5XMM J172904.9+742601
5XMM-DR15 stacked source · SRCID 3001415040100005
Position:
17h29m04.97s +74d26m01.3s
(262.27070°, 74.43369°)
EP flux
1.27e-13
± 2.5e-14
erg cm-2 s-1
CLASSX
Bkg_AGN
(0.378)
Detections
1
| SRCID | 3001415040100005 |
|---|---|
| IAUNAME | 5XMM J172904.9+742601 |
| SC_RA | 17h29m04.97s (262.27070°) |
| SC_DEC | +74d26m01.3s (74.43369°) |
| RADEC_ERR | 0.72 arcsec |
| LII / BII | 105.7871° / 31.5502° |
| N_CONTRIB | 1 (detections) |
| N_OBS | 1 (observations covering the position) |
| MJD_FIRST | 52429.642 (2002-06-04 15:23:49.000 UTC) |
| MJD_LAST | 52429.784 (2002-06-04 18:48:28.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 1.27e-13 ± 2.5e-14 erg cm-2 s-1
Hardness ratios
HR1
0.42
± 0.09
0.2-0.5 / 0.5-1.0 keV
HR2
-0.38
± 0.09
0.5-1.0 / 1.0-2.0 keV
HR3
-0.51
± 0.14
1.0-2.0 / 2.0-4.5 keV
HR4
-0.58
± 0.35
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -2.0)
SUM_FLAG:
0
Long-term lightcurve
No light-curve points available.
Bkg_AGN
CLASSX outlier: 4.12
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
- 4678712
- Match probability
- 0.994
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | 20.447 | 0.146 |
| U | — | — |
| B | — | — |
| V | — | — |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 1.39e-13 (+1.8e-13 / −1.1e-13) erg cm−2 s−1 |
|---|---|
| NH | 8.81e+19 (+4.5e+20 / −2.1e+19) cm−2 |
| Photon index (Γ) | 1.97 (+2.27 / −1.71) |
| DoF | 315 |
| p-value | 0.921 |
| 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.