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 | 1 | X035348.83-102015.7 | chandra | ccd6 | 1118.08 | 784.14 | 78.8073 | 9.53825 | 0.00801001 | 0.000969472 | 31.9463 | 1 | 1.92293 | 1.26959 | 30.4271 | 4.89292 | 56.5528 | 30.4969 | -0.299322 | 0.125117 | F | F | 3.41e+20 | 9.49625e-14 | 1 | dsx |
Report | srcpi bgdpi arf | 1 | X035322.84-102810.4 | chandra | ccd7 | 1224.3 | 617.234 | 45.8919 | 7.26045 | 0.00466447 | 0.000737955 | 36.3914 | 1 | 2.2615 | 1.25271 | 96.2267 | 6.60292 | 42.9681 | 4.45221 | -0.812224 | 0.221183 | F | F | 3.31e+20 | 3.86925e-14 | 1 | dsx |
Report | srcpi bgdpi arf | 11 | X035318.61-102718.9 | chandra | ccd7 | 1350.79 | 721.286 | 25.3921 | 6.3619 | 0.00258086 | 0.000646626 | 15.7235 | 1 | 1.76369 | 1.1809 | 73.9592 | 7.23836 | 22.4898 | 2.92281 | -0.769971 | 0.31246 | F | F | 3.3e+20 | 2.54253e-14 | 1 | dx |
Report | srcpi bgdpi arf | 2 | X035405.43-102116.4 | chandra | ccd6 | 619.889 | 660.278 | 16.8376 | 5.33013 | 0.00171138 | 0.000541756 | 15.6173 | 1 | 1.82556 | 0.963884 | 159.687 | 6.01498 | 11.6871 | 5.23998 | -0.380874 | 0.338774 | A | F | 3.45e+20 | 1.98073e-14 | 1 | dx |
Report | srcpi bgdpi arf | 8 | X035346.68-103127.0 | chandra | ccd7 | 509.495 | 217.731 | 18.1038 | 4.25486 | 0.00184008 | 0.000432467 | 14.356 | 1 | 1.5782 | 1.5782 | 0 | 6.31537 | 12.1533 | 3.81457 | -0.522218 | 0.378612 | F | F | 3.35e+20 | 2.10107e-14 | 1 | dsx |
Report | srcpi bgdpi arf | 7 | X035351.07-102432.2 | chandra | ccd7 | 377.794 | 1060.81 | 14.0779 | 3.83989 | 0.00143088 | 0.000390288 | 11.1635 | 1 | 0.378866 | 0.378866 | 0 | 1.23541 | 10.8305 | 4 | -0.460571 | 0.371183 | F | F | 3.4e+20 | 1.09016e-14 | 1 | dsx |
Report | srcpi bgdpi arf | 5 | X035346.95-102519.8 | chandra | ccd7 | 501.444 | 963.978 | 13.1857 | 3.63121 | 0.0013402 | 0.000369078 | 10.456 | 1 | 0.407445 | 0.316205 | 142.807 | 0.204853 | 9.93417 | 2.93417 | -0.543971 | 0.419464 | F | F | 3.38e+20 | 1.00658e-14 | 1 | dsx |
Report | srcpi bgdpi arf | 6 | X035333.49-102451.1 | chandra | ccd7 | 905.141 | 1022.31 | 11.4788 | 3.38804 | 0.00116671 | 0.000344362 | 9.10248 | 1 | 0.867451 | 0.419018 | 59.6321 | 3.25695 | 7.9591 | 3.63189 | -0.373325 | 0.424125 | F | F | 3.35e+20 | 9.31427e-15 | 1 | dsx |
Report | srcpi bgdpi arf | 3 | X035345.22-102556.7 | chandra | ccd7 | 552.75 | 888.625 | 7.83061 | 3.95804 | 0.000795906 | 0.000402296 | 19.0264 | 1 | 0.492 | 0.492 | 174.608 | 0.882851 | 5 | 3 | -0.25 | 0.515388 | F | F | 3.38e+20 | 5.96097e-15 | 1 | dx |
Report | srcpi bgdpi arf | 2 | X035358.58-102620.8 | chandra | ccd7 | 152.214 | 839.5 | 6.67505 | 3.78388 | 0.000678454 | 0.000384595 | 11.7097 | 1 | 0.513076 | 0.492 | 5.98807 | 3.1658 | 1.91876 | 4.75629 | 0.425094 | 0.623213 | F | F | 3.4e+20 | 5.5834e-15 | 1 | dx |
Report | srcpi bgdpi arf | 10 | X035341.63-102646.2 | chandra | ccd7 | 660.5 | 788 | 5.65822 | 3.59808 | 0.000575103 | 0.000365709 | 9.67847 | 1 | 0.610109 | 0.492 | 64.1837 | 2.05087 | 4 | 1.72658 | -0.396995 | 0.684971 | F | F | 3.36e+20 | 4.33301e-15 | 1 | dx |
Report | srcpi bgdpi arf | 9 | X035330.24-102719.7 | chandra | ccd7 | 1001.83 | 719.833 | 5.48881 | 3.59808 | 0.000557884 | 0.000365709 | 7.67694 | 0.999999 | 0.815949 | 0.492 | 89.2656 | 4.59685 | 0.846644 | 3.79552 | 0.635238 | 0.880328 | A | F | 3.33e+20 | 4.37504e-15 | 1 | dx |
Report | srcpi bgdpi arf | 4 | X035350.21-102533.6 | chandra | ccd7 | 403.25 | 935.5 | 3.83061 | 3.17945 | 0.000389345 | 0.00032316 | 9.30741 | 0.999999 | 0.492 | 0.492 | 180 | 0.964514 | 3 | 0.915307 | -0.532447 | 0.936375 | F | F | 3.39e+20 | 2.93347e-15 | 1 | dx |
Report | srcpi bgdpi arf | 4 | X035400.83-101938.4 | chandra | ccd6 | 757.625 | 859.375 | 9.25386 | 4.27872 | 0.000940565 | 0.00043489 | 10.7131 | 1 | 1.62712 | 0.716909 | 8.40435 | 6.50595 | 5.81347 | 3.4777 | -0.251396 | 0.479051 | A | F | 3.45e+20 | 1.16597e-14 | 1 | dx |
Report | srcpi bgdpi arf | 5 | X035358.37-101745.1 | chandra | ccd6 | 831.346 | 1089.73 | 11.7344 | 4.7081 | 0.00119269 | 0.000478532 | 10.4307 | 1 | 1.91116 | 1.24198 | 172.95 | 7.92595 | 7.83492 | 5.00954 | -0.219969 | 0.388454 | A | F | 3.44e+20 | 1.4778e-14 | 1 | dx |
Report | srcpi bgdpi arf | 6 | X035349.42-102129.1 | chandra | ccd6 | 1100.47 | 635.013 | 18.7437 | 4.3294 | 0.00190511 | 0.000440041 | 7.59817 | 1 | 1.63085 | 0.892752 | 36.3466 | 3.70956 | 10.6755 | 6.5365 | -0.240474 | 0.320221 | T | F | 3.41e+20 | 2.11019e-14 | 1 | dsx |
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