Emma CarliThe University of Manchester · Jodrell Bank Centre for Astrophysics
Emma Carli
Master of Science
Finding new extragalactic pulsars with MeerKAT.
About
5
Publications
546
Reads
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35
Citations
Citations since 2017
Introduction
PhD student. Thesis: Search for extra-galactic radio pulsars with the MeerKAT Telescope. (Jodrell Bank Centre for Astrophysics, Pulsars and Time Domain Astrophysics group, TRAPUM team). Supervisor: Ben Stappers
Skills and Expertise
Additional affiliations
May 2019 - July 2019
Position
- Research Intern
Description
- • Research internship with supervisor Dr. Franca Cassol within the Cherenkov Telescope Array (CTA) group at Marseille's Particle Physics Centre (CPPM). • Study of galactic cosmic ray accelerators in the Milky Way (PeVatrons) for CTA.
May 2018 - July 2019
Position
- Research Intern
Description
- • Research internship with supervisor Dr Alexandre Santerne within the Planetary Systems Group (GSP). • Analysis of photometric and spectroscopic data to better understand the impact of stellar activity on exoplanet-search surveys.
Education
September 2020 - March 2024
September 2015 - June 2020
Publications
Publications (5)
The TRAPUM collaboration has used the MeerKAT telescope to conduct a search for pulsed radio emission from the young Small Magellanic Cloud pulsar J0058−7218 located in the supernova remnant IKT 16, following its discovery in X-rays with XMM-Newton. We report no significant detection of dispersed, pulsed radio emission from this source in three 2-h...
The detection of low-mass transiting exoplanets in multiple systems brings new constraints to planetary formation and evolution processes and challenges the current planet formation theories. Nevertheless, only a mere fraction of the small planets detected by Kepler and K2 have precise mass measurements, which are mandatory to constrain their compo...
The log R HK , a measure of ultraviolet chromospheric emission, is used as a stellar sample selection tool in exoplanet surveys to reduce activity-induced noise. It has indeed been found that above log R HK = −4.7, the Vaughan-Preston gap, photospheric activity increases quite linearly with chromospheric emission [Radick et al., 1998]. In this proj...
