5XMM J072009.9+711258
5XMM-DR15 stacked source · SRCID 3001285010100017
Position:
07h20m09.97s +71d12m58.5s
(110.04153°, 71.21626°)
EP flux
2.65e-14
± 5.3e-15
erg cm-2 s-1
CLASSX
AGN
(0.743)
Detections
5
| SRCID | 3001285010100017 |
|---|---|
| IAUNAME | 5XMM J072009.9+711258 |
| SC_RA | 07h20m09.97s (110.04153°) |
| SC_DEC | +71d12m58.5s (71.21626°) |
| RADEC_ERR | 0.46 arcsec |
| LII / BII | 144.1182° / 27.8739° |
| N_CONTRIB | 5 (detections) |
| N_OBS | 5 (observations covering the position) |
| MJD_FIRST | 52012.712 (2001-04-13 17:05:43.000 UTC) |
| MJD_LAST | 54368.538 (2007-09-25 12:54:08.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 2.65e-14 ± 5.3e-15 erg cm-2 s-1
Hardness ratios
HR1
0.04
± 0.09
0.2-0.5 / 0.5-1.0 keV
HR2
-0.00
± 0.09
0.5-1.0 / 1.0-2.0 keV
HR3
-0.29
± 0.11
1.0-2.0 / 2.0-4.5 keV
HR4
-0.55
± 0.22
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -2.6)
SUM_FLAG:
0
Long-term lightcurve
No light-curve points available.
AGN
CLASSX outlier: 1.25
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
- 2356169
- Match probability
- 0.997
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | — | — |
| U | 21.491 | 0.095 |
| B | — | — |
| V | — | — |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 2.80e-14 (+3.4e-14 / −2.2e-14) erg cm−2 s−1 |
|---|---|
| NH | 7.12e+19 (+3.0e+20 / −1.8e+19) cm−2 |
| Photon index (Γ) | 2.20 (+2.45 / −1.99) |
| DoF | 589 |
| p-value | 0.157 |
| Inter-instrument norm. | 1.71 (1.42–1.91) |
| 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.