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Table B.1.

Summary table of results for individual objects, diffuse emission, and pooling analysis.

Name T0 l b d σd
V2540 Oph 2298.8 9.8 8.2 9.9 4.8 <6.6 <43.5 <2819.3 <963.3
V4743 Sgr 2537.4 14.1 −11.9 4.5 1.8 <6.2 <6.4 <178.8 <30.0
V4744 Sgr 2572.4 4.9 2.1 N/A N/A <6.4 <67.1 <142.5 <149.2
DZ Cru 2640.0 −60.5 2.3 10.7 2.9 <5.2 <4.0 <121.9 <98.1
V475 Sct 2879.6 24.2 −3.9 14.0 6.7 <10.4 <197.9 <27.5 <58.1
V5113 Sgr 2899.5 3.7 −4.1 1.0 0.2 <5.7 <0.2 <18.4 <0.1
DE Cir 2921.0 −40.7 −3.8 N/A N/A <3.8 <24.3 <96.3 <131.8
V1186 Sco 3189.1 −5.6 4.8 4.0 2.2 <6.1 <7.0 <52.6 <13.6
V1187 Sco 3220.6 −4.3 1.5 3.2 0.1 <4.5 <1.3 <27.7 <1.3
V574 Pup 3329.7 −117.4 −2.0 12.4 5.9 <20.7 <253.4 <117.3 <225.8
V382 Nor 3442.3 −27.7 −1.0 4.0 0.5 <4.3 <2.2 <31.8 <2.5
V5115 Sgr 3457.8 6.0 −4.6 3.0 1.0 <3.6 <1.3 <15.9 <0.7
V5116 Sgr 3555.0 2.1 −6.8 1.6 0.7 <7.4 <1.1 <41.4 <0.8
V1047 Cen 3583.0 −53.7 0.0 2.9 2.0 <5.7 <3.2 <93.8 <11.1
V476 Sct 3643.5 24.7 1.2 11.3 1.9 <4.3 <17.8 <19.5 <13.5
V5117 Sgr 3783.4 −5.4 −6.4 1.4 0.3 <6.6 <0.5 <18.2 <0.2
V2576 Oph 3831.6 −3.8 5.4 1.8 1.0 <5.9 <1.6 <17.1 <0.4
V1065 Cen 4123.4 −66.0 3.6 3.3 0.5 <12.7 <4.8 <24.2 <1.3
V1280 Sco 4135.9 −8.7 6.6 1.1 0.5 <6.2 <0.5 <24.4 <0.3
V2467 Cyg 4174.8 80.1 1.8 1.5 0.3 <10.8 <1.0 <81.4 <1.0
V2615 Oph 4178.8 4.1 3.3 2.1 0.8 <6.9 <1.6 <23.1 <0.7
V5558 Sgr 4204.8 11.6 0.2 2.1 0.4 <9.0 <1.4 <30.9 <0.7
V458 Vul 4316.5 58.6 −3.6 4.7 2.1 <11.8 <16.2 <57.2 <11.0
V598 Pup 4320.0 −110.9 −13.8 2.1 0.2 <37.6 <5.0 <9177.2 <173.6
V459 Vul 4459.3 58.2 −2.2 13.6 6.5 <13.4 <172.8 <90.1 <135.5
V2468 Cyg 4532.8 66.8 0.2 6.8 1.0 <6.3 <9.7 <38.2 <8.8
NR TrA 4557.7 −34.1 −7.2 4.5 1.6 <7.9 <6.3 <99.6 <13.8
V2491 Cyg 4566.7 67.2 4.4 2.1 1.4 <14.6 <6.6 <35.3 <2.2
V5579 Sgr 4574.8 3.7 −3.0 12.6 6.1 <10.5 <128.5 <175.6 <354.3
V1212 Cen 4704.0 −46.1 −3.5 N/A N/A <15.9 <114.3 <88.9 <96.4
V1721 Aql 4731.5 41.0 −0.1 7.5 2.0 <9.8 <21.0 <14.0 <5.3
QY Mus 4738.0 −54.7 −4.9 5.6 2.4 <24.3 <45.9 <245.7 <75.1
V679 Car 4796.3 −68.5 −0.5 4.5 2.3 <17.2 <16.5 <43.1 <9.4
V5580 Sgr 4799.0 4.7 −6.5 N/A N/A <6.6 <44.5 <53.9 <74.3
V5582 Sgr 4885.9 7.5 4.7 N/A N/A <8.2 <116.1 <19.5 <25.9
V5581 Sgr 4942.7 2.2 1.8 N/A N/A <6.0 <45.7 <188.8 <206.5
