Skip to content
New issue

Have a question about this project? Sign up for a free GitHub account to open an issue and contact its maintainers and the community.

By clicking “Sign up for GitHub”, you agree to our terms of service and privacy statement. We’ll occasionally send you account related emails.

Already on GitHub? Sign in to your account

Creating pull request for 10.21105.joss.04417 #3295

Closed
wants to merge 3 commits into from
Closed
Show file tree
Hide file tree
Changes from all commits
Commits
File filter

Filter by extension

Filter by extension

Conversations
Failed to load comments.
Loading
Jump to
Jump to file
Failed to load files.
Loading
Diff view
Diff view
329 changes: 329 additions & 0 deletions joss.04417/10.21105.joss.04417.crossref.xml
Original file line number Diff line number Diff line change
@@ -0,0 +1,329 @@
<?xml version="1.0" encoding="UTF-8"?>
<doi_batch xmlns="http://www.crossref.org/schema/5.3.1"
xmlns:ai="http://www.crossref.org/AccessIndicators.xsd"
xmlns:rel="http://www.crossref.org/relations.xsd"
xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
version="5.3.1"
xsi:schemaLocation="http://www.crossref.org/schema/5.3.1 http://www.crossref.org/schemas/crossref5.3.1.xsd">
<head>
<doi_batch_id>20220622T132148-143802ca373313097189b5b559a63d801677f867</doi_batch_id>
<timestamp>20220622132148</timestamp>
<depositor>
<depositor_name>JOSS Admin</depositor_name>
<email_address>[email protected]</email_address>
</depositor>
<registrant>The Open Journal</registrant>
</head>
<body>
<journal>
<journal_metadata>
<full_title>Journal of Open Source Software</full_title>
<abbrev_title>JOSS</abbrev_title>
<issn media_type="electronic">2475-9066</issn>
<doi_data>
<doi>10.21105/joss</doi>
<resource>https://joss.theoj.org/</resource>
</doi_data>
</journal_metadata>
<journal_issue>
<publication_date media_type="online">
<month>06</month>
<year>2022</year>
</publication_date>
<journal_volume>
<volume>7</volume>
</journal_volume>
<issue>74</issue>
</journal_issue>
<journal_article publication_type="full_text">
<titles>
<title>A-SLOTH: Ancient Stars and Local Observables by Tracing
Halos</title>
</titles>
<contributors>
<person_name sequence="first" contributor_role="author">
<given_name>Mattis</given_name>
<surname>Magg</surname>
<ORCID>https://orcid.org/0000-0002-9022-5136</ORCID>
</person_name>
<person_name sequence="additional"
contributor_role="author">
<given_name>Tilman</given_name>
<surname>Hartwig</surname>
<ORCID>https://orcid.org/0000-0001-6742-8843</ORCID>
</person_name>
<person_name sequence="additional"
contributor_role="author">
<given_name>Li-Hsin</given_name>
<surname>Chen</surname>
</person_name>
<person_name sequence="additional"
contributor_role="author">
<given_name>Yuta</given_name>
<surname>Tarumi</surname>
<ORCID>https://orcid.org/0000-0002-9801-7788</ORCID>
</person_name>
</contributors>
<publication_date>
<month>06</month>
<day>22</day>
<year>2022</year>
</publication_date>
<pages>
<first_page>4417</first_page>
</pages>
<publisher_item>
<identifier id_type="doi">10.21105/joss.04417</identifier>
</publisher_item>
<ai:program name="AccessIndicators">
<ai:license_ref applies_to="vor">http://creativecommons.org/licenses/by/4.0/</ai:license_ref>
<ai:license_ref applies_to="am">http://creativecommons.org/licenses/by/4.0/</ai:license_ref>
<ai:license_ref applies_to="tdm">http://creativecommons.org/licenses/by/4.0/</ai:license_ref>
