5XMM J114450.1+193156

5XMM-DR15 stacked source · SRCID 3006174010100279
Position: 11h44m50.12s +19d31m56.4s (176.20882°, 19.53233°)
EP flux
9.53e-15 ± 6.9e-15 erg cm-2 s-1
CLASSX
Bkg_AGN (0.529)
Detections
3

SRCID 3006174010100279
IAUNAME 5XMM J114450.1+193156
SC_RA 11h44m50.12s (176.20882°)
SC_DEC +19d31m56.4s (19.53233°)
RADEC_ERR 1.76 arcsec
LII / BII 235.8489° / 72.9511°
N_CONTRIB 3 (detections)
N_OBS 7 (observations covering the position)
MJD_FIRST 52055.830 (2001-05-26 19:55:46.000 UTC)
MJD_LAST 59188.831 (2020-12-05 19:57:01.000 UTC)

Stacked EPIC flux

EP flux (0.2-12 keV): 9.53e-15 ± 6.9e-15 erg cm-2 s-1

Hardness ratios
HR1
0.51 ± 0.16
0.2-0.5 / 0.5-1.0 keV
HR2
-0.23 ± 0.18
0.5-1.0 / 1.0-2.0 keV
HR3
-0.98 ± 0.21
1.0-2.0 / 2.0-4.5 keV
HR4
0.90 ± 0.90
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: 4.79

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
3086304
Match probability
0.947
FilterMag (AB)Err
UVW2 — —
UVM2 — —
UVW1 18.579 0.032
U — —
B — —
V — —
Gaia DR3
Source ID
3975779006033114624
Match probability
0.905
Magnitudes
G=19.08, BP=16.09, RP=14.73
AllWISE
Name
J114450.14+193158.2
Match probability
0.991
BandMagErr
W1 11.325 0.023
W2 11.426 0.021
W3 10.823 0.107
W4 8.322 —
CLASSOPT
Class
Galaxy
Star
0.00
AGN
0.00
Galaxy
1.00

No redshift estimate available for this source.

Stacked power-law fit
Unabsorbed flux 5.30e-15 (+1.1e-14 / −2.4e-15) erg cm−2 s−1
NH 4.14e+20 (+2.5e+22 / −3.8e+19) cm−2
Photon index (Γ) 2.15 (+2.68 / −1.46)
DoF 284
p-value 0.48
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

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