5XMM J173036.9+742235
5XMM-DR15 stacked source · SRCID 3001415040100002
Position:
17h30m36.92s +74d22m35.4s
(262.65383°, 74.37650°)
EP flux
3.26e-13
± 2.4e-14
erg cm-2 s-1
CLASSX
Extended
(0.995)
Detections
1
| SRCID | 3001415040100002 |
|---|---|
| IAUNAME | 5XMM J173036.9+742235 |
| SC_RA | 17h30m36.92s (262.65383°) |
| SC_DEC | +74d22m35.4s (74.37650°) |
| RADEC_ERR | 0.93 arcsec |
| LII / BII | 105.6965° / 31.4613° |
| 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): 3.26e-13 ± 2.4e-14 erg cm-2 s-1
Hardness ratios
HR1
0.75
± 0.04
0.2-0.5 / 0.5-1.0 keV
HR2
-0.40
± 0.05
0.5-1.0 / 1.0-2.0 keV
HR3
-0.67
± 0.08
1.0-2.0 / 2.0-4.5 keV
HR4
-0.97
± 0.11
2.0-4.5 / 4.5-12.0 keV
Extent:
7.61
± 0.68
arcsec
(ML 79.2)
SUM_FLAG:
1
Long-term lightcurve
No light-curve points available.
Extended
CLASSX outlier: 3.26
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
- 4685415
- Match probability
- 0.992
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | 19.090 | 0.069 |
| U | — | — |
| B | — | — |
| V | — | — |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 2.08e-13 (+2.2e-13 / −1.9e-13) erg cm−2 s−1 |
|---|---|
| NH | 2.04e+21 (+2.3e+21 / −1.8e+21) cm−2 |
| Photon index (Γ) | 2.95 (+2.99 / −2.87) |
| DoF | 315 |
| p-value | 0.001 |
| Quality flag | 7 |
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.