5XMM J001541.2-391506

5XMM-DR15 stacked source · SRCID 3002874010100044
Position: 00h15m41.20s -39d15m06.5s (3.92168°, -39.25179°)
EP flux
5.07e-15 ± 3.7e-16 erg cm-2 s-1
CLASSX
Extragal_XRB (0.535)
Detections
10

SRCID 3002874010100044
IAUNAME 5XMM J001541.2-391506
SC_RA 00h15m41.20s (3.92168°)
SC_DEC -39d15m06.5s (-39.25179°)
RADEC_ERR 0.26 arcsec
LII / BII 332.2409° / -75.7728°
N_CONTRIB 10 (detections)
N_OBS 10 (observations covering the position)
MJD_FIRST 52227.605 (2001-11-14 14:31:49.000 UTC)
MJD_LAST 59561.812 (2021-12-13 19:29:06.000 UTC)

Stacked EPIC flux

EP flux (0.2-12 keV): 5.07e-15 ± 3.7e-16 erg cm-2 s-1

Hardness ratios
HR1
0.83 ± 0.02
0.2-0.5 / 0.5-1.0 keV
HR2
-0.49 ± 0.03
0.5-1.0 / 1.0-2.0 keV
HR3
-0.98 ± 0.03
1.0-2.0 / 2.0-4.5 keV
HR4
0.22 ± 1.06
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML 49.1) SUM_FLAG: 1
Long-term lightcurve

Extragal_XRB

CLASSX outlier: 4.13

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
24746
Match probability
0.671
FilterMag (AB)Err
UVW2 16.314 0.010
UVM2 16.310 0.005
UVW1 16.204 0.004
U
B
V 16.443 0.011
Gaia DR3
Source ID
4997969952487162880
Match probability
0.986
Parallax
0.655 ± 0.518 mas
Proper motion
(0.14, 3.42) mas/yr
Magnitudes
G=19.70, BP=17.89, RP=17.43
CLASSOPT
Class
QSO
Star
0.00
AGN
0.62
Galaxy
0.38

No redshift estimate available for this source.

Stacked power-law fit
Unabsorbed flux 7.18e-15 (+7.9e-15 / −6.5e-15) erg cm−2 s−1
NH 1.75e+21 (+2.0e+21 / −1.4e+21) cm−2
Photon index (Γ) 2.88 (+2.97 / −2.72)
DoF 464
p-value 0.04
Inter-instrument norm. 0.72 (0.60–0.86)
Quality flag 0

APPROX_SOURCE_VAR 27.200 (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.