Current suggested sky model to use is:
srclist_pumav3_EoR0LoBES_EoR1pietro_CenA-GP_2023-11-07.fits
srclist_pumav3_EoR0LoBES_EoR1pietro_CenA-GP_2023-11-07.fits
srclist_pumav3_EoR0LoBES_EoR1pietro_CenA-GP_2023-11-07.yaml
- LoBES (Lynch et al 2021) in EoR0 field
- Procopio et al 2017 with a few added shapelet models in EoR1 field (including Fornax A model from Line et 2020)
- Cook et all 2022 for Cen A and Galactic Plane SNR
- Everything is either a power-law or curved power-law SED
srclist_pumav3_EoR0aegean_EoR1pietro+ForA_phase1+2.txt
- Added a much improved Fornax A model using both phase 1 and phase 2 extended data
srclist_pumav3_EoR0aegean_EoR1pietro+ForA_phase1+2_TGSSgalactic.txt
- New ForA model plus attempt at filling galactic plane with TGSS sources
srclist_pumav3_EoR0aegean_EoR1pietro+ForA_TGSSgalactic.txt
- Attempt to fill in the galactic plane with TGSS sources
srclist_pumav3_EoR0aegean_EoR1pietro+ForA.txt
The main features of this srclist are:
- Based off of the GLEAM catalogue
- Matched to TGSS, VLSSr, SUMMS, and NVSS
- Has PUMA based extended models up to 20 deg away from EoR0
- Has Pietro's extended models up to 10 deg away from EoR1
- Outside of those areas, it is the PUMA matched GLEAM catalogue if a GLEAM source failed the PUMA tests, it has been included but just as a GLEAM source - it has not been eyeballed
- Also has Jenny's shapelet model for Fornax A
srclist_puma-v2_complete.txt
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Added the most up to date and complete PUMA srclist, srclist_puma-v2_complete.txt. This srclist covers the full southern sky, using either mwacs or mrc as a base. It is complete with point source extended models between 22h < RA < 6h, -57deg < Dec < +3deg (2 hours about EoR0 and EoR1). Elsewhere, only the sources accepted by PUMA are currently included.
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In ./puma_v2, the separate srclists used to create srclist_puma-v2_complete.txt are stored and explained
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In ./extended, information and plots of all the extended sources in srclist_puma-v2_complete.txt are included
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srclist_by_beam.py will take a srclist, and return a given number of sources in a megapatch srclist. These will be brightest sources once convolved with the beam, as defined by the pointing given by a designated metafits file. The sources are also confined to a user specified distance of the pointing centre. To use the plotting option (-p), wscaxes module is needed.