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Merge pull request #644 from MESAHub/EbF/add_lanl_OPLIB_type1_opacity…
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Add lanl oplib type1 opacity tables, new abundances, new lowT tables
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@Debraheem
Debraheem authored May 21, 2024
2 parents e90790f + 0e18e00 commit 8ede8e7
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233 changes: 231 additions & 2 deletions chem/public/chem_def.f90
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Original file line number Diff line number Diff line change
Expand Up @@ -55,6 +55,8 @@ module chem_def
!AGSS09 m,s s, with some m
!L09 m,s,r r
!A09_Prz modified AGSS09 - he, c, n, o, ne, mg, al, si, s, ar, fe.
!MB22 m,s s, with some m, supplimented with agss09
!AAG21 m,s s, with some m

! storage for Lodders (2003) isotopic percentages
type isotopic_abundance_table_type
Expand Down Expand Up @@ -280,6 +282,8 @@ module chem_def
real(dp), parameter :: AGSS09_zsol = 0.0134d0
real(dp), parameter :: L09_zsol = 0.0154d0
real(dp), parameter :: A09_Prz_zsol = 0.014d0
real(dp), parameter :: MB22_photospheric_zsol = 0.0169d0
real(dp), parameter :: AAG21_photospheric_zsol = 0.0139d0

real(dp), parameter :: AG89_ysol = 0.2485d0
real(dp), parameter :: GN93_ysol = 0.2485d0
Expand All @@ -289,6 +293,8 @@ module chem_def
real(dp), parameter :: AGSS09_ysol = 0.2485d0
real(dp), parameter :: L09_ysol = 0.2751d0
real(dp), parameter :: A09_Prz_ysol = 0.276d0
real(dp), parameter :: MB22_photospheric_ysol = 0.2485
real(dp), parameter :: AAG21_photospheric_ysol = 0.2485

character(len=iso_name_length) :: chem_element_main_iso_name(num_chem_elements)
integer, parameter :: chem_element_name_len = iso_name_length
Expand All @@ -306,6 +312,8 @@ module chem_def
integer, parameter :: AGSS09_zfracs = 6
integer, parameter :: L09_zfracs = 7
integer, parameter :: A09_Prz_zfracs = 8
integer, parameter :: MB22_photospheric_zfracs = 9
integer, parameter :: AAG21_photospheric_zfracs = 10


real(dp) :: AG89_element_zfrac(num_chem_elements) ! fraction by mass of total Z
Expand Down Expand Up @@ -351,7 +359,12 @@ module chem_def
! eps_S = 7.14
! eps_Ar = 6.50
! eps_Fe = 7.52


real(dp) :: MB22_photospheric_element_zfrac(num_chem_elements) ! fraction by mass of total Z
! Ekaterina Magg et al. , A&A 661, A140 (2022) photospheric abundance.

real(dp) :: AAG21_photospheric_element_zfrac(num_chem_elements) ! fraction by mass of total Z
! Asplund et al. A&A 653, A141 (2021) photospheric abundance.

type (integer_dict), pointer :: chem_element_names_dict

Expand Down Expand Up @@ -550,6 +563,10 @@ subroutine init_chem_tables
call init_AGSS09_data

call init_A09_Przybilla_data

call init_MB22_photospheric_data

call init_AAG21_photospheric_data

call init_L09_data

Expand Down Expand Up @@ -1718,7 +1735,219 @@ subroutine init_A09_Przybilla_data ! fraction by mass of total Z
end do

end subroutine init_A09_Przybilla_data


subroutine init_MB22_photospheric_data ! fraction by mass of total Z
! Ekaterina Magg et al. , A&A 661, A140 (2022) photospheric abundance.
! supplimented with Asplund, Grevesse, Sauval, and Scott 2009 abundances
integer :: i
real(dp) :: z_sum
include 'formats'

