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 | X120247.63-535007.7 | chandra | ccd2 | 732.012 | 1076.99 | 693.286 | 27.0182 | 0.215342 | 0.00839213 | 114.442 | 1 | 0.626363 | 0.514665 | 100.692 | 1.868 | F | F | 1.38e+21 | 5.3143e-12 | 1 | dsxf | ||||
| Report | srcpi bgdpi arf | 2 | X120242.50-534616.3 | chandra | ccd3 | 994.097 | 507.301 | 15.2589 | 3.90626 | 0.00473955 | 0.00121332 | 33.6842 | 1 | 0.752183 | 0.369121 | 131.956 | 3.05084 | F | F | 1.36e+21 | 5.32793e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 1 | X120214.58-534448.2 | chandra | ccd1 | 455.875 | 537.625 | 7.95555 | 2.82843 | 0.00247104 | 0.000878528 | 17.4341 | 1 | 0.68468 | 0.492 | 79.5571 | 5.4713 | F | F | 1.37e+21 | 2.91494e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 1 | X120311.06-534713.7 | chandra | ccd3 | 479.167 | 389.5 | 5.90816 | 2.44949 | 0.00183511 | 0.000760828 | 13.0423 | 1 | 0.702326 | 0.492 | 70.8549 | 5.44886 | F | F | 1.35e+21 | 2.24638e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 3 | X120231.85-534654.2 | chandra | ccd1 | 144.5 | 281.7 | 4.97466 | 2.23607 | 0.00154516 | 0.000694537 | 10.9017 | 1 | 0.492 | 0.492 | 2.38941e-08 | 2.40072 | F | F | 1.37e+21 | 1.69346e-14 | 1 | dx | ||||
| Report | 5 | X120247.54-534618.3 | chandra | ccd3 | 902.75 | 502.75 | 3.9791 | 2 | 0.00123593 | 0.000621213 | 8.78392 | 0.999997 | 0.492 | 0.492 | 45 | 3.31007 | F | T | 1.36e+21 | 0 | 1 | d | |||||
| Report | srcpi bgdpi arf | 3 | X120313.02-534458.3 | chandra | ccd3 | 443.25 | 664.75 | 3.85242 | 2 | 0.00119659 | 0.000621214 | 8.50428 | 0.999997 | 1.20567 | 0.492 | 125.242 | 6.83595 | A | F | 1.34e+21 | 1.53447e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 4 | X120247.65-534236.3 | chandra | ccd3 | 900.5 | 954 | 3.80934 | 2.00001 | 0.00118321 | 0.000621214 | 8.40918 | 0.999997 | 0.793862 | 0.492 | 73.155 | 6.79076 | A | F | 1.34e+21 | 1.48385e-14 | 1 | dx | ||||
| Report | 2 | X120225.85-534716.8 | chandra | ccd1 | 252.5 | 235.833 | 2.94781 | 1.73205 | 0.000915607 | 0.000537986 | 6.45994 | 0.999934 | 0.492 | 0.492 | 130.269 | 2.49405 | F | F | 1.38e+21 | 0 | 1 | d | |||||
| Report | srcpi bgdpi arf | 1 | X120223.47-535144.3 | chandra | ccd0 | 129 | 705 | 1.97196 | 1.41421 | 0.000612504 | 0.000439264 | 4.53315 | 0.999019 | 0.492 | 0.492 | 45 | 3.19978 | F | F | 1.4e+21 | 6.78649e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 2 | X120156.45-535558.4 | chandra | ccd0 | 613.5 | 187.9 | 4.21244 | 2.23609 | 0.00130841 | 0.000694544 | 9.68356 | 0.999998 | 2.96414 | 0.536332 | 44.3757 | 9.00006 | A | F | 1.44e+21 | 1.70875e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 3 | X120144.43-535240.1 | chandra | ccd0 | 830.5 | 590.3 | 4.63537 | 2.23608 | 0.00143978 | 0.00069454 | 10.6558 | 0.999998 | 1.46499 | 0.492 | 40.8084 | 8.447 | A | F | 1.43e+21 | 1.84452e-14 | 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