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 | 9 | X111238.11+132245.0 | chandra | ccd2 | 761.425 | 911.901 | 61.4777 | 8.2774 | 0.012512 | 0.00168462 | 30.2338 | 1 | 0.933177 | 0.379471 | 7.64377 | 4.02016 | A | F | 1.57e+20 | 0 | 1 | ds | |||||
Report | srcpi bgdpi arf | 4 | X111255.58+133205.7 | chandra | ccd1 | 391.451 | 614.629 | 33.1575 | 5.75825 | 0.00674822 | 0.00117192 | 50.0534 | 1 | 2.18604 | 0.851058 | 300.139 | 6.2449 | A | F | 1.57e+20 | 8.44679e-14 | 1 | dsx | ||||
Report | srcpi bgdpi arf | 6 | X111218.04+132108.3 | chandra | ccd2 | 1356.82 | 715.456 | 33.1506 | 5.86365 | 0.00674682 | 0.00119337 | 16.3029 | 1 | 4.51885 | 2.66725 | 351.865 | 8.44505 | F | F | 1.53e+20 | 9.42344e-14 | 1 | dsx | ||||
Report | srcpi bgdpi arf | 3 | X111253.84+133305.9 | chandra | ccd1 | 442.389 | 736.389 | 8.27143 | 3.00002 | 0.00168339 | 0.00061056 | 12.4863 | 1 | 1.27331 | 0.744247 | 67.5638 | 7.03833 | A | F | 1.56e+20 | 2.25766e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 8 | X111253.53+132030.1 | chandra | ccd2 | 303.5 | 637.125 | 7.29792 | 2.82844 | 0.00148526 | 0.000575641 | 3.589 | 0.998793 | 1.58821 | 0.842185 | 149.034 | 6.21618 | A | F | 1.58e+20 | 1.97512e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 1 | X111204.39+132717.0 | chandra | ccd0 | 1106.62 | 628.75 | 6.08379 | 2.82847 | 0.00123973 | 0.000576374 | 9.81029 | 1 | 2.07941 | 1.39494 | 5.25787 | 9.96858 | F | F | 1.51e+20 | 1.81792e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 2 | X111216.31+133055.7 | chandra | ccd0 | 753.083 | 1073 | 9.70976 | 3.46414 | 0.00197862 | 0.000705909 | 15.6573 | 1 | 3.19375 | 2.08459 | 179.611 | 8.37291 | A | F | 1.52e+20 | 2.75233e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 3 | X111217.58+133000.4 | chandra | ccd0 | 715.458 | 960.625 | 22.4267 | 4.899 | 0.00457003 | 0.000998298 | 36.1638 | 1 | 1.6893 | 1.16828 | 26.989 | 7.63714 | F | F | 1.52e+20 | 6.4623e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 2 | X111259.76+132532.3 | chandra | ccd3 | 905.833 | 666.5 | 5.67738 | 2.4495 | 0.00115545 | 0.000498519 | 5.89697 | 0.999948 | 0.610139 | 0.492 | 19.6447 | 3.6341 | F | F | 1.57e+20 | 1.40295e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 5 | X111249.74+132025.3 | chandra | ccd2 | 415.833 | 627.5 | 5.60864 | 2.4495 | 0.00114146 | 0.000498519 | 2.75824 | 0.989929 | 1.04324 | 0.492 | 172.868 | 6.05804 | A | F | 1.58e+20 | 1.50676e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 1 | X111254.41+132607.0 | chandra | ccd3 | 1064.64 | 736.928 | 5.28598 | 2.64579 | 0.0010758 | 0.000538468 | 5.49044 | 0.999948 | 0.591467 | 0.492 | 80.2317 | 2.24876 | F | F | 1.57e+20 | 1.30489e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 3 | X111256.43+132740.8 | chandra | ccd3 | 1004.7 | 927.7 | 4.79377 | 2.23607 | 0.000975623 | 0.000455083 | 4.97919 | 0.999599 | 0.492 | 0.492 | 45 | 3.01966 | F | F | 1.57e+20 | 1.14492e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 4 | X111207.39+133037.0 | chandra | ccd0 | 1017.5 | 1035.1 | 4.56539 | 2.23608 | 0.000930316 | 0.00045566 | 7.36182 | 0.999949 | 0.990526 | 0.492 | 178.355 | 10.1268 | A | F | 1.51e+20 | 1.37978e-14 | 1 | dx | ||||
Report | 5 | X111218.59+133128.3 | chandra | ccd0 | 685.5 | 1139.17 | 5.79989 | 2.44949 | 0.00118188 | 0.000499148 | 9.35249 | 1 | 0.492 | 0.492 | 90 | 8.23746 | F | F | 1.52e+20 | 0 | 1 | d | |||||
Report | srcpi bgdpi arf | 1 | X111231.96+133509.2 | chandra | ccd1 | 1091.1 | 987.1 | 4.33457 | 2.23609 | 0.000882167 | 0.000455086 | 6.54333 | 0.999906 | 0.893328 | 0.793052 | 97.4657 | 9.34815 | F | F | 1.55e+20 | 1.43872e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 6 | X111226.51+132523.1 | chandra | ccd0 | 450.833 | 396.833 | 2.95939 | 1.73205 | 0.000603053 | 0.00035295 | 4.77211 | 0.999329 | 0.492 | 0.492 | 45 | 4.65686 | F | F | 1.52e+20 | 7.43535e-15 | 1 | dx | ||||
Report | srcpi bgdpi arf | 7 | X111223.52+132716.1 | chandra | ccd0 | 539.5 | 626.5 | 2.96924 | 1.73205 | 0.000605059 | 0.00035295 | 4.78799 | 0.999329 | 0.492 | 0.492 | 90 | 5.35118 | F | F | 1.52e+20 | 7.69993e-15 | 1 | dx | ||||
Report | srcpi bgdpi arf | 5 | X111258.01+132733.5 | chandra | ccd3 | 957.833 | 912.833 | 2.8855 | 1.73205 | 0.000587254 | 0.000352506 | 2.99711 | 0.98517 | 0.492 | 0.492 | 45 | 3.32536 | F | F | 1.57e+20 | 6.93911e-15 | 1 | dx | ||||
Report | 8 | X111215.41+132527.6 | chandra | ccd0 | 780.167 | 406.167 | 2.84489 | 1.73206 | 0.00057972 | 0.000352951 | 4.58747 | 0.999329 | 0.492 | 0.492 | 45 | 7.30793 | F | F | 1.52e+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