5XMM J105410.4+573039
5XMM-DR15 stacked source · SRCID 3002274010100018
Position:
10h54m10.44s +57d30m39.7s
(163.54351°, 57.51104°)
EP flux
3.02e-14
± 1.2e-15
erg cm-2 s-1
CLASSX
Gal_XRB
(0.495)
Detections
14
| SRCID | 3002274010100018 |
|---|---|
| IAUNAME | 5XMM J105410.4+573039 |
| SC_RA | 10h54m10.44s (163.54351°) |
| SC_DEC | +57d30m39.7s (57.51104°) |
| RADEC_ERR | 0.13 arcsec |
| LII / BII | 149.0193° / 53.2682° |
| N_CONTRIB | 14 (detections) |
| N_OBS | 21 (observations covering the position) |
| MJD_FIRST | 51661.158 (2000-04-27 03:47:47.000 UTC) |
| MJD_LAST | 52615.196 (2002-12-07 04:41:59.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 3.02e-14 ± 1.2e-15 erg cm-2 s-1
Hardness ratios
HR1
0.35
± 0.02
0.2-0.5 / 0.5-1.0 keV
HR2
-0.30
± 0.02
0.5-1.0 / 1.0-2.0 keV
HR3
-0.64
± 0.03
1.0-2.0 / 2.0-4.5 keV
HR4
-0.84
± 0.10
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML 264.2)
SUM_FLAG:
1
Long-term lightcurve
No light-curve points available.
Gal_XRB
CLASSX outlier: 1.14
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
- 2963178
- Match probability
- 0.89
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | 22.555 | 0.472 |
| UVM2 | — | — |
| UVW1 | 21.438 | 0.060 |
| U | 20.312 | 0.040 |
| B | 18.264 | 0.011 |
| V | — | — |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 3.54e-14 (+3.8e-14 / −3.3e-14) erg cm−2 s−1 |
|---|---|
| NH | 1.37e+21 (+1.5e+21 / −1.1e+21) cm−2 |
| Photon index (Γ) | 2.88 (+2.97 / −2.72) |
| DoF | 2308 |
| p-value | 0.032 |
| Inter-instrument norm. | 0.71 (0.65–0.77) |
| 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.