5XMM J184500.5+005332
5XMM-DR15 stacked source · SRCID 3001774020100019
Position:
18h45m00.57s +00d53m32.6s
(281.25235°, 0.89239°)
EP flux
1.10e-14
± 5.8e-15
erg cm-2 s-1
CLASSX
Star
(0.837)
Detections
3
| SRCID | 3001774020100019 |
|---|---|
| IAUNAME | 5XMM J184500.5+005332 |
| SC_RA | 18h45m00.57s (281.25235°) |
| SC_DEC | +00d53m32.6s (0.89239°) |
| RADEC_ERR | 1.06 arcsec |
| LII / BII | 32.9935° / 1.8372° |
| N_CONTRIB | 3 (detections) |
| N_OBS | 3 (observations covering the position) |
| MJD_FIRST | 52921.032 (2003-10-09 00:45:48.000 UTC) |
| MJD_LAST | 52925.324 (2003-10-13 07:46:48.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 1.10e-14 ± 5.8e-15 erg cm-2 s-1
Hardness ratios
HR1
0.92
± 0.11
0.2-0.5 / 0.5-1.0 keV
HR2
-0.16
± 0.13
0.5-1.0 / 1.0-2.0 keV
HR3
-0.58
± 0.20
1.0-2.0 / 2.0-4.5 keV
HR4
0.12
± 0.54
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML 5.5)
SUM_FLAG:
1
Long-term lightcurve
No light-curve points available.
Star
CLASSX outlier: 6.03
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
- 5635966
- Match probability
- 0.956
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | — | — |
| U | — | — |
| B | — | — |
| V | 18.647 | 0.023 |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 1.60e-14 (+2.2e-14 / −1.2e-14) erg cm−2 s−1 |
|---|---|
| NH | 2.72e+21 (+4.3e+21 / −8.0e+20) cm−2 |
| Photon index (Γ) | 2.32 (+2.82 / −1.65) |
| DoF | 146 |
| p-value | 0.817 |
| 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.