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 | 1 | X143215.12+350525.4 | chandra | ccd2 | 1075 | 693.533 | 26.0418 | 5.47727 | 0.00556331 | 0.00117011 | 40.3345 | 1 | 2.3987 | 1.643 | 81.4889 | 8.8888 | F | F | 1.11e+20 | 7.58501e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 5 | X143244.25+350100.6 | chandra | ccd3 | 1115.97 | 808.05 | 25.9099 | 5.36023 | 0.00553519 | 0.00114512 | 15.4231 | 1 | 1.5802 | 0.52402 | 350.093 | 5.31394 | A | F | 1.09e+20 | 6.81099e-14 | 1 | dsx | ||||
Report | srcpi bgdpi arf | 4 | X143231.77+350243.8 | chandra | ccd2 | 659.857 | 364.5 | 13.1844 | 3.74167 | 0.00281659 | 0.000799333 | 20.4205 | 1 | 1.42518 | 0.850491 | 42.6081 | 6.11403 | A | F | 1.1e+20 | 3.51127e-14 | 1 | dx | ||||
Report | 3 | X143312.56+350841.4 | chandra | ccd1 | 1101.38 | 913.125 | 7.92498 | 2.82843 | 0.00169189 | 0.000603838 | 12.4473 | 1 | 0.559828 | 0.492 | 120.128 | 4.3332 | F | F | 1.09e+20 | 0 | 1 | d | |||||
Report | srcpi bgdpi arf | 2 | X143257.64+350301.9 | chandra | ccd3 | 781.125 | 1053.88 | 7.90946 | 2.82843 | 0.0016897 | 0.000604237 | 4.70819 | 0.999825 | 0.492 | 0.492 | 125.41 | 2.41109 | F | F | 1.09e+20 | 1.89872e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 1 | X143310.29+351409.0 | chandra | ccd0 | 350.167 | 965.833 | 7.83902 | 3.00003 | 0.00167354 | 0.000640472 | 11.8944 | 1 | 1.87102 | 1.10432 | 55.9007 | 9.03781 | A | F | 1.09e+20 | 2.60302e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 2 | X143255.12+351539.2 | chandra | ccd0 | 727.833 | 1149.17 | 8.09736 | 3.00002 | 0.0017287 | 0.00064047 | 12.2864 | 1 | 1.39182 | 0.737554 | 152.19 | 10.2428 | A | F | 1.1e+20 | 2.40176e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 3 | X143257.57+351137.5 | chandra | ccd0 | 666.955 | 657.955 | 10.1434 | 3.31664 | 0.0021655 | 0.000708065 | 15.3909 | 1 | 1.77553 | 1.08312 | 101.125 | 6.19401 | A | F | 1.1e+20 | 2.66929e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 3 | X143302.51+350435.7 | chandra | ccd3 | 659.786 | 1244.5 | 6.8998 | 2.64575 | 0.001474 | 0.000565213 | 4.10717 | 0.9993 | 0.492 | 0.492 | 130.935 | 1.16406 | F | F | 1.09e+20 | 1.61209e-14 | 1 | dx | ||||
Report | 3 | X143237.17+350421.3 | chandra | ccd2 | 525.071 | 562.5 | 6.88096 | 2.64575 | 0.00146998 | 0.000565213 | 10.6575 | 1 | 0.623724 | 0.492 | 90 | 4.51018 | F | F | 1.1e+20 | 0 | 1 | d | |||||
Report | srcpi bgdpi arf | 2 | X143334.03+350534.7 | chandra | ccd1 | 565.357 | 534.071 | 6.47004 | 2.64576 | 0.00138128 | 0.00056484 | 10.1621 | 1 | 1.05962 | 0.823329 | 91.0738 | 7.25558 | F | F | 1.08e+20 | 1.70389e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 1 | X143312.69+350752.0 | chandra | ccd1 | 1097.9 | 812.7 | 4.89803 | 2.23607 | 0.00104567 | 0.000477376 | 7.69307 | 0.999996 | 0.804089 | 0.492 | 102.09 | 3.77561 | A | F | 1.09e+20 | 1.17691e-14 | 1 | dx | ||||
Report | 1 | X143303.48+350209.4 | chandra | ccd3 | 635.5 | 947.3 | 4.88626 | 2.23607 | 0.00104385 | 0.000477692 | 2.9086 | 0.991502 | 0.492 | 0.492 | 36.6504 | 3.42801 | F | F | 1.08e+20 | 0 | 1 | d | |||||
Report | 2 | X143244.39+350246.4 | chandra | ccd2 | 344.833 | 369.5 | 2.94146 | 1.73205 | 0.000628384 | 0.000370019 | 4.55584 | 0.999096 | 0.492 | 0.492 | 90 | 3.93684 | F | F | 1.09e+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