5XMM J121845.5+472420
5XMM-DR15 stacked source · SRCID 3003214010100013
Position:
12h18m45.55s +47d24m20.8s
(184.68978°, 47.40578°)
EP flux
1.49e-13
± 5.4e-15
erg cm-2 s-1
CLASSX
Extragal_XRB
(0.618)
Detections
7
| SRCID | 3003214010100013 |
|---|---|
| IAUNAME | 5XMM J121845.5+472420 |
| SC_RA | 12h18m45.55s (184.68978°) |
| SC_DEC | +47d24m20.8s (47.40578°) |
| RADEC_ERR | 0.14 arcsec |
| LII / BII | 138.3097° / 68.7349° |
| N_CONTRIB | 7 (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): 1.49e-13 ± 5.4e-15 erg cm-2 s-1
Hardness ratios
HR1
0.85
± 0.02
0.2-0.5 / 0.5-1.0 keV
HR2
0.54
± 0.02
0.5-1.0 / 1.0-2.0 keV
HR3
-0.34
± 0.02
1.0-2.0 / 2.0-4.5 keV
HR4
-0.74
± 0.03
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -4.2)
SUM_FLAG:
1
Long-term lightcurve
No light-curve points available.
Extragal_XRB
CLASSX outlier: 2.21
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
- 3190742
- Match probability
- 0.997
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | 20.641 | 0.092 |
| U | 19.859 | 0.048 |
| B | 21.537 | 0.280 |
| V | — | — |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 1.53e-13 (+1.6e-13 / −1.4e-13) erg cm−2 s−1 |
|---|---|
| NH | 5.12e+21 (+6.1e+21 / −4.4e+21) cm−2 |
| Photon index (Γ) | 2.39 (+2.59 / −2.23) |
| DoF | 433 |
| p-value | 0.961 |
| 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.