5XMM J084830.5+740153
5XMM-DR15 stacked source · SRCID 3002554040100002
Position:
08h48m30.51s +74d01m53.7s
(132.12713°, 74.03158°)
EP flux
6.60e-14
± 6.6e-15
erg cm-2 s-1
CLASSX
AGN
(0.871)
Detections
3
| SRCID | 3002554040100002 |
|---|---|
| IAUNAME | 5XMM J084830.5+740153 |
| SC_RA | 08h48m30.51s (132.12713°) |
| SC_DEC | +74d01m53.7s (74.03158°) |
| RADEC_ERR | 0.36 arcsec |
| LII / BII | 139.7432° / 33.9238° |
| 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): 6.60e-14 ± 6.6e-15 erg cm-2 s-1
Hardness ratios
HR1
-0.09
± 0.06
0.2-0.5 / 0.5-1.0 keV
HR2
-0.06
± 0.06
0.5-1.0 / 1.0-2.0 keV
HR3
-0.61
± 0.08
1.0-2.0 / 2.0-4.5 keV
HR4
-0.72
± 0.20
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -3.1)
SUM_FLAG:
0
Long-term lightcurve
No light-curve points available.
AGN
CLASSX outlier: 0.214
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
- 2635358
- Match probability
- 0.999
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | — | — |
| U | 20.209 | 0.057 |
| B | — | — |
| V | — | — |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 5.02e-14 (+5.6e-14 / −4.5e-14) erg cm−2 s−1 |
|---|---|
| NH | 5.03e+19 (+1.8e+20 / −1.6e+19) cm−2 |
| Photon index (Γ) | 2.35 (+2.51 / −2.23) |
| DoF | 296 |
| p-value | 0.361 |
| Inter-instrument norm. | 1.87 (1.72–1.96) |
| Quality flag | 0 |
| APPROX_SOURCE_VAR | 6.400 (approximate flux variability amplitude) |
|---|
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.