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 | 2 | X220538.65-053532.3 | chandra | ccd3 | 907.286 | 139.228 | 48.2194 | 16.4483 | 0.00485988 | 0.00165777 | 5.54688 | 1 | 0.504882 | 0.504882 | 0 | 1.00655 | F | F | 5.18e+20 | 5.52734e-14 | 1 | dsx | ||||
Report | srcpi bgdpi arf | 8 | X220521.73-053331.1 | chandra | ccd1 | 404.618 | 571.448 | 36.2129 | 6.11137 | 0.00365094 | 0.000616141 | 41.7311 | 1 | 0.812951 | 0.812951 | 0 | 5.00678 | F | F | 5.15e+20 | 4.62917e-14 | 1 | dsx | ||||
Report | srcpi bgdpi arf | 3 | X220512.01-053352.9 | chandra | ccd1 | 699.798 | 527.12 | 30.9973 | 5.56752 | 0.00312511 | 0.000561311 | 35.7208 | 1 | 1.71356 | 0.907962 | 359.668 | 6.9432 | F | F | 5.12e+20 | 3.96236e-14 | 1 | dsx | ||||
Report | srcpi bgdpi arf | 1 | X220626.43-053644.5 | chandra | ccd6 | 1025.59 | 946.191 | 37.6817 | 8.12748 | 0.00379782 | 0.000819144 | 7.07405 | 1 | 7.1408 | 7.1408 | 0 | 12.0824 | F | F | 5.27e+20 | 5.27617e-14 | 1 | dsx | ||||
Report | srcpi bgdpi arf | 1 | X220527.74-054155.9 | chandra | ccd0 | 411.287 | 580.461 | 24.6154 | 6.1614 | 0.0024809 | 0.000620987 | 10.6309 | 1 | 1.08756 | 1.08756 | 0 | 5.9619 | F | F | 5.1e+20 | 3.14485e-14 | 1 | dsx | ||||
Report | srcpi bgdpi arf | 2 | X220517.10-054057.8 | chandra | ccd0 | 734.058 | 698.604 | 26.9472 | 5.26586 | 0.00271592 | 0.000530729 | 11.6379 | 1 | 1.99595 | 1.99595 | 0 | 6.8035 | F | F | 5.08e+20 | 3.50586e-14 | 1 | dsx | ||||
Report | srcpi bgdpi arf | 3 | X220516.84-053804.7 | chandra | ccd0 | 742.104 | 1050.3 | 38.2307 | 6.74882 | 0.00385315 | 0.000680192 | 16.511 | 1 | 1.5 | 0.797388 | 15.5527 | 5.4488 | F | F | 5.11e+20 | 4.75166e-14 | 1 | dsx | ||||
Report | srcpi bgdpi arf | 1 | X220539.52-053323.4 | chandra | ccd3 | 880.819 | 401.057 | 16.738 | 4.20225 | 0.00168697 | 0.000423532 | 1.92544 | 0.971248 | 0.703992 | 0.356755 | 114.94 | 3.15983 | F | F | 5.19e+20 | 1.97208e-14 | 1 | dsx | ||||
Report | srcpi bgdpi arf | 2 | X220507.58-053418.8 | chandra | ccd1 | 833.5 | 474 | 16.9384 | 4.24266 | 0.0017077 | 0.000427737 | 19.5195 | 1 | 1.21009 | 0.801493 | 123.487 | 7.84019 | A | F | 5.11e+20 | 2.35356e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 11 | X220546.47-053538.9 | chandra | ccd3 | 670.066 | 125.799 | 15.5905 | 4.36476 | 0.00157131 | 0.000439909 | 1.79344 | 0.963419 | 0.589597 | 0.589597 | 0 | 2.32186 | F | F | 5.19e+20 | 1.85274e-14 | 1 | dsx | ||||