MB22_photospheric_element_zfrac(:) = -20.0d0

! first store log abundances from the paper
MB22_photospheric_element_zfrac(e_li) = 3.26d0 ! AGSS09
MB22_photospheric_element_zfrac(e_be) = 1.38d0 ! AGSS09
MB22_photospheric_element_zfrac(e_b ) = 2.70d0 ! AGSS09
MB22_photospheric_element_zfrac(e_c ) = 8.56d0
MB22_photospheric_element_zfrac(e_n ) = 7.98d0
MB22_photospheric_element_zfrac(e_o ) = 8.77d0
MB22_photospheric_element_zfrac(e_f ) = 4.40d0
MB22_photospheric_element_zfrac(e_ne) = 8.15d0
MB22_photospheric_element_zfrac(e_na) = 6.29d0
MB22_photospheric_element_zfrac(e_mg) = 7.55d0
MB22_photospheric_element_zfrac(e_al) = 6.43d0
MB22_photospheric_element_zfrac(e_si) = 7.59d0
MB22_photospheric_element_zfrac(e_p ) = 5.41d0
MB22_photospheric_element_zfrac(e_s ) = 7.16d0
MB22_photospheric_element_zfrac(e_cl) = 5.25d0
MB22_photospheric_element_zfrac(e_ar) = 6.50d0
MB22_photospheric_element_zfrac(e_k ) = 5.14d0
MB22_photospheric_element_zfrac(e_ca) = 6.37d0
MB22_photospheric_element_zfrac(e_sc) = 3.07d0
MB22_photospheric_element_zfrac(e_ti) = 4.94d0
MB22_photospheric_element_zfrac(e_v ) = 3.89d0
MB22_photospheric_element_zfrac(e_cr) = 5.74d0
MB22_photospheric_element_zfrac(e_mn) = 5.52d0
MB22_photospheric_element_zfrac(e_fe) = 7.50d0
MB22_photospheric_element_zfrac(e_co) = 4.95d0
MB22_photospheric_element_zfrac(e_ni) = 6.24d0
MB22_photospheric_element_zfrac(e_cu) = 4.19d0 ! AGSS09
MB22_photospheric_element_zfrac(e_zn) = 4.56d0 ! AGSS09
MB22_photospheric_element_zfrac(e_ga) = 3.04d0 ! AGSS09
MB22_photospheric_element_zfrac(e_ge) = 3.65d0 ! AGSS09
MB22_photospheric_element_zfrac(e_as) = 2.30d0 !meteor AGSS09
MB22_photospheric_element_zfrac(e_se) = 3.34d0 !meteor AGSS09
MB22_photospheric_element_zfrac(e_br) = 2.54d0 !meteor AGSS09
MB22_photospheric_element_zfrac(e_kr) = 3.25d0 !indirect AGSS09
MB22_photospheric_element_zfrac(e_rb) = 2.52d0 ! AGSS09
MB22_photospheric_element_zfrac(e_sr) = 2.87d0 ! AGSS09
MB22_photospheric_element_zfrac(e_y ) = 2.21d0 ! AGSS09
MB22_photospheric_element_zfrac(e_zr) = 2.58d0 ! AGSS09
MB22_photospheric_element_zfrac(e_nb) = 1.46d0 ! AGSS09
MB22_photospheric_element_zfrac(e_mo) = 1.88d0 ! AGSS09
MB22_photospheric_element_zfrac(e_Ru) = 1.75d0 ! AGSS09
MB22_photospheric_element_zfrac(e_Rh) = 0.91d0 ! AGSS09
MB22_photospheric_element_zfrac(e_Pd) = 1.57d0 ! AGSS09
MB22_photospheric_element_zfrac(e_Ag) = 0.94d0 ! AGSS09
MB22_photospheric_element_zfrac(e_Cd) = 1.71d0 ! AGSS09
MB22_photospheric_element_zfrac(e_In) = 0.80d0 ! AGSS09
MB22_photospheric_element_zfrac(e_Sn) = 2.04d0 ! AGSS09
MB22_photospheric_element_zfrac(e_Sb) = 1.01d0 ! AGSS09
MB22_photospheric_element_zfrac(e_Te) = 2.18d0 ! AGSS09
MB22_photospheric_element_zfrac(e_I ) = 1.55d0 ! AGSS09
MB22_photospheric_element_zfrac(e_Xe) = 2.24d0 ! AGSS09
MB22_photospheric_element_zfrac(e_Cs) = 1.08d0 ! AGSS09
MB22_photospheric_element_zfrac(e_Ba) = 2.18d0 ! AGSS09
MB22_photospheric_element_zfrac(e_La) = 1.10d0 ! AGSS09
MB22_photospheric_element_zfrac(e_Ce) = 1.58d0 ! AGSS09
MB22_photospheric_element_zfrac(e_Pr) = 0.72d0 ! AGSS09
MB22_photospheric_element_zfrac(e_Nd) = 1.42d0 ! AGSS09
MB22_photospheric_element_zfrac(e_Sm) = 0.96d0 ! AGSS09
MB22_photospheric_element_zfrac(e_Eu) = 0.52d0 ! AGSS09
MB22_photospheric_element_zfrac(e_Gd) = 1.07d0 ! AGSS09
MB22_photospheric_element_zfrac(e_Tb) = 0.30d0 ! AGSS09
MB22_photospheric_element_zfrac(e_Dy) = 1.10d0 ! AGSS09
MB22_photospheric_element_zfrac(e_Ho) = 0.48d0 ! AGSS09
MB22_photospheric_element_zfrac(e_Er) = 0.92d0 ! AGSS09
MB22_photospheric_element_zfrac(e_Tm) = 0.10d0 ! AGSS09
MB22_photospheric_element_zfrac(e_Yb) = 0.84d0 ! AGSS09
MB22_photospheric_element_zfrac(e_Lu) = 0.10d0 ! AGSS09
MB22_photospheric_element_zfrac(e_Hf) = 0.85d0 ! AGSS09
MB22_photospheric_element_zfrac(e_Ta) = -0.12d0 ! AGSS09
MB22_photospheric_element_zfrac(e_W ) = 0.85d0 ! AGSS09
MB22_photospheric_element_zfrac(e_Re) = 0.26d0 ! AGSS09
MB22_photospheric_element_zfrac(e_Os) = 1.40d0 ! AGSS09
MB22_photospheric_element_zfrac(e_Ir) = 1.38d0 ! AGSS09
MB22_photospheric_element_zfrac(e_Pt) = 1.62d0 ! AGSS09
MB22_photospheric_element_zfrac(e_Au) = 0.92d0 ! AGSS09
MB22_photospheric_element_zfrac(e_Hg) = 1.17d0 ! AGSS09
MB22_photospheric_element_zfrac(e_Tl) = 0.90d0 ! AGSS09
MB22_photospheric_element_zfrac(e_Pb) = 1.75d0 ! AGSS09
MB22_photospheric_element_zfrac(e_Bi) = 0.65d0 ! AGSS09
MB22_photospheric_element_zfrac(e_Th) = 0.02d0 ! AGSS09
MB22_photospheric_element_zfrac(e_U) = -0.54d0 ! AGSS09

