5XMM J193540.2-525144
5XMM-DR15 stacked source · SRCID 3005161010100013
Position:
19h35m40.20s -52d51m44.3s
(293.91750°, -52.86231°)
EP flux
1.57e-14
± 5.9e-15
erg cm-2 s-1
CLASSX
Star
(0.997)
Detections
1
| SRCID | 3005161010100013 |
|---|---|
| IAUNAME | 5XMM J193540.2-525144 |
| SC_RA | 19h35m40.20s (293.91750°) |
| SC_DEC | -52d51m44.3s (-52.86231°) |
| RADEC_ERR | 1.07 arcsec |
| LII / BII | 344.9917° / -27.8114° |
| N_CONTRIB | 1 (detections) |
| N_OBS | 1 (observations covering the position) |
| MJD_FIRST | 52361.583 (2002-03-28 13:59:56.000 UTC) |
| MJD_LAST | 52361.838 (2002-03-28 20:07:09.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 1.57e-14 ± 5.9e-15 erg cm-2 s-1
Hardness ratios
HR1
0.89
± 0.11
0.2-0.5 / 0.5-1.0 keV
HR2
-0.42
± 0.13
0.5-1.0 / 1.0-2.0 keV
HR3
-0.82
± 0.19
1.0-2.0 / 2.0-4.5 keV
HR4
0.34
± 0.54
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -1.7)
SUM_FLAG:
0
Long-term lightcurve
No light-curve points available.
Star
CLASSX outlier: 2.38
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
- 5965199
- Match probability
- 0.997
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | 18.668 | 0.075 |
| UVM2 | — | — |
| UVW1 | — | — |
| U | — | — |
| B | — | — |
| V | — | — |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 1.28e-14 (+1.7e-14 / −9.5e-15) erg cm−2 s−1 |
|---|---|
| NH | 6.52e+20 (+1.5e+21 / −6.8e+19) cm−2 |
| Photon index (Γ) | 2.43 (+2.82 / −1.98) |
| DoF | 352 |
| p-value | 0.357 |
| 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.