</ai:program>
<rel:program>
<rel:related_item>
<rel:description>Software archive</rel:description>
<rel:inter_work_relation relationship-type="references" identifier-type="doi">10.5281/zenodo.6683682</rel:inter_work_relation>
</rel:related_item>
<rel:related_item>
<rel:description>GitHub review issue</rel:description>
<rel:inter_work_relation relationship-type="hasReview" identifier-type="uri">https://github.com/openjournals/joss-reviews/issues/4417</rel:inter_work_relation>
</rel:related_item>
</rel:program>
<doi_data>
<doi>10.21105/joss.04417</doi>
<resource>https://joss.theoj.org/papers/10.21105/joss.04417</resource>
<collection property="text-mining">
<item>
<resource mime_type="application/pdf">https://joss.theoj.org/papers/10.21105/joss.04417.pdf</resource>
</item>
</collection>
</doi_data>
<citation_list>
<citation key="Parkinson2008">
<article_title>Generating dark matter halo merger
trees</article_title>
<author>Parkinson</author>
<journal_title>Monthly Notices of the Royal Astronomical
Society</journal_title>
<volume>383</volume>
<doi>10.1111/j.1365-2966.2007.12517.x</doi>
<cYear>2008</cYear>
<unstructured_citation>Parkinson, H., Cole, S., &amp; Helly,
J. (2008). Generating dark matter halo merger trees. Monthly Notices of
the Royal Astronomical Society, 383, 557–564.
https://doi.org/10.1111/j.1365-2966.2007.12517.x</unstructured_citation>
</citation>
<citation key="Hartwig15b">
<article_title>Constraining the primordial initial mass
function with stellar archaeology</article_title>
<author>Hartwig</author>
<journal_title>Monthly Notices of the Royal Astronomical
Society</journal_title>
<volume>447</volume>
<doi>10.1093/mnras/stu2740</doi>
<cYear>2015</cYear>
<unstructured_citation>Hartwig, T., Bromm, V., Klessen, R.
S., &amp; Glover, S. C. O. (2015). Constraining the primordial initial
mass function with stellar archaeology. Monthly Notices of the Royal
Astronomical Society, 447, 3892–3908.
https://doi.org/10.1093/mnras/stu2740</unstructured_citation>
</citation>
<citation key="Hartwig16b">
<article_title>Exploring the nature of the Lyman-\alpha
emitter CR7</article_title>
<author>Hartwig</author>
<journal_title>Monthly Notices of the Royal Astronomical
Society</journal_title>
<volume>462</volume>
<doi>10.1093/mnras/stw1775</doi>
<cYear>2016</cYear>
<unstructured_citation>Hartwig, T., Latif, M. A., Magg, M.,
Bromm, V., Klessen, R. S., Glover, S. C. O., Whalen, D. J., Pellegrini,
E. W., &amp; Volonteri, M. (2016). Exploring the nature of the
Lyman-\alpha emitter CR7. Monthly Notices of the Royal Astronomical
Society, 462, 2184–2202.
https://doi.org/10.1093/mnras/stw1775</unstructured_citation>
</citation>
<citation key="Hartwig16a">
<article_title>Gravitational waves from the remnants of the
first stars</article_title>
<author>Hartwig</author>
<journal_title>Monthly Notices of the Royal Astronomical
Society</journal_title>
<volume>460</volume>
<doi>10.1093/mnrasl/slw074</doi>
<cYear>2016</cYear>
<unstructured_citation>Hartwig, T., Volonteri, M., Bromm,
V., Klessen, R. S., Barausse, E., Magg, M., &amp; Stacy, A. (2016).
Gravitational waves from the remnants of the first stars. Monthly
Notices of the Royal Astronomical Society, 460, L74–L78.
https://doi.org/10.1093/mnrasl/slw074</unstructured_citation>
</citation>
<citation key="Hartwig18a">
<article_title>Descendants of the first stars: the distinct