Report | srcpi bgdpi arf | 4 | X220610.55-053851.9 | chandra | ccd2 | 127.967 | 734.767 | 12.5327 | 3.87303 | 0.00126313 | 0.00039035 | 13.1899 | 1 | 2.82048 | 1.20628 | 125.835 | 8.47439 | A | F | 5.22e+20 | 1.84129e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 1 | X220545.90-054423.5 | chandra | ccd2 | 875.833 | 61.0557 | 8.14361 | 3.00002 | 0.000820768 | 0.000302362 | 8.57065 | 1 | 1.20415 | 1.06081 | 105.94 | 8.12421 | F | F | 5.12e+20 | 1.2393e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 1 | X220513.32-053652.7 | chandra | ccd1 | 659.375 | 161.125 | 7.27721 | 2.82844 | 0.000733675 | 0.000285158 | 8.38613 | 1 | 1.28714 | 0.492 | 175.831 | 6.10628 | A | F | 5.1e+20 | 9.13393e-15 | 1 | dx | ||||
Report | srcpi bgdpi arf | 4 | X220519.38-054252.5 | chandra | ccd0 | 664.5 | 464.833 | 5.52517 | 2.4495 | 0.000556864 | 0.000246877 | 2.3862 | 0.978483 | 0.996397 | 0.492 | 162.652 | 7.83915 | A | F | 5.07e+20 | 7.49112e-15 | 1 | dx | ||||
Report | srcpi bgdpi arf | 2 | X220558.02-054350.1 | chandra | ccd2 | 508.333 | 128.833 | 5.18449 | 2.44951 | 0.000522528 | 0.000246878 | 5.45635 | 0.999956 | 1.44798 | 1.20305 | 60.2243 | 8.87467 | F | F | 5.15e+20 | 8.48852e-15 | 1 | dx | ||||
Report | srcpi bgdpi arf | 6 | X220522.95-053109.8 | chandra | ccd1 | 367.3 | 858.1 | 4.67627 | 2.23608 | 0.000471453 | 0.000225437 | 5.38885 | 0.999867 | 0.605406 | 0.492 | 14.2215 | 6.50964 | F | F | 5.16e+20 | 5.91887e-15 | 1 | dx | ||||
Report | 4 | X220520.31-053337.7 | chandra | ccd1 | 447.5 | 557.5 | 3.83816 | 2 | 0.000386956 | 0.000201637 | 4.42303 | 0.998916 | 0.607126 | 0.492 | 22.5 | 5.2297 | F | F | 5.14e+20 | 0 | 1 | d | |||||
Report | srcpi bgdpi arf | 3 | X220555.72-053649.1 | chandra | ccd2 | 578 | 984.5 | 3.76291 | 2.00001 | 0.000379251 | 0.000201574 | 3.96022 | 0.997624 | 0.492 | 0.492 | 180 | 4.46265 | F | F | 5.21e+20 | 4.73451e-15 | 1 | dx | ||||
Report | srcpi bgdpi arf | 6 | X220542.70-053733.5 | chandra | ccd2 | 973 | 894.25 | 3.75211 | 2.00001 | 0.000378162 | 0.000201574 | 3.94886 | 0.997624 | 0.492 | 0.492 | 104.872 | 1.59783 | F | F | 5.17e+20 | 4.40952e-15 | 1 | dx | ||||
Report | srcpi bgdpi arf | 6 | X220530.73-053950.1 | chandra | ccd0 | 320.642 | 836.106 | 20.7778 | 4.55827 | 0.00209413 | 0.000459414 | 8.97349 | 1 | 0.673119 | 0.673119 | 0 | 3.7543 | F | F | 5.12e+20 | 2.48866e-14 | 1 | dsx | ||||
Report | srcpi bgdpi arf | 5 | X220526.22-053003.8 | chandra | ccd1 | 268 | 992.25 | 3.4759 | 2.00002 | 0.000350434 | 0.000201638 | 4.00556 | 0.998916 | 0.897942 | 0.492 | 19.7087 | 7.07136 | A | F | 5.18e+20 | 4.60065e-15 | 1 | dx | ||||
Report | srcpi bgdpi arf | 5 | X220556.38-054012.8 | chandra | ccd2 | 557.833 | 570.5 | 2.93004 | 1.73205 | 0.000295309 | 0.000174568 | 3.08368 | 0.986401 | 0.510281 | 0.492 | 28.155 | 5.91371 | F | F | 5.18e+20 | 4.07344e-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