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Happy Birthday, SVOM!

22 June 2025 marks the first anniversary of the SVOM satellite in orbit. One year ago, the satellite was launched from the Xichang base in China at 07:00 UTC. Following the launch, the subsequent phases took place:

  • in-orbit commissioning phase from late June to late September 2024: commissioning of all platform functions and gradual activation of the instruments;
  • validation phase from October 2024 to mid-January 2025: adjustment of system parameters, instruments, and scientific calibration;
  • from mid-January 2025 onwards: start of the scientific operations phase.

The map below shows the exposure time of different regions of the sky (in galactic coordinates) during this first year for the ECLAIRs telescope. The most exposed regions are the galactic poles, in line with the planned SVOM attitude law.

Exposure time map (in days) of various sky regions (in galactic coordinates) during this first year for the ECLAIRs telescope. The map is based on recurring messages sent by the satellite via the VHF network. Exposure does not account for the sensitivity of the ECLAIRs telescope.

The map below shows the pointing directions of the platform during this first year (in galactic coordinates). The colours indicate the nature of the pointings:

  • in blue: general programme pointings, observing predefined areas of the sky while awaiting potential gamma-ray bursts;
  • in green: target of opportunity pointings, observing known astrophysically interesting targets.

In total, SVOM devoted 35% of its available time to observing targets of opportunity, with half of that time spent revisiting gamma-ray bursts to build their visible light curves using the VT. Over two-thirds of these revisits were conducted for SVOM-detected bursts.

Platform pointing directions during this first year (in galactic coordinates).

Thanks to the observing strategy applied this first year, SVOM successfully detected and observed 132 bursts, including:

  • 111 detected by GRM;
  • 47 detected and localised by ECLAIRs;
  • and among these, 89 were also detected by other missions (Einstein Probe, Neil Gehrels Swift Observatory, Fermi).
Map of SVOM triggers (in galactic coordinates) during this first year, including sources identified as gamma-ray bursts and alerts due to known sources, mainly binary sources in the galactic plane.

Thanks to the responsiveness of the SVOM system and its teams, and the excellent multi-wavelength follow-up from our partners, around fifty gamma-ray bursts were observed in soft X-rays, about thirty in visible light, and redshift was successfully measured for 26 events. In particular this year:

The results of this first year speak for themselves. Detections and observations by SVOM and its partners have generated over 900 scientific circulars. The next step is to continue fine-tuning the mission and instruments. Meanwhile, a series of scientific publications is being prepared to formally present these results to the scientific community.


Happy Birthday SVOM, and congratulations to all the teams!

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