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Table 4

Rotation and glide of the position system of planetary ephemerides with respect to that of DE440 in the equatorial coordinate system.

Ephemeris RX (µas) RY (µas) RZ (µas) GX (µas) GY (µas) GZ (µas)
DE200 −2291(22) −12432(19) −12428(13) 8(14) −1(17) −17(25)
DE403 −1838(13) 597(13) −2309(8) 10(9) −17(12) −6(16)
DE405 −1623(13) 248(12) 891(9) 6(9) −8(11) −5(16)
DE410 −66(9) −665(8) −219(5) 2(5) −1(7) −1(11)
DE421 −33(7) −227(7) −184(4) −2(3) −3(5) −0(8)
DE430 −106(7) −14(7) 101(3) 1(3) −1(6) 2(9)
EPM2011 −113(8) 132(8) 327(4) −1(4) −6(7) 2(9)
EPM2015 −204(8) 97(7) 258(5) −2(5) −2(7) −1(10)
EPM2017 −192(8) 140(8) 223(4) −1(4) −4(7) 0(10)
EPM2021 −58(6) 8(6) 120(3) 1(3) −1(5) 2(7)
INPOP06c 3(11) −275(10) −308(7) 1(8) −3(10) −5(13)
INPOP08a 244(9) 32(9) −572(5) 2(4) −6(7) 0(10)
INPOP10a 116(10) −66(8) −116(5) −3(6) 6(9) −9(12)
INPOP10b 38(12) 388(10) 29(7) 2(7) −5(10) 1(16)
INPOP10e −229(8) −74(7) −202(5) 0(5) −5(6) −1(10)
INPOP13c −107(7) −86(6) −218(4) −3(4) 1(6) 0(8)
INPOP17a −176(9) 208(10) −81(4) 1(4) −4(7) 1(10)
INPOP19a −83(6) 246(6) 4(3) −2(3) −2(5) −1(7)
INPOP21a −237(4) 405(5) 3(3) −3(3) −2(5) 2(6)

Notes. The uncertainties for the estimates given in parentheses were obtained from the least-squares fit and could be underestimated several times, as suggested by the bootstrap fit.

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