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 | 6 | X192606.32+505257.0 | chandra | ccd7 | 550.865 | 457.064 | 267.294 | 16.9206 | 0.0912999 | 0.00577957 | 90.7869 | 1 | 0.44856 | 0.386292 | 351.423 | 0.438049 | F | F | 8.39e+20 | 8.54793e-13 | 1 | dsxf | ||||
Report | srcpi bgdpi arf | 1 | X192538.17+504613.6 | chandra | ccd2 | 348.206 | 1033.15 | 16.0642 | 4.12312 | 0.00548725 | 0.00140839 | 3.81407 | 0.999615 | 1.62631 | 0.909127 | 70.888 | 8.10009 | A | F | 7.97e+20 | 7.51002e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 2 | X192523.65+504105.4 | chandra | ccd2 | 630.19 | 407.935 | 47.0842 | 7.69159 | 0.0160832 | 0.00262732 | 11.179 | 1 | 9.83189 | 9.83189 | 0 | 13.6589 | F | F | 7.75e+20 | 2.37949e-13 | 1 | dsx | ||||
Report | srcpi bgdpi arf rmf | 3 | X192502.16+504316.1 | chandra | ccd2 | 1044.45 | 674.915 | 858.112 | 29.6903 | 0.293118 | 0.0101417 | 203.739 | 1 | 9.35205 | 9.35205 | 0 | 14.1149 | F | F | 7.77e+20 | 4.75456e-12 | 1 | dsxf | ||||
Report | srcpi bgdpi arf | 1 | X192633.10+504457.0 | chandra | ccd6 | 571.376 | 317.77 | 26.8644 | 5.18309 | 0.00917621 | 0.00177041 | 53.7022 | 1 | 4.3655 | 4.3655 | 0 | 8.71311 | F | F | 8.04e+20 | 1.10775e-13 | 1 | dscx | ||||
Report | srcpi bgdpi arf | 5 | X192541.88+505641.8 | chandra | ccd7 | 1020.29 | 914.405 | 20.7155 | 5.26394 | 0.00707579 | 0.001798 | 7.03605 | 1 | 1.22325 | 1.22325 | 0 | 5.80864 | F | F | 8.45e+20 | 5.72392e-14 | 1 | dsx | ||||
Report | srcpi bgdpi arf | 3 | X192626.04+504331.8 | chandra | ccd6 | 706.889 | 143.944 | 14.5499 | 4.2427 | 0.00496987 | 0.00144919 | 29.0855 | 1 | 2.8195 | 2.32372 | 132.944 | 9.60009 | F | F | 7.97e+20 | 6.21001e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 1 | X192606.40+505306.1 | chandra | ccd7 | 549.24 | 475.62 | 11.6903 | 3.41911 | 0.00399308 | 0.00116787 | 3.97063 | 0.999728 | 0.697907 | 0.697907 | 0 | 0.519915 | F | F | 8.4e+20 | 3.20517e-14 | 1 | dsx | ||||
Report | srcpi bgdpi arf | 2 | X192633.44+504503.7 | chandra | ccd6 | 564.333 | 330.917 | 10.2778 | 3.46413 | 0.00351061 | 0.00118325 | 20.5454 | 1 | 2.24272 | 2.10713 | 77.683 | 8.60645 | F | F | 8.05e+20 | 4.23069e-14 | 1 | dcx | ||||
Report | srcpi bgdpi arf | 4 | X192616.44+504633.1 | chandra | ccd6 | 892.3 | 512.3 | 4.75993 | 2.23607 | 0.00162586 | 0.000763783 | 9.51515 | 1 | 1.56421 | 0.492 | 118.42 | 6.29948 | A | F | 8.07e+20 | 1.94082e-14 | 1 | dx | ||||
Report | 7 | X192615.91+504727.8 | chandra | ccd6 | 902.5 | 623.5 | 2.96617 | 1.73205 | 0.00101316 | 0.000591622 | 5.9294 | 0.999866 | 0.492 | 0.492 | 45 | 5.38952 | F | F | 8.12e+20 | 0 | 1 | d | |||||
Report | 1 | X192518.44+505041.0 | chandra | ccd3 | 171.167 | 712.5 | 2.8103 | 1.73206 | 0.000959935 | 0.000591632 | 6.10955 | 0.999929 | 0.903862 | 0.492 | 90 | 8.1963 | A | F | 8.07e+20 | 0 | 1 | d | |||||
Report | srcpi bgdpi arf | 5 | X192642.03+505045.8 | chandra | ccd6 | 400 | 1026.5 | 1.97277 | 1.41421 | 0.000673846 | 0.000483057 | 3.94359 | 0.997832 | 0.492 | 0.492 | 180 | 5.61111 | F | F | 8.44e+20 | 8.28854e-15 | 1 | dx | ||||
Report | srcpi bgdpi arf | 6 | X192636.76+505105.0 | chandra | ccd6 | 501.5 | 1065.5 | 0.946684 | 1 | 0.000323361 | 0.000341574 | 1.89243 | 0.973453 | 0.492 | 0.492 | 90 | 4.71953 | F | F | 8.43e+20 | 3.83905e-15 | 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