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 | X094519.03+100449.8 | chandra | ccd7 | 774.4 | 230.85 | 18.9558 | 5.55522 | 0.00626228 | 0.00183523 | 18.5505 | 1 | 1.59592 | 0.984061 | 26.5453 | 6.42132 | 14.5823 | 3.53012 | -0.6102 | 0.353925 | A | F | 2.4e+20 | 5.07212e-14 | 1 | dx |
| Report | srcpi bgdpi arf | 1 | X094544.03+101211.2 | chandra | ccd6 | 439.1 | 160.9 | 4.87091 | 3.39792 | 0.00160916 | 0.00112254 | 13.5572 | 1 | 0.645531 | 0.492 | 175.136 | 3.25689 | 2 | 2.87091 | 0.178799 | 0.719412 | F | F | 2.4e+20 | 1.73689e-14 | 1 | dx |
| Report | srcpi bgdpi arf | 2 | X094531.79+101253.5 | chandra | ccd6 | 806.3 | 246.9 | 4.76801 | 3.39792 | 0.00157517 | 0.00112254 | 9.8992 | 1 | 0.539019 | 0.492 | 139.933 | 2.80505 | 0.845338 | 3.92267 | 0.645412 | 0.861063 | F | F | 2.4e+20 | 1.69517e-14 | 1 | dx |
| Report | srcpi bgdpi arf | 3 | X094536.89+101355.3 | chandra | ccd6 | 653.25 | 372.625 | 8.93488 | 4.1225 | 0.00295174 | 0.00136192 | 35.0144 | 1 | 0.639741 | 0.492 | 60.7929 | 3.87063 | 5 | 3.93488 | -0.119209 | 0.469144 | F | F | 2.4e+20 | 3.36912e-14 | 1 | dx |
| Report | 1 | X094533.28+100810.5 | chandra | ccd7 | 346.5 | 638.833 | 2.91067 | 1.73205 | 0.000961573 | 0.000572204 | 3.50142 | 0.994498 | 0.627179 | 0.492 | 90 | 1.95658 | F | F | 2.4e+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