5XMM J022151.6-041225
5XMM-DR15 stacked source · SRCID 3003798220107398
Position:
02h21m51.62s -04d12m25.8s
(35.46509°, -4.20716°)
EP flux
1.23e-14
± 2.7e-15
erg cm-2 s-1
CLASSX
Bkg_AGN
(0.629)
Detections
7
| SRCID | 3003798220107398 |
|---|---|
| IAUNAME | 5XMM J022151.6-041225 |
| SC_RA | 02h21m51.62s (35.46509°) |
| SC_DEC | -04d12m25.8s (-4.20716°) |
| RADEC_ERR | 5.87 arcsec |
| LII / BII | 170.1690° / -58.5231° |
| N_CONTRIB | 7 (detections) |
| N_OBS | 372 (observations covering the position) |
| MJD_FIRST | 52667.803 (2003-01-28 19:16:33.000 UTC) |
| MJD_LAST | 57758.217 (2017-01-05 05:11:54.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 1.23e-14 ± 2.7e-15 erg cm-2 s-1
Hardness ratios
HR1
0.25
± 0.19
0.2-0.5 / 0.5-1.0 keV
HR2
0.15
± 0.16
0.5-1.0 / 1.0-2.0 keV
HR3
-0.22
± 0.16
1.0-2.0 / 2.0-4.5 keV
HR4
-0.34
± 0.21
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML 23.6)
SUM_FLAG:
1
Long-term lightcurve
No light-curve points available.
Bkg_AGN
CLASSX outlier: 1.55
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
- 790482
- Match probability
- 0.861
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | 22.597 | 0.192 |
| U | — | — |
| B | — | — |
| V | — | — |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 2.56e-14 (+3.3e-14 / −2.0e-14) erg cm−2 s−1 |
|---|---|
| NH | 1.69e+20 (+6.9e+20 / −2.7e+19) cm−2 |
| Photon index (Γ) | 2.27 (+2.60 / −1.97) |
| DoF | 100 |
| p-value | 0.985 |
| 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.