! convert to fraction of Z by mass
z_sum = 0
do i = e_li, e_u
MB22_photospheric_element_zfrac(i) = &
exp10(MB22_photospheric_element_zfrac(i))*element_atomic_weight(i)
z_sum = z_sum + MB22_photospheric_element_zfrac(i)
end do
do i = e_li, e_u
MB22_photospheric_element_zfrac(i) = MB22_photospheric_element_zfrac(i) / z_sum
end do

end subroutine init_MB22_photospheric_data




subroutine init_AAG21_photospheric_data ! fraction by mass of total Z
! Asplund et al. A&A 653, A141 (2021) photospheric abundance.
! Supplimented with meteoric values
integer :: i
real(dp) :: z_sum
include 'formats'

AAG21_photospheric_element_zfrac(:) = -20.0d0

! first store log abundances from the paper
AAG21_photospheric_element_zfrac(e_li) = 0.96 !± 0.013
AAG21_photospheric_element_zfrac(e_be) = 1.38 !± 0.09
AAG21_photospheric_element_zfrac(e_b ) = 2.70 !± 0.20
AAG21_photospheric_element_zfrac(e_c ) = 8.46 !± 0.04
AAG21_photospheric_element_zfrac(e_n ) = 7.83 !± 0.07
AAG21_photospheric_element_zfrac(e_o ) = 8.69 !± 0.04
AAG21_photospheric_element_zfrac(e_f ) = 4.40 !± 0.25
AAG21_photospheric_element_zfrac(e_ne) = 8.06 !± 0.05
AAG21_photospheric_element_zfrac(e_na) = 6.22 !± 0.03
AAG21_photospheric_element_zfrac(e_mg) = 7.55 !± 0.03
AAG21_photospheric_element_zfrac(e_al) = 6.43 !± 0.03
AAG21_photospheric_element_zfrac(e_si) = 7.51 !± 0.03
AAG21_photospheric_element_zfrac(e_p ) = 5.41 !± 0.03
AAG21_photospheric_element_zfrac(e_s ) = 7.12 !± 0.03
AAG21_photospheric_element_zfrac(e_cl) = 5.31 !± 0.20
AAG21_photospheric_element_zfrac(e_ar) = 6.38 !± 0.10
AAG21_photospheric_element_zfrac(e_k ) = 5.07 !± 0.03
AAG21_photospheric_element_zfrac(e_ca) = 6.30 !± 0.03
AAG21_photospheric_element_zfrac(e_sc) = 3.14 !± 0.04
AAG21_photospheric_element_zfrac(e_ti) = 4.97 !± 0.05
AAG21_photospheric_element_zfrac(e_v ) = 3.90 !± 0.08
AAG21_photospheric_element_zfrac(e_cr) = 5.62 !± 0.04
AAG21_photospheric_element_zfrac(e_mn) = 5.42 !± 0.06
AAG21_photospheric_element_zfrac(e_fe) = 7.46 !± 0.04
AAG21_photospheric_element_zfrac(e_co) = 4.94 !± 0.05
AAG21_photospheric_element_zfrac(e_ni) = 6.20 !± 0.04
AAG21_photospheric_element_zfrac(e_cu) = 4.18 !± 0.05
AAG21_photospheric_element_zfrac(e_zn) = 4.56 !± 0.05
AAG21_photospheric_element_zfrac(e_ga) = 3.02 !± 0.05
AAG21_photospheric_element_zfrac(e_ge) = 3.62 !± 0.10
AAG21_photospheric_element_zfrac(e_as) = 2.30 !± 0.04 meteorites
AAG21_photospheric_element_zfrac(e_se) = 3.34 !± 0.03 meteorites
AAG21_photospheric_element_zfrac(e_br) = 2.54 !± 0.06 meteorites
AAG21_photospheric_element_zfrac(e_kr) = 3.12 !± 0.10
AAG21_photospheric_element_zfrac(e_rb) = 2.32 !± 0.08
