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 | 7 | X053747.33-691020.1 | chandra | ccd3 | 668.52 | 423.003 | 323.127 | 21.5038 | 0.308059 | 0.020501 | 43.4587 | 1 | 2.03228 | 2.03228 | 0 | 6.86878 | F | F | 2.94e+21 | 0 | 1 | ds | |||||
Report | 6 | X053745.38-691009.9 | chandra | ccd3 | 689.756 | 443.605 | 135.725 | 12.7393 | 0.129396 | 0.0121452 | 18.2542 | 1 | 4.20094 | 4.20094 | 0 | 6.86595 | T | F | 2.93e+21 | 0 | 1 | ds | |||||
Report | 1 | X053844.28-690606.2 | chandra | ccd3 | 51.2687 | 940.421 | 51.1586 | 7.15252 | 0.048773 | 0.00681899 | 6.88053 | 1 | 0.506829 | 0.506829 | 0 | 0.360645 | F | F | 3.03e+21 | 0 | 1 | ds | |||||
Report | 2 | X053842.88-690604.9 | chandra | ccd3 | 65.9165 | 942.417 | 23.5932 | 4.89898 | 0.0224923 | 0.00467038 | 3.17315 | 0.998443 | 0.512437 | 0.492 | 173.815 | 0.374657 | F | F | 3.03e+21 | 0 | 1 | dpb | |||||
Report | 4 | X053841.61-690513.8 | chandra | ccd2 | 166.288 | 10.7941 | 19.0218 | 4.55989 | 0.0181348 | 0.00434726 | 14.2944 | 1 | 0.370883 | 0.370883 | 0 | 0.582341 | F | F | 3.01e+21 | 0 | 1 | ds | |||||
Report | 3 | X053809.65-685656.6 | chandra | ccd2 | 516.1 | 1020.5 | 7.33718 | 2.82844 | 0.00699481 | 0.00269646 | 5.5137 | 0.999983 | 1.31446 | 0.61199 | 56.1148 | 9.34293 | A | F | 2.83e+21 | 0 | 1 | d | |||||
Report | 1 | X053830.72-690345.5 | chandra | ccd2 | 284.5 | 189.75 | 3.95513 | 2 | 0.00377057 | 0.00190667 | 2.97218 | 0.990362 | 0.492 | 0.492 | 2.35032e-08 | 2.34449 | F | F | 2.97e+21 | 0 | 1 | d | |||||
Report | 2 | X053754.38-690222.4 | chandra | ccd2 | 681 | 357.75 | 3.94224 | 2 | 0.00375828 | 0.00190668 | 2.96249 | 0.990362 | 0.504692 | 0.492 | 127.982 | 5.61676 | F | F | 2.87e+21 | 0 | 1 | d | |||||
Report | 1 | X053907.74-685721.5 | chandra | ccd0 | 921 | 1052.25 | 3.59915 | 2.00001 | 0.00343121 | 0.00190668 | 8.57107 | 0.999965 | 1.76023 | 0.60431 | 151.721 | 8.63647 | A | F | 2.93e+21 | 0 | 1 | d |
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