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 | X212700.21+101119.2 | chandra | ccd7 | 922.982 | 903.864 | 313.833 | 18.1814 | 0.156609 | 0.00907285 | 108.51 | 1 | 0.449675 | 0.387851 | 337.339 | 0.290563 | F | F | 3.72e+20 | 1.35232e-12 | 1 | dsxf | ||||
| Report | srcpi bgdpi arf | 7 | X212706.05+101021.0 | chandra | ccd7 | 747.707 | 785.587 | 13.2327 | 3.63768 | 0.00660335 | 0.00181527 | 4.5753 | 0.999937 | 0.516976 | 0.516976 | 0 | 2.01648 | F | F | 3.7e+20 | 4.93389e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 1 | X212746.22+101559.9 | chandra | ccd3 | 589.333 | 541.278 | 13.7205 | 4.24272 | 0.00684664 | 0.00211716 | 32.8527 | 1 | 5.7711 | 3.5401 | 177.709 | 12.4663 | A | F | 3.71e+20 | 1.02023e-13 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 3 | X212702.10+101240.6 | chandra | ccd7 | 865.8 | 1068.8 | 9.89421 | 3.16228 | 0.0049373 | 0.00157801 | 3.42099 | 0.998916 | 0.492 | 0.492 | 67.0304 | 1.46205 | F | F | 3.74e+20 | 3.69504e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 2 | X212656.94+101137.1 | chandra | ccd7 | 1020.64 | 939.643 | 6.94363 | 2.64575 | 0.00346494 | 0.00132026 | 2.40081 | 0.987911 | 0.492 | 0.492 | 69.6994 | 0.567284 | F | F | 3.73e+20 | 2.59449e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 5 | X212700.06+100923.3 | chandra | ccd7 | 927.167 | 667.667 | 5.87696 | 2.44949 | 0.00293266 | 0.00122232 | 2.032 | 0.975677 | 0.511691 | 0.492 | 8.70899 | 2.04187 | F | F | 3.7e+20 | 2.20302e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 1 | X212640.17+101504.8 | chandra | ccd6 | 691.7 | 678.9 | 4.94605 | 2.23607 | 0.00246812 | 0.00111582 | 11.504 | 1 | 0.657652 | 0.492 | 162.344 | 5.92448 | F | F | 3.81e+20 | 2.94356e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 2 | X212736.09+101423.3 | chandra | ccd3 | 893.1 | 344.7 | 4.20823 | 2.23609 | 0.00209995 | 0.00111583 | 10.0763 | 0.999999 | 2.60088 | 0.801625 | 104.24 | 9.57481 | A | F | 3.71e+20 | 2.95067e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 1 | X212622.43+101649.4 | chandra | ccd5 | 490.9 | 228.7 | 3.82753 | 2.2361 | 0.00190997 | 0.00111584 | 4.65307 | 0.999324 | 1.31281 | 0.492 | 77.8954 | 10.5171 | A | F | 3.88e+20 | 1.8231e-14 | 1 | dx | ||||
| Report | 2 | X212640.31+101350.3 | chandra | ccd6 | 687.5 | 527.5 | 0.990083 | 1 | 0.000494061 | 0.00049901 | 2.30283 | 0.984882 | 0.492 | 0.492 | 90 | 5.2175 | F | F | 3.79e+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