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 | 4 | X224017.06+080313.3 | chandra | ccd7 | 564.44 | 281.021 | 691.101 | 28.8557 | 0.141213 | 0.0058961 | 58.0882 | 1 | 1.39722 | 1.39722 | 0 | 0.380412 | T | F | 6.39e+20 | 1.40823e-12 | 1 | dsxf | ||||
Report | srcpi bgdpi arf | 1 | X224021.35+075403.7 | chandra | ccd6 | 572.053 | 197.792 | 32.746 | 5.85956 | 0.006691 | 0.00119729 | 24.7057 | 1 | 5.925 | 2.88783 | 36.0483 | 9.00801 | F | F | 6.27e+20 | 8.11668e-14 | 1 | dsx | ||||
Report | srcpi bgdpi arf | 4 | X224021.41+080024.5 | chandra | ccd6 | 570.162 | 971.792 | 21.8556 | 4.87655 | 0.00446578 | 0.000996429 | 16.4893 | 1 | 0.929654 | 0.292714 | 235.085 | 2.73865 | A | F | 6.35e+20 | 4.73786e-14 | 1 | dsx | ||||
Report | srcpi bgdpi arf | 2 | X223942.33+080703.0 | chandra | ccd3 | 243.25 | 725.5 | 10.2765 | 3.46413 | 0.00209979 | 0.000707828 | 16.4314 | 1 | 2.81725 | 1.39198 | 31.8507 | 9.78895 | A | F | 6.49e+20 | 2.92455e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 2 | X223953.02+075345.0 | chandra | ccd2 | 49.0835 | 136.5 | 8.98289 | 3.46418 | 0.00183548 | 0.000707837 | 15.1976 | 1 | 4.11369 | 1.37873 | 143.045 | 11.223 | A | F | 6.3e+20 | 2.86999e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 1 | X223857.39+075354.9 | chandra | ccd0 | 706.136 | 302.5 | 8.20051 | 3.31669 | 0.00167561 | 0.000677701 | 13.6745 | 1 | 4.17817 | 2.83269 | 45.3554 | 22.0428 | F | F | 6.39e+20 | 3.08478e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 2 | X224036.05+075644.7 | chandra | ccd6 | 127.611 | 524.611 | 8.11093 | 3.00002 | 0.00165731 | 0.000612996 | 6.11941 | 0.999984 | 1.58501 | 0.775207 | 64.6447 | 7.6654 | A | F | 6.29e+20 | 2.07851e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 1 | X223948.68+080045.0 | chandra | ccd2 | 180 | 990.167 | 5.56573 | 2.4495 | 0.00113725 | 0.000500507 | 9.41634 | 0.999998 | 1.32678 | 0.894553 | 112.58 | 7.71284 | F | F | 6.4e+20 | 1.63134e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 1 | X223943.50+080227.2 | chandra | ccd3 | 208.333 | 165 | 5.38478 | 2.44951 | 0.00110028 | 0.000500509 | 8.60992 | 0.999996 | 1.07481 | 0.664001 | 102.197 | 8.66567 | A | F | 6.43e+20 | 1.4723e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 3 | X224029.51+075935.5 | chandra | ccd6 | 325.25 | 871.75 | 3.93261 | 2 | 0.000803551 | 0.000408661 | 2.96701 | 0.990704 | 0.557057 | 0.492 | 101.815 | 4.4121 | F | F | 6.34e+20 | 9.29782e-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