5XMM J215133.6-273552
5XMM-DR15 stacked source · SRCID 3006294040100006
Position:
21h51m33.68s -27d35m52.2s
(327.89034°, -27.59784°)
EP flux
8.55e-14
± 2.8e-14
erg cm-2 s-1
CLASSX
AGN
(0.946)
Detections
1
| SRCID | 3006294040100006 |
|---|---|
| IAUNAME | 5XMM J215133.6-273552 |
| SC_RA | 21h51m33.68s (327.89034°) |
| SC_DEC | -27d35m52.2s (-27.59784°) |
| RADEC_ERR | 0.82 arcsec |
| LII / BII | 21.5219° / -50.2870° |
| 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): 8.55e-14 ± 2.8e-14 erg cm-2 s-1
Hardness ratios
HR1
0.16
± 0.13
0.2-0.5 / 0.5-1.0 keV
HR2
-0.07
± 0.12
0.5-1.0 / 1.0-2.0 keV
HR3
-0.40
± 0.15
1.0-2.0 / 2.0-4.5 keV
HR4
-0.05
± 0.32
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -2.2)
SUM_FLAG:
1
Long-term lightcurve
No light-curve points available.
AGN
CLASSX outlier: -0.49
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
- 6400393
- Match probability
- 0.99
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | — | — |
| U | — | — |
| B | — | — |
| V | 19.910 | 0.254 |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 6.41e-14 (+7.4e-14 / −5.5e-14) erg cm−2 s−1 |
|---|---|
| NH | 7.87e+19 (+3.7e+20 / −1.8e+19) cm−2 |
| Photon index (Γ) | 2.21 (+2.42 / −2.03) |
| DoF | 124 |
| p-value | 0.78 |
| 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.