5XMM J000305.5-295200
5XMM-DR15 stacked source · SRCID 3004175010100074
Position:
00h03m05.59s -29d52m00.5s
(0.77331°, -29.86679°)
EP flux
1.01e-14
± 3.2e-15
erg cm-2 s-1
CLASSX
Bkg_AGN
(0.97)
Detections
1
| SRCID | 3004175010100074 |
|---|---|
| IAUNAME | 5XMM J000305.5-295200 |
| SC_RA | 00h03m05.59s (0.77331°) |
| SC_DEC | -29d52m00.5s (-29.86679°) |
| RADEC_ERR | 0.83 arcsec |
| LII / BII | 15.6349° / -79.0371° |
| 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): 1.01e-14 ± 3.2e-15 erg cm-2 s-1
Hardness ratios
HR1
0.57
± 0.09
0.2-0.5 / 0.5-1.0 keV
HR2
-0.36
± 0.09
0.5-1.0 / 1.0-2.0 keV
HR3
-0.55
± 0.14
1.0-2.0 / 2.0-4.5 keV
HR4
-0.63
± 0.53
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML 1.9)
SUM_FLAG:
0
Long-term lightcurve
No light-curve points available.
Bkg_AGN
CLASSX outlier: 4.03
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
- 9190
- Match probability
- 0.919
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | — | — |
| U | 18.210 | 0.012 |
| B | — | — |
| V | 15.427 | 0.005 |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 6.28e-15 (+7.7e-15 / −5.0e-15) erg cm−2 s−1 |
|---|---|
| NH | 1.87e+20 (+6.7e+20 / −2.5e+19) cm−2 |
| Photon index (Γ) | 2.53 (+2.82 / −2.25) |
| DoF | 109 |
| p-value | 0.039 |
| 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.