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 | X040046.49+714510.9 | chandra | ccd2 | 727.264 | 519.224 | 99.7859 | 11.0907 | 0.0200527 | 0.00222876 | 154.482 | 1 | 5.97843 | 4.35208 | 94.2743 | 11.9437 | F | F | 1.36e+21 | 2.94666e-13 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 4 | X040202.31+714031.9 | chandra | ccd6 | 934.916 | 952.959 | 81.7019 | 9.48578 | 0.0164186 | 0.00190624 | 28.3967 | 1 | 2.54794 | 2.54794 | 0 | 6.34267 | F | F | 1.34e+21 | 1.89074e-13 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 3 | X040316.90+714318.8 | chandra | ccd7 | 897.93 | 486.432 | 65.5508 | 8.95588 | 0.013173 | 0.00179976 | 34.2441 | 1 | 0.394059 | 0.394059 | 0 | 0.289069 | F | F | 1.3e+21 | 1.00978e-13 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 2 | X040148.61+713656.8 | chandra | ccd6 | 1068.37 | 515.967 | 48.9071 | 7.48338 | 0.00982825 | 0.00150384 | 16.9984 | 1 | 2.83881 | 2.2687 | 176.226 | 9.20128 | F | F | 1.35e+21 | 1.18874e-13 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 1 | X040259.07+714404.4 | chandra | ccd7 | 1068.32 | 579.253 | 25.9721 | 5.09628 | 0.0052193 | 0.00102414 | 13.568 | 1 | 0.472642 | 0.472642 | 0 | 1.71677 | F | F | 1.31e+21 | 4.03998e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 2 | X040240.52+714455.7 | chandra | ccd7 | 1245.36 | 683.8 | 16.7799 | 4.09633 | 0.00337205 | 0.000823189 | 8.76591 | 1 | 0.892397 | 0.422502 | 319.538 | 3.39672 | F | F | 1.31e+21 | 2.81059e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 3 | X040201.34+713953.4 | chandra | ccd6 | 944.115 | 874.192 | 12.11 | 3.60557 | 0.0024336 | 0.000724565 | 4.20901 | 0.999851 | 1.34937 | 1.15789 | 74.9964 | 6.67976 | F | F | 1.34e+21 | 2.81435e-14 | 1 | dbx | ||||
| Report | srcpi bgdpi arf | 7 | X040340.57+714317.3 | chandra | ccd7 | 671.598 | 483.479 | 10.6238 | 3.25942 | 0.00213495 | 0.000655008 | 5.54993 | 0.999993 | 0.63875 | 0.63875 | 0 | 1.91103 | F | F | 1.3e+21 | 1.65489e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 6 | X040327.73+714928.8 | chandra | ccd7 | 794.5 | 1238 | 8.86716 | 3.1623 | 0.00178192 | 0.000635487 | 4.63225 | 0.999881 | 1.49565 | 0.702172 | 133.993 | 6.51333 | A | F | 1.29e+21 | 1.56201e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 1 | X040225.70+714219.3 | chandra | ccd6 | 709.5 | 1169.79 | 6.78929 | 2.64576 | 0.00136436 | 0.000531684 | 2.35972 | 0.988936 | 0.552602 | 0.492 | 74.8718 | 4.04196 | F | F | 1.32e+21 | 1.47941e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 6 | X040246.28+714022.3 | chandra | ccd6 | 513 | 931.5 | 5.90573 | 2.44949 | 0.0011868 | 0.000492243 | 2.05262 | 0.977525 | 0.820364 | 0.492 | 150.767 | 3.55707 | A | F | 1.32e+21 | 1.26501e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 5 | X040322.60+714632.9 | chandra | ccd7 | 843.167 | 880.333 | 5.82636 | 2.44949 | 0.00117085 | 0.000492244 | 3.04372 | 0.99546 | 0.628774 | 0.492 | 77.5598 | 3.55344 | F | F | 1.3e+21 | 9.29386e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 1 | X040204.86+714844.7 | chandra | ccd3 | 643 | 154 | 5.66005 | 2.4495 | 0.00113743 | 0.000492245 | 9.06294 | 1 | 0.668969 | 0.492 | 8.34962 | 8.0023 | F | F | 1.32e+21 | 1.46301e-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