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 | X110223.38+223920.7 | chandra | ccd7 | 99.6096 | 750.253 | 569.994 | 24.1939 | 0.0629837 | 0.0026734 | 208.431 | 1 | 0.388512 | 0.388512 | 0 | 0.583012 | F | T | 1.12e+20 | 3.67496e-13 | 1 | dsxf | ||||
| Report | srcpi bgdpi arf | 2 | X110224.96+224053.0 | chandra | ccd7 | 55.3149 | 937.652 | 11.9193 | 3.45243 | 0.00131707 | 0.00038149 | 4.35856 | 0.999893 | 0.487408 | 0.487408 | 0 | 0.99545 | F | F | 1.12e+20 | 8.66228e-15 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 3 | X110223.59+223811.6 | chandra | ccd7 | 93.6332 | 609.721 | 33.1854 | 6.34576 | 0.00366695 | 0.000701199 | 12.135 | 1 | 0.451442 | 0.451442 | 0 | 1.72082 | F | F | 1.12e+20 | 2.43589e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 4 | X110223.20+224029.4 | chandra | ccd7 | 104.25 | 889.25 | 7.48919 | 2.82844 | 0.000827546 | 0.000312539 | 2.73859 | 0.98998 | 0.492 | 0.492 | 18.4349 | 0.601828 | F | F | 1.12e+20 | 5.44476e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 5 | X110224.84+223942.8 | chandra | ccd7 | 57.9285 | 794.643 | 6.33062 | 2.64577 | 0.000699525 | 0.000292354 | 2.31493 | 0.978885 | 0.513024 | 0.492 | 75.3211 | 0.286631 | F | F | 1.12e+20 | 4.59274e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 6 | X110221.53+223655.7 | chandra | ccd7 | 151.167 | 454.944 | 8.31502 | 3.00002 | 0.000918799 | 0.000331498 | 3.04057 | 0.995512 | 0.543753 | 0.492 | 29.2243 | 3.03714 | F | F | 1.11e+20 | 6.2605e-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