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 | 5 | X035217.04-735701.3 | chandra | ccd1 | 198.939 | 724.204 | 96.7106 | 10.9452 | 0.0107921 | 0.0012214 | 23.3837 | 1 | 1.80446 | 0.897601 | 322.04 | 6.36751 | 70.4416 | 40.0313 | -0.275274 | 0.109632 | F | F | 9.51e+20 | 1.33363e-13 | 1 | dsx |
| Report | srcpi bgdpi arf | 2 | X035542.19-741408.0 | chandra | ccd6 | 456.635 | 491.975 | 79.5588 | 10.4736 | 0.00887808 | 0.00116877 | 25.8926 | 1 | 4.86654 | 4.45746 | 44.4071 | 17.1056 | 57.3025 | 20.5092 | -0.472851 | 0.147572 | F | F | 1.03e+21 | 1.33685e-13 | 1 | dx |
| Report | srcpi bgdpi arf | 1 | X035543.82-741344.7 | chandra | ccd6 | 442.539 | 539.231 | 87.5974 | 11.0374 | 0.00977512 | 0.00123168 | 24.8734 | 1 | 7.3417 | 4.20833 | 119.948 | 16.9526 | 62.644 | 24.3912 | -0.43951 | 0.138054 | A | F | 1.03e+21 | 1.59935e-13 | 1 | dx |
| Report | srcpi bgdpi arf | 1 | X035317.15-740116.8 | chandra | ccd3 | 673.066 | 487.2 | 12.0446 | 3.47053 | 0.00134408 | 0.000387283 | 8.09997 | 1 | 0.895587 | 0.895587 | 0 | 3.97552 | 5.40715 | 5.66123 | 0.0229554 | 0.41621 | F | F | 9.73e+20 | 1.66543e-14 | 1 | dsx |
| Report | srcpi bgdpi arf | 3 | X035119.02-735553.2 | chandra | ccd1 | 688.706 | 861.2 | 10.3316 | 4.63194 | 0.00115293 | 0.000516889 | 2.49808 | 0.99048 | 1.82349 | 1.82349 | 0 | 8.84588 | 2.81462 | 6.96791 | 0.424563 | 0.526583 | F | F | 9.41e+20 | 1.53696e-14 | 1 | dsx |
| Report | srcpi bgdpi arf | 1 | X035042.21-735944.4 | chandra | ccd1 | 995.346 | 388.961 | 11.0942 | 4.7081 | 0.00123801 | 0.000525383 | 8.03621 | 1 | 1.78036 | 1.3818 | 80.3308 | 8.11062 | 3.34281 | 7.81707 | 0.400923 | 0.45776 | F | F | 9.53e+20 | 1.61215e-14 | 1 | dx |
| Report | srcpi bgdpi arf | 4 | X035140.57-735506.2 | chandra | ccd1 | 506.633 | 956.967 | 11.033 | 4.96863 | 0.00123119 | 0.000554456 | 5.53939 | 0.999996 | 3.21942 | 1.60465 | 53.3292 | 8.86536 | 6.1009 | 5.0587 | -0.0933906 | 0.449994 | A | F | 9.4e+20 | 1.65253e-14 | 1 | dbx |
| Report | srcpi bgdpi arf | 6 | X035314.86-740732.6 | chandra | ccd2 | 433.3 | 734 | 9.92386 | 4.27872 | 0.00110742 | 0.000477468 | 35.9641 | 1 | 0.547593 | 0.492 | 106.934 | 5.29111 | 8.92386 | 1 | -0.798465 | 0.556622 | F | F | 1e+21 | 1.43488e-14 | 1 | dx |
| Report | srcpi bgdpi arf | 2 | X035322.46-740859.5 | chandra | ccd2 | 370.6 | 557 | 8.62092 | 4.1225 | 0.00096202 | 0.000460035 | 14.0019 | 1 | 1.47954 | 0.602185 | 120.361 | 6.77238 | 3.89661 | 4.7243 | 0.0960095 | 0.485032 | A | F | 1.01e+21 | 1.47707e-14 | 1 | dx |
| Report | srcpi bgdpi arf | 3 | X035307.95-740702.9 | chandra | ccd2 | 490.722 | 794.5 | 8.72085 | 4.1225 | 0.000973172 | 0.000460035 | 16.5059 | 1 | 0.746745 | 0.492 | 152.064 | 4.61146 | 3.94417 | 4.77668 | 0.095462 | 0.479449 | A | F | 9.97e+20 | 1.20671e-14 | 1 | dx |
| Report | srcpi bgdpi arf | 1 | X035110.44-740423.2 | chandra | ccd0 | 460 | 814.75 | 7.93967 | 3.95804 | 0.000886306 | 0.000441836 | 32.3259 | 1 | 0.690336 | 0.492 | 21.8014 | 5.40863 | 3 | 4.93967 | 0.244301 | 0.518615 | F | F | 9.75e+20 | 1.09691e-14 | 1 | dx |
| Report | srcpi bgdpi arf | 1 | X035219.32-740333.9 | chandra | ccd2 | 896.786 | 1219.64 | 6.22573 | 3.78388 | 0.000694738 | 0.000422249 | 7.07529 | 0.999998 | 0.538267 | 0.492 | 86.9638 | 0.619375 | 4.45801 | 1.69029 | -0.45016 | 0.682863 | F | F | 9.76e+20 | 9.21075e-15 | 1 | dx |
| Report | srcpi bgdpi arf | 5 | X035258.77-740931.6 | chandra | ccd2 | 568 | 492.5 | 5.59603 | 3.59808 | 0.000624469 | 0.000401514 | 8.80455 | 1 | 0.722036 | 0.492 | 16.4143 | 6.53086 | 4.82687 | 1.76916 | -0.463568 | 0.639745 | F | F | 1.01e+21 | 8.19072e-15 | 1 | dx |
| Report | srcpi bgdpi arf | 4 | X035255.97-740516.3 | chandra | ccd2 | 590.3 | 1011.3 | 4.74592 | 3.39792 | 0.000529604 | 0.000379178 | 9.41532 | 1 | 0.492 | 0.492 | 35.1731 | 2.72751 | 2.74592 | 2 | -0.157171 | 0.735755 | F | F | 9.86e+20 | 6.37504e-15 | 1 | dx |
| Report | 3 | X035138.11-740554.5 | chandra | ccd0 | 227.833 | 630.167 | 2.89751 | 1.73205 | 0.00032345 | 0.000193349 | 3.60702 | 0.995664 | 0.543766 | 0.492 | 145.278 | 4.26046 | F | F | 9.85e+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