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 | 1 | X162039.66+050731.5 | chandra | ccd2 | 561.589 | 501.633 | 73.6785 | 10.6307 | 0.00988966 | 0.00142693 | 17.2132 | 1 | 7.50804 | 4.82086 | 32.566 | 13.109 | 51.1828 | 23.2569 | -0.375149 | 0.152714 | A | F | 4.9e+20 | 1.40011e-13 | 1 | dx |
| Report | srcpi bgdpi arf | 12 | X161940.51+050635.1 | chandra | ccd7 | 771.447 | 554.277 | 18.6294 | 4.32196 | 0.00250058 | 0.000580127 | 14.9374 | 1 | 0.885842 | 0.382983 | 115.701 | 3.91073 | 18.8901 | 0.853508 | -0.913541 | 0.382977 | F | F | 4.88e+20 | 1.93329e-14 | 1 | dsx |
| Report | srcpi bgdpi arf | 6 | X161940.08+050450.7 | chandra | ccd7 | 784 | 341.5 | 16.5695 | 5.21307 | 0.00222407 | 0.000699737 | 25.2525 | 1 | 0.836498 | 0.596254 | 94.2654 | 5.53966 | 10.9385 | 5.75398 | -0.31059 | 0.328872 | F | F | 4.89e+20 | 1.77341e-14 | 1 | dx |
| Report | 4 | X161943.09+051050.0 | chandra | ccd7 | 693.015 | 1072.32 | 12.2139 | 3.49484 | 0.00163945 | 0.000469106 | 9.79333 | 1 | 0.351479 | 0.351479 | 0 | 1.46524 | F | T | 4.83e+20 | 0 | 1 | ds | |||||
| Report | srcpi bgdpi arf | 7 | X161939.95+050453.9 | chandra | ccd7 | 787.833 | 348 | 15.875 | 5.09268 | 0.00213086 | 0.000683576 | 44.9028 | 1 | 0.711689 | 0.492 | 105.274 | 5.50121 | 12 | 3.9375 | -0.505882 | 0.360241 | F | F | 4.89e+20 | 1.68958e-14 | 1 | dbx |
| Report | srcpi bgdpi arf | 1 | X162007.07+051645.3 | chandra | ccd6 | 423.872 | 858.459 | 30.545 | 5.52675 | 0.00409999 | 0.000741844 | 38.7898 | 1 | 3.25508 | 3.25508 | 0 | 8.20164 | 16.8832 | 9.17362 | -0.295875 | 0.27339 | F | F | 4.74e+20 | 4.98257e-14 | 1 | dsx |
| Report | srcpi bgdpi arf | 1 | X161940.30+050714.4 | chandra | ccd7 | 777.838 | 634.064 | 9.68186 | 3.11157 | 0.00129958 | 0.00041766 | 7.76309 | 1 | 0.876743 | 0.419211 | 110.63 | 3.37809 | 6.87851 | 2.87851 | -0.409961 | 0.478147 | F | F | 4.87e+20 | 1.0002e-14 | 1 | dsx |
| Report | srcpi bgdpi arf | 2 | X161950.97+051458.1 | chandra | ccd6 | 912.1 | 640.2 | 10.8902 | 4.42783 | 0.00146176 | 0.000594335 | 32.8608 | 1 | 0.759252 | 0.492 | 115.29 | 5.00209 | 5.89017 | 5 | -0.0817409 | 0.411287 | A | F | 4.75e+20 | 1.63677e-14 | 1 | dx |
| Report | srcpi bgdpi arf | 3 | X162001.57+051228.1 | chandra | ccd6 | 590.389 | 335.167 | 8.81595 | 4.1225 | 0.00118334 | 0.000553352 | 20.5493 | 1 | 0.679174 | 0.492 | 108.752 | 4.17437 | 5 | 3.81595 | -0.134308 | 0.47637 | F | F | 4.81e+20 | 1.36747e-14 | 1 | dx |
| Report | srcpi bgdpi arf | 5 | X161949.53+051227.6 | chandra | ccd6 | 956.056 | 334.278 | 8.92901 | 4.1225 | 0.00119852 | 0.000553352 | 33.5135 | 1 | 0.587111 | 0.492 | 10.2361 | 2.46789 | 2 | 6 | 0.5 | 0.559017 | F | F | 4.81e+20 | 1.27609e-14 | 1 | dx |
