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@ARTICLE{Snellen:2010, | ||
author = {{Snellen}, Ignas A.~G. and {de Kok}, Remco J. and | ||
{de Mooij}, Ernst J.~W. and {Albrecht}, Simon}, | ||
title = "{The orbital motion, absolute mass and high-altitude winds of exoplanet HD209458b}", | ||
journal = {\nat}, | ||
keywords = {Astrophysics - Earth and Planetary Astrophysics}, | ||
year = "2010", | ||
month = "Jun", | ||
volume = {465}, | ||
number = {7301}, | ||
pages = {1049-1051}, | ||
doi = {10.1038/nature09111}, | ||
archivePrefix = {arXiv}, | ||
eprint = {1006.4364}, | ||
primaryClass = {astro-ph.EP}, | ||
adsurl = {https://ui.adsabs.harvard.edu/abs/Snellen2010}, | ||
adsnote = {Provided by the SAO/NASA Astrophysics Data System} | ||
} | ||
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@ARTICLE{Brogi:2012, | ||
author = {{Brogi}, Matteo and {Snellen}, Ignas A.~G. and {de Kok}, Remco J. and | ||
{Albrecht}, Simon and {Birkby}, Jayne and {de Mooij}, Ernst J.~W.}, | ||
title = "{The signature of orbital motion from the dayside of the planet {\ensuremath{\tau}} Bo{\"o}tis b}", | ||
journal = {\nat}, | ||
keywords = {Astrophysics - Earth and Planetary Astrophysics}, | ||
year = "2012", | ||
month = "Jun", | ||
volume = {486}, | ||
number = {7404}, | ||
pages = {502-504}, | ||
doi = {10.1038/nature11161}, | ||
archivePrefix = {arXiv}, | ||
eprint = {1206.6109}, | ||
primaryClass = {astro-ph.EP}, | ||
adsurl = {https://ui.adsabs.harvard.edu/abs/Brogi2012}, | ||
adsnote = {Provided by the SAO/NASA Astrophysics Data System} | ||
} | ||
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--- | ||
title: 'hipparchus: Cross-correlation functions via the weighted mean' | ||
tags: | ||
- Python | ||
- astronomy | ||
- high resolution spectroscopy | ||
authors: | ||
- name: Brett M. Morris | ||
orcid: 0000-0003-2528-3409 | ||
affiliation: 1 | ||
affiliations: | ||
- name: Center for Space and Habitability, University of Bern, Switzerland | ||
index: 1 | ||
date: January 2020 | ||
bibliography: paper.bib | ||
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aas-doi: 10.3847/xxxxx | ||
aas-journal: Astrophysical Journal | ||
--- | ||
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# Summary | ||
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The presence of starspots on exoplanet host stars potentially hinders the | ||
interpretation of planet observations. We must know the starspot covering | ||
fractions of stars in order to interpret the transmission and day-side | ||
spectra of small exoplanets, because the spectral features generated by | ||
exoplanet atmospheres are degenerate with the signatures of starspots. If we | ||
seek to measure starspot coverages with sufficient precision to mitigate | ||
the effects of starspots on planet characterization, we must develop new | ||
techniques to measure the spatial extent of starspots. This is difficult to do | ||
in practice because starspots are dim compared to the rest of the stellar | ||
photosphere, and take up a small fraction of the stellar surface area. | ||
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An analogous contrast-ratio problem occurs when detecting the emission or | ||
transmission spectra from exoplanet atmospheres, which has been addressed using | ||
the cross-correlation function (CCF) technique applied to high resolution | ||
spectroscopy [@Snellen:2010, @Brogi:2012]. The CCF is sensitive to both strong | ||
and weak absorption features that occur at *all* wavelengths throughout the | ||
spectrum of the planet, constructively co-adding the absorption lines into a | ||
single average when a template spectrum is matched with the observed spectrum | ||
at the correct Doppler velocity. | ||
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We introduce ``hipparchus``, a pure Python, open source package designed for | ||
cross-correlating HARPS with synthetic spectral templates. The | ||
accompanying submitted paper to AAS Journals applies the package to the problem | ||
of hunting for cool starspots on stellar photospheres, but it could be used | ||
more generally to measure the CCF in a variety of contexts. ``hipparchus`` | ||
computes the CCF via the weighted mean, with the help of array broadcasting to | ||
simultaneously compute the CCF efficiently at many velocities. It includes | ||
convenience functions for reading and continuum normalizing HARPS(-N) E2DS | ||
spectra, along with an object-oriented framework for computing CCFs. | ||
Contributions to ``hipparchus`` from the community are welcome. | ||
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# Acknowledgements | ||
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We acknowledge valuable advice from H. Jens Hoeijmakers, and spectral templates | ||
from Daniel Kitzmann. | ||
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# References |