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 | 5 | X140337.36+393633.2 | chandra | ccd7 | 667.934 | 317.181 | 55.4374 | 7.44563 | 0.0305234 | 0.00409951 | 100.598 | 1 | 1.12424 | 0.508579 | 20.5503 | 4.15847 | 40 | 5.9234 | -0.742031 | 0.21301 | F | F | 1.16e+20 | 2.43851e-13 | 1 | dsx |
Report | srcpi bgdpi arf | 1 | X140358.18+394625.0 | chandra | ccd3 | 776.389 | 249.056 | 8.58983 | 4.1225 | 0.00473783 | 0.00227382 | 13.4123 | 1 | 2.83401 | 1.9612 | 92.7889 | 9.06677 | 6.88281 | 1.70702 | -0.602548 | 0.565724 | F | F | 1.19e+20 | 6.81166e-14 | 1 | dx |
Report | srcpi bgdpi arf | 3 | X140336.82+394108.2 | chandra | ccd7 | 680.5 | 875.5 | 3.93231 | 3.17945 | 0.00216507 | 0.00175056 | 15.1144 | 1 | 0.615332 | 0.492 | 52.0181 | 2.55069 | 2 | 2 | 0 | 0.559017 | F | F | 1.18e+20 | 1.64178e-14 | 1 | dx |
Report | 4 | X140358.19+394142.1 | chandra | ccd7 | 179.25 | 945 | 3.76903 | 2.00001 | 0.00207517 | 0.00110117 | 6.83937 | 0.999983 | 1.0632 | 0.653408 | 27.6743 | 6.61023 | A | T | 1.17e+20 | 0 | 1 | d | |||||
Report | srcpi bgdpi arf | 1 | X140322.33+394032.8 | chandra | ccd7 | 1020.5 | 803.5 | 2.91531 | 2.93649 | 0.00160512 | 0.00161679 | 10.0175 | 0.999998 | 0.492 | 0.492 | 90 | 0.778028 | 0.915307 | 1 | 0.0442192 | 1.42782 | F | F | 1.19e+20 | 1.21114e-14 | 1 | dx |
Report | 2 | X140322.00+394233.3 | chandra | ccd7 | 1028.17 | 1048.5 | 2.962 | 1.73205 | 0.00163083 | 0.000953641 | 5.37491 | 0.999722 | 0.627179 | 0.492 | 123.69 | 2.6521 | F | F | 1.2e+20 | 0 | 1 | d |
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