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 | 2 | X020504.48+645052.3 | chandra | ccd7 | 733.418 | 428.346 | 135.734 | 11.6699 | 0.00363015 | 0.000312105 | 10.9487 | 1 | 1.01563 | 1.01563 | 0 | 4.31054 | F | T | 5.56e+21 | 7.17159e-14 | 1 | dbsxf | ||||
Report | srcpi bgdpi arf rmf | 8 | X020533.63+644931.0 | chandra | ccd7 | 355.828 | 262.463 | 129.077 | 22.855 | 0.00345211 | 0.000611246 | 10.4117 | 1 | 2.34239 | 2.34239 | 0 | 1.00866 | T | T | 5.58e+21 | 3.35139e-14 | 1 | dsx | ||||
Report | srcpi bgdpi arf | 6 | X020534.85+644940.6 | chandra | ccd7 | 339.923 | 281.905 | 40.034 | 19.3315 | 0.00107069 | 0.00051701 | 3.22927 | 0.999027 | 0.84089 | 0.84089 | 0 | 0.888054 | F | T | 5.57e+21 | 1.03817e-14 | 1 | dsx | ||||
Report | srcpi bgdpi arf | 3 | X020505.28+645103.3 | chandra | ccd7 | 722.967 | 450.651 | 55.288 | 8.77588 | 0.00147865 | 0.000234707 | 4.4597 | 0.999987 | 0.789636 | 0.789636 | 0 | 4.28659 | F | F | 5.56e+21 | 1.49379e-14 | 1 | dsx | ||||
Report | srcpi bgdpi arf | 10 | X020538.12+645012.2 | chandra | ccd7 | 297.498 | 346.107 | 64.1086 | 16.7652 | 0.00171455 | 0.000448378 | 5.1712 | 0.999999 | 1.5 | 1.5 | 0 | 0.794431 | T | T | 5.56e+21 | 1.66316e-14 | 1 | dsx | ||||
Report | srcpi bgdpi arf | 5 | X020443.34+644816.5 | chandra | ccd7 | 1008.62 | 112.588 | 33.5713 | 8.66271 | 0.000897848 | 0.00023168 | 2.70796 | 0.995955 | 1.5337 | 1.5337 | 0 | 6.51309 | F | F | 5.62e+21 | 9.74052e-15 | 1 | dsx | ||||
Report | srcpi bgdpi arf | 1 | X020516.32+644953.0 | chandra | ccd7 | 580.26 | 307.348 | 34.0591 | 9.2355 | 0.000910894 | 0.000246999 | 2.74731 | 0.995955 | 0.771714 | 0.771714 | 0 | 2.87237 | F | F | 5.58e+21 | 9.02939e-15 | 1 | dsx | ||||
Report | srcpi bgdpi arf | 7 | X020531.35+644955.4 | chandra | ccd7 | 385.337 | 312.155 | 57.6426 | 15.1123 | 0.00154162 | 0.000404171 | 4.64963 | 0.999995 | 1.64281 | 1.64281 | 0 | 1.32485 | T | F | 5.57e+21 | 1.49968e-14 | 1 | dsx | ||||
Report | srcpi bgdpi arf | 1 | X020638.62+645022.6 | chandra | ccd6 | 555.375 | 364.518 | 11.9021 | 4.48715 | 0.000318315 | 0.000120006 | 3.06919 | 0.996576 | 1.06905 | 1.06905 | 0 | 5.93139 | F | F | 5.54e+21 | 4.00614e-15 | 1 | dsx | ||||
Report | srcpi bgdpi arf | 4 | X020628.26+645053.2 | chandra | ccd6 | 689.786 | 426.293 | 9.68645 | 4.2639 | 0.000259059 | 0.000114036 | 2.49784 | 0.988513 | 0.699553 | 0.699553 | 0 | 4.95458 | F | F | 5.53e+21 | 3.26867e-15 | 1 | dsx | ||||
Report | srcpi bgdpi arf | 5 | X020630.28+645129.9 | chandra | ccd6 | 663.375 | 500.5 | 14.7588 | 4.47223 | 0.000394709 | 0.000119605 | 3.80584 | 0.999564 | 0.798939 | 0.511504 | 27.2124 | 5.35014 | A | F | 5.52e+21 | 4.90109e-15 | 1 | dx | ||||
Report | srcpi bgdpi arf | 6 | X020650.20+644811.6 | chandra | ccd6 | 403.567 | 98.3667 | 9.99573 | 3.87306 | 0.000267326 | 0.000103581 | 2.5776 | 0.993622 | 1.71988 | 0.99381 | 157.077 | 7.26378 | A | T | 5.57e+21 | 3.70323e-15 | 1 | dx | ||||
Report | srcpi bgdpi arf | 9 | X020614.73+644924.9 | chandra | ccd6 | 864.807 | 246.333 | 21.6644 | 7.07479 | 0.000579405 | 0.000189212 | 5.58659 | 0.999999 | 0.803519 | 0.803519 | 0 | 3.35652 | F | T | 5.56e+21 | 6.91098e-15 | 1 | dsx |
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