5XMM J084652.4+740754
5XMM-DR15 stacked source · SRCID 3002554040100007
Position:
08h46m52.44s +74d07m54.6s
(131.71850°, 74.13182°)
EP flux
2.32e-14
± 6.8e-15
erg cm-2 s-1
CLASSX
Extragal_XRB
(0.491)
Detections
3
| SRCID | 3002554040100007 |
|---|---|
| IAUNAME | 5XMM J084652.4+740754 |
| SC_RA | 08h46m52.44s (131.71850°) |
| SC_DEC | +74d07m54.6s (74.13182°) |
| RADEC_ERR | 0.73 arcsec |
| LII / BII | 139.6773° / 33.7837° |
| N_CONTRIB | 3 (detections) |
| N_OBS | 3 (observations covering the position) |
| MJD_FIRST | 52171.074 (2001-09-19 01:46:16.000 UTC) |
| MJD_LAST | 52352.738 (2002-03-19 17:43:09.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 2.32e-14 ± 6.8e-15 erg cm-2 s-1
Hardness ratios
HR1
0.57
± 0.12
0.2-0.5 / 0.5-1.0 keV
HR2
-0.14
± 0.11
0.5-1.0 / 1.0-2.0 keV
HR3
-0.86
± 0.13
1.0-2.0 / 2.0-4.5 keV
HR4
0.68
± 0.50
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -2.3)
SUM_FLAG:
1
Long-term lightcurve
No light-curve points available.
Extragal_XRB
CLASSX outlier: 3.94
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
- 2627343
- Match probability
- 0.997
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | — | — |
| U | 21.551 | 0.100 |
| B | — | — |
| V | — | — |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 4.37e-14 (+5.3e-14 / −3.7e-14) erg cm−2 s−1 |
|---|---|
| NH | 4.50e+20 (+1.2e+21 / −3.9e+19) cm−2 |
| Photon index (Γ) | 2.62 (+2.89 / −2.34) |
| DoF | 71 |
| p-value | 0.199 |
| 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.