AAG21_photospheric_element_zfrac(e_sr) = 2.83 !± 0.06
AAG21_photospheric_element_zfrac(e_y ) = 2.21 !± 0.05
AAG21_photospheric_element_zfrac(e_zr) = 2.59 !± 0.04
AAG21_photospheric_element_zfrac(e_nb) = 1.47 !± 0.06
AAG21_photospheric_element_zfrac(e_mo) = 1.88 !± 0.09
AAG21_photospheric_element_zfrac(e_Ru) = 1.75 !± 0.08
AAG21_photospheric_element_zfrac(e_Rh) = 0.78 !± 0.11
AAG21_photospheric_element_zfrac(e_Pd) = 1.57 !± 0.10
AAG21_photospheric_element_zfrac(e_Ag) = 0.96 !± 0.10
AAG21_photospheric_element_zfrac(e_Cd) = 1.71 !± 0.03 meteorites
AAG21_photospheric_element_zfrac(e_In) = 0.80 !± 0.20
AAG21_photospheric_element_zfrac(e_Sn) = 2.02 !± 0.10
AAG21_photospheric_element_zfrac(e_Sb) = 1.01 !± 0.06 meteorites
AAG21_photospheric_element_zfrac(e_Te) = 2.18 !± 0.03 meteorites
AAG21_photospheric_element_zfrac(e_I ) = 1.55 !± 0.08 meteorites
AAG21_photospheric_element_zfrac(e_Xe) = 2.22 !± 0.05
AAG21_photospheric_element_zfrac(e_Cs) = 1.08 !± 0.03 meteorites
AAG21_photospheric_element_zfrac(e_Ba) = 2.27 !± 0.05
AAG21_photospheric_element_zfrac(e_La) = 1.11 !± 0.04
AAG21_photospheric_element_zfrac(e_Ce) = 1.58 !± 0.04
AAG21_photospheric_element_zfrac(e_Pr) = 0.75 !± 0.05
AAG21_photospheric_element_zfrac(e_Nd) = 1.42 !± 0.04
AAG21_photospheric_element_zfrac(e_Sm) = 0.95 !± 0.04
AAG21_photospheric_element_zfrac(e_Eu) = 0.52 !± 0.04
AAG21_photospheric_element_zfrac(e_Gd) = 1.08 !± 0.04
AAG21_photospheric_element_zfrac(e_Tb) = 0.31 !± 0.10
AAG21_photospheric_element_zfrac(e_Dy) = 1.10 !± 0.04
AAG21_photospheric_element_zfrac(e_Ho) = 0.48 !± 0.11
AAG21_photospheric_element_zfrac(e_Er) = 0.93 !± 0.05
AAG21_photospheric_element_zfrac(e_Tm) = 0.11 !± 0.04
AAG21_photospheric_element_zfrac(e_Yb) = 0.85 !± 0.11
AAG21_photospheric_element_zfrac(e_Lu) = 0.10 !± 0.09
AAG21_photospheric_element_zfrac(e_Hf) = 0.85 !± 0.05
AAG21_photospheric_element_zfrac(e_Ta) = -0.15 !± 0.04 meteorites
AAG21_photospheric_element_zfrac(e_W ) = 0.79 !± 0.11
AAG21_photospheric_element_zfrac(e_Re) = 0.26 !± 0.02 meteorites
AAG21_photospheric_element_zfrac(e_Os) = 1.35 !± 0.12
AAG21_photospheric_element_zfrac(e_Ir) = 1.32 !± 0.02 meteorites
AAG21_photospheric_element_zfrac(e_Pt) = 1.61 !± 0.02 meteorites
AAG21_photospheric_element_zfrac(e_Au) = 0.91 !± 0.12
AAG21_photospheric_element_zfrac(e_Hg) = 1.17 !± 0.18 meteorites
AAG21_photospheric_element_zfrac(e_Tl) = 0.92 !± 0.17
AAG21_photospheric_element_zfrac(e_Pb) = 1.95 !± 0.08
AAG21_photospheric_element_zfrac(e_Bi) = 0.65 !± 0.04 meteorites
AAG21_photospheric_element_zfrac(e_Th) = 0.03 !± 0.10
AAG21_photospheric_element_zfrac(e_U) = -0.54 !± 0.03 meteorites

