SSDC-resident Catalogs

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Energy Band / Catalog Name				Options	Help
Radio
AT
AT20GCAT ( flux 20 GHz)				U
AT20GCAT ( flux 5 GHz)				U
AT20GCAT ( flux 8 GHz)				U
ATCAPMN ( flux 3.6 cm)				U
ATCAPMN ( flux 6 cm)				U
ATPMNCAT				U
CLASSSCAT				U
CRATES				U
DIXON				U
FIRST				U
GBT
GB6				U
GB87CAT				U
NORTH20CM (flux 20 cm)				U
NORTH20CM (flux 6 cm)				U
NORTH20CM (flux 80 cm)				U
JVASPOL				U
KUEHR				U
NIEPPOCAT				U
NVSS				U
PKSCAT90				U
PMN				U
Planck
ERCSC030				U
ERCSC044				U
ERCSC070				U
ERCSC100				U
ERCSC143				U
ERCSC217				U
ERCSC353				U
ERCSC545				U
ERCSC857				U
PCCS1F030				U
PCCS1F044				U
PCCS1F070				U
PCCS1F100				U
PCCS1F143				U
PCCS1F217				U
PCCS1F353				U
PCCS1F545				U
PCCS1F857				U
PCCS2E100				U
PCCS2E143				U
PCCS2E217				U
PCCS2E353				U
PCCS2E545				U
PCCS2E857				U
PCCS2F030				U
PCCS2F044				U
PCCS2F070				U
PCCS2F100				U
PCCS2F143				U
PCCS2F217				U
PCCS2F353				U
PCCS2F545				U
PCCS2F857				U
SUMSS				U
VLANEP				U
VLSSr				U
WENSS				U
WMAP
WMAP5 (Freq. 23e9 Hz)				U
WMAP5 (Freq. 33e9 Hz)				U
WMAP5 (Freq. 41e9 Hz)				U
WMAP5 (Freq. 61e9 Hz)				U
WMAP5 (Freq. 94e9 Hz)				U
Infrared
AKARI/FIS
AKARIBSC 065				U
AKARIBSC 090				U
AKARIBSC 140				U
AKARIBSC 160				U
AKARI/IRC
AKARIPSC 09				U
AKARIPSC 18				U
DENIS
DENIS_3_i				U
DENIS_3_j				U
DENIS_3_k				U
HATLASDR1
hatlasdr1 (100um)				U
hatlasdr1 (160um)				U
hatlasdr1 (250um)				U
hatlasdr1 (350um)				U
hatlasdr1 (500um)				U
HERSCHEL
HGOODSDR1 (100um)				U
HGOODSDR1 (160um)				U
HGOODSDR1 (250um)				U
HGOODSDR1 (350um)				U
HGOODSDR1 (500um)				U
IRAS
IRASFSC 12				U
IRASFSC 25				U
IRASFSC 60				U
IRASFSC100				U
IRASPSC 12				U
IRASPSC 25				U
IRASPSC 60				U
IRASPSC100				U
WISE
allwise w1				U
allwise w2				U
allwise w3				U
allwise w4				U
WISE W1 ExtEll				U
WISE W1 PointPsf				U
WISE W2 ExtEll				U
WISE W2 PointPsf				U
WISE W3 ExtEll				U
WISE W3 PointPsf				U
WISE W4 ExtEll				U
WISE W4 PointPsf				U
Optical UV
GALEX
GALEXAISFUV				U
GALEXAISNUV				U
GALEXMISFUV				U
GALEXMISNUV				U
Swift
UVOTPLKSED				U
UVOTSSC v				U
UVOTSSC b				U
UVOTSSC u				U
UVOTSSC uvw1				U
UVOTSSC uvm2				U
UVOTSSC uvw2				U
Soft X-Ray
ASCA
ASCASIS (0.5-12 keV)				U
Ariel V
ARIEL3A				U
BeppoSAX
SAXMECS				U
WFCCAT				U
WFCCAT FULL				U
CHANDRA
CHANDRASRC (0.2-0.5 keV)				U
CHANDRASRC (0.5-1.2 keV)				U
CHANDRASRC (1.2-2.0 keV)				U
CHANDRASRC (2.0-7.0 keV)				U
EXOSAT
CMA				U
Einstein
IPC				U
IPCSLEW				U
HEAO-1
A2PIC				U
ROSAT
BMW				U
RASS				U
RXS2CAT				U
SKYROSAT				U
WGACAT2				U
Swift
1SWXRT (0.1-10 keV)				U
1SWXRT (0.1-2.4 keV)				U
1SWXRT (2-10 keV)				U
1SXPS(0.3-1keV)				U
1SXPS(0.3—10 keV)				U
1SXPS(1-2keV)				U
1SXPS(2—10 keV)				U
XRTGRBDEEP				U
UHURU
UHURU4				U
XMM
XMMSL2 (0.2-12 keV)				U
XMMSL2 (0.2-2 keV)				U
XMMSL2 (2-12 keV)				U
4XMM-DR12 (0.5-1 keV)				U
4XMM-DR12 (1-2 keV)				U
4XMM-DR12 (2-4.5 keV)				U
4XMM-DR12 (4.5-12 keV)				U
eROSITA DR1 Main
band 1 (0.2 - 2.3 keV)				U
band P1 (0.2 - 0.5 keV)				U
band P2 (0.5 - 1 keV)				U
band P3 (1 - 2 keV)				U
band P4 (2 - 5 keV)				U
band P5 (5 - 8 keV)				U
eROSITA DR1 hard
band 0 (0.2 - 5.0 keV)				U
band 1 (0.2 - 0.6 keV)				U
band 2 (0.6 - 2.3 keV)				U
band 3 (2.3 - 5.0 keV)				U
eROSITA DR1 suppl
suppl band 1 (0.2 - 2.3 keV)				U
suppl band P1 (0.2 - 0.5 keV)				U
suppl band P2 (0.5 - 1 keV)				U
suppl band P3 (1 - 2 keV)				U
suppl band P4 (2 - 5 keV)				U
suppl band P5 (5 - 8 keV)				U
Hard X-Ray
HEAO-1
A4 (13-25 keV)				U
A4 (25-40 keV)				U
A4 (40-80 keV)				U
A4 (80-180 keV)				U
INTEGRAL
IBISSG4CAT (20-40 keV)				U
IBISSG4CAT (40-100 keV)				U
MAXIGSC				U
MAXIGSCHGL-HB				U
MAXIGSCHGL-SB				U
Swift
BAT39MCAT (10-150keV)				U
BAT39MCAT (15-30keV)				U
BAT54MCAT (15-150keV)				U
BAT54MCAT (15-50keV)				U
BAT60AGN (15 - 55 keV)				U
BATPA100				U
SWBAT105 (14-195 keV)				U
SWBAT70M (14-195 keV)				U
Gamma-Ray
AGILE Grid				U
EGRET3				U
Fermi
2FHL (1081GeV)				U
2FHL (316GeV)				U
2FHL (92GeV)				U
Fermi 4FGL-DR3 (0.05-0.1 GeV)				U
Fermi 4FGL-DR3 (0.1-0.3 GeV)				U
Fermi 4FGL-DR3 (0.3-1 GeV)				U
Fermi 4FGL-DR3 (1-3 GeV)				U
Fermi 4FGL-DR3 (10-30 GeV)				U
Fermi 4FGL-DR3 (100-1000 GeV)				U
Fermi 4FGL-DR3 (3-10 GeV)				U
Fermi 4FGL-DR3 (30-100 GeV)				U
Fermi1FGL (200 Mev)				U
Fermi1FGL (2Gev)				U
Fermi1FGL (600 Mev)				U
Fermi1FGL (60Gev)				U
Fermi1FGL (6Gev)				U
Fermi2FGL (200 Mev)				U
Fermi2FGL (2Gev)				U
Fermi2FGL (600 Mev)				U
Fermi2FGL (60Gev)				U
Fermi2FGL (6Gev)				U
Fermi2FglLC				U
Fermi3FGL (200 Mev)				U
Fermi3FGL (2Gev)				U
Fermi3FGL (600 Mev)				U
Fermi3FGL (60Gev)				U
Fermi3FGL (6Gev)				U
VHE
ARGO2LAC				U
HESS				U
MAGIC				U
VERITAS				U

