Source List

Observation details report
Detailed source parameters (including errors) in a comma-separated values file

Click on source number for detailed analysis, including spectral fits if applicable

data idnum idradec telescope instrument x y cnts cntserr rate rateerr SNR poisprob sigmaj sigmin incang offax cnts_soft cnts_hard hr hr_err ext var N_H flux vign flags
Report srcpi bgdpi 1 X070542.66-381440.4 xmm pn 293.156 275.351 3566.68 67.9659 0.70335 0.0134029 109.93 1 6.23665 5.77637 350.795 1.72731 F T 3.81333 0 1 ds
Report srcpi bgdpi 1 X070542.64-381439.1 xmm mos1 293.197 275.649 650.5 29.7939 0.160276 0.00734087 42.2387 1 5.13503 4.35339 341.626 1.68777 F T 3.81315 0 1 ds
Report srcpi bgdpi 1 X070542.57-381440.2 xmm mos2 293.408 275.394 607.241 29.8885 0.14469 0.00712166 56.7051 1 5.43217 5.43217 0 1.72449 F T 3.8135 0 1 dbs
Report srcpi bgdpi 2 X070600.17-381359.2 xmm mos2 245.727 284.807 437.704 25.4269 0.0927885 0.00539022 40.8735 1 10.875 10.875 0 3.94717 F T 3.75624 0 1 d
Report srcpi bgdpi 4 X070516.10-380427.2 xmm mos2 365.25 416.34 24.3365 6.71515 0.00466139 0.00128621 2.27258 0.987969 10.875 10.875 0 9.82504 F F 3.82409 0 1 d

counts and rate are bgd.-subtracted, based on simple spatial fitting (if done) or extracted counts from aperture otherwise (N.B., in either case aperture counts are given csv file).
cntserr, rateerr = Error on (source) counts and count rate, based on error in total counts
SNR = signal-to-noise ratio, computed using Nsrc/sqrt(Nbgd)
poisprob = Poisson probability of observing total counts given bgd. counts
sigmaj, sigmin = source extent (from detection output or spatial fitting) in units of arcsecs.
incang = position angle of source (inclination from x-axis)
cnts_soft = bgd.-subtracted counts in soft band (0.50 - 2.00 KeV, always taken directly from source aperture rather than model fitting)
cnts_hard = bgd.-subtracted counts in hard band (2.00 - 10.00 KeV, always taken directly from source aperture rather than model fitting)
hr, hr_err = hardness ratio ([cnts_hard-cnts_soft]/[cnts_hard+cnts_soft]) and error
ext = source extension flag: F = false (not extended), A = true (extended), A = asymetric (ratio of sigmaj/sigmin > 1 + x, where x = 0.5 by default)
var = variability flag: U = unknown, F = false (is not variable), T = true
N_H = Galactic column density as determined from LHEASOFT nh program
flux = flux determined from count rate using pimms (in the 0.30-8.00 keV bandpass for a power-law model with ph. index = 1.8)
vign = vignetting correction
Flags: d = detection parameters, s = simple spatial fitting parameters, b = simple spatial fitting failed, p = poor simple spatial fit, x = extracted events parameters, t = temporal anaylsis parameters, i = psf spatial fitting parameters, f = spectral fitting parameters, c = source is confused, u = user-defined source, v = detected source coincident with user-defined source, r = source is in region-of-interest