5XMM J132505.4+301815
5XMM-DR15 stacked source · SRCID 3002574020100034
Position:
13h25m05.44s +30d18m15.6s
(201.27268°, 30.30433°)
EP flux
1.97e-14
± 4.4e-15
erg cm-2 s-1
CLASSX
AGN
(0.89)
Detections
1
| SRCID | 3002574020100034 |
|---|---|
| IAUNAME | 5XMM J132505.4+301815 |
| SC_RA | 13h25m05.44s (201.27268°) |
| SC_DEC | +30d18m15.6s (30.30433°) |
| RADEC_ERR | 0.65 arcsec |
| LII / BII | 58.2062° / 81.9701° |
| N_CONTRIB | 1 (detections) |
| N_OBS | 1 (observations covering the position) |
| MJD_FIRST | 52255.718 (2001-12-12 17:14:17.000 UTC) |
| MJD_LAST | 52256.169 (2001-12-13 04:02:51.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 1.97e-14 ± 4.4e-15 erg cm-2 s-1
Hardness ratios
HR1
0.02
± 0.11
0.2-0.5 / 0.5-1.0 keV
HR2
-0.05
± 0.11
0.5-1.0 / 1.0-2.0 keV
HR3
-0.06
± 0.12
1.0-2.0 / 2.0-4.5 keV
HR4
-0.67
± 0.17
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -2.3)
SUM_FLAG:
0
Long-term lightcurve
No light-curve points available.
AGN
CLASSX outlier: -0.467
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
- 3473060
- Match probability
- 0.961
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | — | — |
| U | 22.699 | 0.336 |
| B | — | — |
| V | — | — |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 2.10e-14 (+2.5e-14 / −1.8e-14) erg cm−2 s−1 |
|---|---|
| NH | 4.07e+19 (+1.7e+20 / −1.5e+19) cm−2 |
| Photon index (Γ) | 1.72 (+1.86 / −1.56) |
| DoF | 296 |
| p-value | 0.709 |
| Inter-instrument norm. | 0.92 (0.75–1.12) |
| 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.