5XMM J132457.2+300728
5XMM-DR15 stacked source · SRCID 3002574020100040
Position:
13h24m57.28s +30d07m28.7s
(201.23868°, 30.12464°)
EP flux
1.98e-14
± 5.6e-15
erg cm-2 s-1
CLASSX
Extended
(0.999)
Detections
1
| SRCID | 3002574020100040 |
|---|---|
| IAUNAME | 5XMM J132457.2+300728 |
| SC_RA | 13h24m57.28s (201.23868°) |
| SC_DEC | +30d07m28.7s (30.12464°) |
| RADEC_ERR | 1.46 arcsec |
| LII / BII | 57.0705° / 82.0610° |
| 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): 1.98e-14 ± 5.6e-15 erg cm-2 s-1
Hardness ratios
HR1
0.56
± 0.07
0.2-0.5 / 0.5-1.0 keV
HR2
-0.53
± 0.07
0.5-1.0 / 1.0-2.0 keV
HR3
-0.98
± 0.11
1.0-2.0 / 2.0-4.5 keV
HR4
0.98
± 0.40
2.0-4.5 / 4.5-12.0 keV
Extent:
8.43
± 0.98
arcsec
(ML 36.3)
SUM_FLAG:
1
Long-term lightcurve
No light-curve points available.
Extended
CLASSX outlier: 2.68
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
- 3472601
- Match probability
- 0.989
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | — | — |
| U | 21.796 | 0.167 |
| B | — | — |
| V | — | — |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 5.73e-15 (+6.9e-15 / −4.7e-15) erg cm−2 s−1 |
|---|---|
| NH | 6.97e+20 (+1.2e+21 / −1.0e+20) cm−2 |
| Photon index (Γ) | 2.73 (+2.92 / −2.40) |
| DoF | 80 |
| p-value | 0.168 |
| 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.