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 | X024532.96+364039.4 | chandra | ccd6 | 515.737 | 867.415 | 76.7097 | 10.8631 | 0.00736565 | 0.00104307 | 93.4328 | 1 | 6.70753 | 4.34545 | 107.95 | 13.2069 | A | F | 5.71e+20 | 1.05016e-13 | 1 | dcx | ||||
Report | srcpi bgdpi arf | 2 | X024632.96+365107.3 | chandra | ccd3 | 222.15 | 743.476 | 68.6103 | 8.28313 | 0.00658796 | 0.000795346 | 45.0031 | 1 | 2.45849 | 1.45448 | 43.7734 | 7.14171 | F | F | 5.83e+20 | 8.62129e-14 | 1 | dsx | ||||
Report | srcpi bgdpi arf | 1 | X024527.32+365928.5 | chandra | ccd0 | 749.042 | 759.124 | 45.1438 | 7.3006 | 0.00433471 | 0.000701003 | 15.8084 | 1 | 3.93871 | 1.94834 | 300.316 | 9.06202 | F | F | 5.67e+20 | 7.31281e-14 | 1 | dsx | ||||
Report | srcpi bgdpi arf | 8 | X024553.66+365232.8 | chandra | ccd2 | 147.705 | 953.701 | 26.5461 | 5.4801 | 0.00254895 | 0.000526198 | 22.4321 | 1 | 0.589246 | 0.589246 | 0 | 0.976547 | F | F | 5.74e+20 | 2.99832e-14 | 1 | dsx | ||||
Report | srcpi bgdpi arf | 4 | X024603.97+365418.1 | chandra | ccd1 | 891.533 | 89.6188 | 49.8727 | 9.1483 | 0.00478878 | 0.00087842 | 8.57599 | 1 | 1.62762 | 1.62762 | 0 | 1.83819 | T | F | 5.76e+20 | 5.58141e-14 | 1 | dsx | ||||
Report | srcpi bgdpi arf | 1 | X024543.56+364532.1 | chandra | ccd2 | 394.091 | 98.1365 | 20.3055 | 4.69044 | 0.00194972 | 0.000450375 | 17.1586 | 1 | 1.56345 | 1.0539 | 28.6796 | 7.88687 | F | F | 5.74e+20 | 2.82299e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 3 | X024607.76+370142.2 | chandra | ccd1 | 798.792 | 991.833 | 20.0217 | 4.89903 | 0.00192248 | 0.000470404 | 3.44289 | 0.999165 | 3.44586 | 2.08924 | 62.5322 | 9.05362 | A | F | 5.76e+20 | 2.95711e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 7 | X024529.60+364554.6 | chandra | ccd2 | 735.577 | 144.709 | 27.2193 | 5.21721 | 0.00261359 | 0.000500956 | 23.001 | 1 | 4.89258 | 4.89258 | 0 | 9.01962 | F | F | 5.71e+20 | 3.93827e-14 | 1 | dsx | ||||
Report | srcpi bgdpi arf | 1 | X024559.72+365214.4 | chandra | ccd3 | 1033.13 | 879.278 | 15.928 | 4.68684 | 0.0015294 | 0.00045003 | 10.4476 | 1 | 0.351389 | 0.351389 | 0 | 0.6711 | F | F | 5.76e+20 | 1.74506e-14 | 1 | dsx | ||||
Report | srcpi bgdpi arf | 2 | X024624.49+370016.4 | chandra | ccd1 | 391.605 | 817.763 | 16.0342 | 4.35894 | 0.0015396 | 0.000418544 | 2.75721 | 0.994571 | 2.34126 | 1.44801 | 161.591 | 9.08195 | A | F | 5.8e+20 | 2.23843e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 3 | X024535.00+364034.9 | chandra | ccd6 | 465.833 | 858.292 | 12.1161 | 4.89917 | 0.00116339 | 0.000470417 | 14.7575 | 1 | 6.25746 | 1.98373 | 103.73 | 13.1247 | A | F | 5.72e+20 | 1.88713e-14 | 1 | dcx | ||||
