5XMM J215220.6-273028
5XMM-DR15 stacked source · SRCID 3006294040100027
Position:
21h52m20.63s -27d30m28.2s
(328.08596°, -27.50785°)
EP flux
7.06e-14
± 4.4e-14
erg cm-2 s-1
CLASSX
Extended
(0.999)
Detections
1
| SRCID | 3006294040100027 |
|---|---|
| IAUNAME | 5XMM J215220.6-273028 |
| SC_RA | 21h52m20.63s (328.08596°) |
| SC_DEC | -27d30m28.2s (-27.50785°) |
| RADEC_ERR | 6.50 arcsec |
| LII / BII | 21.7088° / -50.4418° |
| N_CONTRIB | 1 (detections) |
| N_OBS | 1 (observations covering the position) |
| MJD_FIRST | 52221.582 (2001-11-08 13:57:33.000 UTC) |
| MJD_LAST | 52221.659 (2001-11-08 15:49:33.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 7.06e-14 ± 4.4e-14 erg cm-2 s-1
Hardness ratios
HR1
0.20
± 0.19
0.2-0.5 / 0.5-1.0 keV
HR2
-0.26
± 0.19
0.5-1.0 / 1.0-2.0 keV
HR3
-0.32
± 0.28
1.0-2.0 / 2.0-4.5 keV
HR4
0.40
± 0.48
2.0-4.5 / 4.5-12.0 keV
Extent:
21.78
± 3.67
arcsec
(ML 15.3)
SUM_FLAG:
0
Long-term lightcurve
No light-curve points available.
Extended
CLASSX outlier: 2.98
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
- 6401482
- Match probability
- 0.77
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | — | — |
| U | — | — |
| B | — | — |
| V | 16.264 | 0.026 |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 7.11e-15 (+1.1e-14 / −5.1e-15) erg cm−2 s−1 |
|---|---|
| NH | 2.43e+20 (+1.2e+21 / −3.0e+19) cm−2 |
| Photon index (Γ) | 2.20 (+2.67 / −1.76) |
| DoF | 62 |
| p-value | 0.824 |
| 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.