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 | 1 | X142044.90+533913.9 | chandra | ccd7 | 241.761 | 965.005 | 151.896 | 12.8004 | 0.0282801 | 0.00238319 | 105.282 | 1 | 2.13914 | 2.13914 | 0 | 6.4768 | F | F | 1.09e+20 | 1.99108e-13 | 1 | dsxf | ||||
| Report | srcpi bgdpi arf | 1 | X142038.39+532414.4 | chandra | ccd6 | 194.323 | 168.177 | 25.9376 | 5.83104 | 0.00399098 | 0.000897214 | 28.2987 | 1 | 3.13314 | 2.40737 | 16.001 | 9.67549 | F | F | 1.04e+20 | 4.94821e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 9 | X142013.19+533304.9 | chandra | ccd7 | 815.266 | 214.936 | 19.6184 | 4.43232 | 0.00365257 | 0.000825214 | 13.5979 | 1 | 0.441415 | 0.441415 | 0 | 1.54411 | F | F | 1.06e+20 | 2.52657e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 8 | X142021.45+533900.6 | chandra | ccd7 | 665.526 | 937.754 | 22.4571 | 4.74054 | 0.00418109 | 0.000882599 | 15.5655 | 1 | 1.51087 | 1.51087 | 0 | 5.36697 | F | T | 1.1e+20 | 3.09038e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 1 | X141924.56+533158.8 | chandra | ccd2 | 211.961 | 705.885 | 16.9503 | 5.09914 | 0.00260812 | 0.000784597 | 19.0439 | 1 | 4.37759 | 2.57831 | 110.426 | 8.82106 | A | F | 1.08e+20 | 3.46579e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 4 | X142039.81+533423.8 | chandra | ccd7 | 332.633 | 374.833 | 13.416 | 3.87301 | 0.0020643 | 0.000595934 | 9.2989 | 1 | 0.541695 | 0.492 | 140.978 | 2.62501 | F | F | 1.06e+20 | 1.46128e-14 | 1 | dpx | ||||
| Report | srcpi bgdpi arf | 3 | X142019.79+533049.7 | chandra | ccd6 | 532.795 | 972.138 | 9.81029 | 3.13214 | 0.00172502 | 0.000550749 | 10.7033 | 1 | 1.08462 | 1.08462 | 0 | 2.84781 | F | F | 1.06e+20 | 1.77608e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 5 | X142014.79+533609.0 | chandra | ccd7 | 786.061 | 589.004 | 7.86607 | 2.80465 | 0.00146452 | 0.000522174 | 5.45213 | 0.999936 | 0.595324 | 0.595324 | 0 | 2.78811 | F | F | 1.07e+20 | 1.04446e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 2 | X142010.81+533348.6 | chandra | ccd7 | 858.268 | 303.707 | 8.27912 | 2.87735 | 0.00154142 | 0.000535708 | 5.73842 | 0.999988 | 0.436452 | 0.436452 | 0 | 1.80009 | F | F | 1.07e+20 | 1.07105e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 7 | X142022.08+533700.7 | chandra | ccd7 | 653.7 | 693.6 | 8.39721 | 3.16231 | 0.00129207 | 0.00048658 | 5.82028 | 0.999988 | 0.652793 | 0.511345 | 158.003 | 3.37727 | F | F | 1.07e+20 | 9.21986e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 3 | X142041.33+533355.3 | chandra | ccd7 | 305.056 | 317.056 | 7.79521 | 3.00002 | 0.00119944 | 0.00046161 | 5.40302 | 0.999936 | 0.675534 | 0.492 | 72.6708 | 2.75339 | F | F | 1.06e+20 | 8.56452e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 6 | X142050.74+533515.1 | chandra | ccd7 | 134.928 | 479.357 | 6.08471 | 2.64577 | 0.000936247 | 0.000407101 | 4.21744 | 0.999683 | 0.625587 | 0.492 | 125.515 | 4.4389 | F | F | 1.06e+20 | 7.65333e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 2 | X142012.52+533138.4 | chandra | ccd6 | 663.9 | 1070.5 | 4.7037 | 2.23608 | 0.000723753 | 0.000344062 | 5.13189 | 0.999761 | 0.537677 | 0.492 | 47.287 | 2.52206 | F | F | 1.06e+20 | 7.43334e-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