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 | 8 | X130211.04+000004.8 | chandra | ccd7 | 798.39 | 503.303 | 41.5128 | 6.44304 | 0.00847687 | 0.00131566 | 48.479 | 1 | 0.464849 | 0.464849 | 0 | 0.586092 | F | F | 1.42e+20 | 0 | 1 | ds | |||||
| Report | 2 | X130215.84+000053.1 | chandra | ccd7 | 652.167 | 601.509 | 34.5122 | 5.92426 | 0.00704736 | 0.00120973 | 40.3036 | 1 | 0.446807 | 0.446807 | 0 | 2.01701 | F | F | 1.42e+20 | 0 | 1 | ds | |||||
| Report | 3 | X130220.95+000133.8 | chandra | ccd7 | 496.472 | 684.182 | 29.0579 | 5.61744 | 0.00593359 | 0.00114707 | 33.9341 | 1 | 0.993779 | 0.470183 | 93.3114 | 3.44896 | F | F | 1.42e+20 | 0 | 1 | ds | |||||
| Report | 2 | X130147.01-000645.1 | chandra | ccd6 | 996.719 | 522.688 | 28.3882 | 5.6569 | 0.00579683 | 0.00115513 | 51.9291 | 1 | 3.66441 | 2.38657 | 149.062 | 8.51197 | A | F | 1.43e+20 | 0 | 1 | d | |||||
| Report | 1 | X130216.68+000042.5 | chandra | ccd7 | 626.532 | 579.91 | 10.8278 | 3.29056 | 0.00221103 | 0.000671931 | 12.6448 | 1 | 0.777797 | 0.337683 | 96.9522 | 2.08938 | F | F | 1.42e+20 | 0 | 1 | ds | |||||
| Report | 1 | X130146.30-000545.0 | chandra | ccd6 | 1018.1 | 644.8 | 9.089 | 3.1623 | 0.00185596 | 0.000645736 | 16.6261 | 1 | 1.30876 | 1.06118 | 50.1465 | 7.91588 | F | F | 1.43e+20 | 0 | 1 | d | |||||
| Report | 4 | X130211.44+000205.0 | chandra | ccd7 | 785.786 | 747.071 | 6.84186 | 2.64575 | 0.0013971 | 0.000540259 | 7.98998 | 0.999999 | 0.536031 | 0.492 | 108.592 | 2.49195 | F | F | 1.42e+20 | 0 | 1 | d | |||||
| Report | 1 | X130136.24+000158.4 | chandra | ccd2 | 239.929 | 749.786 | 5.87388 | 2.64578 | 0.00119944 | 0.000540265 | 11.0959 | 1 | 1.92827 | 1.3806 | 152.82 | 8.63594 | F | F | 1.42e+20 | 0 | 1 | d | |||||
| Report | 5 | X130210.15+000303.2 | chandra | ccd7 | 825 | 865.333 | 5.86822 | 2.44949 | 0.00119828 | 0.000500183 | 6.85296 | 0.999988 | 0.52308 | 0.492 | 12.5574 | 3.41787 | F | F | 1.42e+20 | 0 | 1 | d | |||||
| Report | 3 | X130143.88-000353.9 | chandra | ccd6 | 1092.1 | 870.7 | 4.88868 | 2.23607 | 0.000998261 | 0.000456603 | 8.94262 | 0.999999 | 0.558616 | 0.492 | 104.221 | 7.31657 | F | F | 1.43e+20 | 0 | 1 | d | |||||
| Report | 7 | X130205.86+000616.0 | chandra | ccd7 | 955.9 | 1257.3 | 4.63289 | 2.23608 | 0.000946031 | 0.000456604 | 5.41034 | 0.999884 | 1.06001 | 0.492 | 2.46961 | 6.69015 | A | F | 1.42e+20 | 0 | 1 | d | |||||
| Report | 1 | X130134.77+000641.5 | chandra | ccd3 | 815.9 | 438.1 | 4.59087 | 2.44953 | 0.00093745 | 0.00050019 | 8.68269 | 0.999989 | 1.53164 | 0.623054 | 37.7499 | 11.1864 | A | F | 1.42e+20 | 0 | 1 | d | |||||
| Report | 6 | X130222.59+000315.2 | chandra | ccd7 | 445.75 | 889.75 | 3.83753 | 2.00001 | 0.000783619 | 0.000408398 | 4.4815 | 0.999036 | 0.565893 | 0.492 | 69.407 | 4.87649 | F | F | 1.42e+20 | 0 | 1 | d | |||||
| Report | 5 | X130201.45-000606.3 | chandra | ccd6 | 556.5 | 601.5 | 2.91421 | 1.73205 | 0.000595077 | 0.000353683 | 5.33082 | 0.999738 | 0.492 | 0.492 | 90 | 6.08665 | F | F | 1.43e+20 | 0 | 1 | d | |||||
| Report | 4 | X130208.99-000244.3 | chandra | ccd6 | 326.5 | 1012.17 | 2.81604 | 1.73205 | 0.000575032 | 0.000353683 | 5.15125 | 0.999738 | 0.529672 | 0.492 | 169.722 | 2.38003 | F | F | 1.42e+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