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 | 1 | X125520.27+000829.6 | chandra | ccd7 | 422.401 | 914.306 | 80.1158 | 9.01775 | 0.0169275 | 0.00190534 | 72.8359 | 1 | 0.472418 | 0.472418 | 0 | 0.945381 | F | F | 1.4e+20 | 0 | 1 | ds | |||||
| Report | 3 | X125512.30+000751.9 | chandra | ccd7 | 665.39 | 837.835 | 42.7284 | 6.85423 | 0.009028 | 0.00144822 | 38.8458 | 1 | 0.414137 | 0.414137 | 0 | 1.6028 | F | F | 1.4e+20 | 0 | 1 | ds | |||||
| Report | 2 | X125519.20+000942.6 | chandra | ccd7 | 455.29 | 1062.8 | 29.9588 | 5.47346 | 0.00632994 | 0.00115648 | 27.2365 | 1 | 0.554255 | 0.379004 | 80.439 | 0.929681 | F | F | 1.4e+20 | 0 | 1 | ds | |||||
| Report | 1 | X125607.69+000209.5 | chandra | ccd3 | 122.849 | 909.815 | 46.1137 | 8.82734 | 0.00974328 | 0.00186511 | 8.17636 | 1 | 10.633 | 6.67941 | 10.4241 | 14.3741 | F | F | 1.39e+20 | 0 | 1 | ds | |||||
| Report | 9 | X125527.56+000618.8 | chandra | ccd7 | 200.301 | 648.573 | 23.8323 | 4.88183 | 0.00503548 | 0.00103147 | 21.6667 | 1 | 1.12179 | 0.690462 | 357.262 | 3.73506 | A | F | 1.39e+20 | 0 | 1 | ds | |||||
| Report | 6 | X125526.03+000418.9 | chandra | ccd7 | 246.84 | 404.901 | 28.4823 | 5.71773 | 0.00601797 | 0.00120809 | 25.8942 | 1 | 1.20095 | 1.20095 | 0 | 5.16914 | F | F | 1.39e+20 | 0 | 1 | ds | |||||
| Report | 4 | X125513.46+000911.7 | chandra | ccd7 | 630.184 | 999.955 | 17.8916 | 4.22985 | 0.00378028 | 0.000893715 | 16.2658 | 1 | 0.427652 | 0.427652 | 0 | 0.913092 | F | F | 1.4e+20 | 0 | 1 | ds | |||||
| Report | 2 | X125545.32-000023.3 | chandra | ccd3 | 804.29 | 598.71 | 13.2624 | 4.35901 | 0.00280217 | 0.000921001 | 2.35154 | 0.989464 | 5.56771 | 3.13409 | 28.6319 | 11.7299 | A | F | 1.39e+20 | 0 | 1 | d | |||||
| Report | 5 | X125517.27+000959.9 | chandra | ccd7 | 513.5 | 1097.5 | 8.84525 | 3 | 0.00186889 | 0.000633861 | 8.04151 | 1 | 0.492 | 0.492 | 124.099 | 1.03964 | F | F | 1.4e+20 | 0 | 1 | d | |||||
| Report | 1 | X125613.21+000803.2 | chandra | ccd2 | 405.9 | 649.3 | 7.55434 | 3.16233 | 0.00159613 | 0.000668159 | 13.6747 | 1 | 3.41474 | 1.51078 | 3.0672 | 14.0849 | A | F | 1.39e+20 | 0 | 1 | d | |||||
| Report | 7 | X125503.18+000938.5 | chandra | ccd7 | 943 | 1054 | 3.90821 | 2 | 0.000825754 | 0.000422574 | 3.55309 | 0.998437 | 0.492 | 0.492 | 45 | 3.51865 | F | F | 1.4e+20 | 0 | 1 | d | |||||
| Report | 8 | X125506.14+000406.8 | chandra | ccd7 | 852.75 | 379.75 | 3.84437 | 2 | 0.000812265 | 0.000422575 | 3.49504 | 0.998437 | 0.513971 | 0.492 | 155.817 | 5.55529 | F | F | 1.4e+20 | 0 | 1 | d | |||||
| Report | 2 | X125554.19+000949.7 | chandra | ccd2 | 985.75 | 865.75 | 3.58471 | 2.00001 | 0.000757402 | 0.000422577 | 6.48897 | 0.999717 | 0.492 | 0.492 | 154.33 | 9.34119 | F | F | 1.39e+20 | 0 | 1 | d | |||||
| Report | 2 | X125521.82+001159.0 | chandra | ccd6 | 853.833 | 393.5 | 2.9554 | 1.73205 | 0.000624437 | 0.00036596 | 5.05232 | 0.999565 | 0.492 | 0.492 | 180 | 3.25376 | F | F | 1.4e+20 | 0 | 1 | d | |||||
| Report | 1 | X125524.57+001332.5 | chandra | ccd6 | 769.833 | 583.5 | 2.92433 | 1.73205 | 0.000617874 | 0.00036596 | 4.99921 | 0.999565 | 0.678423 | 0.492 | 118.155 | 4.95649 | F | F | 1.4e+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