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 | X123227.93+112811.6 | chandra | ccd5 | 414.04 | 250.677 | 79.8577 | 13.1039 | 0.0156894 | 0.00257448 | 8.33239 | 1 | 7.31784 | 7.31784 | 0 | 12.2236 | F | F | 2.41e+20 | 1.48267e-13 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 12 | X123220.46+111238.6 | chandra | ccd7 | 606.512 | 435.299 | 21.0594 | 4.58905 | 0.00413749 | 0.000901601 | 18.0864 | 1 | 0.816169 | 0.42723 | 329.742 | 3.43507 | F | F | 2.42e+20 | 3.16208e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 2 | X123216.43+111650.9 | chandra | ccd7 | 726.903 | 948.225 | 11.436 | 3.80464 | 0.00224681 | 0.00074749 | 9.82157 | 1 | 0.698256 | 0.272428 | 104.916 | 1.75543 | A | F | 2.41e+20 | 1.6652e-14 | 1 | dsx | ||||
| Report | 9 | X123222.23+111810.3 | chandra | ccd6 | 569 | 68 | 9.87843 | 3.16228 | 0.00194078 | 0.000621283 | 13.1868 | 1 | 0.492 | 0.492 | 151.845 | 2.14422 | F | F | 2.42e+20 | 0 | 1 | d | |||||
| Report | srcpi bgdpi arf | 3 | X123207.09+112013.7 | chandra | ccd6 | 1021.38 | 318.875 | 7.75786 | 2.82843 | 0.00152416 | 0.000555693 | 10.3561 | 1 | 0.606139 | 0.540486 | 156.355 | 5.68935 | F | F | 2.4e+20 | 1.83324e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 4 | X123211.78+111453.1 | chandra | ccd7 | 865.5 | 708.25 | 7.75428 | 2.82843 | 0.00152346 | 0.000555693 | 6.65961 | 0.999998 | 0.662419 | 0.492 | 69.1832 | 2.92732 | F | F | 2.41e+20 | 1.17163e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 6 | X123207.54+111722.6 | chandra | ccd7 | 992 | 1012.12 | 7.60052 | 2.82844 | 0.00149325 | 0.000555694 | 6.52755 | 0.999987 | 0.759414 | 0.492 | 91.0273 | 3.96631 | A | F | 2.4e+20 | 1.28244e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 3 | X123220.45+111430.4 | chandra | ccd7 | 606.071 | 662.072 | 6.70534 | 2.64576 | 0.00131738 | 0.000519803 | 5.75874 | 0.999987 | 0.688669 | 0.492 | 79.8118 | 1.62642 | T | F | 2.42e+20 | 9.71469e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 8 | X123208.09+112559.8 | chandra | ccd6 | 991.5 | 1022.38 | 6.30661 | 2.82848 | 0.00123904 | 0.000555701 | 8.41876 | 0.999998 | 2.639 | 0.492 | 60.7543 | 10.5949 | A | F | 2.39e+20 | 1.62836e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 1 | X123220.98+111640.3 | chandra | ccd7 | 590.167 | 926 | 5.85473 | 2.44949 | 0.00115026 | 0.000481244 | 5.02821 | 0.999914 | 0.492 | 0.492 | 120.779 | 0.77405 | F | F | 2.42e+20 | 8.52891e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 9 | X123225.96+111102.8 | chandra | ccd7 | 441.5 | 240.167 | 5.66472 | 2.4495 | 0.00111293 | 0.000481245 | 4.86503 | 0.999914 | 0.615146 | 0.492 | 12.6731 | 5.04538 | F | F | 2.43e+20 | 8.68982e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 1 | X123230.95+111823.7 | chandra | ccd6 | 308.3 | 95.2998 | 4.8739 | 2.23607 | 0.00095756 | 0.000439313 | 6.50623 | 0.999973 | 0.605247 | 0.492 | 147.732 | 3.1008 | F | F | 2.43e+20 | 1.02406e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 4 | X123213.45+111819.8 | chandra | ccd6 | 831.5 | 87.2998 | 4.87322 | 2.23607 | 0.000957426 | 0.000439313 | 6.50533 | 0.999973 | 0.673358 | 0.492 | 167.778 | 3.24009 | F | F | 2.41e+20 | 1.0254e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 5 | X123223.35+111546.6 | chandra | ccd7 | 519.5 | 816.9 | 4.75437 | 2.23607 | 0.000934075 | 0.000439314 | 4.08319 | 0.999484 | 0.492 | 0.492 | 2.77269e-08 | 0.292622 | F | F | 2.42e+20 | 6.84628e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 11 | X123209.18+111308.6 | chandra | ccd7 | 943.25 | 495.75 | 3.79903 | 2.00001 | 0.000746384 | 0.000392935 | 3.26272 | 0.997261 | 0.492 | 0.492 | 45 | 4.40912 | F | F | 2.41e+20 | 6.10614e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 8 | X123227.13+111033.6 | chandra | ccd7 | 406.5 | 180.75 | 3.77089 | 2.00001 | 0.000740853 | 0.000392935 | 3.23855 | 0.997261 | 0.538384 | 0.492 | 14.4433 | 5.57511 | F | F | 2.43e+20 | 5.90619e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 10 | X123235.74+111131.5 | chandra | ccd7 | 148.833 | 298.5 | 3.63328 | 2.00001 | 0.000713819 | 0.000392936 | 3.12037 | 0.987422 | 0.492 | 0.492 | 180 | 5.51674 | F | F | 2.44e+20 | 6.17333e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 7 | X123219.65+110954.1 | chandra | ccd7 | 630 | 100.5 | 3.39587 | 2.00002 | 0.000667175 | 0.000392937 | 2.91647 | 0.987422 | 0.760713 | 0.521845 | 2.35031e-08 | 6.17676 | F | F | 2.43e+20 | 5.45302e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 7 | X123218.17+112124.2 | chandra | ccd6 | 690.167 | 462.167 | 2.94674 | 1.73205 | 0.000578936 | 0.000340291 | 3.93364 | 0.997351 | 0.492 | 0.492 | 45 | 5.48884 | F | F | 2.41e+20 | 6.41181e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 6 | X123218.06+112120.9 | chandra | ccd6 | 693.5 | 455.5 | 2.88362 | 1.73206 | 0.000566535 | 0.000340291 | 3.84938 | 0.997351 | 0.521845 | 0.492 | 2.35031e-08 | 5.44107 | F | F | 2.41e+20 | 6.26053e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 5 | X123220.15+111957.5 | chandra | ccd6 | 631.167 | 285.833 | 2.87774 | 1.73206 | 0.00056538 | 0.000340291 | 3.84153 | 0.997351 | 0.492 | 0.492 | 16.845 | 3.97841 | F | F | 2.41e+20 | 6.08734e-15 | 1 | dx | ||||
| Report | 2 | X123208.51+111947.4 | chandra | ccd6 | 979 | 265.5 | 1.94993 | 1.41422 | 0.000383096 | 0.000277846 | 2.60298 | 0.980547 | 0.492 | 0.492 | 180 | 5.13204 | F | F | 2.4e+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