5XMM J182854.5-112656

5XMM-DR15 stacked source · SRCID 3005194060100097
Position: 18h28m54.52s -11d26m56.0s (277.22716°, -11.44890°)
EP flux
5.41e-14 ± 5.5e-15 erg cm-2 s-1
CLASSX
Bkg_AGN (0.47)
Detections
2

SRCID 3005194060100097
IAUNAME 5XMM J182854.5-112656
SC_RA 18h28m54.52s (277.22716°)
SC_DEC -11d26m56.0s (-11.44890°)
RADEC_ERR 0.45 arcsec
LII / BII 20.1922° / -0.2808°
N_CONTRIB 2 (detections)
N_OBS 71 (observations covering the position)
MJD_FIRST 51990.864 (2001-03-22 20:43:55.000 UTC)
MJD_LAST 56366.500 (2013-03-15 11:59:18.000 UTC)

Stacked EPIC flux

EP flux (0.2-12 keV): 5.41e-14 ± 5.5e-15 erg cm-2 s-1

Hardness ratios
HR1
0.92 ± 0.11
0.2-0.5 / 0.5-1.0 keV
HR2
0.61 ± 0.07
0.5-1.0 / 1.0-2.0 keV
HR3
-0.10 ± 0.07
1.0-2.0 / 2.0-4.5 keV
HR4
-0.60 ± 0.08
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -2.7) SUM_FLAG: 0
Long-term lightcurve

Bkg_AGN

CLASSX outlier: 4.65

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
5438082
Match probability
0.962
FilterMag (AB)Err
UVW2 — —
UVM2 — —
UVW1 — —
U — —
B 19.246 0.063
V 17.765 0.062
Gaia DR3
Source ID
4153358685199735552
Match probability
0.981
Parallax
0.437 ± 0.093 mas
Proper motion
(0.86, -0.22) mas/yr
Magnitudes
G=17.29, BP=18.15, RP=16.36
Distance
950 pc
CLASSOPT
Class
Star
Star
1.00
AGN
0.00
Galaxy
0.00

No redshift estimate available for this source.

Stacked power-law fit
Unabsorbed flux 4.64e-14 (+5.4e-14 / −4.0e-14) erg cm−2 s−1
NH 5.83e+21 (+7.3e+21 / −4.5e+21) cm−2
Photon index (Γ) 2.06 (+2.36 / −1.80)
DoF 260
p-value 0.584
Inter-instrument norm. 1.00 (0.83–1.18)
Quality flag 0

APPROX_SOURCE_VAR 5.500 (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

The per-observation light curve is shown in the X-ray properties section above.