From f3f23c115338c433e4a23c2fe6c60ea7a0d37f99 Mon Sep 17 00:00:00 2001 From: Leo Singer Date: Tue, 18 Feb 2025 17:07:59 -0500 Subject: [PATCH] Fix spelling (American English, not British English) --- app/routes/missions.svom/route.mdx | 12 ++++++------ 1 file changed, 6 insertions(+), 6 deletions(-) diff --git a/app/routes/missions.svom/route.mdx b/app/routes/missions.svom/route.mdx index 924ce1a82..ac8036558 100644 --- a/app/routes/missions.svom/route.mdx +++ b/app/routes/missions.svom/route.mdx @@ -26,7 +26,7 @@ import logo from './logo_svom_black.svg' The [Space-based multi-band astronomical Variable Objects Monitor (SVOM)](https://www.svom.eu/en/the-svom-mission/) is a French-Chinese mission, result of a collaboration between the two national space agencies, [China National Space Administration (CNSA)](https://www.cnsa.gov.cn/english/index.html) and [Centre national d'études spatiales (CNES)](https://cnes.fr/en/projects/svom). SVOM is dedicated to the study of the most powerful transient phenomena, with a particular emphasis on gamma-ray bursts (GRBs). -The SVOM spacecraft carries four multi-wavelength instruments: ECLAIRs, Gamma Ray burst Monitor (GRM), Microchannel X-ray Telescope (MXT) and Visual Telescope (VT). ECLAIRs and GRM can detect gamma-ray transient sources in real-time with localisation capabilities for ECLAIRs. SVOM can transfer the alerts in near real-time with a typical latency of less than 30s and perform autonomous slew to allow x-ray and optical follow-up of the source with the smaller field of view instruments: MXT and VT. +The SVOM spacecraft carries four multi-wavelength instruments: ECLAIRs, Gamma Ray burst Monitor (GRM), Microchannel X-ray Telescope (MXT) and Visual Telescope (VT). ECLAIRs and GRM can detect gamma-ray transient sources in real-time with localization capabilities for ECLAIRs. SVOM can transfer the alerts in near real-time with a typical latency of less than 30s and perform autonomous slew to allow x-ray and optical follow-up of the source with the smaller field of view instruments: MXT and VT.
@@ -63,11 +63,11 @@ Each of the four instruments has its own dedicated topic to stream notices with | Notice Type | Content | Latency | | ------------------------------------------ | -------------------------------------------------------------------- | ------------- | | `grm-trigger` | GRM trigger notice with possible rough localization | ~15 sec | -| `eclairs-wakeup` | ECLAIRs localisation of a GRB candidate | ~15 sec | -| `eclairs-catalog` | ECLAIRs localisation of a flaring source from the on-board catalogue | ~15 sec | +| `eclairs-wakeup` | ECLAIRs localization of a GRB candidate | ~15 sec | +| `eclairs-catalog` | ECLAIRs localization of a flaring source from the on-board catalogue | ~15 sec | | `slewing` /
`not-slewing` 1 | Platform slew status and target coordinates | ~1-8 min | -| 
`mxt-initial_qf#`2
| MXT localisation of a found counterpart (only if platform slews) | ~3 min | -| 
`mxt-update_qf#`2
| MXT updated localisation (qf > mxt-initial_qf) | ~3 min | +| 
`mxt-initial_qf#`2
| MXT localization of a found counterpart (only if platform slews) | ~3 min | +| 
`mxt-update_qf#`2
| MXT updated localization (qf > mxt-initial_qf) | ~3 min |
@@ -76,7 +76,7 @@ the slew threshold (in a maximum time window of 8 min) or if the slew was not possible. The reason is specified in the notice parameters. 2 the value of the quality factor `qf` indicates the accuracy -of the localisation: +of the localization: - `qf1`→ 120'' < R90 < 300''
- `qf2`→ 60'' < R90 < 120''
- `qf3`→ 30'' < R90 < 60''