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 | X143918.20+430525.7 | chandra | ccd5 | 665.127 | 1067.24 | 297.275 | 18.3514 | 0.0801455 | 0.00494754 | 47.3012 | 1 | 9.66118 | 6.41397 | 241.45 | 12.2272 | F | F | 1.44e+20 | 6.40082e-13 | 1 | dsxf | ||||
Report | srcpi bgdpi arf | 4 | X143835.95+431459.2 | chandra | ccd7 | 511.876 | 441.883 | 14.5679 | 3.81679 | 0.0039275 | 0.001029 | 17.484 | 1 | 0.425463 | 0.425463 | 0 | 0.126392 | F | F | 1.46e+20 | 2.82339e-14 | 1 | dsx | ||||
Report | srcpi bgdpi arf | 1 | X143915.17+430729.1 | chandra | ccd6 | 191.131 | 383.858 | 21.9949 | 4.68987 | 0.00592983 | 0.00126439 | 41.1388 | 1 | 7.45123 | 3.10766 | 67.1149 | 10.3078 | F | F | 1.45e+20 | 7.27889e-14 | 1 | dsx | ||||
Report | srcpi bgdpi arf | 2 | X143900.16+431441.7 | chandra | ccd6 | 525.722 | 1262.06 | 8.83511 | 3 | 0.00238193 | 0.000808794 | 16.525 | 1 | 0.82505 | 0.492 | 55.8661 | 4.4749 | A | F | 1.48e+20 | 2.74627e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 6 | X143835.28+431226.0 | chandra | ccd6 | 1078.17 | 986 | 5.95778 | 2.44949 | 0.0016062 | 0.000660377 | 11.1433 | 1 | 0.492 | 0.492 | 133.807 | 2.44431 | F | F | 1.45e+20 | 1.69117e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 3 | X143853.00+431006.1 | chandra | ccd6 | 684.333 | 701.833 | 5.89151 | 2.44949 | 0.00158834 | 0.000660378 | 11.0194 | 1 | 0.729571 | 0.492 | 84.7896 | 5.73079 | F | F | 1.46e+20 | 1.76287e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 1 | X143807.27+431638.7 | chandra | ccd7 | 1148 | 644 | 5.8459 | 2.44949 | 0.00157604 | 0.000660378 | 7.01611 | 0.999992 | 0.608211 | 0.492 | 53.5514 | 5.45344 | F | F | 1.44e+20 | 1.3614e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 3 | X143817.92+432030.0 | chandra | ccd7 | 911.167 | 1113.83 | 5.18862 | 2.44951 | 0.00139884 | 0.000660384 | 6.22726 | 0.999914 | 1.05856 | 0.944249 | 86.2027 | 6.47832 | F | F | 1.46e+20 | 1.12563e-14 | 1 | dx | ||||
Report | 2 | X143822.87+432022.6 | chandra | ccd7 | 801.3 | 1098.7 | 4.61813 | 2.23608 | 0.00124504 | 0.000602842 | 5.54257 | 0.999914 | 0.818482 | 0.594995 | 23.1986 | 5.96705 | F | F | 1.46e+20 | 0 | 1 | d | |||||
Report | srcpi bgdpi arf | 4 | X143826.31+431023.9 | chandra | ccd6 | 1277.75 | 737.75 | 3.92282 | 2 | 0.00105758 | 0.000539196 | 7.33716 | 0.999987 | 0.492 | 0.492 | 45 | 4.78935 | F | F | 1.44e+20 | 1.27138e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 5 | X143910.59+430951.8 | chandra | ccd6 | 293 | 673.25 | 3.82067 | 2.00001 | 0.00103005 | 0.000539197 | 7.14611 | 0.999987 | 0.865382 | 0.732212 | 116.565 | 8.11054 | F | F | 1.46e+20 | 1.21226e-14 | 1 | dx | ||||
Report | 8 | X143831.33+430839.5 | chandra | ccd6 | 1166.17 | 525.5 | 2.8595 | 1.73206 | 0.000770914 | 0.000466959 | 5.34834 | 0.999778 | 0.492 | 0.492 | 180 | 6.26846 | F | F | 1.44e+20 | 0 | 1 | d | |||||
Report | 7 | X143856.87+431233.0 | chandra | ccd6 | 598.5 | 1000.5 | 0.966056 | 1 | 0.000260446 | 0.000269598 | 1.80689 | 0.966156 | 0.492 | 0.492 | 90 | 4.5184 | F | F | 1.47e+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