! convert to fraction of Z by mass
z_sum = 0
do i = e_li, e_u
AAG21_photospheric_element_zfrac(i) = &
exp10(AAG21_photospheric_element_zfrac(i))*element_atomic_weight(i)
z_sum = z_sum + AAG21_photospheric_element_zfrac(i)
end do
do i = e_li, e_u
AAG21_photospheric_element_zfrac(i) = AAG21_photospheric_element_zfrac(i) / z_sum
end do

end subroutine init_AAG21_photospheric_data

subroutine init_L09_data ! fraction by mass of total Z
! Lodders 09
Expand Down
8 changes: 7 additions & 1 deletion chem/public/chem_lib.f90
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Expand Up @@ -705,7 +705,13 @@ real(dp) function chem_M_div_h(x,z,zfrac_choice) ! Returns [M/H]
ysolar = L09_ysol
case(A09_Prz_zfracs)
zsolar = A09_Prz_zsol
ysolar = A09_Prz_ysol
ysolar = A09_Prz_ysol
case(MB22_photospheric_zfracs)
zsolar = MB22_photospheric_zsol
ysolar = MB22_photospheric_ysol
case(AAG21_photospheric_zfracs)
zsolar = AAG21_photospheric_zsol
ysolar = AAG21_photospheric_ysol
case(Custom_zfracs)
call mesa_error(__FILE__,__LINE__,"[M/H] not supported with custom zfracs.")
case default
Expand Down
24 changes: 21 additions & 3 deletions docs/source/kap/overview.rst
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Expand Up @@ -57,10 +57,27 @@ High temperature :math:`(T \gtrsim 10^4\,\rm K)`

The OPAL tables (|OPAL|) with fixed metal distributions are called
Type 1 and cover the region :math:`0.0 \leq X \leq 1-Z` and
:math:`0.0\leq Z \leq 0.1`. Type 1 tables from the Opacity Project
(OP; |OP|) are also available. The set of tables to be used are
:math:`0.0\leq Z \leq 0.1`. The Opacity Project
(OP; |OP|) are also available. Type 1 tables from The Los Alamos
OPLIB database (OPLIB; |OPLIB|) are also available, and cover the
region :math:`0.0 \leq X \leq 1-Z` and
:math:`0.0\leq Z \leq 0.2`. The set of tables to be used are
selected by the option :ref:`kap/defaults:kap_file_prefix`.

A direct comparison between the Type 1 format of OPAL/OP tables and
the OPLIB tables are shown in the figure below
taken from Figure 1 in Farag et al. 2024. Further comparisons
between OP/OPAL/OPLIB can be found in Farag et al. 2024.


