Last Observations
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PuMA Monitoring Program
High-cadence monitoring of southern glitching pulsars
The PuGli-S project tracks bright glitching pulsars in the southern hemisphere at S-band using the two IAR antennas, building a long-baseline dataset for timing analysis, glitch detection, and cadence optimization.
The observing program is designed to support rapid follow-up, residual studies before and after glitches, jitter analysis across timescales, and refreshed post-glitch ToAs for downstream science, including gravitational-wave searches.
Four compact entry points
The site is organized so that the main operational views are reachable in one click and do not require scanning long pages first.
By PSR
Jump to the long-term pulsar view when you want the historical pages and tempo plots grouped by source.
Open pulsar historySummary
Open a generated statistics view with pulsar counts, observations per source, yearly totals, and skipped datasets.
Open summaryPuMA Collaboration
External project and collaboration context remain available through the main PuMA site.
Open collaboration pageMonitored pulsars
The current observing list is kept visible as a compact grid instead of a long inline paragraph, which makes the front page easier to scan and update.
- J0738-4042
- J0742-2822
- J0835-4510
- J1430-6623
- J1644-4559
- J1709-4429
- J1721-3532
- J1731-4744
- J1740-3015
Recent arXiv work connected to the IAR monitoring campaign
A compact set of related papers involving the PuGli-S monitoring effort and publications with Guillermo Gancio or G. Gancio in the author list.
First results of the glitching pulsars monitoring program at the Argentine Institute of Radioastronomy
arXiv:2210.03770, 2022. Early results from the high-cadence IAR campaign, including the Vela glitch and mini-glitches in PSR J1048-5832.
Open on arXivUpdates on the glitching pulsar monitoring campaign performed from IAR
arXiv:2312.08188, 2023. Follow-up campaign update with glitch measurements for Vela, J0742-2822, J1740-3015, and J1048-5832.
Open on arXivTiming irregularities and glitches from the pulsar monitoring campaign at IAR
arXiv:2406.17099, 2024. Daily-cadence timing analysis of young pulsars, including newly reported glitches and timing-noise behaviour.
Open on arXivConstraints on gravitational waves from the 2024 Vela pulsar glitch
arXiv:2512.17990, 2025. Gravitational-wave constraints connected to the 2024 Vela glitch, with G. Gancio in the author list.
Open on arXiv