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 | 1 | X123049.05+122329.6 | chandra | ccd7 | 130.887 | 314.472 | 414.171 | 36.2889 | 0.0886525 | 0.00776757 | 14.7245 | 1 | 1.39248 | 1.39248 | 0 | 0.757157 | T | F | 1.94e+20 | 8.7622e-13 | 1 | dsxf | ||||
| Report | srcpi bgdpi arf rmf | 2 | X123048.64+122332.4 | chandra | ccd7 | 143.128 | 320.224 | 1065.04 | 44.0882 | 0.227969 | 0.00943695 | 37.864 | 1 | 0.483748 | 0.483748 | 0 | 0.773075 | F | F | 1.93e+20 | 1.61069e-12 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 3 | X123048.23+122335.0 | chandra | ccd7 | 155.24 | 325.503 | 94.6705 | 25.5473 | 0.020264 | 0.00546834 | 3.3657 | 0.999509 | 0.841464 | 0.841464 | 0 | 0.809452 | T | F | 1.93e+20 | 1.43144e-13 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 5 | X123047.15+122415.9 | chandra | ccd7 | 187.372 | 408.683 | 59.8135 | 12.702 | 0.012803 | 0.00271884 | 2.12647 | 0.981648 | 0.36105 | 0.36105 | 0 | 1.52011 | F | F | 1.93e+20 | 9.10331e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 9 | X123047.17+122332.0 | chandra | ccd7 | 186.774 | 319.311 | 80.0922 | 17.621 | 0.0171436 | 0.00377173 | 2.84742 | 0.997559 | 1.485 | 1.485 | 0 | 0.804195 | T | F | 1.93e+20 | 1.20999e-13 | 1 | dsx | ||||
| Report | srcpi bgdpi arf rmf | 10 | X123049.38+122328.4 | chandra | ccd7 | 120.919 | 312.135 | 7855.95 | 99.6579 | 1.68155 | 0.0213315 | 279.293 | 1 | 0.548613 | 0.548613 | 0 | 0.750886 | F | F | 1.94e+20 | 1.1897e-11 | 1 | dsx |
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