Dec | Declination | deg | pos.eq.dec;meta.main |
Fermi_gr_slope | Gamma-ray slope | Gamma-ray slope from Fermi | N/A | obs.param |
Fermi_gr_slope_error | Gamma-ray slope error | Error on gamma-ray slope from Fermi | N/A | stat.error;obs.param |
Fermi_name | Fermi name | Fermi designation if any | N/A | meta.id.assoc |
flux_peak | log(flux peak) | Flux peak | log(erg.cm**-2.s**-1) | em.freq |
id | id | Internal id | N/A | meta |
name | name | Designation | N/A | meta.id;meta.main |
nu_flag | nu-flag | Frequency peak measurement quality flag Note nu_flag | N/A | meta.code |
nu_peak | log(nu peak) | Synchroton frequency peak | log(Hz) | em.freq |
radio_flux | Radio flux density | Radio flux density, NVSS or FIRST | mJy | phot.flux;em.radio |
raj2000 | RA | Right ascension | deg | pos.eq.ra;meta.main |
TEV_FOM | TeV FOM | TeV figure-of-merit estimated flux (E>50GeV) | unknown | obs.param |
WISE_mag | IR mag | WISE magnitude | mag | phot.mag;em.IR |
z | z | redshift | N/A | src.redshift |
z_flag | z-flag | redshift quality flag Note z_flag | N/A | meta.code |
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 |
---|---|---|---|---|---|
asdc_link | asdc sed tool | N/A | N/A | N/A | 1 |
name | name | Designation | N/A | meta.id;meta.main | 1 |
raj2000 | RA | Right ascension | deg | pos.eq.ra;meta.main | 1 |
decj2000 | Dec | Declination | deg | pos.eq.dec;meta.main | 1 |
WISE_mag | IR mag | WISE magnitude | mag | phot.mag;em.IR | 1 |
radio_flux | Radio flux density | Radio flux density, NVSS or FIRST | mJy | phot.flux;em.radio | 1 |
z | z | redshift | N/A | src.redshift | 1 |
z_flag | z-flag | redshift quality flag Note z_flag | N/A | meta.code | 1 |
nu_peak | log(nu peak) | Synchroton frequency peak | log(Hz) | em.freq | 1 |
nu_flag | nu-flag | Frequency peak measurement quality flag Note nu_flag | N/A | meta.code | 1 |
flux_peak | log(flux peak) | Flux peak | log(erg.cm**-2.s**-1) | em.freq | 1 |
blazar_type | Blazar type | Blazar extended information flag Note blazar_type | N/A | meta.code | 1 |
Fermi_gr_slope | Gamma-ray slope | Gamma-ray slope from Fermi | N/A | obs.param | 1 |
Fermi_gr_slope_error | Gamma-ray slope error | Error on gamma-ray slope from Fermi | N/A | stat.error;obs.param | 1 |
TEV_FOM | TeV FOM | TeV figure-of-merit estimated flux (E>50GeV) | unknown | obs.param | 1 |
id | id | Internal id | N/A | meta | 20 |
BZcat_name | BZcat name | BZcat designation if any | N/A | meta.id.cross | 20 |
Fermi_name | Fermi name | Fermi designation if any | N/A | meta.id.assoc | 20 |
VOResource XML (that's something exclusively for VO nerds)
Status on previous knowledge of the source
0 | already known HSP |
1 | HSP candidate; lacks optical spectrum |
2 | complementary source from Sedentary catalog |
3 | in WISE database of extended sources |
4 | complementary TeV detected HSPs |
5 | newly identified HSP |
Quality of frequency peak measurement
1 | good estimate |
2 | uncertain |
3 | lower limit |
Quality/source of the redshift value
0 | no redshift |
1 | trustfull redshift |
2 | uncertain value from the literature |
3 | lower limit based on R-magnitude |