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 | 8 | X130320.82+191756.1 | chandra | ccd6 | 592.29 | 673.867 | 211.654 | 14.5483 | 0.0212208 | 0.00145864 | 72.0558 | 1 | 2.47079 | 2.47079 | 0 | 6.24005 | F | F | 2.21e+20 | 2.36656e-13 | 1 | dsxf | ||||
| Report | srcpi bgdpi arf rmf | 1 | X130346.63+191612.9 | chandra | ccd7 | 894.617 | 609.875 | 127.152 | 24.6898 | 0.0127446 | 0.00247469 | 13.2659 | 1 | 1.79323 | 1.79323 | 0 | 0.0945484 | T | F | 2.2e+20 | 5.95713e-14 | 1 | dsxf | ||||
| Report | srcpi bgdpi arf rmf | 3 | X130424.49+192229.3 | chandra | ccd3 | 168.603 | 43.4878 | 144.547 | 12.8493 | 0.0144881 | 0.0012879 | 31.8799 | 1 | 4.20102 | 4.20102 | 0 | 11.0076 | F | F | 2.16e+20 | 1.87983e-13 | 1 | dsxf | ||||
| Report | srcpi bgdpi arf rmf | 2 | X130416.79+192803.6 | chandra | ccd3 | 390.075 | 722.251 | 106.912 | 12.3696 | 0.0107158 | 0.00123981 | 23.5794 | 1 | 6.1376 | 5.91056 | 6.50275 | 13.8845 | F | F | 2.15e+20 | 1.61566e-13 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 5 | X130307.89+191942.4 | chandra | ccd6 | 963.625 | 889.625 | 72.9599 | 9.38094 | 0.00731507 | 0.000940547 | 24.8386 | 1 | 4.1287 | 2.69855 | 84.6333 | 9.70064 | A | F | 2.21e+20 | 9.32155e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 2 | X130317.68+191328.6 | chandra | ccd6 | 682.976 | 130.151 | 14.7778 | 6.73267 | 0.00148165 | 0.000675032 | 5.03098 | 0.999987 | 0.671633 | 0.671633 | 0 | 7.27435 | F | F | 2.23e+20 | 1.94541e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 3 | X130342.20+191543.0 | chandra | ccd7 | 1022.13 | 549.081 | 46.8566 | 7.74656 | 0.00469648 | 0.000776445 | 4.88862 | 0.999997 | 0.381492 | 0.381492 | 0 | 1.06213 | F | F | 2.2e+20 | 3.5607e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 1 | X130338.52+191857.2 | chandra | ccd6 | 82.7837 | 797.816 | 38.4814 | 6.20459 | 0.00385822 | 0.000622085 | 13.1007 | 1 | 0.833903 | 0.833903 | 0 | 3.30099 | F | F | 2.2e+20 | 4.26123e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 2 | X130356.89+191750.1 | chandra | ccd7 | 599.344 | 807.477 | 16.6725 | 4.47734 | 0.0016711 | 0.000448769 | 1.73947 | 0.955742 | 0.429331 | 0.429331 | 0 | 3.004 | F | F | 2.19e+20 | 1.2834e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 1 | X130410.67+192343.5 | chandra | ccd3 | 565.605 | 193.447 | 16.0754 | 4.35894 | 0.00161124 | 0.000436898 | 3.54543 | 0.999311 | 2.48019 | 1.89742 | 38.2716 | 9.4862 | F | F | 2.17e+20 | 2.31266e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 3 | X130328.75+191445.5 | chandra | ccd6 | 364.179 | 286.408 | 11.3673 | 3.91319 | 0.00113971 | 0.000392344 | 3.8699 | 0.999359 | 1.06611 | 1.06611 | 0 | 4.3661 | F | F | 2.21e+20 | 1.44775e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 4 | X130329.96+191511.9 | chandra | ccd6 | 328.9 | 339.4 | 9.49416 | 3.16229 | 0.000951899 | 0.000317056 | 3.23221 | 0.998468 | 0.892666 | 0.492 | 12.726 | 3.96423 | A | F | 2.21e+20 | 1.18861e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 1 | X130330.36+192433.3 | chandra | ccd2 | 703.929 | 158.643 | 6.11528 | 2.64577 | 0.000612936 | 0.000265187 | 8.40376 | 0.999999 | 2.20705 | 0.739995 | 85.1901 | 9.15886 | A | F | 2.18e+20 | 9.57267e-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