Report | srcpi bgdpi arf | 5 | X024528.52+365139.9 | chandra | ccd2 | 760.5 | 846 | 9.9174 | 3.31665 | 0.000952266 | 0.000318463 | 8.38045 | 1 | 0.492 | 0.492 | 153.435 | 6.0732 | F | F | 5.69e+20 | 1.24646e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 2 | X024526.32+365806.0 | chandra | ccd0 | 773.045 | 590.864 | 9.78339 | 3.31665 | 0.000939398 | 0.000318464 | 3.42593 | 0.998047 | 1.5942 | 1.18768 | 53.2076 | 8.27192 | F | F | 5.67e+20 | 1.28448e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 3 | X024529.49+364816.9 | chandra | ccd2 | 737.4 | 433.4 | 9.24081 | 3.16229 | 0.0008873 | 0.000303642 | 7.80871 | 1 | 1.6706 | 0.688651 | 24.8601 | 7.35525 | A | F | 5.7e+20 | 1.21594e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 5 | X024601.35+364921.1 | chandra | ccd3 | 992.833 | 526.5 | 8.67143 | 3.00001 | 0.000832628 | 0.00028806 | 5.68779 | 0.999968 | 0.651301 | 0.492 | 163.764 | 3.54979 | F | F | 5.77e+20 | 1.1199e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 3 | X024539.31+365728.3 | chandra | ccd0 | 456.833 | 513.833 | 8.45362 | 3.00001 | 0.000811714 | 0.00028806 | 2.96027 | 0.995526 | 0.720155 | 0.546207 | 82.0273 | 5.98163 | F | F | 5.7e+20 | 1.04199e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 4 | X024556.36+365448.3 | chandra | ccd0 | 41.5 | 188.5 | 7.28376 | 2.82844 | 0.000699385 | 0.000271587 | 2.55062 | 0.990273 | 0.492 | 0.492 | 4.73116 | 1.99411 | F | F | 5.74e+20 | 7.94254e-15 | 1 | dx | ||||
Report | srcpi bgdpi arf | 2 | X024534.37+364030.9 | chandra | ccd6 | 481.417 | 850.083 | 7.28283 | 3.46421 | 0.000699295 | 0.000332632 | 8.87051 | 0.999999 | 6.12021 | 0.627628 | 89.5512 | 13.2335 | A | F | 5.71e+20 | 1.07201e-14 | 1 | dcx | ||||
Report | srcpi bgdpi arf | 3 | X024607.58+364820.3 | chandra | ccd3 | 840.5 | 402.928 | 6.67146 | 2.64576 | 0.000640592 | 0.000254045 | 4.37597 | 0.99931 | 0.657373 | 0.492 | 60.6319 | 4.87801 | F | F | 5.79e+20 | 8.09455e-15 | 1 | dx | ||||
Report | srcpi bgdpi arf | 4 | X024543.75+365117.6 | chandra | ccd2 | 389.1 | 800.3 | 4.76685 | 2.23607 | 0.000457712 | 0.000214707 | 4.02811 | 0.999377 | 0.492 | 0.492 | 137.382 | 3.30127 | F | F | 5.72e+20 | 5.65919e-15 | 1 | dx | ||||
Report | srcpi bgdpi arf | 2 | X024558.07+364628.1 | chandra | ccd2 | 39.75 | 211.75 | 3.70377 | 2.00001 | 0.000355635 | 0.00019204 | 3.12978 | 0.996794 | 0.614537 | 0.492 | 129.608 | 6.38182 | F | F | 5.77e+20 | 4.77464e-15 | 1 | dx | ||||
Report | srcpi bgdpi arf | 6 | X024517.49+365151.4 | chandra | ccd2 | 1029.5 | 869.75 | 3.57394 | 2.00001 | 0.000343169 | 0.000192041 | 3.02007 | 0.98573 | 1.20958 | 0.492 | 24.9569 | 8.22244 | A | F | 5.67e+20 | 4.85227e-15 | 1 | dx |
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