5XMM J061356.2+710300
5XMM-DR15 stacked source · SRCID 3000922030100018
Position:
06h13m56.29s +71d03m00.7s
(93.48452°, 71.05019°)
EP flux
1.90e-14
± 4.0e-15
erg cm-2 s-1
CLASSX
AGN
(0.922)
Detections
17
| SRCID | 3000922030100018 |
|---|---|
| IAUNAME | 5XMM J061356.2+710300 |
| SC_RA | 06h13m56.29s (93.48452°) |
| SC_DEC | +71d03m00.7s (71.05019°) |
| RADEC_ERR | 0.44 arcsec |
| LII / BII | 143.2381° / 22.5936° |
| N_CONTRIB | 17 (detections) |
| N_OBS | 17 (observations covering the position) |
| MJD_FIRST | 51836.038 (2000-10-19 00:54:32.000 UTC) |
| MJD_LAST | 57132.768 (2015-04-20 18:26:21.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 1.90e-14 ± 4.0e-15 erg cm-2 s-1
Hardness ratios
HR1
0.44
± 0.10
0.2-0.5 / 0.5-1.0 keV
HR2
0.33
± 0.07
0.5-1.0 / 1.0-2.0 keV
HR3
-0.29
± 0.07
1.0-2.0 / 2.0-4.5 keV
HR4
-0.46
± 0.18
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -2.7)
SUM_FLAG:
1
Long-term lightcurve
No light-curve points available.
AGN
CLASSX outlier: 0.167
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
- 2215854
- Match probability
- 0.996
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | — | — |
| U | — | — |
| B | — | — |
| V | 19.492 | 0.115 |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 3.98e-14 (+4.6e-14 / −3.4e-14) erg cm−2 s−1 |
|---|---|
| NH | 6.47e+19 (+2.7e+20 / −1.8e+19) cm−2 |
| Photon index (Γ) | 1.13 (+1.24 / −1.04) |
| DoF | 413 |
| p-value | 0.401 |
| Inter-instrument norm. | 0.84 (0.70–1.05) |
| 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.