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 | 1 | X081825.91+312805.6 | chandra | ccd7 | 1030 | 539.262 | 31.8246 | 5.81435 | 0.00533725 | 0.000975115 | 11.1005 | 1 | 1.18983 | 0.622668 | 305.756 | 4.04723 | A | F | 3.32e+20 | 4.4955e-14 | 1 | dsx | ||||
Report | srcpi bgdpi arf rmf | 8 | X081855.95+312712.1 | chandra | ccd7 | 248.735 | 430.582 | 116.179 | 11.4296 | 0.0194841 | 0.00191683 | 40.5234 | 1 | 1.88298 | 1.02431 | 352.1 | 5.51267 | F | F | 3.31e+20 | 1.63412e-13 | 1 | dspxf | ||||
Report | srcpi bgdpi arf | 4 | X081838.98+313100.1 | chandra | ccd7 | 689.853 | 893.382 | 16.5923 | 4.12311 | 0.00278267 | 0.00069148 | 5.78742 | 0.999998 | 0.537687 | 0.492 | 152.732 | 0.29436 | F | F | 3.32e+20 | 2.06607e-14 | 1 | dbx | ||||
Report | srcpi bgdpi arf | 3 | X081836.90+313043.6 | chandra | ccd7 | 743.7 | 859.8 | 9.77175 | 3.16228 | 0.0016388 | 0.000530341 | 3.4084 | 0.997878 | 0.492 | 0.492 | 50.0623 | 0.539479 | F | F | 3.32e+20 | 1.22284e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 1 | X081829.94+313307.2 | chandra | ccd6 | 654.611 | 136.833 | 8.8811 | 3 | 0.00148945 | 0.000503132 | 12.0905 | 1 | 0.560495 | 0.492 | 59.353 | 2.56895 | F | F | 3.32e+20 | 1.59544e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 2 | X081853.66+313013.0 | chandra | ccd7 | 308.25 | 797.875 | 7.73551 | 2.82843 | 0.00129731 | 0.000474352 | 2.69816 | 0.989589 | 0.492 | 0.492 | 176.073 | 3.48009 | F | F | 3.32e+20 | 1.03206e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 5 | X081825.05+312750.0 | chandra | ccd7 | 1052 | 507 | 6.60463 | 2.64576 | 0.00110765 | 0.000443716 | 2.30371 | 0.978713 | 0.502115 | 0.492 | 65.3006 | 4.36463 | F | F | 3.32e+20 | 1.01077e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 2 | X081829.59+313460.0 | chandra | ccd6 | 663.75 | 366 | 3.94554 | 2 | 0.000661709 | 0.000335421 | 5.37135 | 0.999756 | 0.492 | 0.492 | 160.67 | 4.1916 | F | F | 3.33e+20 | 7.46031e-15 | 1 | dx | ||||
Report | srcpi bgdpi arf | 3 | X081837.91+313611.3 | chandra | ccd6 | 447.5 | 510.833 | 2.94147 | 1.73205 | 0.000493316 | 0.000290484 | 4.00444 | 0.997697 | 0.492 | 0.492 | 90 | 4.97608 | F | F | 3.33e+20 | 5.52594e-15 | 1 | dx | ||||
Report | srcpi bgdpi arf | 4 | X081842.50+313559.2 | chandra | ccd6 | 328.25 | 486.25 | 3.86824 | 2 | 0.000648744 | 0.000335422 | 5.26611 | 0.999756 | 0.492 | 0.492 | 45 | 4.86949 | F | F | 3.33e+20 | 7.42593e-15 | 1 | dx | ||||
Report | srcpi bgdpi arf | 5 | X081846.14+313736.7 | chandra | ccd6 | 233.9 | 684.5 | 4.5721 | 2.23608 | 0.000766789 | 0.000375014 | 6.22432 | 0.999978 | 1.12662 | 0.492 | 44.1408 | 6.63006 | A | F | 3.33e+20 | 9.77917e-15 | 1 | dx | ||||
Report | srcpi bgdpi arf | 6 | X081846.10+313740.9 | chandra | ccd6 | 235 | 693 | 1.74236 | 1.41422 | 0.000292212 | 0.00023718 | 2.372 | 0.982434 | 0.782767 | 0.492 | 45 | 6.69504 | A | F | 3.33e+20 | 3.69806e-15 | 1 | dx | ||||
Report | srcpi bgdpi arf | 7 | X081836.44+313401.0 | chandra | ccd6 | 485.667 | 246 | 5.9235 | 2.44949 | 0.000993434 | 0.000410806 | 8.06409 | 0.999998 | 0.492 | 0.492 | 94.2654 | 2.82416 | F | F | 3.33e+20 | 1.06787e-14 | 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