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 | X043741.62+505646.2 | chandra | ccd1 | 221.756 | 626.596 | 471.234 | 23.1317 | 0.047334 | 0.00232351 | 96.4787 | 1 | 2.72324 | 2.72324 | 0 | 9.19613 | F | F | 6.25e+21 | 5.69237e-13 | 1 | dsxf | ||||
Report | srcpi bgdpi arf | 1 | X043649.46+505243.0 | chandra | ccd3 | 972.51 | 1129.86 | 8.9417 | 4.51329 | 0.000898166 | 0.000453346 | 2.64505 | 0.992974 | 0.97108 | 0.200879 | 93.5852 | 0.26308 | A | F | 6.35e+21 | 1.16354e-14 | 1 | dsx | ||||
Report | srcpi bgdpi arf | 2 | X043702.11+505649.3 | chandra | ccd1 | 980.696 | 631.572 | 10.5719 | 4.02046 | 0.00106192 | 0.000403843 | 2.16445 | 0.980934 | 0.46781 | 0.46781 | 0 | 4.43684 | F | F | 6.3e+21 | 1.48322e-14 | 1 | dsx | ||||
Report | srcpi bgdpi arf | 2 | X043645.42+504556.4 | chandra | ccd3 | 1049.9 | 303 | 8.99707 | 3.1623 | 0.000903727 | 0.000317643 | 2.66142 | 0.992974 | 1.39624 | 0.697456 | 156.727 | 7.0124 | A | F | 6.39e+21 | 1.36375e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 3 | X043711.07+504933.7 | chandra | ccd3 | 555.833 | 744.944 | 8.78196 | 3 | 0.00088212 | 0.000301341 | 2.59779 | 0.992974 | 0.79362 | 0.492 | 160.64 | 4.89671 | A | F | 6.35e+21 | 1.21268e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 4 | X043601.95+504720.7 | chandra | ccd2 | 879.8 | 239.4 | 8.32275 | 3.16231 | 0.000835994 | 0.000317644 | 9.77826 | 1 | 1.90545 | 0.683886 | 54.1317 | 9.24478 | A | F | 6.41e+21 | 1.38711e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 6 | X043653.23+504937.0 | chandra | ccd3 | 899.5 | 751.25 | 7.83941 | 2.82843 | 0.000787444 | 0.000284107 | 2.31898 | 0.986515 | 0.56815 | 0.492 | 52.0181 | 3.39912 | F | F | 6.36e+21 | 1.07046e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 4 | X043648.92+505302.6 | chandra | ccd3 | 982.5 | 1169.25 | 7.60017 | 2.82844 | 0.000763413 | 0.000284108 | 2.24821 | 0.986515 | 0.546906 | 0.492 | 30.7785 | 0.121019 | F | F | 6.35e+21 | 1.2127e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 5 | X043659.44+504908.0 | chandra | ccd3 | 779.786 | 692.357 | 6.80221 | 2.64576 | 0.00068326 | 0.000265758 | 2.01216 | 0.97521 | 0.676719 | 0.492 | 124.538 | 4.17101 | F | F | 6.36e+21 | 9.38563e-15 | 1 | dx | ||||
Report | srcpi bgdpi arf | 1 | X043522.74+503942.0 | chandra | ccd6 | 1118.06 | 572.944 | 6.77891 | 3.00004 | 0.00068092 | 0.000301345 | 7.80566 | 0.999999 | 2.33477 | 1.73135 | 1.33515 | 18.9573 | F | F | 6.49e+21 | 1.31553e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 2 | X043623.09+505401.6 | chandra | ccd2 | 471.214 | 1053.36 | 6.76509 | 2.64576 | 0.000679532 | 0.000265758 | 7.94819 | 0.999999 | 0.763903 | 0.492 | 116.565 | 4.16584 | A | F | 6.37e+21 | 9.22356e-15 | 1 | dx | ||||