V2672 Oph 5059.5 1.0 2.5 3.1 0.7 <8.0 <2.8 <25.4 <1.4
V496 Sct 5112.4 25.3 −1.8 3.2 0.8 <15.8 <6.9 <120.1 <10.5
V5585 Sgr 5216.7 2.3 −4.2 N/A N/A <10.4 <158.4 <52.5 <51.9
V2674 Oph 5245.8 −2.2 3.6 1.6 0.4 <7.3 <0.9 <36.5 <0.7
V1310 Sco 5247.9 −11.5 2.2 N/A N/A <5.6 <28.2 <17.2 <24.3
V5586 Sgr 5309.8 1.5 −1.0 N/A N/A <10.0 <126.6 <114.1 <145.9
V1723 Aql 5450.5 29.1 −0.9 N/A N/A <15.1 <151.2 <78.2 <156.2
V5587 Sgr 5586.9 4.8 2.4 N/A N/A <8.3 <88.2 <53.0 <95.1
V5588 Sgr 5647.8 7.8 −1.9 3.1 0.7 <7.2 <2.9 <50.7 <3.4
V1313 Sco 5810.4 −18.4 3.8 N/A N/A <4.7 <38.3 <18.5 <24.6
V965 Per 5872.0 151.6 −17.9 N/A N/A <15.5 <85.1 <219.8 <325.0
V2676 Oph 6011.8 0.3 5.3 N/A N/A <4.9 <26.6 <45.9 <76.4
V5589 Sgr 6038.0 5.0 3.1 3.3 0.6 <8.9 <3.2 <147.7 <10.0
V1324 Sco 6069.8 −2.6 −2.9 4.3 0.9 <5.3 <4.8 <76.1 <11.5
V5591 Sgr 6104.5 7.2 2.5 3.6 2.3 <6.8 <8.9 <43.9 <8.3
V5592 Sgr 6115.5 4.8 −6.1 N/A N/A <7.7 <99.8 <57.2 <170.7
V5593 Sgr 6124.5 12.4 −1.9 N/A N/A <8.6 <104.7 <36.3 <70.5
V959 Mon 6148.8 −153.7 0.1 1.4 0.4 <17.9 <2.3 <168.5 <2.2
V1724 Aql 6220.4 32.8 −0.4 N/A N/A <8.4 <39.4 <70.9 <152.1
V809 Cep 6325.4 110.6 0.4 N/A N/A <6.5 <38.9 <180.5 <247.5
V1533 Sco 6446.6 −7.4 −1.7 N/A N/A <7.3 <76.4 <81.7 <142.3
V339 Del 6518.6 62.2 −9.4 3.6 2.2 <7.2 <5.6 <169.6 <24.6
V1830 Aql 6593.5 37.1 −1.0 N/A N/A <13.4 <108.3 <1115.5 <978.7
V556 Ser 6620.4 18.1 4.1 N/A N/A <9.5 <59.5 <367.2 <611.7
V5666 Sgr 6683.9 9.9 −4.7 N/A N/A <7.3 <73.7 <168.6 <372.6
V2659 Cyg 6747.8 70.5 −3.3 N/A N/A <2.9 <25.8 <35.1 <48.3
V1535 Sco 7064.8 −10.1 3.9 5.3 1.7 <13.4 <22.7 <23.2 <6.4
V1658 Sco 7068.0 −2.8 −2.4 N/A N/A <7.8 <67.2 <20.7 <31.4
V1404 Cen 7081.3 −48.6 −1.6 N/A N/A <6.5 <54.3 <154.9 <183.9
V5668 Sgr 7096.6 5.4 −9.9 1.4 0.7 <8.2 <0.8 <14.0 <0.3
V2944 Oph 7110.8 6.6 8.6 N/A N/A <9.5 <62.2 <31.4 <54.1
V5669 Sgr 7292.4 2.6 −3.1 N/A N/A <11.6 <123.3 <15.9 <21.7
V1831 Aql 7300.5 49.8 0.3 N/A N/A <9.9 <77.9 <50.4 <55.7
V2949 Oph 7306.4 2.8 4.6 N/A N/A <6.8 <50.2 <22.9 <36.2
V5850 Sgr 7326.4 12.6 −2.6 N/A N/A <8.6 <57.4 <127.1 <195.4
V555 Nor 7455.3 −33.1 1.6 N/A N/A <11.9 <159.9 <57.3 <44.1
V1655 Sco 7549.6 −8.0 −3.2 N/A N/A <5.5 <41.6 <69.9 <138.5
V5854 Sgr 7581.2 0.2 −1.0 N/A N/A <10.3 <121.0 <53.6 <173.0
V5853 Sgr 7608.5 3.8 −1.7 N/A N/A <4.4 <27.4 <31.2 <61.2
