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 | X104303.78+005420.1 | chandra | ccd3 | 694.233 | 1065.81 | 555.156 | 24.5731 | 0.320057 | 0.0141668 | 79.568 | 1 | 3.36292 | 2.31114 | 309.233 | 8.8612 | F | F | 3.87e+20 | 0 | 1 | ds | |||||
| Report | 1 | X104230.14+010223.8 | chandra | ccd7 | 1050.92 | 910.847 | 98.7208 | 9.93583 | 0.0613869 | 0.00617833 | 109.581 | 1 | 1.51791 | 0.663436 | 251.848 | 4.46658 | A | F | 3.92e+20 | 0 | 1 | ds | |||||
| Report | 1 | X104332.92+010107.4 | chandra | ccd2 | 629.575 | 1164.15 | 34.4104 | 6.32462 | 0.0198382 | 0.00364625 | 110.118 | 1 | 4.36164 | 2.38943 | 175.158 | 11.2877 | A | F | 3.77e+20 | 0 | 1 | d | |||||
| Report | 8 | X104230.70+010002.2 | chandra | ccd7 | 1033.79 | 623.009 | 13.3909 | 3.65936 | 0.0083268 | 0.00227548 | 14.864 | 1 | 1.09625 | 0.325552 | 91.5192 | 4.87229 | A | F | 3.93e+20 | 0 | 1 | ds | |||||
| Report | 3 | X104240.49+010254.5 | chandra | ccd7 | 735.196 | 973.21 | 9.1847 | 3.40874 | 0.00571126 | 0.00211964 | 10.1951 | 1 | 0.49559 | 0.49559 | 0 | 1.97853 | F | F | 3.9e+20 | 0 | 1 | ds | |||||
| Report | 6 | X104229.39+010153.6 | chandra | ccd7 | 1073.06 | 849.056 | 8.78924 | 3 | 0.00506714 | 0.00172955 | 9.75615 | 1 | 1.0108 | 0.492 | 104.527 | 4.66509 | A | F | 3.92e+20 | 0 | 1 | d | |||||
| Report | 2 | X104320.66+005954.3 | chandra | ccd2 | 1003.39 | 1015.5 | 8.20502 | 3.00002 | 0.00473033 | 0.00172956 | 26.2572 | 1 | 1.76065 | 1.21758 | 0.535969 | 8.49986 | F | F | 3.78e+20 | 0 | 1 | d | |||||
| Report | 2 | X104248.57+010141.4 | chandra | ccd7 | 488.375 | 824.25 | 7.93753 | 2.82843 | 0.00457612 | 0.00163064 | 8.81074 | 1 | 0.492 | 0.492 | 56.3099 | 0.597881 | F | F | 3.89e+20 | 0 | 1 | d | |||||
| Report | 5 | X104256.15+010123.5 | chandra | ccd7 | 257.5 | 787.833 | 5.9292 | 2.44949 | 0.00341828 | 0.00141217 | 6.58148 | 0.999977 | 0.498199 | 0.492 | 17.3476 | 2.21911 | F | F | 3.87e+20 | 0 | 1 | d | |||||
| Report | 7 | X104233.89+010207.2 | chandra | ccd7 | 936 | 876.667 | 5.86151 | 2.44949 | 0.00337926 | 0.00141217 | 6.50634 | 0.999977 | 0.674648 | 0.492 | 105.206 | 3.5292 | F | F | 3.91e+20 | 0 | 1 | d | |||||
| Report | 3 | X104259.99+010330.0 | chandra | ccd6 | 834.3 | 335.9 | 4.93196 | 2.23607 | 0.00284336 | 0.00128913 | 13.201 | 1 | 0.718226 | 0.492 | 5.81682 | 3.24088 | F | F | 3.85e+20 | 0 | 1 | d | |||||
| Report | 4 | X104249.11+010320.7 | chandra | ccd7 | 471.9 | 1026.1 | 4.90304 | 2.23607 | 0.00282669 | 0.00128913 | 5.44243 | 0.999801 | 0.492 | 0.492 | 156.137 | 1.11079 | F | F | 3.88e+20 | 0 | 1 | d | |||||
| Report | 2 | X104300.45+010744.0 | chandra | ccd6 | 820.5 | 852.3 | 4.82673 | 2.23607 | 0.00278269 | 0.00128913 | 12.9193 | 1 | 0.705388 | 0.492 | 31.3919 | 6.28773 | F | F | 3.83e+20 | 0 | 1 | d | |||||
| Report | 1 | X104248.66+010721.1 | chandra | ccd6 | 1179.75 | 805.75 | 3.93279 | 2 | 0.00226732 | 0.00115304 | 10.5266 | 1 | 0.793565 | 0.492 | 108.435 | 5.08466 | A | F | 3.86e+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