5XMM J021505.4-735529

5XMM-DR15 stacked source · SRCID 3004915010100049
Position: 02h15m05.45s -73d55m29.4s (33.77269°, -73.92484°)
EP flux
4.64e-15 ± 1.2e-15 erg cm-2 s-1
CLASSX
Bkg_AGN (0.542)
Detections
7

SRCID 3004915010100049
IAUNAME 5XMM J021505.4-735529
SC_RA 02h15m05.45s (33.77269°)
SC_DEC -73d55m29.4s (-73.92484°)
RADEC_ERR 0.55 arcsec
LII / BII 295.2960° / -41.9403°
N_CONTRIB 7 (detections)
N_OBS 9 (observations covering the position)
MJD_FIRST 51730.634 (2000-07-05 15:13:30.000 UTC)
MJD_LAST 53386.433 (2005-01-16 10:23:46.000 UTC)

Stacked EPIC flux

EP flux (0.2-12 keV): 4.64e-15 ± 1.2e-15 erg cm-2 s-1

Hardness ratios
HR1
0.57 ± 0.08
0.2-0.5 / 0.5-1.0 keV
HR2
-0.61 ± 0.08
0.5-1.0 / 1.0-2.0 keV
HR3
-0.74 ± 0.17
1.0-2.0 / 2.0-4.5 keV
HR4
-0.53 ± 0.92
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -2.5) SUM_FLAG: 1
Long-term lightcurve

Bkg_AGN

CLASSX outlier: 2.36

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
754225
Match probability
0.992
FilterMag (AB)Err
UVW2 — —
UVM2 — —
UVW1 — —
U 21.694 0.111
B — —
V — —
Gaia DR3
Source ID
4643571447613040256
Match probability
0.981
Magnitudes
G=17.56, BP=18.93, RP=15.87
AllWISE
Name
J021505.68-735529.1
Match probability
0.996
BandMagErr
W1 13.015 0.023
W2 12.812 0.023
W3 12.658 0.352
W4 9.360 —
CLASSOPT
Class
Star
Star
0.98
AGN
0.00
Galaxy
0.01

No redshift estimate available for this source.

Stacked power-law fit
Unabsorbed flux 1.29e-14 (+1.7e-14 / −1.1e-14) erg cm−2 s−1
NH 1.99e+20 (+7.3e+20 / −2.6e+19) cm−2
Photon index (Γ) 2.54 (+2.82 / −2.24)
DoF 44
p-value 0.647
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.