5XMM J021645.0-740556
5XMM-DR15 stacked source · SRCID 3004915010100067
Position:
02h16m45.07s -74d05m56.0s
(34.18780°, -74.09889°)
EP flux
7.88e-15
± 3.2e-15
erg cm-2 s-1
CLASSX
Star
(1)
Detections
6
| SRCID | 3004915010100067 |
|---|---|
| IAUNAME | 5XMM J021645.0-740556 |
| SC_RA | 02h16m45.07s (34.18780°) |
| SC_DEC | -74d05m56.0s (-74.09889°) |
| RADEC_ERR | 0.66 arcsec |
| LII / BII | 295.2581° / -41.7340° |
| N_CONTRIB | 6 (detections) |
| N_OBS | 9 (observations covering the position) |
| MJD_FIRST | 51730.634 (2000-07-05 15:13:30.000 UTC) |
| MJD_LAST | 53386.433 (2005-01-16 10:23:46.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 7.88e-15 ± 3.2e-15 erg cm-2 s-1
Hardness ratios
HR1
0.59
± 0.08
0.2-0.5 / 0.5-1.0 keV
HR2
-0.51
± 0.09
0.5-1.0 / 1.0-2.0 keV
HR3
-0.92
± 0.20
1.0-2.0 / 2.0-4.5 keV
HR4
0.15
± 1.08
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -2.4)
SUM_FLAG:
2
Long-term lightcurve
No light-curve points available.
Star
CLASSX outlier: 2.41
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
- 760415
- Match probability
- 0.992
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | 20.589 | 0.064 |
| U | — | — |
| B | — | — |
| V | — | — |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 1.46e-14 (+2.0e-14 / −1.1e-14) erg cm−2 s−1 |
|---|---|
| NH | 6.86e+20 (+1.7e+21 / −7.3e+19) cm−2 |
| Photon index (Γ) | 2.43 (+2.84 / −1.96) |
| DoF | 78 |
| p-value | 0.223 |
| 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.