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 | 1 | X171943.26-143318.0 | xmm | pn | 177.185 | 342.104 | 229.145 | 17.0857 | 0.0656398 | 0.00489429 | 42.6579 | 1 | 10.875 | 10.875 | 0 | 9.34344 | 190.902 | 24.1636 | -0.775291 | 0.0974091 | F | F | 1.76e+21 | 4.18916e-13 | 1 | dpx |
Report | srcpi bgdpi arf | 1 | X171943.35-143320.6 | xmm | mos1 | 176.865 | 342.057 | 98.9721 | 12.3221 | 0.0212894 | 0.00265055 | 14.7239 | 1 | 7.30088 | 5.46135 | 112.305 | 9.35476 | 79.0123 | 20.8098 | -0.583062 | 0.132109 | F | F | 1.76e+21 | 4.2608e-13 | 1 | dsx |
Report | srcpi bgdpi arf | 2 | X171907.33-143220.8 | xmm | pn | 297.086 | 355.813 | 82.971 | 11.5712 | 0.0237675 | 0.00331463 | 15.6719 | 1 | 10.875 | 10.875 | 0 | 4.16093 | 42.3031 | 34.824 | -0.0969715 | 0.145871 | F | F | 1.77e+21 | 1.14042e-13 | 1 | dx |
Report | srcpi bgdpi arf | 2 | X171859.65-143920.7 | xmm | mos2 | 322.737 | 259.315 | 34.4101 | 8.15158 | 0.0071958 | 0.00170465 | 6.07929 | 1 | 5.23977 | 5.23977 | 0 | 3.35135 | 28.8651 | 2.50925 | -0.840044 | 0.294833 | F | F | 1.78e+21 | 1.0467e-13 | 1 | dsx |
Report | srcpi bgdpi arf | 2 | X171859.77-143920.6 | xmm | mos1 | 322.338 | 259.322 | 24.7256 | 7.88864 | 0.0053186 | 0.00169689 | 3.67837 | 0.999628 | 5.06883 | 2.26062 | 27.1282 | 3.32568 | 22.5759 | 0.974667 | -0.917228 | 0.357012 | F | F | 1.78e+21 | 1.32476e-13 | 1 | dsx |
Report | srcpi bgdpi arf | 1 | X171943.38-143323.9 | xmm | mos2 | 176.794 | 339.384 | 47.6534 | 9.04674 | 0.00996521 | 0.00189184 | 11.7864 | 1 | 10.875 | 10.875 | 0 | 9.30534 | 40.6176 | 6.66849 | -0.717952 | 0.234304 | F | F | 1.76e+21 | 2.57519e-13 | 1 | dpx |
Report | srcpi bgdpi arf | 3 | X171840.49-142700.9 | xmm | pn | 386.731 | 429.366 | 35.1753 | 8.4683 | 0.0100762 | 0.00242579 | 5.81932 | 1 | 8.29608 | 4.26644 | 46.8757 | 11.4581 | 23.9755 | 5.51803 | -0.625814 | 0.289785 | F | F | 1.77e+21 | 1.3744e-13 | 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