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 | X030110.13+445347.1 | chandra | ccd7 | 1024.87 | 512.063 | 118.506 | 11.4181 | 0.0159203 | 0.00153393 | 37.6654 | 1 | 0.333532 | 0.333532 | 0 | 0.743106 | 105 | 15.7456 | -0.739193 | 0.124054 | F | T | 1.51e+21 | 7.41514e-14 | 1 | dsxf |
Report | srcpi bgdpi arf | 1 | X030114.17+445350.5 | chandra | ccd7 | 937.514 | 519.13 | 30.591 | 7.57277 | 0.00410965 | 0.00101734 | 9.72291 | 1 | 0.586127 | 0.586127 | 0 | 0.174893 | 30.6933 | 5.98255 | -0.673761 | 0.245946 | F | F | 1.51e+21 | 3.24024e-14 | 1 | dsx |
Report | srcpi bgdpi arf | 15 | X030115.26+445230.8 | chandra | ccd7 | 914.047 | 356.979 | 20.1278 | 4.4864 | 0.002704 | 0.00060271 | 6.39733 | 1 | 0.405674 | 0.405674 | 0 | 1.16551 | 14.9151 | 4.66049 | -0.523847 | 0.32194 | F | F | 1.51e+21 | 2.15957e-14 | 1 | dsx |
Report | srcpi bgdpi arf | 10 | X030115.07+445515.4 | chandra | ccd7 | 918.079 | 691.536 | 12.9669 | 3.73362 | 0.001742 | 0.000501582 | 4.12134 | 0.999743 | 0.305272 | 0.305272 | 0 | 1.59752 | 9.83053 | 2.91526 | -0.542553 | 0.423245 | F | F | 1.52e+21 | 1.37809e-14 | 1 | dsx |
Report | srcpi bgdpi arf | 4 | X030117.56+445304.2 | chandra | ccd7 | 863.7 | 424.5 | 9.66123 | 4.27872 | 0.0012979 | 0.000574807 | 16.5988 | 1 | 0.492 | 0.492 | 46.4312 | 0.833821 | 6.74592 | 2.91531 | -0.396493 | 0.480637 | F | F | 1.51e+21 | 1.03008e-14 | 1 | dx |
Report | srcpi bgdpi arf | 9 | X030056.14+445508.7 | chandra | ccd7 | 1326.28 | 677.611 | 8.73218 | 4.1225 | 0.00117309 | 0.00055382 | 16.8733 | 1 | 0.622595 | 0.492 | 3.07758 | 3.5338 | 6.79913 | 1.93304 | -0.557259 | 0.545674 | F | F | 1.51e+21 | 1.0286e-14 | 1 | dx |
Report | srcpi bgdpi arf | 8 | X030114.16+445433.2 | chandra | ccd7 | 937.278 | 605.278 | 8.83061 | 4.1225 | 0.00118631 | 0.00055382 | 21.4561 | 1 | 0.492 | 0.492 | 14.5273 | 0.888075 | 4.83061 | 4 | -0.0940607 | 0.473427 | F | F | 1.52e+21 | 9.678e-15 | 1 | dx |
Report | srcpi bgdpi arf | 1 | X030059.04+445246.6 | chandra | ccd6 | 492.875 | 1099.75 | 7.82157 | 3.95804 | 0.00105076 | 0.000531726 | 18.5163 | 1 | 0.7013 | 0.492 | 22.624 | 2.83911 | 3 | 4.82157 | 0.23289 | 0.525092 | F | F | 1.5e+21 | 1.11444e-14 | 1 | dx |
Report | srcpi bgdpi arf | 7 | X030114.90+445401.9 | chandra | ccd7 | 921.214 | 541.643 | 5.54114 | 3.78388 | 0.000744401 | 0.00050833 | 4.58767 | 0.999859 | 0.514009 | 0.492 | 38.1643 | 0.383129 | 5.27057 | 0.351617 | -0.874918 | 0.904788 | F | F | 1.51e+21 | 6.20358e-15 | 1 | dx |
Report | 2 | X030110.50+444956.8 | chandra | ccd6 | 245.3 | 754.5 | 4.85495 | 2.23607 | 0.000652218 | 0.000300396 | 6.79767 | 0.999984 | 0.674536 | 0.492 | 124.099 | 3.77798 | F | T | 1.5e+21 | 0 | 1 | d | |||||
Report | srcpi bgdpi arf | 3 | X030051.26+444824.9 | chandra | ccd6 | 661.643 | 568.143 | 21.4335 | 5.7697 | 0.00287939 | 0.000775106 | 28.4767 | 1 | 1.94154 | 0.618569 | 36.6132 | 6.64689 | 16.8381 | 4.59535 | -0.571199 | 0.311414 | A | F | 1.49e+21 | 3.52158e-14 | 1 | dx |
Report | srcpi bgdpi arf | 4 | X030101.47+445025.5 | chandra | ccd6 | 440.5 | 813 | 5.91531 | 3.59808 | 0.000794667 | 0.000483368 | 20.326 | 1 | 0.492 | 0.492 | 90 | 3.9537 | 2.91531 | 3 | 0.0143177 | 0.616388 | F | F | 1.5e+21 | 9.01197e-15 | 1 | dx |
Report | srcpi bgdpi arf | 5 | X030058.18+444724.5 | chandra | ccd6 | 512.1 | 445.1 | 4.93812 | 3.39792 | 0.000663392 | 0.000456479 | 19.8519 | 1 | 0.71012 | 0.518772 | 38.3038 | 6.87623 | 0 | 4.93812 | 1 | 0.987888 | F | F | 1.49e+21 | 7.74599e-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