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 arf 3 X153924.45-833529.4 chandra ccd3 668.3 399.5 29.4453 7.2803 0.00368606 0.00091137 2.58556 0.99445 0.492 0.492 109.903 2.32464 F F 7.29e+20 4.12938e-14 1 dbx
Report srcpi bgdpi arf 1 X153648.27-833811.0 chandra ccd1 524.092 850.287 16.2828 5.08543 0.00203835 0.000636616 5.26106 0.999991 0.805522 0.805522 0 6.11223 F F 7.34e+20 2.41075e-14 1 dsx
Report srcpi bgdpi arf 2 X153930.74-833522.6 chandra ccd3 647.456 414.015 53.7347 17.2989 0.0067267 0.00216553 4.71837 0.999996 2.0869 2.0869 0 2.32504 T F 7.29e+20 7.55206e-14 1 dsx
Report srcpi bgdpi arf 4 X153758.84-834057.2 chandra ccd1 281.583 515.167 16.3967 4.12311 0.00205258 0.000516144 5.29784 0.999991 0.784951 0.535596 125.184 5.5812 F F 7.32e+20 2.404e-14 1 dx
Report srcpi bgdpi arf 3 X153530.15-833529.9 chandra ccd1 794.5 1172.27 10.4601 3.6056 0.00130942 0.000451359 3.37971 0.99905 2.28456 1.61818 162.559 8.35822 F F 7.37e+20 1.71557e-14 1 dx
Report srcpi bgdpi arf 1 X154353.81-833513.3 chandra ccd2 564.227 1086.32 9.89034 3.31665 0.00123762 0.000415027 11.6016 1 1.45988 0.901402 39.9875 6.11707 A F 7.18e+20 1.60945e-14 1 dx
Report srcpi bgdpi arf 1 X154529.64-833059.4 chandra ccd6 1240.59 682.318 9.11061 3.31666 0.00114005 0.000415029 11.1928 1 2.65493 1.62417 129.44 10.498 A F 7.14e+20 1.48665e-14 1 dx
Report srcpi bgdpi arf 1 X154126.36-834520.7 chandra ccd0 394.773 660.773 8.59198 3.31667 0.00107515 0.00041503 11.0414 1 2.86534 1.43816 56.2574 8.4193 A F 7.24e+20 1.41004e-14 1 dx
Report srcpi bgdpi arf 2 X154201.79-833454.7 chandra ccd2 945.375 1128.38 7.76335 2.82843 0.000971463 0.000353934 9.10657 1 0.57525 0.492 11.1643 3.47642 F F 7.23e+20 1.1877e-14 1 dx
Report srcpi bgdpi arf 2 X153609.93-834028.0 chandra ccd1 648 569.125 7.33677 2.82844 0.000918439 0.000354073 2.37055 0.980998 1.12612 0.630634 162.728 7.81453 A F 7.36e+20 1.21312e-14 1 dx
Report srcpi bgdpi arf 5 X154405.73-834012.7 chandra ccd2 533.333 477.333 5.79154 2.44949 0.000724722 0.000306516 6.7936 0.999989 0.492 0.492 45 6.86205 F T 7.18e+20 9.3295e-15 1 dx
Report 4 X154036.49-833859.6 chandra ccd2 1236.5 631.75 3.93213 2 0.000492045 0.000250269 4.61247 0.999073 0.492 0.492 164.196 1.92371 F F 7.26e+20 0 1 d
Report srcpi bgdpi arf 2 X153954.82-834254.9 chandra ccd0 699 957.5 1.89466 1.41422 0.000237087 0.000176967 2.4348 0.976335 0.492 0.492 180 5.8754 F F 7.28e+20 2.84214e-15 1 dx
Report srcpi bgdpi arf 3 X154012.13-834026.7 chandra ccd0 641.5 1258.83 3.86492 2 0.000483635 0.000250269 4.96675 0.999589 0.492 0.492 90 3.36506 F F 7.27e+20 5.49995e-15 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 - 7.99 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), T = 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