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 | 1 | X231246.83+052125.9 | chandra | ccd7 | 764.93 | 832.46 | 154.094 | 12.6753 | 0.019394 | 0.00159529 | 80.2964 | 1 | 1.34645 | 1.34645 | 0 | 5.30813 | F | F | 5.93e+20 | 1.35007e-13 | 1 | dsxf | ||||
| Report | srcpi bgdpi arf | 5 | X231252.07+051649.8 | chandra | ccd7 | 605.689 | 271.291 | 38.4683 | 6.55197 | 0.00484153 | 0.000824616 | 20.0453 | 1 | 0.404251 | 0.404251 | 0 | 0.803953 | F | F | 5.85e+20 | 3.63108e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 4 | X231301.58+052136.2 | chandra | ccd7 | 316.667 | 852.958 | 23.2275 | 4.89899 | 0.00292335 | 0.000616573 | 12.1036 | 1 | 0.950515 | 0.573845 | 74.4311 | 5.31935 | A | F | 5.94e+20 | 2.33673e-14 | 1 | dpbx | ||||
| Report | srcpi bgdpi arf | 2 | X231238.32+051654.6 | chandra | ccd7 | 1023.11 | 280.963 | 13.5044 | 3.75015 | 0.00169963 | 0.000471984 | 7.03697 | 1 | 0.48668 | 0.48668 | 0 | 4.19012 | F | F | 5.84e+20 | 1.54768e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 3 | X231240.47+051745.7 | chandra | ccd7 | 957.999 | 384.824 | 13.6546 | 3.69521 | 0.00171854 | 0.000465072 | 7.11523 | 1 | 0.923587 | 0.923587 | 0 | 3.83756 | F | F | 5.86e+20 | 1.45125e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 1 | X231257.09+051329.0 | chandra | ccd6 | 534.45 | 892.149 | 12.5707 | 3.54552 | 0.00158212 | 0.000446232 | 16.0276 | 1 | 0.710542 | 0.710542 | 0 | 3.09338 | F | F | 5.77e+20 | 1.69306e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 6 | X231305.13+051622.3 | chandra | ccd7 | 209.352 | 215.389 | 8.15954 | 3.87111 | 0.00102694 | 0.000487209 | 4.25183 | 0.999548 | 0.409534 | 0.409534 | 0 | 2.50657 | F | F | 5.85e+20 | 8.0872e-15 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 9 | X231247.60+051615.4 | chandra | ccd7 | 741 | 200.9 | 9.74681 | 3.16228 | 0.00122671 | 0.000397996 | 5.07893 | 0.999968 | 0.492 | 0.492 | 148.85 | 1.88229 | F | F | 5.83e+20 | 9.31645e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 1 | X231218.56+052132.7 | chandra | ccd3 | 258.346 | 747.808 | 9.04791 | 3.60562 | 0.00113919 | 0.000453971 | 11.538 | 1 | 3.52988 | 2.01807 | 60.4432 | 10.3772 | A | F | 5.87e+20 | 1.64355e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 2 | X231222.60+052024.3 | chandra | ccd3 | 135.944 | 608.871 | 22.9259 | 5.1962 | 0.00288651 | 0.000654235 | 29.2354 | 1 | 2.84485 | 2.19125 | 65.466 | 8.96297 | F | F | 5.86e+20 | 3.97143e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 3 | X231223.16+051614.5 | chandra | ccd3 | 118.944 | 101.167 | 8.4176 | 3.00001 | 0.00105983 | 0.000377721 | 10.7342 | 1 | 1.21765 | 0.676171 | 131.705 | 7.95078 | A | F | 5.78e+20 | 1.42006e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 5 | X231301.48+050948.4 | chandra | ccd6 | 400.5 | 443.25 | 3.6968 | 2.00001 | 0.000465269 | 0.000251716 | 4.71339 | 0.999559 | 0.492 | 0.492 | 129.69 | 6.91655 | F | F | 5.69e+20 | 5.39167e-15 | 1 | dx | ||||
| Report | 2 | X231300.79+051345.8 | chandra | ccd6 | 421.5 | 925.833 | 2.93568 | 1.73205 | 0.000369477 | 0.000217991 | 3.74298 | 0.996333 | 0.492 | 0.492 | 90 | 3.11664 | F | F | 5.78e+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