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 | 5 | X100812.79+115948.9 | chandra | ccd1 | 527.61 | 197.035 | 105.228 | 10.7581 | 0.0339511 | 0.00347102 | 32.4615 | 1 | 0.987901 | 0.381599 | 355.88 | 2.94158 | A | F | 3.57e+20 | 0 | 1 | ds | |||||
| Report | 1 | X100911.33+115804.1 | chandra | ccd7 | 960.61 | 1022.47 | 38.4155 | 6.96366 | 0.0123945 | 0.00224677 | 12.1015 | 1 | 13.2024 | 4.72121 | 95.5836 | 12.1546 | A | F | 3.54e+20 | 0 | 1 | ds | |||||
| Report | 1 | X100842.92+115058.7 | chandra | ccd2 | 247.167 | 438.833 | 15.7078 | 4.24268 | 0.00506794 | 0.00136885 | 34.8706 | 1 | 3.48937 | 1.95338 | 41.3089 | 8.60542 | A | F | 3.53e+20 | 0 | 1 | d | |||||
| Report | 2 | X100828.31+115107.9 | chandra | ccd2 | 682.9 | 457.4 | 9.55707 | 3.16229 | 0.00308347 | 0.00102027 | 21.2163 | 1 | 1.65242 | 0.492 | 122.01 | 6.90435 | A | F | 3.54e+20 | 0 | 1 | d | |||||
| Report | 6 | X100828.65+115604.0 | chandra | ccd2 | 673.056 | 1059.28 | 8.90509 | 3 | 0.00287312 | 0.000967914 | 19.7689 | 1 | 0.492 | 0.492 | 103.628 | 2.45719 | F | F | 3.55e+20 | 0 | 1 | d | |||||
| Report | 2 | X100828.96+120208.1 | chandra | ccd3 | 989.75 | 849.375 | 7.89059 | 2.82843 | 0.0025458 | 0.000912559 | 17.737 | 1 | 0.601302 | 0.492 | 80.7023 | 4.64359 | F | F | 3.57e+20 | 0 | 1 | d | |||||
| Report | 2 | X100936.89+115327.2 | chandra | ccd7 | 196.944 | 459.833 | 7.18456 | 3.00006 | 0.00231801 | 0.000967933 | 2.26326 | 0.984713 | 5.1364 | 2.1878 | 18.7587 | 18.9074 | A | F | 3.5e+20 | 0 | 1 | d | |||||
| Report | 1 | X100849.94+115653.4 | chandra | ccd3 | 363.9 | 209.9 | 4.86077 | 2.23607 | 0.00156827 | 0.000721442 | 10.9264 | 1 | 0.723136 | 0.492 | 0.716048 | 6.97054 | F | F | 3.55e+20 | 0 | 1 | d | |||||
| Report | 4 | X100843.27+115337.1 | chandra | ccd2 | 236.7 | 760.9 | 4.81425 | 2.23607 | 0.00155326 | 0.000721442 | 10.6874 | 1 | 1.26247 | 0.492 | 81.2271 | 6.75773 | A | T | 3.54e+20 | 0 | 1 | d | |||||
| Report | 5 | X100848.14+115505.5 | chandra | ccd2 | 91.5 | 940.5 | 4.78115 | 2.23608 | 0.00154258 | 0.000721443 | 10.6139 | 0.999998 | 0.492 | 0.492 | 90 | 7.02665 | F | F | 3.54e+20 | 0 | 1 | d | |||||
| Report | 3 | X100815.88+115317.5 | chandra | ccd2 | 1053.83 | 720.833 | 2.95992 | 1.73205 | 0.000954982 | 0.000558826 | 6.57089 | 0.99994 | 0.492 | 0.492 | 45 | 4.77032 | F | T | 3.55e+20 | 0 | 1 | d | |||||
| Report | 1 | X100802.61+115422.4 | chandra | ccd0 | 442.833 | 516.833 | 2.95301 | 1.73205 | 0.000952753 | 0.000558826 | 7.04448 | 0.999965 | 0.615 | 0.492 | 45 | 5.82015 | F | F | 3.56e+20 | 0 | 1 | d | |||||
| Report | 2 | X100811.27+115612.3 | chandra | ccd0 | 184.25 | 740.25 | 3.963 | 2 | 0.00127862 | 0.000645276 | 9.45384 | 0.999999 | 0.492 | 0.492 | 90 | 3.03263 | F | F | 3.56e+20 | 0 | 1 | d | |||||
| Report | 3 | X100749.35+115457.8 | chandra | ccd0 | 838.167 | 589 | 5.49653 | 2.4495 | 0.00177339 | 0.000790303 | 13.1121 | 1 | 2.65826 | 0.664406 | 153.029 | 8.42147 | A | T | 3.57e+20 | 0 | 1 | d | |||||
| Report | 4 | X100801.72+115806.3 | chandra | ccd0 | 469.214 | 971.929 | 6.92037 | 2.64575 | 0.00223278 | 0.00085362 | 16.5087 | 1 | 0.492 | 0.492 | 71.565 | 4.89596 | F | T | 3.57e+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