chemical signature of second generation stars</article_title>
<author>Hartwig</author>
<journal_title>Monthly Notices of the Royal Astronomical
Society</journal_title>
<doi>10.1093/mnras/sty1176</doi>
<cYear>2018</cYear>
<unstructured_citation>Hartwig, T., Yoshida, N., Magg, M.,
Frebel, A., Glover, S. C. O., Gómez, F. A., Griffen, B., Ishigaki, M.
N., Ji, A. P., Klessen, R. S., O’Shea, B. W., &amp; Tominaga, N. (2018).
Descendants of the first stars: the distinct chemical signature of
second generation stars. Monthly Notices of the Royal Astronomical
Society. https://doi.org/10.1093/mnras/sty1176</unstructured_citation>
</citation>
<citation key="Magg21b">
<article_title>Effect of the cosmological transition to
metal-enriched star-formation on the hydrogen 21-cm
signal</article_title>
<author>Magg</author>
<journal_title>Monthly Notices of the Royal Astronomical
Society</journal_title>
<doi>10.1093/mnras/stac1664</doi>
<cYear>2022</cYear>
<unstructured_citation>Magg, M., Reis, I., Fialkov, A.,
Barkana, R., Klessen, R. S., Glover, S. C. O., Chen, L.-H., Hartwig, T.,
&amp; Schauer, A. T. P. (2022). Effect of the cosmological transition to
metal-enriched star-formation on the hydrogen 21-cm signal. Monthly
Notices of the Royal Astronomical Society.
https://doi.org/10.1093/mnras/stac1664</unstructured_citation>
</citation>
<citation key="chen22">
<article_title>Tracing stars in Milky Way satellites with
A-SLOTH</article_title>
<author>Chen</author>
<journal_title>arXiv e-prints</journal_title>
<cYear>2022</cYear>
<unstructured_citation>Chen, L.-H., Magg, M., Hartwig, T.,
Glover, S. C. O., Ji, A. P., &amp; Klessen, R. S. (2022). Tracing stars
in Milky Way satellites with A-SLOTH. arXiv e-Prints, arXiv:2202.01220.
https://arxiv.org/abs/2202.01220</unstructured_citation>
</citation>
<citation key="Magg18">
<article_title>Predicting the locations of possible
long-lived low-mass first stars: importance of satellite dwarf
galaxies</article_title>
<author>Magg</author>
<journal_title>Monthly Notices of the Royal Astronomical
Society</journal_title>
<volume>473</volume>
<doi>10.1093/mnras/stx2729</doi>
<cYear>2018</cYear>
<unstructured_citation>Magg, M., Hartwig, T., Agarwal, B.,
Frebel, A., Glover, S. C. O., Griffen, B. F., &amp; Klessen, R. S.
(2018). Predicting the locations of possible long-lived low-mass first
stars: importance of satellite dwarf galaxies. Monthly Notices of the
Royal Astronomical Society, 473, 5308–5323.
https://doi.org/10.1093/mnras/stx2729</unstructured_citation>
</citation>
<citation key="Magg16">
<article_title>A new statistical model for Population III
supernova rates: discriminating between \LambdaCDM and WDM
cosmologies</article_title>
<author>Magg</author>
<journal_title>Monthly Notices of the Royal Astronomical
Society</journal_title>
<volume>462</volume>
<doi>10.1093/mnras/stw1882</doi>
<cYear>2016</cYear>
<unstructured_citation>Magg, M., Hartwig, T., Glover, S. C.
O., Klessen, R. S., &amp; Whalen, D. J. (2016). A new statistical model
for Population III supernova rates: discriminating between \LambdaCDM
and WDM cosmologies. Monthly Notices of the Royal Astronomical Society,
462, 3591–3601.
https://doi.org/10.1093/mnras/stw1882</unstructured_citation>
</citation>
<citation key="Tarumi20">
<article_title>Implications of Inhomogeneous Metal Mixing
for Stellar Archaeology</article_title>
<author>Tarumi</author>
