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 | X190447.48+090241.6 | chandra | ccd2 | 982.127 | 498.692 | 874.459 | 31.0477 | 0.0657732 | 0.00233528 | 117.621 | 1 | 3.28762 | 1.86873 | 111.46 | 7.96682 | A | F | 1.24e+22 | 0 | 1 | ds | |||||
Report | 10 | X190455.39+085953.9 | chandra | ccd2 | 743.974 | 157.807 | 32.4353 | 7.31317 | 0.00243965 | 0.000550066 | 4.36277 | 0.99997 | 1.7479 | 0.43409 | 126.879 | 6.66558 | F | F | 1.25e+22 | 0 | 1 | ds | |||||
Report | 10 | X190546.98+085931.2 | chandra | ccd1 | 643.359 | 363.606 | 41.4173 | 7.62879 | 0.00311524 | 0.000573806 | 13.0697 | 1 | 1.90423 | 1.90423 | 0 | 7.46076 | F | F | 1.34e+22 | 0 | 1 | ds | |||||
Report | 3 | X190543.37+085727.3 | chandra | ccd1 | 751.58 | 111.34 | 23.1948 | 5.00002 | 0.00174461 | 0.00037608 | 7.31939 | 1 | 1.96441 | 0.952786 | 13.3014 | 7.89451 | A | F | 1.34e+22 | 0 | 1 | d | |||||
Report | 7 | X190540.14+090400.9 | chandra | ccd1 | 849.72 | 911.87 | 25.6072 | 5.37686 | 0.00192607 | 0.000404425 | 8.08065 | 1 | 2.16358 | 0.521999 | 19.9254 | 5.17043 | A | F | 1.31e+22 | 0 | 1 | ds | |||||
Report | 1 | X190507.66+085434.4 | chandra | ccd3 | 973.522 | 368.331 | 10.4353 | 4.97254 | 0.000784902 | 0.000374015 | 2.76042 | 0.99359 | 1.37033 | 1.37033 | 0 | 8.73612 | F | F | 1.29e+22 | 0 | 1 | ds | |||||
Report | 1 | X190521.39+090920.4 | chandra | ccd0 | 816.643 | 700.714 | 13.279 | 3.74167 | 0.000999027 | 0.0002815 | 15.9711 | 1 | 1.42595 | 0.842632 | 141.23 | 6.57832 | A | F | 1.27e+22 | 0 | 1 | d | |||||
Report | 2 | X190510.36+085646.5 | chandra | ccd3 | 891.6 | 636.4 | 9.02755 | 3.1623 | 0.000679014 | 0.000237854 | 2.38803 | 0.988314 | 1.19552 | 0.798533 | 119.467 | 6.43113 | F | F | 1.29e+22 | 0 | 1 | d | |||||
Report | 5 | X190515.22+085951.2 | chandra | ccd3 | 745.5 | 1011.62 | 8.79591 | 3 | 0.000661591 | 0.000225647 | 2.32676 | 0.988314 | 0.492 | 0.492 | 122.199 | 3.1293 | F | F | 1.29e+22 | 0 | 1 | d | |||||
Report | 2 | X190527.93+090819.7 | chandra | ccd0 | 619.625 | 577.25 | 7.89068 | 2.82843 | 0.000593646 | 0.000212794 | 9.49044 | 1 | 0.544484 | 0.492 | 168.823 | 5.90951 | F | F | 1.28e+22 | 0 | 1 | d | |||||
Report | 1 | X190538.06+090006.0 | chandra | ccd1 | 911.643 | 433.928 | 6.89126 | 2.64575 | 0.000518331 | 0.000199002 | 2.17462 | 0.97203 | 0.588298 | 0.492 | 155.457 | 5.25259 | F | F | 1.32e+22 | 0 | 1 | d | |||||
Report | 3 | X190531.59+090618.1 | chandra | ccd0 | 509.5 | 330.214 | 6.75921 | 2.64576 | 0.000508521 | 0.00019905 | 8.12957 | 0.999999 | 0.679273 | 0.492 | 136.363 | 4.58157 | F | F | 1.29e+22 | 0 | 1 | d | |||||
Report | 4 | X190517.87+090713.3 | chandra | ccd0 | 922.5 | 442.214 | 6.67814 | 2.64576 | 0.000502422 | 0.000199051 | 8.03207 | 0.999999 | 0.743434 | 0.492 | 113.097 | 4.47023 | A | F | 1.27e+22 | 0 | 1 | d | |||||
Report | 5 | X190529.57+090619.8 | chandra | ccd0 | 570.875 | 334.091 | 11.2923 | 3.3604 | 0.000849565 | 0.000252816 | 13.5817 | 1 | 0.834008 | 0.354532 | 45.5884 | 4.30347 | F | F | 1.29e+22 | 0 | 1 | ds | |||||
Report | 9 | X190551.46+090157.9 | chandra | ccd1 | 508.214 | 661.5 | 6.22759 | 2.64577 | 0.000468413 | 0.000199003 | 1.96519 | 0.97203 | 1.41893 | 0.590424 | 75.3055 | 7.8708 | A | F | 1.33e+22 | 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