Source List

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 X065948.17+141421.2 chandra ccd7 573.15 877.692 751.64 30.1595 0.153484 0.00615855 101.263 1 0.674149 0.674149 0 0.579529 T F 1.36e+21 1.12329e-12 1 dsxf
Report srcpi bgdpi arf 2 X065947.92+141228.0 chandra ccd7 580.479 647.691 32.4429 5.84515 0.00662482 0.00119358 4.37081 0.999973 0.370322 0.370322 0 2.39229 F F 1.37e+21 5.00424e-14 1 dsx
Report srcpi bgdpi arf 8 X065957.03+141220.0 chandra ccd7 311.331 631.519 30.0819 5.97396 0.0061427 0.00121988 4.05273 0.99993 0.847198 0.446017 321.871 3.08228 F F 1.35e+21 4.45466e-14 1 dsx
Report srcpi bgdpi arf 2 X070009.39+142214.2 chandra ccd6 414.861 905.722 31.9141 6.00004 0.00651681 0.0012252 58.2916 1 2.99593 2.10672 78.3574 8.83271 F F 1.31e+21 7.44718e-14 1 dx
Report srcpi bgdpi arf 1 X070010.01+142219.0 chandra ccd6 396.5 915.5 12.5212 3.74168 0.00255682 0.000764046 22.8702 1 0.92082 0.716728 42.4028 8.98229 F F 1.31e+21 2.98321e-14 1 dpx
Report srcpi bgdpi arf 3 X065950.67+142200.6 chandra ccd6 967.864 877.955 10.387 3.31664 0.00212102 0.000677253 18.9721 1 1.03514 0.792266 117.873 7.18797 F F 1.34e+21 2.31865e-14 1 dx
Report srcpi bgdpi arf 4 X065955.47+141809.2 chandra ccd6 825.8 407.6 9.84725 3.16228 0.0020108 0.000645733 17.9862 1 0.623139 0.492 155.478 3.62294 F F 1.34e+21 2.00594e-14 1 dx
Report srcpi bgdpi arf 1 X070036.06+140821.2 chandra ccd3 298.682 946.227 8.54108 3.31668 0.00174408 0.000677262 16.0858 1 5.37066 1.73651 108.314 13.0007 A F 1.29e+21 2.23735e-14 1 dx
Report 10 X065958.82+141553.3 chandra ccd6 727 131.5 7.93332 2.82843 0.00161997 0.000577561 14.4903 1 0.562888 0.492 146.599 2.4851 F F 1.34e+21 0 1 d
Report srcpi bgdpi arf 7 X065948.85+141918.9 chandra ccd6 1021.36 549.357 6.87931 2.64575 0.00140475 0.000540259 12.5652 1 0.656949 0.492 151.535 4.49143 F F 1.34e+21 1.56372e-14 1 dx
Report srcpi bgdpi arf 5 X070007.29+141734.4 chandra ccd6 476.833 337 5.90624 2.44949 0.00120605 0.000500183 10.7878 1 0.593709 0.492 51.1126 5.10101 F F 1.32e+21 1.27883e-14 1 dx
Report 6 X065939.14+141818.6 chandra ccd6 1308.3 426.9 4.92657 2.23607 0.001006 0.000456602 8.99846 0.999999 0.597973 0.492 13.2825 4.29991 F F 1.36e+21 0 1 d
Report srcpi bgdpi arf 8 X070013.60+142030.9 chandra ccd6 290.5 695.75 3.71524 2.00001 0.000758648 0.000408399 6.78595 0.999984 1.03489 0.492 41.9085 8.14281 A F 1.3e+21 8.44345e-15 1 dx
Report srcpi bgdpi arf 9 X065945.46+142153.0 chandra ccd6 1121.5 862.5 1.81084 1.41422 0.000369772 0.000288782 3.30753 0.996409 0.492 0.492 90 7.12495 F F 1.34e+21 4.9547e-15 1 dx

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