5XMM J000302.7-295423
5XMM-DR15 stacked source · SRCID 3004175010100012
Position:
00h03m02.74s -29d54m23.5s
(0.76143°, -29.90652°)
EP flux
4.33e-14
± 3.9e-15
erg cm-2 s-1
CLASSX
AGN
(0.961)
Detections
1
| SRCID | 3004175010100012 |
|---|---|
| IAUNAME | 5XMM J000302.7-295423 |
| SC_RA | 00h03m02.74s (0.76143°) |
| SC_DEC | -29d54m23.5s (-29.90652°) |
| RADEC_ERR | 0.30 arcsec |
| LII / BII | 15.4414° / -79.0190° |
| 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): 4.33e-14 ± 3.9e-15 erg cm-2 s-1
Hardness ratios
HR1
-0.05
± 0.05
0.2-0.5 / 0.5-1.0 keV
HR2
0.05
± 0.05
0.5-1.0 / 1.0-2.0 keV
HR3
-0.53
± 0.05
1.0-2.0 / 2.0-4.5 keV
HR4
-0.54
± 0.13
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -3.3)
SUM_FLAG:
0
Long-term lightcurve
No light-curve points available.
AGN
CLASSX outlier: 0.426
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
- 9059
- Match probability
- 0.989
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | — | — |
| U | 21.277 | 0.057 |
| B | — | — |
| V | 20.384 | 0.099 |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 3.41e-14 (+3.7e-14 / −3.1e-14) erg cm−2 s−1 |
|---|---|
| NH | 4.96e+19 (+1.5e+20 / −1.5e+19) cm−2 |
| Photon index (Γ) | 2.04 (+2.13 / −1.97) |
| DoF | 482 |
| p-value | 0.861 |
| Inter-instrument norm. | 1.05 (0.94–1.16) |
| 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.