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 | 7 | X224030.19+032130.5 | chandra | ccd7 | 319.888 | 308.787 | 169.735 | 13.2315 | 0.0172705 | 0.0013463 | 115.952 | 1 | 0.696562 | 0.696562 | 0 | 0.325376 | T | F | 5.06e+20 | 1.61146e-13 | 1 | dsxf | ||||
| Report | srcpi bgdpi arf | 4 | X224022.87+032450.8 | chandra | ccd7 | 542.634 | 715.997 | 60.5633 | 7.78224 | 0.00616231 | 0.000791842 | 41.3728 | 1 | 0.837967 | 0.837967 | 0 | 4.10632 | F | F | 5.01e+20 | 4.76885e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 5 | X224019.26+032613.6 | chandra | ccd7 | 652.703 | 884.216 | 28.9876 | 5.38401 | 0.00294949 | 0.000547824 | 19.8024 | 1 | 1.18643 | 1.18643 | 0 | 5.76505 | F | F | 5e+20 | 2.35373e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 6 | X224024.22+032638.7 | chandra | ccd7 | 501.538 | 935.187 | 24.4155 | 4.9412 | 0.00248427 | 0.000502767 | 16.6791 | 1 | 1.49832 | 1.49832 | 0 | 5.61677 | F | F | 5e+20 | 1.97623e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 1 | X223926.34+032044.2 | chandra | ccd3 | 1078.8 | 346.587 | 16.6843 | 4.79594 | 0.00169764 | 0.00048799 | 17.3626 | 1 | 4.41862 | 0.492 | 134.817 | 16.2034 | A | F | 5.03e+20 | 4.84895e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 3 | X224021.45+032441.9 | chandra | ccd7 | 585.835 | 697.87 | 15.6248 | 3.95282 | 0.00158982 | 0.000402199 | 10.6738 | 1 | 1.19603 | 0.4837 | 0.170429 | 4.1781 | A | F | 5.01e+20 | 1.23143e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 1 | X224036.54+031519.5 | chandra | ccd6 | 505.346 | 522.269 | 12.1041 | 3.60556 | 0.0012316 | 0.000366867 | 13.0561 | 1 | 1.02877 | 0.824811 | 119.476 | 6.12886 | F | F | 5.15e+20 | 1.39083e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 2 | X224024.48+032354.1 | chandra | ccd7 | 493.753 | 600.762 | 11.7064 | 3.42146 | 0.00119112 | 0.000348133 | 7.99704 | 1 | 0.639749 | 0.639749 | 0 | 3.09154 | F | F | 5.03e+20 | 9.11187e-15 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 7 | X224028.53+031849.9 | chandra | ccd6 | 749.1 | 949.9 | 9.68645 | 3.16228 | 0.0009856 | 0.000321763 | 10.4483 | 1 | 0.746333 | 0.492 | 131.898 | 2.56707 | A | F | 5.1e+20 | 1.02892e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 6 | X224033.84+031509.2 | chandra | ccd6 | 587.5 | 501.25 | 6.78152 | 2.82846 | 0.000690022 | 0.000287796 | 7.3149 | 0.999997 | 1.53491 | 0.539142 | 162.959 | 6.19057 | A | F | 5.15e+20 | 8.27525e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 4 | X224040.19+031613.5 | chandra | ccd6 | 394.1 | 632.1 | 4.89235 | 2.23607 | 0.000497798 | 0.000227521 | 5.27714 | 0.99973 | 0.492 | 0.492 | 79.0993 | 5.55395 | F | F | 5.15e+20 | 5.5443e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 2 | X224039.70+031850.5 | chandra | ccd6 | 408.9 | 951.1 | 4.85946 | 2.23607 | 0.000494452 | 0.000227521 | 5.24167 | 0.99973 | 0.492 | 0.492 | 45 | 3.25072 | F | F | 5.11e+20 | 5.25389e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 3 | X224046.32+031419.8 | chandra | ccd6 | 207.5 | 401 | 3.70988 | 2.00001 | 0.000377482 | 0.000203501 | 4.00167 | 0.998076 | 0.492 | 0.492 | 90 | 7.93047 | F | F | 5.18e+20 | 4.9259e-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