diff --git a/scripts/check_effective_wavelengths.py b/scripts/check_effective_wavelengths.py
index 9ada30b..ec943a3 100644
--- a/scripts/check_effective_wavelengths.py
+++ b/scripts/check_effective_wavelengths.py
@@ -6,10 +6,13 @@
 SPECLITE_SURVEY_PREFIXES = {
     "DES": "decam2014",
     "Euclid_VIS": "Euclid",
+    "Euclid_NISP": "Euclid",
     "HSC": "hsc2017",
     "LSST": "lsst2016",
 }
 
+EUCLID_FILTER_NAMES = {"IE": "VIS", "YE": "Y", "JE": "J", "HE": "H"}
+
 
 def check_effective_wavelengths(survey_name):
     """Compare current effective wavelengths with speclite
@@ -29,10 +32,7 @@ def check_effective_wavelengths(survey_name):
         print("------- | --------- | ---------")
 
         for filter_name in survey.available_filters:
-            if filter_name == "IE":
-                old_filter_name = "VIS"
-            else:
-                old_filter_name = filter_name
+            old_filter_name = EUCLID_FILTER_NAMES.get(filter_name, filter_name)
             speclite_filter_name = f"{speclite_prefix}-{old_filter_name}"
             speclite_filter = load_filter(speclite_filter_name)
             speclite_eff_wl = speclite_filter.effective_wavelength.to(u.nm)
diff --git a/scripts/check_zeropoints.py b/scripts/check_zeropoints.py
index a31c4a0..51f3f16 100644
--- a/scripts/check_zeropoints.py
+++ b/scripts/check_zeropoints.py
@@ -8,10 +8,13 @@
 SPECLITE_SURVEY_PREFIXES = {
     "DES": "decam2014",
     "Euclid_VIS": "Euclid",
+    "Euclid_NISP": "Euclid",
     "HSC": "hsc2017",
     "LSST": "lsst2016",
 }
 
+EUCLID_FILTER_NAMES = {"IE": "VIS", "YE": "Y", "JE": "J", "HE": "H"}
+
 
 def compute_zeropoint_mag(band_name, effective_area, exposure_time=1 * u.s):
     """Compute the zeropoint of a given filter with speclite"""
@@ -42,10 +45,7 @@ def check_zeropoints(survey_name):
         print("------- | --------- | ---------")
 
         for filter_name in survey.available_filters:
-            if filter_name == "IE":
-                old_filter_name = "VIS"
-            else:
-                old_filter_name = filter_name
+            old_filter_name = EUCLID_FILTER_NAMES.get(filter_name, filter_name)
             speclite_filter_name = f"{speclite_prefix}-{old_filter_name}"
             speclite_zp = compute_zeropoint_mag(
                 speclite_filter_name, survey.effective_area
diff --git a/surveycodex/data/Euclid_NISP.yaml b/surveycodex/data/Euclid_NISP.yaml
new file mode 100644
index 0000000..a9ed556
--- /dev/null
+++ b/surveycodex/data/Euclid_NISP.yaml
@@ -0,0 +1,60 @@
+name: "Euclid_NISP"
+description: "Euclid wide-field survey done with the Euclid space telescope and the near-infrared spectrometer and photometer (NISP), photometric channel"
+pixel_scale: 0.30
+gain: 2.0
+mirror_diameter: 1.2
+obscuration: 0.13
+zeropoint_airmass: 0.0
+filters:
+  YE:
+    name: "YE"
+    sky_brightness: 22.1
+    full_exposure_time: 112
+    zeropoint: 24.99
+    psf_fwhm: 0.477
+    effective_wavelength: 1089.014
+  JE:
+    name: "JE"
+    sky_brightness: 22.2
+    full_exposure_time: 112
+    zeropoint: 25.17
+    psf_fwhm: 0.486
+    effective_wavelength: 1379.127
+  HE:
+    name: "HE"
+    sky_brightness: 22.3
+    full_exposure_time: 112
+    zeropoint: 25.11
+    psf_fwhm: 0.492
+    effective_wavelength: 1785.975
+references:
+  pixel_scale:
+    link: "https://arxiv.org/abs/2108.01201"
+    comment: "Euclid preparation I. The Euclid Wide Survey (Scaramella et al. 2022), Sect. 3.2: NISP has a plate scale of 0.3 arcsec/pixel"
+  gain:
+    link: "https://arxiv.org/abs/2405.13496"
+    comment: "Euclid: ERO -- compact- and diffuse-emission photometry pipeline, Sect. 4.3.7: NISP's average gain is 2 electrons per ADU"
+  mirror_diameter:
+    link: "https://arxiv.org/abs/1608.08603"
+    comment: "(v1) See section 3.1 -- NISP shares the same 1.2 m Euclid telescope as VIS, split by a dichroic"
+  obscuration:
+    link: "https://arxiv.org/abs/1608.08603"
+    comment: "(v1) See section 3.1 -- same shared telescope as VIS"
+  zeropoint_airmass:
+    link: ""
+    comment: "Space telescope"
+  sky_brightness:
+    link: "https://arxiv.org/abs/2405.13496"
+    comment: "Euclid: ERO -- compact- and diffuse-emission photometry pipeline, Table 2: median in-flight sky background per band from the 17 ERO fields"
+  full_exposure_time:
+    link: "https://arxiv.org/abs/2108.01201"
+    comment: "Euclid preparation I. The Euclid Wide Survey (Scaramella et al. 2022), Sect. 4.1: each of the three NISP photometric images (Y, J, H) in the reference observing sequence lasts 112 s -- single-pointing exposure, matching the convention used for Euclid_VIS's full_exposure_time"
+  zeropoint:
+    link: "https://speclite.readthedocs.io/en/latest/filters.html"
+    comment: "computed with speclite – see scripts/check_zeropoints.py"
+  psf_fwhm:
+    link: "https://arxiv.org/abs/2405.13496"
+    comment: "Euclid: ERO -- compact- and diffuse-emission photometry pipeline, Table 2: median in-flight FWHM per band, measured on stacked ERO survey images"
+  effective_wavelength:
+    link: "https://speclite.readthedocs.io/en/latest/filters.html"
+    comment: "computed with speclite – see scripts/check_effective_wavelength.py"
diff --git a/surveycodex/rich.py b/surveycodex/rich.py
index 0f0d4dc..41795fd 100644
--- a/surveycodex/rich.py
+++ b/surveycodex/rich.py
@@ -7,7 +7,13 @@
 
 
 def _rich_survey_name(survey):
-    if survey.name in ["Euclid_VIS", "COSMOS", "Roman_WFI", "Roman_WFI_Deep"]:
+    if survey.name in [
+        "Euclid_VIS",
+        "Euclid_NISP",
+        "COSMOS",
+        "Roman_WFI",
+        "Roman_WFI_Deep",
+    ]:
         icon = _SATELLITE
     else:
         icon = _TELESCOPE