5XMM J022102.3-032507
5XMM-DR15 stacked source · SRCID 3003798260102105
Position:
02h21m02.33s -03d25m07.0s
(35.25969°, -3.41862°)
EP flux
5.79e-14
± 1.5e-14
erg cm-2 s-1
CLASSX
AGN
(0.942)
Detections
2
| SRCID | 3003798260102105 |
|---|---|
| IAUNAME | 5XMM J022102.3-032507 |
| SC_RA | 02h21m02.33s (35.25969°) |
| SC_DEC | -03d25m07.0s (-3.41862°) |
| RADEC_ERR | 0.67 arcsec |
| LII / BII | 168.8998° / -58.0554° |
| N_CONTRIB | 2 (detections) |
| N_OBS | 372 (observations covering the position) |
| MJD_FIRST | 52501.025 (2002-08-15 00:36:35.000 UTC) |
| MJD_LAST | 52501.440 (2002-08-15 10:33:08.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 5.79e-14 ± 1.5e-14 erg cm-2 s-1
Hardness ratios
HR1
0.47
± 0.14
0.2-0.5 / 0.5-1.0 keV
HR2
0.09
± 0.14
0.5-1.0 / 1.0-2.0 keV
HR3
-0.34
± 0.13
1.0-2.0 / 2.0-4.5 keV
HR4
-0.40
± 0.27
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -2.4)
SUM_FLAG:
1
Long-term lightcurve
No light-curve points available.
AGN
CLASSX outlier: -0.301
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
- 784999
- Match probability
- 0.838
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | 22.155 | 0.153 |
| U | — | — |
| B | — | — |
| V | — | — |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 3.87e-14 (+4.7e-14 / −3.1e-14) erg cm−2 s−1 |
|---|---|
| NH | 7.81e+19 (+3.6e+20 / −1.8e+19) cm−2 |
| Photon index (Γ) | 1.61 (+1.81 / −1.44) |
| DoF | 139 |
| p-value | 0.838 |
| Inter-instrument norm. | 1.27 (1.00–1.56) |
| 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.