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 | 2 | X033619.86-172806.9 | chandra | ccd7 | 218.551 | 524.528 | 39.7471 | 6.56851 | 0.00364722 | 0.000602732 | 32.8672 | 1 | 0.367024 | 0.367024 | 0 | 0.52029 | 33.9152 | -0.254293 | -1 | 0.28839 | F | F | 6.19e+20 | 2.76803e-14 | 1 | dsx |
| Report | srcpi bgdpi arf | 1 | X033608.19-173949.9 | chandra | ccd3 | 136.944 | 398.13 | 34.6775 | 7.1441 | 0.00318202 | 0.000655547 | 22.7545 | 1 | 3.17682 | 2.12537 | 110.289 | 12.168 | 21.7168 | 12.9607 | -0.2525 | 0.213086 | F | F | 6.01e+20 | 4.68745e-14 | 1 | dpx |
| Report | srcpi bgdpi arf | 2 | X033551.00-173407.1 | chandra | ccd3 | 636.929 | 1094.79 | 38.1026 | 7.46142 | 0.00349632 | 0.000684665 | 22.3846 | 1 | 3.52398 | 2.23316 | 125.156 | 8.94266 | 22.4634 | 16.8001 | -0.144239 | 0.194472 | A | F | 6.07e+20 | 4.91611e-14 | 1 | dx |
| Report | srcpi bgdpi arf | 1 | X033619.77-172756.6 | chandra | ccd7 | 221.239 | 545.534 | 17.3347 | 4.1635 | 0.00159064 | 0.000382045 | 14.3342 | 1 | 0.330307 | 0.330307 | 0 | 0.448706 | 10.9151 | 7 | -0.218537 | 0.306187 | F | F | 6.19e+20 | 1.2087e-14 | 1 | dsx |
| Report | srcpi bgdpi arf | 3 | X033627.09-172826.6 | chandra | ccd6 | 1044.17 | 659.638 | 16.2072 | 4.02582 | 0.00148719 | 0.000369413 | 18.5977 | 1 | 0.837645 | 0.376603 | 317.937 | 2.26001 | 9.92389 | 3.88583 | -0.437232 | 0.385121 | F | F | 6.2e+20 | 1.56523e-14 | 1 | dsx |
| Report | srcpi bgdpi arf | 5 | X033619.52-172840.3 | chandra | ccd7 | 228.469 | 456.627 | 10.7481 | 3.27843 | 0.000986256 | 0.000300832 | 8.88769 | 1 | 0.528835 | 0.181939 | 89.9594 | 0.875639 | 6 | 4.91231 | -0.0996759 | 0.411116 | F | F | 6.18e+20 | 7.48735e-15 | 1 | dsx |
| Report | srcpi bgdpi arf | 3 | X033603.84-173518.4 | chandra | ccd3 | 263.5 | 950.056 | 8.0059 | 4.1225 | 0.000734626 | 0.000378283 | 8.0296 | 1 | 1.40469 | 0.868009 | 87.1526 | 8.14156 | 4.89536 | 3.16286 | -0.214998 | 0.528329 | A | F | 6.07e+20 | 9.90079e-15 | 1 | dx |
| Report | srcpi bgdpi arf | 2 | X033640.17-172636.6 | chandra | ccd6 | 663.333 | 882.5 | 5.58157 | 3.59808 | 0.000512168 | 0.000330162 | 8.62868 | 1 | 0.597959 | 0.492 | 17.0931 | 5.46179 | 2.79078 | 1.86052 | -0.2 | 0.756304 | F | F | 6.41e+20 | 5.78384e-15 | 1 | dx |
| Report | srcpi bgdpi arf | 4 | X033619.24-172505.3 | chandra | ccd7 | 236.1 | 893.3 | 4.66123 | 3.39792 | 0.000427717 | 0.000311795 | 8.0084 | 0.999998 | 0.492 | 0.492 | 35.7825 | 2.81678 | 3 | 1.74592 | -0.264244 | 0.75178 | F | F | 6.25e+20 | 3.45552e-15 | 1 | dx |
| Report | srcpi bgdpi arf | 3 | X033621.61-172747.5 | chandra | ccd7 | 167.1 | 563.5 | 4.74592 | 3.39792 | 0.000435488 | 0.000311795 | 9.41532 | 1 | 0.492 | 0.492 | 101.31 | 0.88979 | 2 | 2.91531 | 0.186216 | 0.713849 | F | F | 6.2e+20 | 3.31995e-15 | 1 | dx |
| Report | 1 | X033639.85-172843.5 | chandra | ccd6 | 672.833 | 624.5 | 2.91689 | 1.73205 | 0.000267656 | 0.000158934 | 3.34713 | 0.99239 | 0.492 | 0.492 | 180 | 5.30004 | F | F | 6.21e+20 | 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