Thursday, March 30th, 12:30 P.M.
The
Chandra Source Catalog version 2.1 (CSC 2.1) adds observations released
publicly between January 1, 2015 and the end of 2021, uncovers a
significant portion of new sky for X-ray exploration, and has a number
of algorithmic enhancements with respect to the previous version. In
this splinter session we will host a hands-on workshop/tutorial for
users to get familiar with the different access interfaces to CSC 2.1,
including our Table Access Protocol (TAP) service that can be used with
Virtual Observatory tools such as astroquery and pyvo. We also introduce
users to a few science threads that exploit the catalog data products,
such as light curves and spectra, and provide Jupyter notebooks that
demonstrate how to access these data products and how to used them for
scientific applications such as AGN selection and transient
identification. This session is complementary to our accepted Special
Session on the science enabled by the CSC.
Thursday, March 30th, 2:00 P.M.
The
new version of the Chandra Source Catalog (CSC 2.1) is a rolling
release currently in production, with processed datasets already
available to the users. The final release, expected in the first half of
2023, expands on version 2.0 by adding over 4,500 observations released
publicly between January 1, 2015 and December 31, 2021, corresponding
to an increase of more than 40% of the sky area covered, relative to
CSC2.0. The nearly 450,000 individual X-ray sources in CSC 2.1, the vast
majority of which are serendipitous, represent a significant
opportunity for population studies and data-driven discovery in high
energy astrophysics, and a rich data repository with many applications
in the era of Big Data and Open Science. In this special session we will
present CSC 2.1 and highlight some relevant, cutting-edge science
questions that the catalog has been used to address, through
presentations on specific science projects. We will introduce attendees
to the diverse dataset of tabulated properties and data products that
make up the catalog, including spectra and light curves, and discuss
features of CSC 2.1 that facilitate multi-wavelength science, such as
our effort to align the catalog astrometry to the Gaia reference frame
and the cross-matching of the CSC with Sloan Digital Sky Survey (SDSS). A
diverse cohort of early career scientists will present their
CSC-enabled research and discuss how CSC can be used to advance high
energy astrophysics.