REVIEW 2 cited by
Observatory science with eXTP
Not yet reviewed by Pith; the record is open.
This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.
SPECIMEN: schema-true, not a live event
T0 review · schema-true
One-sentence machine reading of the paper's core claim.
pith:XXXXXXXX · record.json · timestamp
read the original abstract
In this White Paper we present the potential of the enhanced X-ray Timing and Polarimetry (eXTP) mission for studies related to Observatory Science targets. These include flaring stars, supernova remnants, accreting white dwarfs, low and high mass X-ray binaries, radio quiet and radio loud active galactic nuclei, tidal disruption events, and gamma-ray bursts. eXTP will be excellently suited to study one common aspect of these objects: their often transient nature. Developed by an international Consortium led by the Institute of High Energy Physics of the Chinese Academy of Science, the eXTP mission is expected to be launched in the mid 2020s.
Forward citations
Cited by 2 Pith papers
-
Observatory Science with eXTP
An updated white paper describing the planned observatory science of the eXTP X-ray mission, with simulations of anticipated spectral, timing, and polarization measurements across many astrophysical source classes.
-
Continuum optical-UV and X-ray variability of AGN: current results and future challenges
A comprehensive review of AGN continuum variability from optical/UV to X-rays, with no new data.
Discussion (0). Continue with ORCID to comment.