V1656 Sco 7637.5 −5.2 2.5 N/A N/A <8.9 <82.9 <21.6 <36.4
V1659 Sco 7638.0 −4.1 −1.9 N/A N/A <10.7 <145.0 <20.3 <33.6
V611 Sct 7638.3 21.3 1.2 N/A N/A <15.8 <136.6 <34.1 <40.9
V407 Lup 7655.0 −29.9 9.6 N/A N/A <18.4 <212.1 <90.5 <111.1
V5855 Sgr 7681.4 4.0 −4.0 13.4 6.4 <7.5 <71.4 <43.0 <77.0
V5856 Sgr 7686.0 4.3 −6.5 7.7 3.7 <7.9 <4.8 <91.6 <86.1
V1657 Sco 7785.9 −13.7 3.9 N/A N/A <15.2 <169.8 <36.0 <71.2
V1405 Cen 7868.1 −53.8 −1.0 N/A N/A <11.2 <89.8 <31.7 <42.6
V3662 Oph 7881.8 2.7 3.2 N/A N/A <6.5 <54.6 <124.0 <199.4
V612 Sct 7923.4 18.0 −2.2 4.0 1.0 <12.9 <7.9 <187.6 <22.0
V549 Vel 8020.4 −92.8 −2.3 N/A N/A <36.8 <414.3 <114.5 <202.7
V1660 Sco 8040.0 −3.6 1.6 N/A N/A <8.6 <46.8 <26.2 <33.9
V3663 Oph 8068.4 0.1 7.2 N/A N/A <10.9 <65.5 <135.0 <234.8
V357 Mus 8132.5 −65.7 −4.1 N/A N/A <23.4 <205.1 <56.2 <92.5
V1661 Sco 8135.9 −5.9 3.2 N/A N/A <14.2 <114.7 <44.7 <67.4
FM Cir 8137.7 −51.2 −5.3 N/A N/A <89.6 <497.7 <590.5 <713.8
V1662 Sco 8155.9 −19.6 −0.1 N/A N/A <25.1 <248.5 <27.1 <34.2
V3664 Oph 8161.8 1.3 6.4 N/A N/A <10.8 <66.6 <26.6 <46.0
V1663 Sco 8173.4 −12.6 1.9 N/A N/A <11.9 <68.3 <28.8 <55.9
V3665 Oph 8187.8 −3.7 5.8 N/A N/A <12.0 <91.4 <28.2 <46.5
V906 Car 8197.3 −73.4 −1.1 N/A N/A <26.4 <230.6 <22.8 <18.9
V5857 Sgr 8216.7 11.5 1.8 N/A N/A <39.6 <336.2 <44.0 <43.5
Diffuse – – – – – <39.4 <2.7 <59.8 <4.1
Complete pooling – – – – – – <0.7 (<1.0) – <0.5
Partial pooling – – – – – – <2.0 – <2.5

Notes. From left to right, the columns are the name of the object (or analysis type at the bottom), T0 is the discovery date of the objects in units of MJD-50000, l and b are the Galactic longitude and latitude in degrees, and d and σd are the distance and uncertainty estimates in units of kpc (see Sect. 4). If no distance estimate is available, the generic distance prior (Sect. 4.2) has been used and marked as N/A in the table. is the upper bound (99.85th percentile) of the 1275 keV line flux, the corresponding upper bound on the 22Na ejecta mass, is the upper bound on the 478 keV line flux, and is the corresponding bound on the ejected 7Be mass. Fluxes are given in units of 10−5 ph cm−2 s−1, and ejecta masses in units of 10−7 M⊙.

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