5XMM J031757.2-030421
5XMM-DR15 stacked source · SRCID 3005602220100014
Position:
03h17m57.20s -03d04m21.8s
(49.48833°, -3.07271°)
EP flux
1.77e-14
± 8.0e-15
erg cm-2 s-1
CLASSX
Star
(0.84)
Detections
1
| SRCID | 3005602220100014 |
|---|---|
| IAUNAME | 5XMM J031757.2-030421 |
| SC_RA | 03h17m57.20s (49.48833°) |
| SC_DEC | -03d04m21.8s (-3.07271°) |
| RADEC_ERR | 1.12 arcsec |
| LII / BII | 184.8626° / -47.5313° |
| N_CONTRIB | 1 (detections) |
| N_OBS | 1 (observations covering the position) |
| MJD_FIRST | 52503.423 (2002-08-17 10:08:51.000 UTC) |
| MJD_LAST | 52503.706 (2002-08-17 16:56:53.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 1.77e-14 ± 8.0e-15 erg cm-2 s-1
Hardness ratios
HR1
0.45
± 0.11
0.2-0.5 / 0.5-1.0 keV
HR2
-0.58
± 0.11
0.5-1.0 / 1.0-2.0 keV
HR3
-0.97
± 0.13
1.0-2.0 / 2.0-4.5 keV
HR4
-1.00
± 9.75
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML 3.8)
SUM_FLAG:
0
Long-term lightcurve
No light-curve points available.
Star
CLASSX outlier: 4.89
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
- 925854
- Match probability
- 0.982
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | 22.418 | 0.227 |
| U | — | — |
| B | — | — |
| V | — | — |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 1.94e-14 (+2.4e-14 / −1.6e-14) erg cm−2 s−1 |
|---|---|
| NH | 1.92e+20 (+6.8e+20 / −2.4e+19) cm−2 |
| Photon index (Γ) | 2.59 (+2.85 / −2.32) |
| DoF | 292 |
| p-value | 0.901 |
| Inter-instrument norm. | 0.91 (0.67–1.18) |
| Quality flag | 0 |
| APPROX_SOURCE_VAR | 5.300 (approximate flux variability amplitude) |
|---|
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.