diff --git a/surveycodex/data/Roman_WFI.yaml b/surveycodex/data/Roman_WFI.yaml new file mode 100644 index 0000000..6b2ea41 --- /dev/null +++ b/surveycodex/data/Roman_WFI.yaml @@ -0,0 +1,60 @@ +name: "Roman_WFI" +description: "Roman High-Latitude Wide-Area Survey (HLWAS) medium tier done with the Nancy Grace Roman Space Telescope and the Wide Field Instrument (WFI)" +pixel_scale: 0.11 +gain: 1.67 +mirror_diameter: 2.4 +obscuration: 0.20252763 +zeropoint_airmass: 0.0 +filters: + F106: + name: "F106" + sky_brightness: 22.92 + full_exposure_time: 642 + zeropoint: 26.32 + psf_fwhm: 0.087 + effective_wavelength: 1073.633 + F129: + name: "F129" + sky_brightness: 22.96 + full_exposure_time: 642 + zeropoint: 26.32 + psf_fwhm: 0.106 + effective_wavelength: 1296.861 + F158: + name: "F158" + sky_brightness: 23.06 + full_exposure_time: 642 + zeropoint: 26.32 + psf_fwhm: 0.128 + effective_wavelength: 1596.115 +references: + pixel_scale: + link: "https://github.com/RomanSpaceTelescope/roman-technical-information/blob/main/roman_technical_information/data/WideFieldInstrument/WFI_overview.yaml" + comment: "focal_plane_array.spatial_sampling" + gain: + link: "https://roman-docs.stsci.edu/simulation-tools/roman-wfi-exposure-time-calculator/etc-appendix-inputs-and-calculations" + comment: "IPC-corrected gain, i.e. the typical 1.8 e-/DN divided by the GSFC IPC correction factor of 1.08" + mirror_diameter: + link: "https://github.com/RomanSpaceTelescope/roman-technical-information/blob/main/roman_technical_information/data/Observatory/MissionandObservatoryTechnicalOverview/MissionandObservatory.yaml" + comment: "Telescope_Parameters.primary_mirror_diameter – the aperture stop effective diameter is 2.36 m" + obscuration: + link: "https://roman-docs.stsci.edu/simulation-tools/roman-wfi-exposure-time-calculator/etc-appendix-inputs-and-calculations" + comment: "Using the collecting area coll_area = 36076.8 cm^2, the obscuration is 1-36076.8/(pi*240*240/4)" + zeropoint_airmass: + link: "" + comment: "Space telescope" + sky_brightness: + link: "https://github.com/RomanSpaceTelescope/roman-technical-information/blob/main/roman_technical_information/data/WideFieldInstrument/Imaging/ZodiacalLight/zodiacal_light.ecsv" + comment: "Minimum zodiacal light count rate per pixel converted with the filter zeropoint and the pixel scale – internal thermal background excluded" + full_exposure_time: + link: "https://roman-docs.stsci.edu/roman-community-defined-surveys/high-latitude-wide-area-survey" + comment: "HLWAS medium tier: 107 s per dither, 3 dithers, 2 passes" + zeropoint: + link: "https://github.com/RomanSpaceTelescope/roman-technical-information/blob/main/roman_technical_information/data/WideFieldInstrument/Imaging/ZeroPoints/Roman_zeropoints_20240301.ecsv" + comment: "ABMag zeropoint of detector WFI01 (SCA1), from the effective area curves of 2024-03-01" + psf_fwhm: + link: "https://github.com/RomanSpaceTelescope/roman-technical-information/blob/main/roman_technical_information/data/WideFieldInstrument/Imaging/FiltersSummary/filter_parameters.ecsv" + comment: "Simulated on SCA1 near the centre of the WFI field of view with a K0V input spectrum" + effective_wavelength: + link: "https://github.com/RomanSpaceTelescope/roman-technical-information/blob/main/roman_technical_information/data/WideFieldInstrument/Imaging/EffectiveAreas/Roman_effarea_v8_SCA01_20240301.ecsv" + comment: "Photon-weighted mean wavelength of the SCA1 effective area curve, following the speclite convention" diff --git a/surveycodex/data/Roman_WFI_Deep.yaml b/surveycodex/data/Roman_WFI_Deep.yaml new file mode 100644 index 0000000..97dade3 --- /dev/null +++ b/surveycodex/data/Roman_WFI_Deep.yaml @@ -0,0 +1,88 @@ +name: "Roman_WFI_Deep" +description: "Roman High-Latitude Wide-Area Survey (HLWAS) deep tier done with the Nancy Grace Roman Space Telescope and the Wide Field Instrument (WFI)" +pixel_scale: 0.11 +gain: 1.67 +mirror_diameter: 2.4 +obscuration: 0.20252763 +zeropoint_airmass: 0.0 +filters: + F087: + name: "F087" + sky_brightness: 22.93 + full_exposure_time: 4410 + zeropoint: 26.23 + psf_fwhm: 0.073 + effective_wavelength: 881.180 + F106: + name: "F106" + sky_brightness: 22.92 + full_exposure_time: 4410 + zeropoint: 26.32 + psf_fwhm: 0.087 + effective_wavelength: 1073.633 + F129: + name: "F129" + sky_brightness: 22.96 + full_exposure_time: 4410 + zeropoint: 26.32 + psf_fwhm: 0.106 + effective_wavelength: 1296.861 + F146: + name: "F146" + sky_brightness: 23.01 + full_exposure_time: 5292 + zeropoint: 27.54 + psf_fwhm: 0.105 + effective_wavelength: 1536.573 + F158: + name: "F158" + sky_brightness: 23.06 + full_exposure_time: 4410 + zeropoint: 26.32 + psf_fwhm: 0.128 + effective_wavelength: 1596.115 + F184: + name: "F184" + sky_brightness: 23.19 + full_exposure_time: 4410 + zeropoint: 25.85 + psf_fwhm: 0.146 + effective_wavelength: 1850.203 + F213: + name: "F213" + sky_brightness: 23.34 + full_exposure_time: 4410 + zeropoint: 25.81 + psf_fwhm: 0.169 + effective_wavelength: 2144.099 +references: + pixel_scale: + link: "https://github.com/RomanSpaceTelescope/roman-technical-information/blob/main/roman_technical_information/data/WideFieldInstrument/WFI_overview.yaml" + comment: "focal_plane_array.spatial_sampling" + gain: + link: "https://roman-docs.stsci.edu/simulation-tools/roman-wfi-exposure-time-calculator/etc-appendix-inputs-and-calculations" + comment: "IPC-corrected gain, i.e. the typical 1.8 e-/DN divided by the GSFC IPC correction factor of 1.08" + mirror_diameter: + link: "https://github.com/RomanSpaceTelescope/roman-technical-information/blob/main/roman_technical_information/data/Observatory/MissionandObservatoryTechnicalOverview/MissionandObservatory.yaml" + comment: "Telescope_Parameters.primary_mirror_diameter – the aperture stop effective diameter is 2.36 m" + obscuration: + link: "https://roman-docs.stsci.edu/simulation-tools/roman-wfi-exposure-time-calculator/etc-appendix-inputs-and-calculations" + comment: "Using the collecting area coll_area = 36076.8 cm^2, the obscuration is 1-36076.8/(pi*240*240/4)" + zeropoint_airmass: + link: "" + comment: "Space telescope" + sky_brightness: + link: "https://github.com/RomanSpaceTelescope/roman-technical-information/blob/main/roman_technical_information/data/WideFieldInstrument/Imaging/ZodiacalLight/zodiacal_light.ecsv" + comment: "Minimum zodiacal light count rate per pixel converted with the filter zeropoint and the pixel scale – internal thermal background excluded" + full_exposure_time: + link: "https://roman-docs.stsci.edu/roman-community-defined-surveys/high-latitude-wide-area-survey" + comment: "HLWAS deep tier: 294 s per dither, 3 dithers, 5 passes (6 passes for F146) – see 'Details of Deep Tier Observations'" + zeropoint: + link: "https://github.com/RomanSpaceTelescope/roman-technical-information/blob/main/roman_technical_information/data/WideFieldInstrument/Imaging/ZeroPoints/Roman_zeropoints_20240301.ecsv" + comment: "ABMag zeropoint of detector WFI01 (SCA1), from the effective area curves of 2024-03-01" + psf_fwhm: + link: "https://github.com/RomanSpaceTelescope/roman-technical-information/blob/main/roman_technical_information/data/WideFieldInstrument/Imaging/FiltersSummary/filter_parameters.ecsv" + comment: "Simulated on SCA1 near the centre of the WFI field of view with a K0V input spectrum" + effective_wavelength: + link: "https://github.com/RomanSpaceTelescope/roman-technical-information/blob/main/roman_technical_information/data/WideFieldInstrument/Imaging/EffectiveAreas/Roman_effarea_v8_SCA01_20240301.ecsv" + comment: "Photon-weighted mean wavelength of the SCA1 effective area curve, following the speclite convention" diff --git a/surveycodex/rich.py b/surveycodex/rich.py index 2da6d96..0f0d4dc 100644 --- a/surveycodex/rich.py +++ b/surveycodex/rich.py @@ -7,7 +7,7 @@ def _rich_survey_name(survey): - if survey.name in ["Euclid_VIS", "COSMOS"]: + if survey.name in ["Euclid_VIS", "COSMOS", "Roman_WFI", "Roman_WFI_Deep"]: icon = _SATELLITE else: icon = _TELESCOPE