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 | 3 | X015150.91+004013.0 | chandra | ccd3 | 58.2 | 640.2 | 8.71312 | 3.16231 | 0.00269314 | 0.000977438 | 22.6817 | 1 | 3.84956 | 1.90973 | 78.2109 | 15.6171 | A | F | 2.8e+20 | 3.81083e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 1 | X015047.86+003520.8 | chandra | ccd7 | 643.278 | 61.2778 | 7.97362 | 3.00003 | 0.00246456 | 0.000927277 | 10.3974 | 1 | 1.33284 | 0.59868 | 51.7875 | 6.67714 | A | T | 2.77e+20 | 1.70187e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 6 | X015051.72+004001.6 | chandra | ccd7 | 525.625 | 632 | 7.90574 | 2.82843 | 0.00244358 | 0.000874238 | 10.3089 | 1 | 0.520594 | 0.492 | 28.9973 | 2.1175 | F | F | 2.75e+20 | 1.54684e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 1 | X015045.68+004921.9 | chandra | ccd6 | 560.786 | 717.786 | 6.30217 | 2.64577 | 0.00194794 | 0.00081778 | 14.834 | 1 | 1.01624 | 0.922651 | 114.985 | 7.38819 | F | T | 2.69e+20 | 2.03339e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 3 | X015048.84+004126.2 | chandra | ccd7 | 613.5 | 803.833 | 5.89803 | 2.44949 | 0.00182302 | 0.000757113 | 7.69086 | 0.999997 | 0.492 | 0.492 | 180 | 0.583582 | F | F | 2.74e+20 | 1.12645e-14 | 1 | dx | ||||
Report | 4 | X015042.76+004420.2 | chandra | ccd6 | 649.7 | 104.5 | 4.97856 | 2.23607 | 0.00153882 | 0.000691146 | 11.7185 | 1 | 0.492 | 0.492 | 145.901 | 2.77217 | F | F | 2.71e+20 | 0 | 1 | d | |||||
Report | srcpi bgdpi arf | 1 | X015131.50+004457.9 | chandra | ccd2 | 539.9 | 177.1 | 4.62447 | 2.23608 | 0.00142938 | 0.000691149 | 11.82 | 0.999999 | 1.25332 | 0.492 | 139.037 | 11.06 | A | T | 2.76e+20 | 1.82768e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 5 | X015040.38+003935.9 | chandra | ccd7 | 871.25 | 579.75 | 3.8597 | 2 | 0.00119299 | 0.000618181 | 5.03294 | 0.99964 | 0.5535 | 0.492 | 120.964 | 3.21651 | F | F | 2.74e+20 | 7.69426e-15 | 1 | dx | ||||
Report | 2 | X015056.68+004047.3 | chandra | ccd7 | 374.5 | 724.833 | 2.95104 | 1.73205 | 0.000912136 | 0.00053536 | 3.84807 | 0.996871 | 0.492 | 0.492 | 90 | 2.31107 | F | F | 2.75e+20 | 0 | 1 | d | |||||
Report | srcpi bgdpi arf | 4 | X015057.99+003902.4 | chandra | ccd7 | 334.5 | 511.5 | 2.93049 | 1.73205 | 0.000905785 | 0.00053536 | 3.82128 | 0.996871 | 0.492 | 0.492 | 90 | 3.75498 | F | F | 2.76e+20 | 5.90511e-15 | 1 | dx | ||||
Report | 3 | X015038.54+004942.8 | chandra | ccd6 | 778.5 | 760.167 | 2.91777 | 1.73205 | 0.000901852 | 0.00053536 | 6.86782 | 0.999962 | 0.492 | 0.492 | 151.845 | 8.11372 | F | F | 2.67e+20 | 0 | 1 | d | |||||
Report | 1 | X015120.74+004033.2 | chandra | ccd3 | 977.833 | 681.167 | 2.91715 | 1.73205 | 0.00090166 | 0.00053536 | 7.59381 | 0.999982 | 0.492 | 0.492 | 163.155 | 8.10552 | F | T | 2.79e+20 | 0 | 1 | d | |||||
Report | 2 | X015122.85+003832.3 | chandra | ccd3 | 913.5 | 435.5 | 2.89853 | 1.73205 | 0.000895906 | 0.00053536 | 7.54535 | 0.999982 | 1.34613 | 0.492 | 53.7628 | 9.18449 | A | F | 2.8e+20 | 0 | 1 | d | |||||
Report | 2 | X015054.73+004614.6 | chandra | ccd6 | 285 | 337 | 1.96829 | 1.41421 | 0.000608379 | 0.000437119 | 4.63295 | 0.999144 | 0.492 | 0.492 | 45 | 4.47081 | F | F | 2.72e+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