Inspect.Documentation History
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# Metallicity [Fe/H] (Not required for Fe)
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# Metallicity [Fe/H] (Not required for all elements)
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The output includes equivalent width, LTE and NLTE abundance, NLTE abundance correction, [Fe/H], and [X/Fe].\\
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The output includes equivalent width, LTE and NLTE abundance, NLTE abundance correction, [Fe/H] and/or [X/Fe]. \\
Changed line 13 from:
# Metallicity [Fe/H] (Not for Fe)
to:
# Metallicity [Fe/H] (Not required for Fe)
Added line 13:
# Metallicity [Fe/H] (Not for Fe)
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The output includes equivalent width, LTE and NLTE abundance, and NLTE abundance correction.\\
to:
The output includes equivalent width, LTE and NLTE abundance, NLTE abundance correction, [Fe/H], and [X/Fe].\\
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To access the database, choose an element from the periodic table on the front page. We are working on extending the data grids to cover more elements.
to:
To access the database, choose an element from the periodic table on the front page. We are continuously working on extending the data grids to cover more elements.
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There are two ways of querying data for a given line, either from a pre-computed equivalent width or from a LTE abundance. Choose the method that suits your purpose best. Abundances are specified relative to hydrogen on the common logarithmic scale: \\
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There are two ways of querying data for a given line, either from a pre-computed equivalent width or from a LTE abundance. Choose the method that suits your purpose best by clicking on the corresponding link at the top. Abundances are specified relative to hydrogen on the common logarithmic scale: \\
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Changed lines 1-8 from:
To access the database, click the link 'Periodic Table' in the side bar of the Main Page and select element. Currently available:
* Li
* Na
* Fe
Data to be provided as input:
* Li
* Na
* Fe
Data to be provided as input
to:
To access the database, choose an element from the periodic table on the front page. We are working on extending the data grids to cover more elements.
There are two ways of querying data for a given line, either from a pre-computed equivalent width or from a LTE abundance. Choose the method that suits your purpose best. Abundances are specified relative to hydrogen on the common logarithmic scale: \\
\\
Abundance (X) = log(N(X)/N(H)) + 12
\\
Data to be provided as input:\\
\\
There are two ways of querying data for a given line, either from a pre-computed equivalent width or from a LTE abundance. Choose the method that suits your purpose best. Abundances are specified relative to hydrogen on the common logarithmic scale: \\
\\
Abundance (X) = log(N(X)/N(H)) + 12
\\
Data to be provided as input:\\
\\
Changed lines 14-18 from:
# Wavelength must be chosen from the list. For the available spectral lines, check the {+Line data+} link at the top of each page.
The output includes equivalent width, LTE and NLTE abundance, and NLTE abundance correction
For each element, ADS-links to one or two references are listed, in which the NLTE calculations are described.If you use the data from INSPECT in your work, please cite the relevant articles and include a comment of the following kind:
The output includes equivalent width, LTE and NLTE abundance, and NLTE abundance correction
For each element, ADS-links to one or two references are listed, in which the NLTE calculations are described.
to:
# Wavelength must be chosen from the list. For the available spectral lines, check the {+Line data+} link at the top of each page.\\
The output includes equivalent width, LTE and NLTE abundance, and NLTE abundance correction.\\
For each element, ADS-links to one or two references are listed, in which the NLTE calculations are described. Here you will find more information about the model atmospheres, atomic data, treatment of fine and hyperfine structure etc.\\
If you use the data from INSPECT in your work, please cite the relevant articles and include a comment of the following kind:\\
The output includes equivalent width, LTE and NLTE abundance, and NLTE abundance correction.\\
For each element, ADS-links to one or two references are listed, in which the NLTE calculations are described. Here you will find more information about the model atmospheres, atomic data, treatment of fine and hyperfine structure etc.\\
If you use the data from INSPECT in your work, please cite the relevant articles and include a comment of the following kind:\\
Changed lines 11-12 from:
# Logarithm of surface gravity [cm s-2]
# Microturbulence [km s-1]
# Microturbulence [km s-1]
to:
# Logarithm of surface gravity [cm s'^-2^']
# Microturbulence [km s'^-1^']
# Microturbulence [km s'^-1^']
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# Equivalent width [Å] or LTE abundance
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# Equivalent width [mÅ] or LTE abundance
Changed line 9 from:
# Equivalent width [pm = 0.1 A] or LTE abundance
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# Equivalent width [Å] or LTE abundance
Changed line 17 from:
For each element, ADS-links to one or two references are listed where the calculations are described. If you use the data from INSPECT in your work, please cite the relevant articles and include a comment of the following kind:
to:
For each element, ADS-links to one or two references are listed, in which the NLTE calculations are described. If you use the data from INSPECT in your work, please cite the relevant articles and include a comment of the following kind:
Added lines 17-22:
For each element, ADS-links to one or two references are listed where the calculations are described. If you use the data from INSPECT in your work, please cite the relevant articles and include a comment of the following kind:
"Data obtained from the INSPECT database, version 1.0 (www.inspect-stars.net)"
"Data obtained from the INSPECT database, version 1.0 (www.inspect-stars.net)"
Changed lines 1-2 from:
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To access the database, click the link 'Periodic Table' in the side bar of the Main Page and select element. Currently available:
Changed lines 7-11 from:
Data to be provided as an input:
# Equivalent width, in pm (0.1 A)
# Effective temperature, in K
# Logarithm of surface gravity, cgs (cm s-2)
# Microturbulence, in km/s
# Equivalent width
# Effective temperature, in K
# Logarithm of surface
to:
Data to be provided as input:
# Equivalent width [pm = 0.1 A] or LTE abundance
# Effective temperature [K]
# Logarithm of surface gravity [cm s-2]
# Microturbulence [km s-1]
# Equivalent width [pm = 0.1 A] or LTE abundance
# Effective temperature [K]
# Logarithm of surface gravity [cm s-2]
# Microturbulence [km s-1]
Changed lines 15-18 from:
The output includes either
* LTE and NLTE equivalent widths
or
* LTE and NLTE abundance corrections
*
or
* LTE and NLTE abundance corrections
to:
The output includes equivalent width, LTE and NLTE abundance, and NLTE abundance correction
Added lines 1-19:
'''INSPECT Documentation'''
----
For a simple query, click the link 'Database' in the side bar of the Main Page and select element. Currently available:
* Li
* Na
* Fe
Data to be provided as an input:
# Equivalent width, in pm (0.1 A)
# Effective temperature, in K
# Logarithm of surface gravity, cgs (cm s-2)
# Microturbulence, in km/s
# Wavelength must be chosen from the list. For the available spectral lines, check the {+Line data+} link at the top of each page.
The output includes either
* LTE and NLTE equivalent widths
or
* LTE and NLTE abundance corrections
----
For a simple query, click the link 'Database' in the side bar of the Main Page and select element. Currently available:
* Li
* Na
* Fe
Data to be provided as an input:
# Equivalent width, in pm (0.1 A)
# Effective temperature, in K
# Logarithm of surface gravity, cgs (cm s-2)
# Microturbulence, in km/s
# Wavelength must be chosen from the list. For the available spectral lines, check the {+Line data+} link at the top of each page.
The output includes either
* LTE and NLTE equivalent widths
or
* LTE and NLTE abundance corrections