5XMM J153244.0+324245
5XMM-DR15 stacked source · SRCID 3003914010100015
Position:
15h32m44.03s +32d42m45.8s
(233.18344°, 32.71273°)
EP flux
3.52e-14
± 5.1e-15
erg cm-2 s-1
CLASSX
Bkg_AGN
(0.515)
Detections
3
| SRCID | 3003914010100015 |
|---|---|
| IAUNAME | 5XMM J153244.0+324245 |
| SC_RA | 15h32m44.03s (233.18344°) |
| SC_DEC | +32d42m45.8s (32.71273°) |
| RADEC_ERR | 0.75 arcsec |
| LII / BII | 52.0255° / 54.8185° |
| N_CONTRIB | 3 (detections) |
| N_OBS | 4 (observations covering the position) |
| MJD_FIRST | 52485.506 (2002-07-30 12:08:00.000 UTC) |
| MJD_LAST | 53369.317 (2004-12-30 07:36:59.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 3.52e-14 ± 5.1e-15 erg cm-2 s-1
Hardness ratios
HR1
-0.09
± 0.09
0.2-0.5 / 0.5-1.0 keV
HR2
0.05
± 0.09
0.5-1.0 / 1.0-2.0 keV
HR3
-0.38
± 0.10
1.0-2.0 / 2.0-4.5 keV
HR4
-0.35
± 0.17
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML 26.5)
SUM_FLAG:
1
Long-term lightcurve
No light-curve points available.
Bkg_AGN
CLASSX outlier: 2.18
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
- 3936537
- Match probability
- 0.999
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | 20.713 | 0.173 |
| UVM2 | 20.254 | 0.084 |
| UVW1 | 20.276 | 0.066 |
| U | 20.314 | 0.080 |
| B | 20.212 | 0.122 |
| V | — | — |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 3.04e-14 (+3.9e-14 / −2.4e-14) erg cm−2 s−1 |
|---|---|
| NH | 4.25e+19 (+1.6e+20 / −1.6e+19) cm−2 |
| Photon index (Γ) | 1.89 (+2.10 / −1.70) |
| DoF | 974 |
| p-value | 0.103 |
| Inter-instrument norm. | 1.31 (1.09–1.60) |
| 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.