5XMM J000221.5-300646
5XMM-DR15 stacked source · SRCID 3004175010100083
Position:
00h02m21.52s -30d06m46.7s
(0.58966°, -30.11296°)
EP flux
1.34e-14
± 3.4e-15
erg cm-2 s-1
CLASSX
AGN
(0.933)
Detections
1
| SRCID | 3004175010100083 |
|---|---|
| IAUNAME | 5XMM J000221.5-300646 |
| SC_RA | 00h02m21.52s (0.58966°) |
| SC_DEC | -30d06m46.7s (-30.11296°) |
| RADEC_ERR | 0.80 arcsec |
| LII / BII | 14.5527° / -78.8303° |
| N_CONTRIB | 1 (detections) |
| N_OBS | 1 (observations covering the position) |
| MJD_FIRST | 52440.823 (2002-06-15 19:44:59.000 UTC) |
| MJD_LAST | 52441.421 (2002-06-16 10:06:17.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 1.34e-14 ± 3.4e-15 erg cm-2 s-1
Hardness ratios
HR1
-0.09
± 0.20
0.2-0.5 / 0.5-1.0 keV
HR2
0.47
± 0.14
0.5-1.0 / 1.0-2.0 keV
HR3
-0.10
± 0.12
1.0-2.0 / 2.0-4.5 keV
HR4
-0.61
± 0.18
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -2.0)
SUM_FLAG:
0
Long-term lightcurve
No light-curve points available.
AGN
CLASSX outlier: -0.242
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
- 7652
- Match probability
- 0.975
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | — | — |
| U | 20.940 | 0.107 |
| B | — | — |
| V | 20.280 | 0.131 |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 1.64e-14 (+2.1e-14 / −1.3e-14) erg cm−2 s−1 |
|---|---|
| NH | 1.19e+21 (+3.3e+21 / −1.1e+20) cm−2 |
| Photon index (Γ) | 1.55 (+2.07 / −1.24) |
| DoF | 86 |
| p-value | 0.423 |
| 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.