Report | srcpi bgdpi arf | 3 | X043609.30+504739.0 | chandra | ccd2 | 738.071 | 276.357 | 6.18218 | 2.64577 | 0.00062098 | 0.000265759 | 7.26334 | 0.999989 | 1.31028 | 0.840396 | 50.0679 | 8.14831 | A | F | 6.4e+21 | 9.80319e-15 | 1 | dx | ||||
Report | 15 | X043711.26+504516.6 | chandra | ccd3 | 551.643 | 222.214 | 6.16115 | 2.64577 | 0.000618868 | 0.000265759 | 1.82253 | 0.956416 | 0.523195 | 0.492 | 142.161 | 8.4553 | F | T | 6.37e+21 | 0 | 1 | d | |||||
Report | 8 | X043704.25+504819.3 | chandra | ccd3 | 687 | 593.5 | 5.91884 | 2.44949 | 0.000594528 | 0.000246044 | 1.75085 | 0.956416 | 0.492 | 0.492 | 180 | 5.23524 | F | T | 6.36e+21 | 0 | 1 | d | |||||
Report | srcpi bgdpi arf | 7 | X043652.58+504522.2 | chandra | ccd3 | 911.833 | 233.333 | 5.59912 | 2.4495 | 0.000562413 | 0.000246044 | 1.65628 | 0.956416 | 0.492 | 0.492 | 122.886 | 7.59228 | F | F | 6.38e+21 | 8.54966e-15 | 1 | dx | ||||
Report | srcpi bgdpi arf | 6 | X043728.23+505725.7 | chandra | ccd1 | 478.6 | 705.8 | 8.8348 | 3.1623 | 0.000887427 | 0.000317643 | 1.8088 | 0.956246 | 1.38897 | 0.999108 | 98.767 | 7.69626 | F | F | 6.26e+21 | 1.26718e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 8 | X043701.67+505437.1 | chandra | ccd1 | 988.82 | 362.781 | 16.5385 | 4.32143 | 0.00166124 | 0.000434075 | 3.38603 | 0.999116 | 0.452888 | 0.452888 | 0 | 2.66229 | F | T | 6.32e+21 | 2.16109e-14 | 1 | dsx | ||||
Report | srcpi bgdpi arf | 1 | X043629.47+504909.1 | chandra | ccd2 | 349.1 | 458.7 | 4.87364 | 2.23607 | 0.000489542 | 0.000224606 | 5.72596 | 0.999892 | 0.558616 | 0.492 | 104.221 | 4.83936 | F | F | 6.38e+21 | 6.92646e-15 | 1 | dx | ||||
Report | srcpi bgdpi arf | 6 | X043636.31+505302.7 | chandra | ccd2 | 217 | 933.5 | 3.90739 | 2 | 0.000392485 | 0.000200894 | 4.59073 | 0.999086 | 0.492 | 0.492 | 121.717 | 1.93836 | F | F | 6.36e+21 | 5.29857e-15 | 1 | dx | ||||
Report | srcpi bgdpi arf | 5 | X043630.98+505147.2 | chandra | ccd2 | 319.75 | 780 | 3.88799 | 2 | 0.000390536 | 0.000200894 | 4.56793 | 0.999086 | 0.492 | 0.492 | 14.8724 | 3.00563 | F | F | 6.37e+21 | 5.25294e-15 | 1 | dx | ||||
Report | srcpi bgdpi arf | 8 | X043634.53+505011.7 | chandra | ccd2 | 251.5 | 585.833 | 2.90688 | 1.73205 | 0.000291987 | 0.000173979 | 3.41524 | 0.993524 | 0.492 | 0.492 | 90 | 3.52541 | F | T | 6.37e+21 | 4.00566e-15 | 1 | dx | ||||
Report | 7 | X043607.31+505406.5 | chandra | ccd2 | 774.5 | 1064 | 2.71733 | 1.73206 | 0.000272947 | 0.00017398 | 3.19254 | 0.993524 | 0.492 | 0.492 | 90 | 6.61297 | F | F | 6.38e+21 | 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