5XMM J130038.0+280325
5XMM-DR15 stacked source · SRCID 3012471090100420
Position:
13h00m38.01s +28d03m25.0s
(195.15840°, 28.05695°)
EP flux
1.82e-14
± 4.0e-15
erg cm-2 s-1
CLASSX
Bkg_AGN
(0.927)
Detections
8
| SRCID | 3012471090100420 |
|---|---|
| IAUNAME | 5XMM J130038.0+280325 |
| SC_RA | 13h00m38.01s (195.15840°) |
| SC_DEC | +28d03m25.0s (28.05695°) |
| RADEC_ERR | 0.54 arcsec |
| LII / BII | 57.9655° / 87.7609° |
| N_CONTRIB | 8 (detections) |
| N_OBS | 60 (observations covering the position) |
| MJD_FIRST | 51693.537 (2000-05-29 12:52:43.000 UTC) |
| MJD_LAST | 53540.273 (2005-06-19 06:33:16.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 1.82e-14 ± 4.0e-15 erg cm-2 s-1
Hardness ratios
HR1
0.70
± 0.06
0.2-0.5 / 0.5-1.0 keV
HR2
-0.65
± 0.06
0.5-1.0 / 1.0-2.0 keV
HR3
-0.72
± 0.16
1.0-2.0 / 2.0-4.5 keV
HR4
-0.42
± 0.59
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML 16.0)
SUM_FLAG:
2
Long-term lightcurve
No light-curve points available.
Bkg_AGN
CLASSX outlier: 2.8
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
- 3369333
- Match probability
- 0.774
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | — | — |
| U | 16.245 | 0.013 |
| B | — | — |
| V | — | — |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 3.64e-14 (+4.5e-14 / −2.9e-14) erg cm−2 s−1 |
|---|---|
| NH | 5.75e+20 (+1.3e+21 / −8.0e+19) cm−2 |
| Photon index (Γ) | 2.18 (+2.66 / −1.87) |
| DoF | 452 |
| p-value | 0.641 |
| Inter-instrument norm. | 1.36 (1.12–1.63) |
| 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.