5XMM J074032.3+702222
5XMM-DR15 stacked source · SRCID 3002854020100001
Position:
07h40m32.37s +70d22m22.1s
(115.13486°, 70.37281°)
EP flux
1.22e-13
± 7.9e-15
erg cm-2 s-1
CLASSX
AGN
(0.639)
Detections
3
| SRCID | 3002854020100001 |
|---|---|
| IAUNAME | 5XMM J074032.3+702222 |
| SC_RA | 07h40m32.37s (115.13486°) |
| SC_DEC | +70d22m22.1s (70.37281°) |
| RADEC_ERR | 0.21 arcsec |
| LII / BII | 145.0961° / 29.5412° |
| N_CONTRIB | 3 (detections) |
| N_OBS | 3 (observations covering the position) |
| MJD_FIRST | 52171.579 (2001-09-19 13:53:26.000 UTC) |
| MJD_LAST | 52578.796 (2002-10-31 19:06:04.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 1.22e-13 ± 7.9e-15 erg cm-2 s-1
Hardness ratios
HR1
0.16
± 0.04
0.2-0.5 / 0.5-1.0 keV
HR2
0.08
± 0.03
0.5-1.0 / 1.0-2.0 keV
HR3
-0.38
± 0.04
1.0-2.0 / 2.0-4.5 keV
HR4
-0.49
± 0.07
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -3.8)
SUM_FLAG:
1
Long-term lightcurve
No light-curve points available.
AGN
CLASSX outlier: -0.47
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
- 2408109
- Match probability
- 0.956
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | 21.334 | 0.064 |
| U | — | — |
| B | — | — |
| V | 20.055 | 0.153 |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 1.22e-13 (+1.3e-13 / −1.1e-13) erg cm−2 s−1 |
|---|---|
| NH | 7.28e+19 (+3.1e+20 / −2.2e+19) cm−2 |
| Photon index (Γ) | 1.93 (+2.07 / −1.83) |
| DoF | 262 |
| p-value | 0.972 |
| 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.