5XMM J021432.5-734612
5XMM-DR15 stacked source · SRCID 3004915010100059
Position:
02h14m32.57s -73d46m12.5s
(33.63569°, -73.77014°)
EP flux
2.54e-14
± 5.8e-15
erg cm-2 s-1
CLASSX
AGN
(0.943)
Detections
5
| SRCID | 3004915010100059 |
|---|---|
| IAUNAME | 5XMM J021432.5-734612 |
| SC_RA | 02h14m32.57s (33.63569°) |
| SC_DEC | -73d46m12.5s (-73.77014°) |
| RADEC_ERR | 0.68 arcsec |
| LII / BII | 295.2537° / -42.0965° |
| N_CONTRIB | 5 (detections) |
| N_OBS | 9 (observations covering the position) |
| MJD_FIRST | 51730.634 (2000-07-05 15:13:30.000 UTC) |
| MJD_LAST | 53386.433 (2005-01-16 10:23:46.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 2.54e-14 ± 5.8e-15 erg cm-2 s-1
Hardness ratios
HR1
0.54
± 0.10
0.2-0.5 / 0.5-1.0 keV
HR2
0.05
± 0.09
0.5-1.0 / 1.0-2.0 keV
HR3
-0.37
± 0.10
1.0-2.0 / 2.0-4.5 keV
HR4
-0.03
± 0.21
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -2.0)
SUM_FLAG:
2
Long-term lightcurve
No light-curve points available.
AGN
CLASSX outlier: -0.411
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
- 752444
- Match probability
- 0.988
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | 22.287 | 0.158 |
| U | 21.592 | 0.100 |
| B | — | — |
| V | — | — |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 1.79e-14 (+2.6e-14 / −1.3e-14) erg cm−2 s−1 |
|---|---|
| NH | 1.30e+20 (+9.3e+20 / −2.3e+19) cm−2 |
| Photon index (Γ) | 1.58 (+1.98 / −1.24) |
| DoF | 54 |
| p-value | 0.588 |
| 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.