<journal_title>Astrophysical Journal</journal_title>
<issue>1</issue>
<volume>897</volume>
<doi>10.3847/1538-4357/ab960d</doi>
<cYear>2020</cYear>
<unstructured_citation>Tarumi, Y., Hartwig, T., &amp; Magg,
M. (2020). Implications of Inhomogeneous Metal Mixing for Stellar
Archaeology. Astrophysical Journal, 897(1), 58.
https://doi.org/10.3847/1538-4357/ab960d</unstructured_citation>
</citation>
<citation key="GreifReview">
<article_title>The numerical frontier of the high-redshift
Universe</article_title>
<author>Greif</author>
<journal_title>Computational Astrophysics and
Cosmology</journal_title>
<volume>2</volume>
<doi>10.1186/s40668-014-0006-2</doi>
<cYear>2015</cYear>
<unstructured_citation>Greif, T. H. (2015). The numerical
frontier of the high-redshift Universe. Computational Astrophysics and
Cosmology, 2, 3.
https://doi.org/10.1186/s40668-014-0006-2</unstructured_citation>
</citation>
<citation key="deBennassuti17">
<article_title>Limits on Population III star formation with
the most iron-poor stars</article_title>
<author>de Bennassuti</author>
<journal_title>Monthly Notices of the Royal Astronomical
Society</journal_title>
<volume>465</volume>
<doi>10.1093/mnras/stw2687</doi>
<cYear>2017</cYear>
<unstructured_citation>de Bennassuti, M., Salvadori, S.,
Schneider, R., Valiante, R., &amp; Omukai, K. (2017). Limits on
Population III star formation with the most iron-poor stars. Monthly
Notices of the Royal Astronomical Society, 465, 926–940.
https://doi.org/10.1093/mnras/stw2687</unstructured_citation>
</citation>
<citation key="Visbal18">
<article_title>Self-consistent semi-analytic models of the
first stars</article_title>
<author>Visbal</author>
<journal_title>Monthly Notices of the Royal Astronomical
Society</journal_title>
<issue>4</issue>
<volume>475</volume>
<doi>10.1093/mnras/sty142</doi>
<cYear>2018</cYear>
<unstructured_citation>Visbal, E., Haiman, Z., &amp; Bryan,
G. L. (2018). Self-consistent semi-analytic models of the first stars.
Monthly Notices of the Royal Astronomical Society, 475(4), 5246–5256.
https://doi.org/10.1093/mnras/sty142</unstructured_citation>
</citation>
<citation key="Brauer2019">
<article_title>The Origin of r-process Enhanced Metal-poor
Halo Stars In Now-destroyed Ultra-faint Dwarf Galaxies</article_title>
<author>Brauer</author>
<journal_title>Astrophysical Journal</journal_title>
<issue>2</issue>
<volume>871</volume>
<doi>10.3847/1538-4357/aafafb</doi>
<cYear>2019</cYear>
<unstructured_citation>Brauer, K., Ji, A. P., Frebel, A.,
Dooley, G. A., Gómez, F. A., &amp; O’Shea, B. W. (2019). The Origin of
r-process Enhanced Metal-poor Halo Stars In Now-destroyed Ultra-faint
Dwarf Galaxies. Astrophysical Journal, 871(2), 247.
https://doi.org/10.3847/1538-4357/aafafb</unstructured_citation>
</citation>
<citation key="Ishiyama16">
<article_title>Where are the Low-mass Population III
Stars?</article_title>
<author>Ishiyama</author>
<journal_title>Astrophysical Journal</journal_title>
<volume>826</volume>
<doi>10.3847/0004-637X/826/1/9</doi>
<cYear>2016</cYear>
<unstructured_citation>Ishiyama, T., Sudo, K., Yokoi, S.,
Hasegawa, K., Tominaga, N., &amp; Susa, H. (2016). Where are the
Low-mass Population III Stars? Astrophysical Journal, 826, 9.
https://doi.org/10.3847/0004-637X/826/1/9</unstructured_citation>
</citation>
</citation_list>
</journal_article>
</journal>
</body>
</doi_batch>
Loading