5XMM J000319.2-300217
5XMM-DR15 stacked source · SRCID 3004175010100029
Position:
00h03m19.25s -30d02m17.8s
(0.83019°, -30.03827°)
EP flux
3.96e-14
± 5.9e-15
erg cm-2 s-1
CLASSX
AGN
(0.889)
Detections
1
| SRCID | 3004175010100029 |
|---|---|
| IAUNAME | 5XMM J000319.2-300217 |
| SC_RA | 00h03m19.25s (0.83019°) |
| SC_DEC | -30d02m17.8s (-30.03827°) |
| RADEC_ERR | 0.45 arcsec |
| LII / BII | 14.6986° / -79.0497° |
| 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): 3.96e-14 ± 5.9e-15 erg cm-2 s-1
Hardness ratios
HR1
0.27
± 0.07
0.2-0.5 / 0.5-1.0 keV
HR2
-0.07
± 0.07
0.5-1.0 / 1.0-2.0 keV
HR3
-0.39
± 0.08
1.0-2.0 / 2.0-4.5 keV
HR4
-0.13
± 0.16
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -2.8)
SUM_FLAG:
0
Long-term lightcurve
No light-curve points available.
AGN
CLASSX outlier: -0.186
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
- 9701
- Match probability
- 0.992
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | — | — |
| U | 22.585 | 0.172 |
| B | — | — |
| V | 21.340 | 0.331 |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 2.66e-14 (+3.0e-14 / −2.4e-14) erg cm−2 s−1 |
|---|---|
| NH | 7.35e+19 (+2.8e+20 / −1.8e+19) cm−2 |
| Photon index (Γ) | 1.75 (+1.88 / −1.65) |
| DoF | 579 |
| p-value | 0.895 |
| Inter-instrument norm. | 0.90 (0.77–1.05) |
| 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.