5XMM J005802.1-721902
5XMM-DR15 stacked source · SRCID 3001854010101309
Position:
00h58m02.19s -72d19m02.0s
(14.50913°, -72.31723°)
EP flux
1.23e-15
± 3.9e-16
erg cm-2 s-1
CLASSX
Bkg_AGN
(0.582)
Detections
20
| SRCID | 3001854010101309 |
|---|---|
| IAUNAME | 5XMM J005802.1-721902 |
| SC_RA | 00h58m02.19s (14.50913°) |
| SC_DEC | -72d19m02.0s (-72.31723°) |
| RADEC_ERR | 1.33 arcsec |
| LII / BII | 302.2258° / -44.8020° |
| N_CONTRIB | 20 (detections) |
| N_OBS | 182 (observations covering the position) |
| MJD_FIRST | 51834.632 (2000-10-17 15:10:35.000 UTC) |
| MJD_LAST | 58925.579 (2020-03-17 13:54:08.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 1.23e-15 ± 3.9e-16 erg cm-2 s-1
Hardness ratios
HR1
0.33
± 0.11
0.2-0.5 / 0.5-1.0 keV
HR2
-0.45
± 0.12
0.5-1.0 / 1.0-2.0 keV
HR3
-0.87
± 0.22
1.0-2.0 / 2.0-4.5 keV
HR4
-0.92
± 3.34
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -0.2)
SUM_FLAG:
0
Long-term lightcurve
No light-curve points available.
Bkg_AGN
CLASSX outlier: 4.44
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
- 371787
- Match probability
- 0.704
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | 19.425 | 0.092 |
| U | 19.359 | 0.065 |
| B | — | — |
| V | — | — |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 2.68e-15 (+3.4e-15 / −2.0e-15) erg cm−2 s−1 |
|---|---|
| NH | 5.01e+19 (+2.2e+20 / −1.6e+19) cm−2 |
| Photon index (Γ) | 2.71 (+2.92 / −2.39) |
| DoF | 644 |
| p-value | 0.541 |
| 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.