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Jesse Mason

Publications and source records attributed to Jesse Mason.

4 recordsLinked to original sources

Improved rainfall forecasts in daily use over East Africa

Ensemble forecasting has proven to be a vital tool for predicting extreme, life-threatening or only partially predictable weather events. As well as providing probabilistic products, individual ensemble members provide context and realisations of possible extreme weather. However, many National Meteorological Services in East Africa do not have the computing resources to enable them to run their local area models in ensemble mode over the full period of the two-week medium range. In this paper we test the performance of a forecast system, comprising the global ECMWF ensemble forecast, post-processed using cGAN, a neural network model, and forecasts calibrated using IDR, a recent statistical method, against the probabilistic climatology. cGAN provides comparable levels of probabilistic skill as IDR applied to the ECMWF ensemble or IDR applied to the machine-learning models FuXi and GraphCast. These methods improve the raw ECMWF ensemble forecast substantially, which is itself an improvement on deterministic forecasts. The ability of cGAN to produce individual realisations of future rainfall was important when assessed in an operational context by the National Meteorological and Hydrological Services of Kenya and Ethiopia. Moreover, in common with IDR, cGAN is cheap to train/run and requires no additional post-processing. It is run on laptops to generate many thousands of ensemble members, making it suitable for Meteorological Services with limited computational facilities.

physics.ao-ph

Observational Astrophysics Research through Cross Institutional Research Partnerships

Undergraduate research in STEM can be a transformative experience, especially for Community College students, many of whom come from under-represented backgrounds. However, undergraduate research at Community Colleges is relatively rare, due in part to their focus on teaching excellence. Research partnerships with four year colleges about exciting and accessible science topics, facilitated by researchers such as postdoctoral fellows, can be a powerful path forward. We describe our program, the Dead Stars Society (DSS), as a successful example of such a research partnership, focused on the topic of observational astronomy, specifically stellar science with the Vera C. Rubin Observatory, and X-ray astronomy with Chandra, NICER and NuSTAR.

physics.ed-ph

Classifying Compact Radio Emission in Nearby Galaxies: a 10GHz Study of Active Galactic Nuclei, Supernovae, Anomalous Microwave Emission and Star Forming Regions

We present 115 compact radio point sources in three galaxies, NGC 5474, NGC 4631 and M51, taken in the most extended (A-)configuration of the Karl G. Jansky Very Large Array at 10GHz. Several of these compact radio point sources have diffuse counterparts identified in previous multi-band studies of resolved radio continuum emission. We find compact counterparts to eight star forming regions, four anomalous microwave emission candidates, and one supernova remnant (SN 2011dh). Nine of the compact radio sources match X-ray counterparts, the majority of which are background galaxies. These AGN are all within the D25 (isophotal diameter) of the host galaxy and might act as contaminants for X-ray binary population studies, highlighting the need for high-resolution multi-band imaging. This study showcases the broad number of science cases that require sensitive radio facilities, like the upcoming Square Kilometre Array and the planned next generation Very Large Array.

astro-ph.GA

Detecting the Black Hole Candidate Population in M51's Young Massive Star Clusters: Constraints on Accreting Intermediate Mass Black Holes

Intermediate mass black holes (10^2 < M_BH< 10^5 Msun) are an open question in our understanding of black hole evolution and growth. They have long been linked to dense star cluster environments thanks to cluster dynamics, but there are a limited number of secure detections. We leverage existing X-ray observations from Chandra X-ray Observatory and optical catalogs from Hubble Space Telescope with new radio observations from the Karl G. Jansky Very Large Array to search for any evidence of accreting black holes in young massive clusters in the nearby galaxy M51. We find that of 43 bright ($L_X > 10^{38}$ erg/s) X-ray point sources in M51, 24 had probable matches to objects including possible associated star clusters in the HST Legacy Extragalactic UV Survey catalog, seven of which were classified as contaminants (background galaxies or foreground stars). We explore the optical properties of the remaining 17 sources, including cluster age and mass estimates, and search for radio counterparts in the 8-12 GHz band. The lack of radio counterparts to X-ray sources we know to be associated with young massive clusters in M51 suggests that we do not significantly detect hard-state IMBHs ~ 10^4 Msun or above. However, more sensitive radio facilities like the Square Kilometre Array and next generation Very Large Array may be able to provide evidence for IMBHs with masses down to ~ 10^3 Msun.

astro-ph.HE