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