5XMM J084855.3+741035
5XMM-DR15 stacked source · SRCID 3002554040100006
Position:
08h48m55.34s +74d10m35.1s
(132.23057°, 74.17642°)
EP flux
8.68e-14
± 2.1e-14
erg cm-2 s-1
CLASSX
AGN
(0.954)
Detections
3
| SRCID | 3002554040100006 |
|---|---|
| IAUNAME | 5XMM J084855.3+741035 |
| SC_RA | 08h48m55.34s (132.23057°) |
| SC_DEC | +74d10m35.1s (74.17642°) |
| RADEC_ERR | 0.70 arcsec |
| LII / BII | 139.5679° / 33.8989° |
| 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): 8.68e-14 ± 2.1e-14 erg cm-2 s-1
Hardness ratios
HR1
0.18
± 0.14
0.2-0.5 / 0.5-1.0 keV
HR2
0.40
± 0.09
0.5-1.0 / 1.0-2.0 keV
HR3
-0.34
± 0.10
1.0-2.0 / 2.0-4.5 keV
HR4
-0.40
± 0.23
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -2.2)
SUM_FLAG:
1
Long-term lightcurve
No light-curve points available.
AGN
CLASSX outlier: -0.0038
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
- 2640325
- Match probability
- 0.997
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | — | — |
| U | 21.533 | 0.098 |
| B | — | — |
| V | — | — |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 5.43e-14 (+7.3e-14 / −4.1e-14) erg cm−2 s−1 |
|---|---|
| NH | 3.01e+20 (+1.9e+21 / −2.8e+19) cm−2 |
| Photon index (Γ) | 1.43 (+1.92 / −1.15) |
| DoF | 54 |
| p-value | 0.944 |
| 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.