5XMM J002733.9+171155
5XMM-DR15 stacked source · SRCID 3005014020100014
Position:
00h27m33.92s +17d11m55.4s
(6.89132°, 17.19873°)
EP flux
2.90e-14
± 5.7e-15
erg cm-2 s-1
CLASSX
Star
(0.981)
Detections
1
| SRCID | 3005014020100014 |
|---|---|
| IAUNAME | 5XMM J002733.9+171155 |
| SC_RA | 00h27m33.92s (6.89132°) |
| SC_DEC | +17d11m55.4s (17.19873°) |
| RADEC_ERR | 0.63 arcsec |
| LII / BII | 114.8146° / -45.2964° |
| N_CONTRIB | 1 (detections) |
| N_OBS | 1 (observations covering the position) |
| MJD_FIRST | 51915.674 (2001-01-06 16:10:21.000 UTC) |
| MJD_LAST | 51916.277 (2001-01-07 06:39:29.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 2.90e-14 ± 5.7e-15 erg cm-2 s-1
Hardness ratios
HR1
0.41
± 0.07
0.2-0.5 / 0.5-1.0 keV
HR2
-0.32
± 0.07
0.5-1.0 / 1.0-2.0 keV
HR3
-0.83
± 0.08
1.0-2.0 / 2.0-4.5 keV
HR4
-1.00
± 0.59
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -2.7)
SUM_FLAG:
0
Long-term lightcurve
No light-curve points available.
Star
CLASSX outlier: 2.81
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.
No multi-wavelength counterpart data available for this source.
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 2.40e-14 (+2.7e-14 / −2.1e-14) erg cm−2 s−1 |
|---|---|
| NH | 1.02e+21 (+1.3e+21 / −7.0e+20) cm−2 |
| Photon index (Γ) | 2.88 (+2.97 / −2.67) |
| DoF | 819 |
| p-value | 0.038 |
| Inter-instrument norm. | 1.09 (0.90–1.31) |
| Quality flag | 0 |
| APPROX_SOURCE_VAR | 8.600 (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.