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 | X143624.27+353709.7 | chandra | ccd3 | 921.235 | 930.529 | 32.6602 | 5.83097 | 0.00682988 | 0.00121937 | 54.0926 | 1 | 1.80879 | 1.02164 | 38.156 | 7.40425 | A | F | 1.03e+20 | 0 | 1 | d | |||||
| Report | 4 | X143624.61+352537.1 | chandra | ccd2 | 907.244 | 568.419 | 21.0749 | 4.68734 | 0.00440437 | 0.000979592 | 22.2607 | 1 | 1.147 | 0.45179 | 43.7078 | 4.1713 | F | F | 1.02e+20 | 0 | 1 | ds | |||||
| Report | 1 | X143543.36+353653.7 | chandra | ccd1 | 891.3 | 901.9 | 17.283 | 4.47218 | 0.00361421 | 0.00093522 | 29.5937 | 1 | 4.2553 | 1.93904 | 38.607 | 10.6432 | A | F | 1.05e+20 | 0 | 1 | d | |||||
| Report | 3 | X143541.70+353210.9 | chandra | ccd1 | 933.25 | 327.188 | 13.8165 | 4.00004 | 0.0028893 | 0.000836486 | 23.6581 | 1 | 2.80977 | 1.77622 | 113.739 | 8.59109 | A | F | 1.05e+20 | 0 | 1 | d | |||||
| Report | 1 | X143641.30+352537.2 | chandra | ccd2 | 492 | 568.2 | 9.8119 | 3.16228 | 0.00205053 | 0.000660867 | 10.364 | 1 | 0.500337 | 0.492 | 100.77 | 5.68414 | F | F | 1.02e+20 | 0 | 1 | d | |||||
| Report | 2 | X143629.43+353359.5 | chandra | ccd3 | 793.167 | 543.944 | 8.88363 | 3 | 0.00185774 | 0.000627359 | 14.7133 | 1 | 0.87514 | 0.492 | 41.4711 | 4.46993 | A | F | 1.03e+20 | 0 | 1 | d | |||||
| Report | 5 | X143647.29+353042.0 | chandra | ccd3 | 349.928 | 142.929 | 6.8701 | 2.64575 | 0.00143667 | 0.000553279 | 11.3784 | 1 | 0.492 | 0.492 | 177.28 | 5.18583 | F | F | 1.02e+20 | 0 | 1 | d | |||||
| Report | 2 | X143617.76+353728.1 | chandra | ccd1 | 38.5 | 971 | 5.62877 | 2.4495 | 0.00117709 | 0.000512238 | 9.63819 | 0.999998 | 0.888424 | 0.861692 | 37.9819 | 7.75293 | F | F | 1.03e+20 | 0 | 1 | d | |||||
| Report | 3 | X143624.74+353520.5 | chandra | ccd3 | 909.7 | 708.7 | 4.92049 | 2.23607 | 0.00102897 | 0.000467606 | 8.14944 | 0.999998 | 0.640153 | 0.492 | 25.0972 | 5.5969 | F | F | 1.03e+20 | 0 | 1 | d | |||||
| Report | 3 | X143644.37+352712.7 | chandra | ccd2 | 415.9 | 762.5 | 4.90549 | 2.23607 | 0.00102517 | 0.000467303 | 5.1815 | 0.999664 | 0.756439 | 0.492 | 75.8035 | 5.18382 | A | F | 1.02e+20 | 0 | 1 | d | |||||
| Report | 1 | X143601.13+352641.3 | chandra | ccd0 | 453.833 | 697.5 | 2.96421 | 1.73205 | 0.000619472 | 0.000361971 | 5.11596 | 0.999595 | 0.561105 | 0.492 | 115.097 | 5.28504 | F | F | 1.03e+20 | 0 | 1 | d | |||||
| Report | 2 | X143559.82+352401.3 | chandra | ccd0 | 487.204 | 372.87 | 20.75 | 4.55522 | 0.00433647 | 0.000951979 | 35.8127 | 1 | 2.71467 | 1.23346 | 11.537 | 7.34518 | F | F | 1.04e+20 | 0 | 1 | ds | |||||
| Report | 5 | X143605.97+353201.6 | chandra | ccd1 | 331.167 | 307.5 | 2.94737 | 1.73205 | 0.000616353 | 0.000362206 | 5.0468 | 0.99957 | 0.492 | 0.492 | 180 | 4.00412 | F | F | 1.04e+20 | 0 | 1 | d | |||||
| Report | 4 | X143633.42+353639.5 | chandra | ccd3 | 694.5 | 869.167 | 2.8451 | 1.73206 | 0.000594967 | 0.000362207 | 4.71214 | 0.999449 | 0.799252 | 0.492 | 4.26538 | 7.25543 | A | F | 1.03e+20 | 0 | 1 | d | |||||
| Report | 4 | X143618.19+353550.4 | chandra | ccd1 | 28 | 772.5 | 1.95978 | 1.41422 | 0.000409829 | 0.00029574 | 3.35575 | 0.994869 | 0.5535 | 0.492 | 180 | 6.12722 | F | F | 1.03e+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