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 | 1 | X091946.79+334458.8 | chandra | ccd3 | 253.757 | 918.076 | 41.6752 | 8.77499 | 0.0138556 | 0.00291739 | 7.01188 | 1 | 1.5 | 1.5 | 0 | 1.76236 | T | F | 1.38e+20 | 0 | 1 | ds | |||||
Report | 2 | X091915.73+334411.1 | chandra | ccd3 | 1040.58 | 821.083 | 23.687 | 4.89898 | 0.00787511 | 0.00162875 | 3.98535 | 0.999903 | 1.4894 | 0.777907 | 70.6648 | 6.77574 | A | F | 1.37e+20 | 0 | 1 | d | |||||
Report | 1 | X092002.90+335545.2 | chandra | ccd0 | 703.643 | 1027.55 | 19.2338 | 4.5826 | 0.0063946 | 0.00152356 | 41.469 | 1 | 3.48194 | 1.79271 | 123.149 | 9.67931 | A | F | 1.39e+20 | 0 | 1 | d | |||||
Report | 2 | X091912.27+334616.2 | chandra | ccd2 | 952.929 | 27.5 | 6.65355 | 2.64576 | 0.00221208 | 0.000879626 | 13.512 | 1 | 1.10243 | 0.492 | 77.2889 | 7.00934 | A | F | 1.38e+20 | 0 | 1 | d | |||||
Report | 1 | X092018.72+334220.2 | chandra | ccd1 | 487.333 | 425.667 | 5.60902 | 2.4495 | 0.00186481 | 0.000814376 | 11.8988 | 1 | 0.895288 | 0.645248 | 99.7512 | 8.11478 | F | F | 1.38e+20 | 0 | 1 | d | |||||
Report | 3 | X091958.27+334306.6 | chandra | ccd1 | 1006 | 519.5 | 3.97038 | 2 | 0.00132002 | 0.000664933 | 8.42267 | 0.999996 | 0.492 | 0.492 | 2.35031e-08 | 4.44449 | F | F | 1.38e+20 | 0 | 1 | d | |||||
Report | 2 | X092007.32+334541.1 | chandra | ccd1 | 776.833 | 833.833 | 2.97346 | 1.73205 | 0.000988574 | 0.000575849 | 6.30782 | 0.999915 | 0.492 | 0.492 | 45 | 4.5683 | F | F | 1.39e+20 | 0 | 1 | d | |||||
Report | 1 | X091928.84+334742.5 | chandra | ccd2 | 532.833 | 202.5 | 2.95185 | 1.73205 | 0.000981389 | 0.000575849 | 5.99459 | 0.999881 | 0.627179 | 0.492 | 56.3099 | 3.67985 | F | F | 1.38e+20 | 0 | 1 | d | |||||
Report | 2 | X091948.02+335443.8 | chandra | ccd0 | 1080.17 | 902.5 | 2.82791 | 1.73206 | 0.000940184 | 0.00057585 | 6.09709 | 0.999925 | 1.0113 | 0.492 | 116.736 | 8.00264 | A | F | 1.39e+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