| Report | srcpi bgdpi arf | 3 | X161948.07+050953.0 | chandra | ccd7 | 541.25 | 956 | 7.00337 | 3.95804 | 0.000940043 | 0.000531277 | 7.01521 | 0.999999 | 0.58578 | 0.492 | 36.5046 | 0.141212 | 4.57287 | 2.64406 | -0.267262 | 0.573705 | F | F | 4.84e+20 | 7.04067e-15 | 1 | dx |
| Report | srcpi bgdpi arf | 9 | X161957.08+050932.2 | chandra | ccd7 | 267.625 | 913.75 | 7.37078 | 3.95804 | 0.000989359 | 0.000531277 | 9.29206 | 1 | 0.595866 | 0.492 | 22.6897 | 2.31777 | 6.86017 | 0.930087 | -0.761218 | 0.6453 | F | F | 4.85e+20 | 7.6294e-15 | 1 | dx |
| Report | srcpi bgdpi arf | 8 | X161936.27+050727.5 | chandra | ccd7 | 899.625 | 660.25 | 7.51829 | 3.95804 | 0.00100916 | 0.000531277 | 10.8325 | 1 | 0.605664 | 0.492 | 94.0179 | 3.88339 | 6.93118 | 0.724738 | -0.810673 | 0.672587 | F | F | 4.87e+20 | 7.83469e-15 | 1 | dx |
| Report | srcpi bgdpi arf | 2 | X161939.74+050831.9 | chandra | ccd7 | 794.214 | 791.072 | 6.77493 | 3.78388 | 0.00090938 | 0.0005079 | 14.2805 | 1 | 0.555158 | 0.492 | 67.5 | 2.53677 | 4.92498 | 1.92498 | -0.437959 | 0.610149 | F | F | 4.86e+20 | 6.93219e-15 | 1 | dx |
| Report | srcpi bgdpi arf | 10 | X161933.23+050956.3 | chandra | ccd7 | 991.786 | 962.786 | 6.5983 | 3.78388 | 0.000885672 | 0.0005079 | 10.4108 | 1 | 0.62254 | 0.492 | 48.8334 | 3.6728 | 4.79915 | 0.93305 | -0.674453 | 0.76715 | F | F | 4.84e+20 | 7.4837e-15 | 1 | dx |
| Report | srcpi bgdpi arf | 1 | X162009.71+050016.5 | chandra | ccd3 | 1004.12 | 571.375 | 8.56694 | 4.27872 | 0.00114992 | 0.000574321 | 7.15638 | 1 | 2.70291 | 1.03967 | 168.172 | 11.148 | 3.70687 | 4.9252 | 0.14114 | 0.505024 | A | F | 4.94e+20 | 1.73016e-14 | 1 | dx |
| Report | srcpi bgdpi arf | 11 | X161933.77+051131.0 | chandra | ccd7 | 975.333 | 1155.17 | 5.83879 | 3.59808 | 0.000783724 | 0.00048296 | 14.5419 | 1 | 0.517376 | 0.492 | 55.278 | 3.83943 | 2.91939 | 2.91939 | 0 | 0.453134 | F | F | 4.82e+20 | 7.35521e-15 | 1 | dx |
| Report | srcpi bgdpi arf | 4 | X161944.74+051557.0 | chandra | ccd6 | 1101.3 | 759.9 | 4.90529 | 3.39792 | 0.000658423 | 0.000456093 | 15.939 | 1 | 0.879798 | 0.492 | 14.2371 | 5.98233 | 4 | 1.90529 | -0.354718 | 0.655061 | A | T | 4.73e+20 | 8.02573e-15 | 1 | dx |
| Report | srcpi bgdpi arf | 5 | X161936.49+051135.1 | chandra | ccd7 | 892.833 | 1163.5 | 2.83061 | 2.93649 | 0.000379945 | 0.000394157 | 6.87766 | 0.99997 | 0.492 | 0.492 | 180 | 3.25918 | 2.83061 | 0 | -1 | 1.49884 | F | F | 4.82e+20 | 3.21632e-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