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 | X014419.02+173108.6 | chandra | ccd5 | 679.558 | 1073.91 | 17.3104 | 8.1894 | 0.00548992 | 0.00259724 | 2.45406 | 0.99196 | 2.12514 | 2.12514 | 0 | 10.9864 | F | F | 4.71e+20 | 5.21803e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 1 | X014409.68+173245.7 | chandra | ccd6 | 616.032 | 300.122 | 23.7269 | 4.87103 | 0.00752488 | 0.00154482 | 45.3929 | 1 | 4.44945 | 4.44945 | 0 | 8.72872 | F | F | 4.72e+20 | 9.26123e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 8 | X014355.31+173917.3 | chandra | ccd7 | 696.646 | 120.192 | 16.7265 | 4.0898 | 0.00530475 | 0.00129707 | 6.2071 | 0.999999 | 0.675333 | 0.675333 | 0 | 2.33808 | F | F | 4.73e+20 | 4.02934e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 6 | X014342.56+174527.3 | chandra | ccd7 | 1066.98 | 872.337 | 11.041 | 5.05611 | 0.00350162 | 0.00160353 | 4.09725 | 0.999795 | 0.954907 | 0.954907 | 0 | 6.06234 | F | F | 4.73e+20 | 2.82867e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 5 | X014342.87+174526.7 | chandra | ccd7 | 1057.3 | 870.5 | 13.8888 | 3.873 | 0.00440473 | 0.00122829 | 5.15406 | 0.999992 | 0.937615 | 0.771393 | 107.556 | 5.98855 | F | F | 4.73e+20 | 3.54313e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 3 | X014411.48+174315.5 | chandra | ccd7 | 226.5 | 603.722 | 8.86228 | 3 | 0.0028106 | 0.000951427 | 3.28874 | 0.998593 | 0.798593 | 0.492 | 56.479 | 3.25845 | A | F | 4.73e+20 | 2.25825e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 4 | X014406.91+174452.8 | chandra | ccd7 | 359.5 | 801.625 | 7.72499 | 2.82843 | 0.00244992 | 0.000897015 | 2.8667 | 0.992169 | 0.896206 | 0.492 | 76.9638 | 3.92876 | A | F | 4.73e+20 | 1.91661e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 7 | X014349.53+174621.4 | chandra | ccd7 | 864.125 | 981.625 | 7.64143 | 2.82843 | 0.00242342 | 0.000897016 | 2.83569 | 0.992169 | 0.66219 | 0.492 | 46.5264 | 5.77803 | F | F | 4.73e+20 | 1.90687e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 5 | X014360.00+173900.8 | chandra | ccd6 | 897.167 | 1062.17 | 5.90542 | 2.44949 | 0.00187286 | 0.000776837 | 11.2979 | 1 | 0.662511 | 0.492 | 88.6368 | 2.22826 | F | F | 4.73e+20 | 1.95561e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 2 | X014418.45+173514.4 | chandra | ccd6 | 360.7 | 602.1 | 4.84506 | 2.23607 | 0.00153657 | 0.000709153 | 9.26927 | 1 | 0.959552 | 0.492 | 162.588 | 7.32843 | A | T | 4.71e+20 | 1.92122e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 1 | X014339.63+173328.1 | chandra | ccd2 | 144.1 | 616.1 | 4.54176 | 2.23608 | 0.00144038 | 0.000709156 | 8.88095 | 0.999992 | 1.68116 | 1.49993 | 123.898 | 9.25452 | F | F | 4.73e+20 | 2.01796e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 4 | X014352.71+173820.0 | chandra | ccd6 | 1108.75 | 979.25 | 3.95723 | 2 | 0.001255 | 0.000634285 | 7.57073 | 0.99999 | 0.492 | 0.492 | 45 | 3.47682 | F | F | 4.73e+20 | 1.36184e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 3 | X014417.54+173748.1 | chandra | ccd6 | 387.5 | 914.5 | 2.91549 | 1.73205 | 0.000924625 | 0.000549307 | 5.57774 | 0.999813 | 0.624964 | 0.492 | 106.845 | 5.26845 | F | F | 4.72e+20 | 1.07163e-14 | 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