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 | X083642.74+532837.7 | chandra | ccd7 | 813.904 | 233.859 | 167.57 | 81.3966 | 0.0105166 | 0.00510843 | 4.16298 | 0.999978 | 2.12573 | 2.12573 | 0 | 6.01584 | F | T | 3.61e+20 | 7.10737e-14 | 1 | dsxf | ||||
| Report | srcpi bgdpi arf rmf | 16 | X083645.03+532753.1 | chandra | ccd7 | 772.321 | 143.127 | 177.747 | 13.5681 | 0.0111553 | 0.000851527 | 4.41581 | 0.999993 | 2.77296 | 1.67576 | 335.71 | 6.77192 | F | F | 3.6e+20 | 9.15255e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf rmf | 7 | X083642.82+533432.6 | chandra | ccd7 | 812.364 | 955.149 | 129.012 | 12.0751 | 0.00809675 | 0.00075783 | 3.20508 | 0.999247 | 0.429589 | 0.429589 | 0 | 0.12297 | F | F | 3.61e+20 | 5.865e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 1 | X083736.11+534214.8 | chandra | ccd2 | 728.54 | 552.088 | 72.8036 | 10.3529 | 0.00457001 | 0.000649873 | 12.4165 | 1 | 6.38854 | 3.97457 | 38.8348 | 10.8773 | F | T | 3.45e+20 | 6.17046e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 1 | X083821.73+533853.7 | chandra | ccd3 | 337.377 | 1101.34 | 43.903 | 10.1001 | 0.00275533 | 0.000633874 | 42.1446 | 1 | 4.23563 | 3.64824 | 80.072 | 15.2164 | F | T | 3.38e+20 | 3.96843e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 4 | X083740.86+533516.7 | chandra | ccd3 | 1074.56 | 657.062 | 41.0088 | 6.92827 | 0.00257369 | 0.000434814 | 39.3663 | 1 | 3.89354 | 1.82372 | 161.699 | 8.5801 | A | F | 3.44e+20 | 3.48277e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 1 | X083602.49+534131.4 | chandra | ccd6 | 1114.5 | 839.133 | 41.6421 | 6.45873 | 0.00261446 | 0.000405505 | 39.8171 | 1 | 5.4772 | 5.4772 | 0 | 9.12713 | F | T | 3.67e+20 | 3.09489e-14 | 1 | dbsx | ||||
| Report | srcpi bgdpi arf | 6 | X083628.77+533619.9 | chandra | ccd6 | 640.582 | 205.39 | 26.8889 | 5.18545 | 0.00168819 | 0.000325563 | 25.7105 | 1 | 0.838761 | 0.838761 | 0 | 2.72011 | F | F | 3.63e+20 | 1.75121e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 4 | X083638.80+533833.3 | chandra | ccd6 | 459.092 | 476.269 | 13.8564 | 3.72242 | 0.000869958 | 0.000233708 | 13.2491 | 1 | 0.891045 | 0.891045 | 0 | 3.95154 | F | F | 3.62e+20 | 9.21502e-15 | 1 | dsx | ||||
| Report | 3 | X083625.16+534033.8 | chandra | ccd6 | 704.833 | 720.833 | 5.54967 | 2.4495 | 0.00034843 | 0.000153789 | 5.30646 | 0.999856 | 0.492 | 0.492 | 145.278 | 6.48665 | F | F | 3.64e+20 | 0 | 1 | d | |||||
| Report | srcpi bgdpi arf | 2 | X083619.30+533842.2 | chandra | ccd6 | 810.9 | 494.3 | 4.84669 | 2.23607 | 0.000304294 | 0.000140389 | 4.63428 | 0.99906 | 0.492 | 0.492 | 144.217 | 5.38254 | F | T | 3.65e+20 | 3.29621e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 3 | X083736.07+533446.1 | chandra | ccd3 | 1161 | 594.5 | 3.66672 | 2.00001 | 0.000230121 | 0.00012552 | 3.51986 | 0.99486 | 0.492 | 0.492 | 26.5651 | 7.84843 | F | F | 3.45e+20 | 3.11416e-15 | 1 | dx | ||||
| Report | 2 | X083737.67+533518.2 | chandra | ccd3 | 1132.17 | 659.833 | 2.48147 | 1.73207 | 0.000155736 | 0.000108704 | 2.38208 | 0.975338 | 0.639127 | 0.492 | 101.31 | 8.11096 | F | T | 3.45e+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