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Advanced Spectroscopy Observations with NIRSpec and MIRI Across Multiple Wavelengths

This project focuses on high-resolution spectroscopy utilizing the NIRSpec and MIRI instruments across a range of wavelengths from 0.6 to 28 micrometers. We explore detailed spectral analysis with resolutions from R~30 to R~3500. The observations include multiple visits to ensure robust data collection, employing filters such as F322W2 and F444W. This comprehensive study aims to investigate various celestial phenomena, offering insights into the chemical compositions and physical conditions of distant astronomical objects.

tara-nelson
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Advanced Spectroscopy Observations with NIRSpec and MIRI Across Multiple Wavelengths

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  1. NIRSpec R~500-1300, or ~1500-3500 R~700-1300, or ~2000-3500 R~700-1300 or ~2000-3500 R~30-100 0.6um 1um 2um 3um 4um 5um R~150 NIRCam NIRISS R~430-1350, SOSS R~1700 (F322W2) R~1700 (F444W) LRS, R~100 R>1600, 3 visits R>800, 3 visits R>2400, 3 visits MIRI 5um 10um 15um 20um 25um 28um

  2. R~500-1300, or ~1500-3500 R~700-1300, or ~2000-3500 R~700-1300 or ~2000-3500 NIRSpec R~30-100 0.6um 1um 2um 3um 4um 5um R~150 NIRISS R~430-1350, SOSS NIRCam R~1700 (F444W) R~1700 (F322W2) LRS, R~100 R>2400, 3 visits R>1600, 3 visits R>800, 3 visits MIRI 5um 10um 15um 20um 25um 28um

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