Data from external services and catalogs

Name			Credits		Search	Options
BSDC-MAGIC						U
BSDC-Veritas						U
Catalina RTS						U
NED					IRAS 18162-2048IRAS18162-2048	U
VizieR photometry						U
2MASS						U
SDSS19						U
USNO A2.0						U

• SSC (Numerical)

Log R(cm)			B (Gauss)
δ			N
Log (γ min)			Log (γ max)

Power Law

α

Power Law + Cut Off

α
Log (γ cut)

Broken Power Law

α 1
α 2
Log (γ b)

Log Parabola

Log (γ 0)
r
s

Power Law + Log Parabola

Log (γ 0)
r
s

Synchrotron self-absorption

YES NO

fast accurate

    

• Polynomial

y(x) =a+b * x+c * x^2+d * x^3   Polinomial degree

a
b
c
d

Interval for X-Axis limits for FIT

Log X min

Log X max

Max value of Log vf(v)
v_max = v(Log vf(v)_max)
StdError
Correlation Coefficient
Num Terms

     

Photometric redshift estimation

Please choose the type of templates to be used for the fit of the data: Power Law  (F ∝ λ^{-β} (0.05<β<2))(2012, A&A 538, A26) Composite QSO optical spectrum  (2001, ApJ 122, 549) Giant Elliptical galaxy template (1980, ApJS 43,393) (Optional) Add a systematic error (in terms of fraction (%) of flux) to the flux errors (see Note 2): 0 1 5 10 20 50 Run Please note that this is a Beta Version. Use it with caution and at your own risk. Note 1: The tool uses the current nufnu data (in units of [erg/cm^2/s]) in the frequency range between 1.0E14 and 5.0E15 Hz. If multiple nufnu values for the same frequency are present, the average value will be used for the photo-redshift estimation. Note2: When the chi2 explodes and/or both the integrated prob. p(z) around the best solution and the chi2 prob. are very low or zero, it might be possible to improve the goodness of the fit by adding a systematic error to the measurements (see the Tutorial for more details). Exit

Composite QSO sp. and Standard X-ray emission	αro Update
Giant Elliptical
Ibm type (NGC4449)	scaling factor Update
Sb type (M31)	scaling factor Update
Sbc type (NGC2903)	scaling factor Update
Scd type (NGC4559)	scaling factor Update

Instrument Sensitivity for selected instruments

	Name
	Planck-HFI
	Planck-LFI
	Swift UVOT
	NuSTAR
	Super-Agile
	Swift XRT
	Agile-Grid
	ASTROGAM
	EGRET
	Fermi 2yr (2FGL)
	Fermi 4yr (3FGL)
	Integral ISGRI
	Integral PICsIT
	Swift BAT
	CTA_NORTH
	CTA_SOUTH
	HESS
	MAGIC high
	MAGIC low
	Veritas