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 | 5 | X155252.48+320150.8 | chandra | ccd7 | 275.245 | 626.426 | 48.8006 | 6.98574 | 0.0156336 | 0.00223792 | 82.476 | 1 | 0.493018 | 0.493018 | 0 | 0.13764 | F | F | 2.31e+20 | 0 | 1 | ds | |||||
Report | srcpi bgdpi arf | 2 | X155251.37+314949.0 | chandra | ccd3 | 326.692 | 520.769 | 31.3678 | 6.63341 | 0.0100487 | 0.00212503 | 77.6459 | 1 | 3.89929 | 3.30191 | 33.4257 | 11.946 | F | F | 2.27e+20 | 1.37392e-13 | 1 | dx | ||||
Report | srcpi bgdpi arf | 1 | X155222.45+315158.5 | chandra | ccd3 | 1075.44 | 784.375 | 13.4055 | 4.00006 | 0.00429447 | 0.00128143 | 33.1831 | 1 | 5.56381 | 3.60497 | 107.166 | 11.7324 | A | T | 2.26e+20 | 6.25261e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 3 | X155245.15+320511.3 | chandra | ccd7 | 464.762 | 1033.91 | 10.0223 | 3.1658 | 0.00321069 | 0.00101418 | 16.9383 | 1 | 1.56436 | 0.576586 | 1.5874 | 3.80971 | F | F | 2.32e+20 | 2.63841e-14 | 1 | dsx | ||||
Report | srcpi bgdpi arf | 1 | X155324.72+315210.4 | chandra | ccd2 | 479.1 | 655.767 | 10.7653 | 3.87308 | 0.00344868 | 0.00124075 | 27.0553 | 1 | 4.51493 | 3.08858 | 177.628 | 11.7128 | F | T | 2.31e+20 | 5.18359e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 4 | X155228.40+320340.3 | chandra | ccd7 | 897.1 | 848.7 | 9.7556 | 3.16228 | 0.00312523 | 0.00101304 | 16.4876 | 1 | 0.845112 | 0.589781 | 129.429 | 5.54921 | F | F | 2.3e+20 | 2.41447e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 4 | X155302.45+320258.3 | chandra | ccd6 | 1045.12 | 612.125 | 7.96049 | 2.82843 | 0.00255016 | 0.000906093 | 19.3745 | 1 | 0.492 | 0.492 | 45 | 2.34676 | F | F | 2.32e+20 | 2.66881e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 1 | X155312.65+320232.1 | chandra | ccd6 | 781.5 | 559 | 5.93645 | 2.44949 | 0.00190175 | 0.000784699 | 14.4483 | 1 | 0.618902 | 0.492 | 140.884 | 4.24184 | F | T | 2.33e+20 | 2.10606e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 2 | X155312.97+320401.3 | chandra | ccd6 | 773.5 | 740.3 | 4.91937 | 2.23607 | 0.00157593 | 0.00071633 | 11.9729 | 1 | 1.08148 | 0.492 | 38.1951 | 4.80323 | A | F | 2.34e+20 | 1.76031e-14 | 1 | dx | ||||
Report | 1 | X155237.60+320139.4 | chandra | ccd7 | 659.5 | 602.75 | 3.94254 | 2 | 0.001263 | 0.000640705 | 6.66313 | 0.999967 | 0.504598 | 0.492 | 110.05 | 3.26105 | F | T | 2.3e+20 | 0 | 1 | d | |||||
Report | 2 | X155232.57+320423.2 | chandra | ccd7 | 789.167 | 935.833 | 2.94358 | 1.73205 | 0.000942982 | 0.000554867 | 4.97483 | 0.999526 | 0.492 | 0.492 | 45 | 5.06039 | F | F | 2.3e+20 | 0 | 1 | d | |||||
Report | srcpi bgdpi arf | 3 | X155314.29+320524.3 | chandra | ccd6 | 739.5 | 909 | 1.96758 | 1.41421 | 0.000630317 | 0.000453047 | 4.78875 | 0.999293 | 0.492 | 0.492 | 153.435 | 5.80451 | F | F | 2.35e+20 | 7.18338e-15 | 1 | dx | ||||
Report | srcpi bgdpi arf | 2 | X155309.32+315427.3 | chandra | ccd2 | 878 | 933.5 | 1.92191 | 1.41422 | 0.000615688 | 0.000453047 | 4.83015 | 0.999412 | 0.492 | 0.492 | 180 | 8.08405 | F | F | 2.3e+20 | 8.22863e-15 | 1 | dx | ||||
Report | srcpi bgdpi arf | 3 | X155309.41+315421.2 | chandra | ccd2 | 875.786 | 921.214 | 6.78677 | 2.64576 | 0.00217415 | 0.000847574 | 17.0565 | 1 | 1.06382 | 0.534291 | 19.3005 | 8.18288 | A | F | 2.3e+20 | 2.92661e-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