5XMM J121930.2+472201
5XMM-DR15 stacked source · SRCID 3005914010100112
Position:
12h19m30.27s +47d22m01.2s
(184.87614°, 47.36700°)
EP flux
4.97e-15
± 3.0e-15
erg cm-2 s-1
CLASSX
Star
(0.747)
Detections
6
| SRCID | 3005914010100112 |
|---|---|
| IAUNAME | 5XMM J121930.2+472201 |
| SC_RA | 12h19m30.27s (184.87614°) |
| SC_DEC | +47d22m01.2s (47.36700°) |
| RADEC_ERR | 0.80 arcsec |
| LII / BII | 138.0196° / 68.8148° |
| N_CONTRIB | 6 (detections) |
| N_OBS | 8 (observations covering the position) |
| MJD_FIRST | 51886.934 (2000-12-08 22:25:31.000 UTC) |
| MJD_LAST | 54057.366 (2006-11-18 08:47:36.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 4.97e-15 ± 3.0e-15 erg cm-2 s-1
Hardness ratios
HR1
0.39
± 0.11
0.2-0.5 / 0.5-1.0 keV
HR2
-0.58
± 0.12
0.5-1.0 / 1.0-2.0 keV
HR3
-0.76
± 0.30
1.0-2.0 / 2.0-4.5 keV
HR4
0.86
± 0.59
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -2.0)
SUM_FLAG:
1
Long-term lightcurve
No light-curve points available.
Star
CLASSX outlier: 3.47
Class probabilities
Class taxonomy
- AGN — active galactic nucleus.
- Bkg_AGN — background AGN.
- Star — Galactic star.
- Gal_XRB — Galactic X-ray binary.
- Extragal_XRB — extragalactic X-ray binary.
- CV — cataclysmic variable.
- Extended — cluster or galaxy.
Optical Monitor (OM)
- OM Source ID
- 3193877
- Match probability
- 0.996
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | — | — |
| U | — | — |
| B | 20.611 | 0.061 |
| V | — | — |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 6.18e-15 (+8.5e-15 / −4.5e-15) erg cm−2 s−1 |
|---|---|
| NH | 1.62e+20 (+7.8e+20 / −2.2e+19) cm−2 |
| Photon index (Γ) | 2.48 (+2.81 / −2.08) |
| DoF | 57 |
| p-value | 0.884 |
| Quality flag | 0 |
No variability data available for this source.
No contributing observations found.
Sky view (optical)
DSS2 colour optical image. The header thumbnail shows the XMM-Newton X-ray image; use the layers menu in the toolbar to switch surveys.
Hardness-ratio diagram
No hardness-ratio pairs available for this source.
The per-observation light curve is shown in the X-ray properties section above.