5XMM J072315.3+711656
5XMM-DR15 stacked source · SRCID 3001285010100038
Position:
07h23m15.37s +71d16m56.0s
(110.81405°, 71.28223°)
EP flux
1.10e-14
± 4.0e-15
erg cm-2 s-1
CLASSX
AGN
(0.931)
Detections
5
| SRCID | 3001285010100038 |
|---|---|
| IAUNAME | 5XMM J072315.3+711656 |
| SC_RA | 07h23m15.37s (110.81405°) |
| SC_DEC | +71d16m56.0s (71.28223°) |
| RADEC_ERR | 0.92 arcsec |
| LII / BII | 144.0548° / 28.1246° |
| 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): 1.10e-14 ± 4.0e-15 erg cm-2 s-1
Hardness ratios
HR1
-0.12
± 0.19
0.2-0.5 / 0.5-1.0 keV
HR2
0.46
± 0.14
0.5-1.0 / 1.0-2.0 keV
HR3
-0.39
± 0.15
1.0-2.0 / 2.0-4.5 keV
HR4
-0.42
± 0.34
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -1.8)
SUM_FLAG:
1
Long-term lightcurve
No light-curve points available.
AGN
CLASSX outlier: -0.602
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
- 2367728
- Match probability
- 0.98
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | — | — |
| U | 21.946 | 0.255 |
| B | — | — |
| V | 21.110 | 0.258 |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 3.20e-14 (+4.1e-14 / −2.2e-14) erg cm−2 s−1 |
|---|---|
| NH | 5.27e+20 (+2.2e+21 / −4.1e+19) cm−2 |
| Photon index (Γ) | 1.42 (+1.93 / −1.15) |
| DoF | 213 |
| p-value | 0.555 |
| 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.