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 rmf | 1 | X095238.36-622315.6 | chandra | ccd2 | 736.132 | 1046.63 | 209.109 | 14.5309 | 0.0606088 | 0.00421167 | 207.2 | 1 | 1.47071 | 1.21652 | 342.285 | 5.88672 | F | F | 2.29e+21 | 5.20537e-13 | 1 | dsxf | ||||
Report | srcpi bgdpi arf | 1 | X095220.14-623236.1 | chandra | ccd3 | 94.5 | 432.5 | 55.8222 | 8.3067 | 0.0161796 | 0.00240763 | 103.691 | 1 | 0.492 | 0.492 | 90 | 9.70155 | F | F | 2.18e+21 | 3.79261e-13 | 1 | dx | ||||
Report | srcpi bgdpi arf | 3 | X095110.11-622818.3 | chandra | ccd3 | 1080.17 | 956.405 | 20.6681 | 4.58258 | 0.0059905 | 0.00132823 | 38.3914 | 1 | 0.970752 | 0.688629 | 117.631 | 6.36323 | F | F | 2.19e+21 | 7.89701e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 1 | X095039.23-621942.2 | chandra | ccd7 | 1019.96 | 751.833 | 17.8845 | 4.89906 | 0.00518368 | 0.00141996 | 22.6455 | 1 | 3.93367 | 2.24435 | 155.619 | 8.86632 | A | F | 2.25e+21 | 4.9862e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 2 | X095033.81-622135.0 | chandra | ccd7 | 1095.6 | 522.15 | 14.2127 | 4.47222 | 0.00411945 | 0.00129624 | 17.9963 | 1 | 4.06998 | 2.83102 | 84.7376 | 8.8079 | F | F | 2.23e+21 | 4.01852e-14 | 1 | dx | ||||
Report | 4 | X095214.35-622522.3 | chandra | ccd2 | 1075.96 | 790.017 | 10.8529 | 3.29437 | 0.00314565 | 0.000954854 | 10.7538 | 1 | 0.716296 | 0.716296 | 0 | 3.53343 | F | F | 2.25e+21 | 0 | 1 | ds | |||||
Report | 1 | X095153.59-622010.8 | chandra | ccd6 | 891.214 | 136.929 | 6.88188 | 2.64575 | 0.00199466 | 0.000766851 | 13.0084 | 1 | 0.721722 | 0.492 | 131.786 | 3.54346 | F | F | 2.29e+21 | 0 | 1 | d | |||||
Report | srcpi bgdpi arf | 1 | X095327.37-623009.7 | chandra | ccd0 | 567.5 | 1114 | 6.63869 | 2.82846 | 0.00192417 | 0.000819808 | 13.4067 | 1 | 2.85984 | 0.492 | 21.2257 | 13.2389 | A | F | 2.25e+21 | 2.7432e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 2 | X095157.50-623044.0 | chandra | ccd3 | 412.643 | 660.928 | 6.38584 | 2.64577 | 0.00185089 | 0.000766855 | 11.8618 | 1 | 1.37607 | 0.578822 | 166.306 | 7.16755 | A | F | 2.19e+21 | 2.27275e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 3 | X095142.51-622156.6 | chandra | ccd7 | 124 | 480.833 | 5.88627 | 2.44949 | 0.00170609 | 0.000709967 | 7.45325 | 0.999996 | 0.492 | 0.492 | 16.4847 | 1.81404 | F | F | 2.26e+21 | 1.59045e-14 | 1 | dx | ||||
Report | 5 | X095139.11-622927.5 | chandra | ccd3 | 671.5 | 816.3 | 4.96508 | 2.23607 | 0.00143909 | 0.000648107 | 9.22271 | 0.999999 | 0.492 | 0.492 | 90 | 5.88666 | F | F | 2.19e+21 | 0 | 1 | d | |||||
Report | srcpi bgdpi arf | 2 | X095222.25-622806.6 | chandra | ccd2 | 964.7 | 455.3 | 4.79533 | 2.23607 | 0.00138989 | 0.000648109 | 4.75156 | 0.999347 | 0.86246 | 0.623717 | 53.9394 | 5.98696 | F | F | 2.23e+21 | 1.65617e-14 | 1 | dx | ||||
Report | 4 | X095139.37-622645.8 | chandra | ccd3 | 668 | 1145 | 3.96712 | 2 | 0.00114984 | 0.000579685 | 7.36897 | 0.999987 | 0.492 | 0.492 | 157.5 | 3.25252 | F | F | 2.22e+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