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 arf rmf | 1 | X141315.00-031228.8 | xmm | pn | 293.969 | 275.067 | 91437.5 | 337.44 | 8.60559 | 0.031758 | 610.554 | 1 | 6.1733 | 6.1733 | 0 | 1.727 | F | F | 3.80928 | 6.13484e-11 | 1 | dsxf | ||||
| Report | srcpi bgdpi arf rmf | 3 | X141315.04-031228.9 | xmm | mos1 | 293.837 | 275.039 | 40926.2 | 227.222 | 3.094 | 0.0171779 | 395.58 | 1 | 6.23742 | 6.0579 | 338.752 | 1.73083 | F | F | 3.80923 | 6.68412e-11 | 1 | dsxf | ||||
| Report | srcpi bgdpi arf rmf | 1 | X141315.05-031229.5 | xmm | mos2 | 293.797 | 274.899 | 45281.9 | 226.261 | 3.42311 | 0.0171043 | 821.288 | 1 | 7.02517 | 7.02517 | 0 | 1.72696 | F | F | 3.8093 | 7.87207e-11 | 1 | dsxf | ||||
| Report | srcpi bgdpi arf | 4 | X141318.35-031215.1 | xmm | mos2 | 282.408 | 277.712 | 183.181 | 22.5465 | 0.0158343 | 0.00194893 | 3.3224 | 0.999517 | 10.875 | 10.875 | 0 | 1.89952 | F | F | 3.80516 | 1.62352e-13 | 1 | dbcx | ||||
| Report | srcpi bgdpi arf | 3 | X141316.64-031311.2 | xmm | mos2 | 288.298 | 264.798 | 153.951 | 20.193 | 0.0138583 | 0.00181772 | 2.79224 | 0.997163 | 10.875 | 10.875 | 0 | 2.54721 | F | F | 3.79568 | 1.45558e-13 | 1 | dbx | ||||
| Report | srcpi bgdpi arf | 2 | X141318.34-031238.5 | xmm | mos2 | 282.453 | 272.839 | 168.986 | 22.7982 | 0.0136177 | 0.00183719 | 3.06493 | 0.998791 | 10.875 | 10.875 | 0 | 2.18792 | F | F | 3.79968 | 1.34609e-13 | 1 | dpcx | ||||
| Report | srcpi bgdpi arf | 13 | X141320.72-031211.5 | xmm | mos2 | 274.266 | 278.881 | 102.193 | 16.4876 | 0.00799002 | 0.00128909 | 1.85351 | 0.968112 | 10.875 | 10.875 | 0 | 2.25409 | F | F | 3.80084 | 7.71581e-14 | 1 | dbx | ||||
| Report | srcpi bgdpi arf rmf | 12 | X141321.62-031126.9 | xmm | mos2 | 271.158 | 289.277 | 112.319 | 16.7326 | 0.00849084 | 0.00126491 | 2.03716 | 0.978975 | 15.1524 | 15.1524 | 0 | 2.29528 | T | F | 3.80948 | 7.87661e-14 | 1 | dsx |
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