5XMM J230043.4+585029

5XMM-DR15 stacked source · SRCID 3003814010100002
Position: 23h00m43.40s +58d50m29.9s (345.18082°, 58.84164°)
EP flux
1.92e-13 ± 9.5e-15 erg cm-2 s-1
CLASSX
CV (0.861)
Detections
5

SRCID 3003814010100002
IAUNAME 5XMM J230043.4+585029
SC_RA 23h00m43.40s (345.18082°)
SC_DEC +58d50m29.9s (58.84164°)
RADEC_ERR 0.16 arcsec
LII / BII 109.0231° / -1.0077°
N_CONTRIB 5 (detections)
N_OBS 13 (observations covering the position)
MJD_FIRST 52296.715 (2002-01-22 17:09:56.000 UTC)
MJD_LAST 52464.768 (2002-07-09 18:25:34.000 UTC)

Stacked EPIC flux

EP flux (0.2-12 keV): 1.92e-13 ± 9.5e-15 erg cm-2 s-1

Hardness ratios
HR1
0.64 ± 0.03
0.2-0.5 / 0.5-1.0 keV
HR2
0.19 ± 0.03
0.5-1.0 / 1.0-2.0 keV
HR3
-0.38 ± 0.03
1.0-2.0 / 2.0-4.5 keV
HR4
-0.57 ± 0.05
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -3.5) SUM_FLAG: 1
Long-term lightcurve

CV

CLASSX outlier: 4.6

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
6516620
Match probability
0.972
FilterMag (AB)Err
UVW2 — —
UVM2 — —
UVW1 — —
U — —
B — —
V 19.778 0.119
Gaia DR3
Source ID
2013339454141087616
Match probability
0.992
Parallax
2.018 ± 0.816 mas
Proper motion
(-0.89, -2.38) mas/yr
Magnitudes
G=20.68, BP=20.84, RP=20.63
CLASSOPT
Class
QSO
Star
0.00
AGN
1.00
Galaxy
0.00

No redshift estimate available for this source.

Stacked power-law fit
Unabsorbed flux 1.37e-13 (+1.6e-13 / −1.2e-13) erg cm−2 s−1
NH 1.05e+21 (+1.4e+21 / −6.4e+20) cm−2
Photon index (Γ) 1.95 (+2.10 / −1.78)
DoF 578
p-value 0.902
Inter-instrument norm. 1.03 (0.91–1.16)
Quality flag 0

APPROX_SOURCE_VAR 39.400 (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.