
<script type="text/javascript">
<!--
document.write('<div id="oa_widget"></div>');
document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=undefined&type=result"></script>');
-->
</script>The Eureka! Control Files (.ecf files) and Eureka! Parameter Files (.epf files) used for the reduction and fitting of the JWST NIRCam/F322W2, NIRCam/F444W, and MIRI/LRS eclipse observations of WASP-69 b as presented in Schlawin et al. 2024 (AAS Journals). These analyses used version 0.10 of the Eureka! pipeline; jwst package version 1.10.2; CRDS version 11.17.0; and CRDS context 1094 for NIRCam/F322W2 and NIRCam/F444W, and 1097 for MIRI/LRS. For the MIRI observations, the Eureka! pipeline was modified to include the custom 390 Hz noise removal step which was later merged through PR #556.
| citations This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically). | 1 | |
| popularity This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network. | Average | |
| influence This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically). | Average | |
| impulse This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network. | Average |
