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 | X002141.01+003841.7 | chandra | ccd6 | 669.986 | 826.903 | 155.738 | 12.5858 | 0.0568789 | 0.00459661 | 95.4088 | 1 | 1.49265 | 1.49265 | 0 | 4.66268 | F | F | 2.79e+20 | 0 | 1 | dsc | |||||
| Report | 1 | X002125.99+004510.4 | chandra | ccd7 | 738.878 | 637.129 | 76.1123 | 8.72424 | 0.0277036 | 0.00317548 | 116.258 | 1 | 0.717785 | 0.387814 | 356.753 | 2.85685 | F | F | 2.81e+20 | 0 | 1 | ds | |||||
| Report | 2 | X002133.27+004301.1 | chandra | ccd7 | 516.889 | 374.132 | 50.7137 | 7.17781 | 0.0184589 | 0.0026126 | 77.4628 | 1 | 0.399628 | 0.399628 | 0 | 0.114111 | F | F | 2.8e+20 | 0 | 1 | ds | |||||
| Report | 8 | X002132.60+004200.8 | chandra | ccd7 | 536.9 | 251.1 | 9.94178 | 3.16228 | 0.00361858 | 0.001151 | 15.1856 | 1 | 0.492 | 0.492 | 117.231 | 0.915511 | F | F | 2.8e+20 | 0 | 1 | d | |||||
| Report | 4 | X002119.39+004124.2 | chandra | ccd7 | 939.4 | 176.8 | 9.87463 | 3.16228 | 0.00359414 | 0.001151 | 15.083 | 1 | 0.492516 | 0.492 | 42.842 | 3.72948 | F | F | 2.81e+20 | 0 | 1 | d | |||||
| Report | 3 | X002132.74+004338.4 | chandra | ccd7 | 532.611 | 449.5 | 8.93527 | 3 | 0.00325223 | 0.00109193 | 13.6482 | 1 | 0.492 | 0.492 | 70.9765 | 0.720966 | F | F | 2.8e+20 | 0 | 1 | d | |||||
| Report | 5 | X002128.66+004626.9 | chandra | ccd7 | 656.929 | 792.071 | 6.87046 | 2.64575 | 0.00250069 | 0.000962993 | 10.4943 | 1 | 0.536403 | 0.492 | 30.2111 | 3.6912 | F | F | 2.8e+20 | 0 | 1 | d | |||||
| Report | 7 | X002132.07+004955.5 | chandra | ccd7 | 552.9 | 1215.9 | 4.52918 | 2.23608 | 0.00164852 | 0.000813883 | 6.91811 | 0.999916 | 1.20702 | 0.59273 | 47.8272 | 7.00599 | A | F | 2.8e+20 | 0 | 1 | d | |||||
| Report | 2 | X002136.17+003808.5 | chandra | ccd6 | 817 | 759 | 3.96463 | 2 | 0.00144794 | 0.000730426 | 2.42883 | 0.980687 | 0.492 | 0.492 | 90 | 4.84498 | F | F | 2.79e+20 | 0 | 1 | d | |||||
| Report | 3 | X002146.30+003858.9 | chandra | ccd6 | 508.115 | 861.5 | 12.7767 | 3.60556 | 0.0046662 | 0.0013168 | 7.82728 | 1 | 0.951622 | 0.69875 | 32.3111 | 5.15239 | F | F | 2.78e+20 | 0 | 1 | d | |||||
| Report | 4 | X002126.99+003929.7 | chandra | ccd6 | 1097 | 924 | 7.88254 | 2.82843 | 0.00287881 | 0.00103298 | 4.82903 | 0.999893 | 0.792796 | 0.492 | 124.481 | 3.74499 | A | F | 2.8e+20 | 0 | 1 | d | |||||
| Report | 5 | X002126.82+003946.3 | chandra | ccd6 | 1102.1 | 957.7 | 4.94034 | 2.23607 | 0.00180427 | 0.000816642 | 3.02657 | 0.99386 | 0.504374 | 0.492 | 166.717 | 3.5121 | F | F | 2.8e+20 | 0 | 1 | d | |||||
| Report | 6 | X002127.49+003538.6 | chandra | ccd6 | 1081.5 | 454.3 | 4.48325 | 2.23608 | 0.00163734 | 0.000816647 | 2.74655 | 0.99386 | 1.58629 | 0.532129 | 16.2249 | 7.40911 | A | F | 2.8e+20 | 0 | 1 | d | |||||
| Report | 7 | X002140.95+003839.7 | chandra | ccd6 | 671.211 | 822.344 | 44.2091 | 6.70821 | 0.0161457 | 0.00244993 | 27.0836 | 1 | 0.789133 | 0.542732 | 21.4954 | 4.69985 | F | F | 2.79e+20 | 0 | 1 | dc | |||||
| Report | 6 | X002141.16+004821.7 | chandra | ccd7 | 275.75 | 1025.25 | 3.83155 | 2.00001 | 0.0013946 | 0.000727956 | 5.85252 | 0.999916 | 0.556826 | 0.492 | 16.0027 | 5.80713 | F | F | 2.79e+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