Description This new version of hoki contains the data analysis pipelines used to fit BPASS SEDs to observed SEDs using ppxf, as well as utility functions that streamline the exploration of the stellar models to make finding transient progenitors faster than ever and easy to automate. These tools were created for the analysis that resulted in the publication Stevance et al. 2023 (in press. with Nature Astronomy). New features and data sedfitting subpackage which contains the kvn and lordcommander modules which contain helper tools to create SED templates to fit observed SEDs with ppxf and retrieve stellar formation histories and metallicities for individual spectra and data cubes. (NOTE: i want, in time, to rename and refactor these utilit...
Current time domain facilities are discovering hundreds of new galactic and extra-galactic transient...
Artículo de publicación ISIContext. The Public European Southern Observatory Spectroscopic Survey of...
In this paper, I present a new set of synthetic spectral energy distributions (SEDs) for young stell...
New Features csp subpackage: Create Complex Stellar Populations from the BPASS Simple Stellar Popul...
Jupyter notebooks and data for the tutorials on SED fitting using the BPASSv2.2.1 models and the hok...
Spectral energy distributions (SEDs) are useful primary and complementary tools in the analysis of o...
Summary At the core of v1.5 is the age_utils module and the AgeWizard pipeline. The utilities provi...
This data set is made of 26 binary files (.pckl) that contain pandas DataFrames compiling all the BP...
This is a database of spec-SEDs and phot-SEDs of CCSN progenitors. There are two sub-databases for ...
FITS file containing the pre-computed grid of Done or Nemmen model SEDs. See Table 2 in the publicat...
Measuring the cosmic star formation history (SFH) is essential to our understanding of the build-up ...
The Dense Basis SED fitting method reveals previously inaccessible information about the number and ...
EvE contains a number of tables summarising the BPASSv2.2.1 stellar library to facilitate identifyin...
This is a curated starter-kit that contains a subset of the full data in BPASSv2.2.1. For the full d...
SED template fits to various public spectroscopic redshift surveys cross matched to publicly availab...
Current time domain facilities are discovering hundreds of new galactic and extra-galactic transient...
Artículo de publicación ISIContext. The Public European Southern Observatory Spectroscopic Survey of...
In this paper, I present a new set of synthetic spectral energy distributions (SEDs) for young stell...
New Features csp subpackage: Create Complex Stellar Populations from the BPASS Simple Stellar Popul...
Jupyter notebooks and data for the tutorials on SED fitting using the BPASSv2.2.1 models and the hok...
Spectral energy distributions (SEDs) are useful primary and complementary tools in the analysis of o...
Summary At the core of v1.5 is the age_utils module and the AgeWizard pipeline. The utilities provi...
This data set is made of 26 binary files (.pckl) that contain pandas DataFrames compiling all the BP...
This is a database of spec-SEDs and phot-SEDs of CCSN progenitors. There are two sub-databases for ...
FITS file containing the pre-computed grid of Done or Nemmen model SEDs. See Table 2 in the publicat...
Measuring the cosmic star formation history (SFH) is essential to our understanding of the build-up ...
The Dense Basis SED fitting method reveals previously inaccessible information about the number and ...
EvE contains a number of tables summarising the BPASSv2.2.1 stellar library to facilitate identifyin...
This is a curated starter-kit that contains a subset of the full data in BPASSv2.2.1. For the full d...
SED template fits to various public spectroscopic redshift surveys cross matched to publicly availab...
Current time domain facilities are discovering hundreds of new galactic and extra-galactic transient...
Artículo de publicación ISIContext. The Public European Southern Observatory Spectroscopic Survey of...
In this paper, I present a new set of synthetic spectral energy distributions (SEDs) for young stell...