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 | 2 | X043113.54+585813.1 | chandra | ccd7 | 916.395 | 459.618 | 248.636 | 15.9509 | 0.0499491 | 0.00320441 | 142.78 | 1 | 0.400376 | 0.345368 | 89.952 | 0.336386 | 208.781 | 8 | -0.926193 | 0.0991225 | F | T | 3.36e+21 | 2.24171e-13 | 1 | dsxf |
| Report | srcpi bgdpi arf | 1 | X043056.09+585858.5 | chandra | ccd7 | 1190.47 | 551.888 | 38.5933 | 6.47278 | 0.00775311 | 0.00130033 | 22.1623 | 1 | 0.528319 | 0.277569 | 334.919 | 2.06934 | 8.95544 | 29.9109 | 0.539167 | 0.214102 | F | F | 3.37e+21 | 7.07009e-14 | 1 | dsx |
| Report | srcpi bgdpi arf | 1 | X043054.39+585733.7 | chandra | ccd6 | 412.453 | 1002.65 | 15.6824 | 3.9601 | 0.00315048 | 0.000795556 | 24.6198 | 1 | 0.633782 | 0.363629 | 330.62 | 2.3909 | 8.95139 | 5.85418 | -0.209192 | 0.345021 | F | F | 3.37e+21 | 3.52846e-14 | 1 | dsx |
| Report | srcpi bgdpi arf | 5 | X043121.87+585759.0 | chandra | ccd7 | 785.421 | 430.891 | 14.2104 | 3.76967 | 0.00285476 | 0.000757298 | 8.16037 | 1 | 0.574169 | 0.295738 | 53.227 | 1.40043 | 7.95639 | 4.91279 | -0.236503 | 0.378615 | F | F | 3.35e+21 | 2.72166e-14 | 1 | dsx |
| Report | srcpi bgdpi arf | 4 | X043105.60+585607.8 | chandra | ccd6 | 236.216 | 827.877 | 12.8704 | 3.58753 | 0.00258558 | 0.000720712 | 20.2053 | 1 | 0.779194 | 0.779194 | 0 | 2.44367 | 0.830785 | 11.9154 | 0.869642 | 0.493 | F | F | 3.36e+21 | 2.91083e-14 | 1 | dsx |
| Report | srcpi bgdpi arf | 3 | X043130.18+590216.5 | chandra | ccd7 | 654.928 | 953.929 | 6.77627 | 3.78388 | 0.0013613 | 0.000760151 | 14.3261 | 1 | 0.745448 | 0.492 | 69.6994 | 4.51183 | 2.88813 | 4 | 0.161417 | 0.562995 | A | F | 3.35e+21 | 1.25309e-14 | 1 | dx |
| Report | srcpi bgdpi arf | 1 | X043102.39+590757.3 | chandra | ccd3 | 341.357 | 455.5 | 6.11574 | 3.78388 | 0.0012286 | 0.000760151 | 6.50366 | 0.999996 | 3.18851 | 1.23331 | 97.0315 | 9.5813 | 1.8035 | 4.44324 | 0.42258 | 0.665343 | A | F | 3.36e+21 | 1.72669e-14 | 1 | dx |
| Report | srcpi bgdpi arf | 2 | X043052.75+590818.5 | chandra | ccd3 | 492.1 | 498.7 | 4.67115 | 3.39792 | 0.000938395 | 0.000682614 | 8.14557 | 0.999999 | 1.01338 | 0.492 | 156.949 | 10.1547 | 2.87668 | 1.83557 | -0.220936 | 0.749679 | A | T | 3.36e+21 | 1.38275e-14 | 1 | dx |
| Report | srcpi bgdpi arf | 4 | X043204.05+585934.6 | chandra | ccd7 | 122.5 | 626 | 3.60834 | 3.17945 | 0.000724886 | 0.000638726 | 5.76571 | 0.999944 | 1.48912 | 0.492 | 87.2798 | 6.84822 | 2.91607 | 0.748218 | -0.591616 | 1.02612 | A | F | 3.33e+21 | 7.43865e-15 | 1 | dx |
| Report | srcpi bgdpi arf | 3 | X043028.43+585406.1 | chandra | ccd6 | 821.167 | 580.833 | 2.81041 | 2.93649 | 0.000564589 | 0.000589918 | 6.45449 | 0.999954 | 0.878912 | 0.492 | 59.3052 | 7.0665 | 1.85781 | 0.952603 | -0.32209 | 1.12146 | A | F | 3.39e+21 | 8.46779e-15 | 1 | dx |
| Report | 2 | X043026.52+585655.9 | chandra | ccd6 | 850.167 | 926.167 | 2.77973 | 1.73206 | 0.000558426 | 0.000347957 | 4.36391 | 0.999182 | 0.649604 | 0.492 | 164.872 | 6.00737 | F | T | 3.39e+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