5XMM J215224.5-272930
5XMM-DR15 stacked source · SRCID 3006294040100024
Position:
21h52m24.52s -27d29m30.5s
(328.10217°, -27.49179°)
EP flux
8.32e-14
± 4.0e-14
erg cm-2 s-1
CLASSX
Extended
(0.998)
Detections
1
| SRCID | 3006294040100024 |
|---|---|
| IAUNAME | 5XMM J215224.5-272930 |
| SC_RA | 21h52m24.52s (328.10217°) |
| SC_DEC | -27d29m30.5s (-27.49179°) |
| RADEC_ERR | 4.07 arcsec |
| LII / BII | 21.7376° / -50.4531° |
| 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): 8.32e-14 ± 4.0e-14 erg cm-2 s-1
Hardness ratios
HR1
0.34
± 0.20
0.2-0.5 / 0.5-1.0 keV
HR2
0.11
± 0.16
0.5-1.0 / 1.0-2.0 keV
HR3
-0.74
± 0.21
1.0-2.0 / 2.0-4.5 keV
HR4
0.68
± 0.29
2.0-4.5 / 4.5-12.0 keV
Extent:
10.05
± 1.96
arcsec
(ML 9.1)
SUM_FLAG:
1
Long-term lightcurve
No light-curve points available.
Extended
CLASSX outlier: 3.2
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
- 6401592
- Match probability
- 0.791
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | — | — |
| U | — | — |
| B | — | — |
| V | 19.044 | 0.133 |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 1.96e-14 (+2.7e-14 / −1.4e-14) erg cm−2 s−1 |
|---|---|
| NH | 5.63e+19 (+2.2e+20 / −1.7e+19) cm−2 |
| Photon index (Γ) | 1.59 (+1.94 / −1.30) |
| DoF | 84 |
| p-value | 0.701 |
| 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.