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 | 3 | X033330.49+311050.5 | xmm | mos2 | 275.105 | 355.798 | 42.1627 | 19.9266 | 0.00416166 | 0.00196685 | 2.44717 | 0.992436 | 3.23424 | 3.23424 | 0 | 4.49764 | 29.1591 | 11.4627 | -0.435639 | 0.236572 | F | F | 1.16e+21 | 1.08202e-13 | 1 | dsx |
Report | srcpi bgdpi arf | 7 | X033344.85+310359.2 | xmm | mos2 | 232.662 | 261.318 | 51.2215 | 16.3216 | 0.00505581 | 0.00161102 | 3.7887 | 0.999881 | 10.875 | 10.875 | 0 | 5.47559 | 15.3745 | 40.9588 | 0.454158 | 0.31324 | F | T | 1.16e+21 | 8.86835e-14 | 1 | dbx |
Report | srcpi bgdpi arf | 8 | X033256.79+310344.6 | xmm | mos2 | 374.606 | 258.191 | 18.1903 | 16.9609 | 0.00179547 | 0.00167412 | 1.18457 | 0.887297 | 10.875 | 10.875 | 0 | 6.24572 | -2.09901 | 13.4584 | 1 | 1.71936 | F | F | 1.14e+21 | 2.60069e-14 | 1 | dbx |
Report | srcpi bgdpi arf | 9 | X033309.53+310245.5 | xmm | mos2 | 336.992 | 243.74 | 34.9552 | 17.7854 | 0.00345025 | 0.00175551 | 2.22846 | 0.986772 | 10.875 | 10.875 | 0 | 4.85166 | 4.25053 | 32.0767 | 0.765987 | 0.604449 | F | F | 1.14e+21 | 4.77939e-14 | 1 | dbx |
Report | srcpi bgdpi arf | 4 | X033259.70+310146.0 | xmm | mos2 | 366.052 | 229.736 | 53.8316 | 16.3867 | 0.00531344 | 0.00161744 | 3.98842 | 0.999943 | 10.875 | 10.875 | 0 | 6.98848 | 14.9996 | 34.0066 | 0.387849 | 0.346518 | F | F | 1.14e+21 | 9.11351e-14 | 1 | dbx |
Report | srcpi bgdpi arf | 5 | X033343.82+310452.7 | xmm | mos2 | 235.693 | 272.782 | 38.4496 | 16.3867 | 0.00379516 | 0.00161744 | 2.7356 | 0.996516 | 10.875 | 10.875 | 0 | 4.91449 | 6.3487 | 32.4796 | 0.672986 | 0.49773 | F | F | 1.16e+21 | 6.21906e-14 | 1 | dbpx |
Report | srcpi bgdpi arf | 6 | X033259.38+310408.0 | xmm | mos2 | 366.955 | 262.782 | 6.15311 | 16.9922 | 0.000607342 | 0.00167721 | 0.390057 | 0.666554 | 10.875 | 10.875 | 0 | 5.5999 | -0.701976 | 2.52508 | 1 | 9.20037 | F | F | 1.14e+21 | 8.42806e-15 | 1 | dx |
Report | srcpi bgdpi arf | 10 | X033357.71+311532.6 | xmm | mos2 | 194.878 | 420.708 | 56.6638 | 17.1885 | 0.00559299 | 0.00169658 | 3.28883 | 0.999315 | 24.5663 | 7.41393 | 354.216 | 11.7092 | 17.986 | 29.5242 | 0.242856 | 0.34728 | F | F | 1.18e+21 | 1.86683e-13 | 1 | dsx |
Report | srcpi bgdpi arf | 2 | X033351.46+311226.2 | xmm | mos2 | 213.266 | 377.35 | 51.7938 | 15.6884 | 0.0051123 | 0.00154852 | 4.05424 | 0.999954 | 10.875 | 10.875 | 0 | 8.41794 | 22.8435 | 26.0377 | 0.065346 | 0.313319 | F | F | 1.17e+21 | 1.18366e-13 | 1 | dx |
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