.. figure:: type1_format.png
:alt: kap blends in solar-like compositions

Location of each Type-1 opacity table in the :math:`X–Z` plane (left panel) and the
log:math:`T`–log:math:`R` plane (right panel). Orange circles mark the location of
the 126 OPAL Type-1 tables (Rogers & Iglesias 1992). Blue circles
mark the location of the new 1194 Type-1 opacity tables (Farag et al. 2024).

Additionally, there is support for the OPAL Type 2 tables that allow
for varying amounts of C and O beyond that accounted for by :math:`Z`;
these are needed during helium burning and beyond. These have a range
Expand Down Expand Up @@ -164,8 +181,9 @@ degeneracy, the additional correction formulae of |B20| are applied.

.. |OPAL| replace:: Iglesias & Rogers `1993 <https://ui.adsabs.harvard.edu/abs/1993ApJ...412..752I/abstract>`__, `1996 <https://ui.adsabs.harvard.edu/abs/1996ApJ...464..943I/abstract>`__

.. |OP| replace:: `Seaton 2005 <https://ui.adsabs.harvard.edu/abs/2005MNRAS.362L...1S/abstract>`__

.. |OP| replace:: `Seaton 2005 <https://ui.adsabs.harvard.edu/abs/2005MNRAS.362L...1S/abstract>`__
.. |OPLIB| replace:: `Colgan 2016 <https://ui.adsabs.harvard.edu/abs/2016ApJ...817..116C/abstract>`__

.. |Cassisi| replace:: `Cassisi et al. (2007) <https://ui.adsabs.harvard.edu/abs/2007ApJ...661.1094C/abstract>`__

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23 changes: 22 additions & 1 deletion kap/defaults/kap.defaults
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Expand Up @@ -33,11 +33,26 @@
! These tables use the value of ``Zbase`` for Z, unless ``use_Zbase_for_Type1 = .false.``.

! The Type1 tables cover a wider range of X and have a higher resolution in
! Z for each X than Type2. The Type1 tables are for (X,Z) pairs from the following sets:
! Z for each X than Type2. The OPAL/OP Type1 tables are for 126 (X,Z) pairs from the following sets:
!
! + X: 0.0, 0.1, 0.2, 0.35, 0.5, 0.7, 0.8, 0.9, 0.95, 1-Z
! + Z: 0.0, 1e-4, 3e-4, 1e-3, 2e-3, 4e-3, 1e-2, 2e-2, 3e-2, 4e-2, 6e-2, 8e-1, 1e-1

!The OPLIB Type1 tables offer additional table density, for 1194 (X,Z) pairs from the following sets:
!
! + X: 0.0, 0.000001, 0.00001, 0.0001, 0.001, 0.01, 0.05, 0.1,
! + 0.15, 0.2, 0.25, 0.3, 0.35, 0.4, 0.45, 0.5,
! + 0.55, 0.6, 0.65, 0.7, 0.75, 0.8, 0.85, 0.9,
! + 0.91, 0.92, 0.93, 0.94, 0.95, 0.96, 0.97,
! + 0.98, 0.99, 1-Z
! +
! + Z: 0.0, 0.000001, 0.00001, 0.00003, 0.00007, 0.0001,
! + 0.0003, 0.0007, 0.001, 0.002, 0.003, 0.004,0.006,
! + 0.008, 0.01, 0.012, 0.014, 0.015, 0.016, 0.017, 0.018,
! + 0.019, 0.02, 0.021, 0.022, 0.023, 0.024, 0.025, 0.026,
! + 0.028, 0.03, 0.035, 0.04, 0.05, 0.06, 0.07, 0.08,
! + 0.09, 0.1, 0.15, 0.2


! Available options:

Expand All @@ -46,6 +61,10 @@
! + ``'a09'``
! + ``'OP_gs98'``
! + ``'OP_a09_nans_removed_by_hand'``
! + ``'oplib_gs98``'
! + ``'oplib_agss09``'
! + ``'oplib_aag21``'
! + ``'oplib_mb22``'
!
! ::

Expand Down Expand Up @@ -88,6 +107,8 @@

! Available options:

! + ``'lowT_fa05_mb22'``
! + ``'lowT_fa05_aag21'``
! + ``'lowT_Freedman11'``
! + ``'lowT_fa05_gs98'``
! + ``'lowT_fa05_gn93'``
Expand Down
4 changes: 2 additions & 2 deletions kap/kap_data.tar.xz
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