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 | 2 | X174732.30-315730.5 | chandra | ccd2 | 945.25 | 798 | 7.92566 | 3.95804 | 0.00407313 | 0.0020341 | 29.0684 | 1 | 0.560473 | 0.492 | 149.405 | 2.75681 | 5.92566 | 2 | -0.49531 | 0.563206 | F | F | 6.29e+21 | 5.41096e-14 | 1 | dx |
Report | srcpi bgdpi arf | 1 | X174751.80-320125.2 | chandra | ccd2 | 441.333 | 320.833 | 5.84113 | 3.59808 | 0.00300186 | 0.00184911 | 14.6546 | 1 | 0.696505 | 0.652995 | 82.5343 | 7.63009 | 2.92056 | 2.92056 | 0 | 0.452952 | F | F | 6.02e+21 | 4.68883e-14 | 1 | dx |
Report | 1 | X174710.27-314803.1 | chandra | ccd1 | 661.167 | 806.833 | 2.99369 | 1.73205 | 0.00153851 | 0.00089013 | 8.91888 | 0.999994 | 0.759546 | 0.492 | 93.7973 | 8.41458 | A | F | 6.76e+21 | 0 | 1 | d | |||||
Report | 1 | X174727.72-315614.9 | chandra | ccd0 | 12.8335 | 819.5 | 2.96708 | 1.73205 | 0.00152483 | 0.000890131 | 8.75548 | 0.999993 | 0.627179 | 0.492 | 180 | 1.99835 | F | F | 6.36e+21 | 0 | 1 | d | |||||
Report | srcpi bgdpi arf | 2 | X174714.16-315620.1 | chandra | ccd0 | 363.75 | 808.75 | 4.94586 | 3.39792 | 0.00254176 | 0.00174625 | 21.2569 | 1 | 0.769917 | 0.492 | 156.915 | 4.50771 | 0 | 4.94586 | 1 | 0.986342 | A | F | 6.46e+21 | 3.55333e-14 | 1 | dx |
Report | 1 | X174750.91-315245.5 | chandra | ccd3 | 628.5 | 381 | 1.9753 | 1.41421 | 0.00101514 | 0.000726789 | 5.68344 | 0.999732 | 0.492 | 0.492 | 153.435 | 4.10145 | F | F | 6.27e+21 | 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