Discussion Overview
The discussion revolves around the differences between 1D and 2D spectra, particularly in the context of astronomical data obtained from spectrographs. Participants explore definitions, processing methods, and software tools related to these spectra.
Discussion Character
- Technical explanation
- Meta-discussion
Main Points Raised
- One participant inquires about the definitions of 1D and 2D spectra, indicating a lack of clear information in available documents.
- Another participant explains that 2D spectra are generated on a CCD after exposure, where the object being observed typically spans multiple pixels. They describe the process of converting a 2D spectrum into a 1D spectrum by summing pixel counts.
- Several participants share links to documents for further reading, although access issues arise with one of the links, prompting alternative suggestions.
- There is a discussion about the software needed to read PostScript files, with participants suggesting programs like Ghostview and Ghostscript, and discussing file compression formats.
- One participant mentions the complexity of processing Echelle spectra, which can show multiple orders of the same spectrum, and also refers to multi-object spectrographs that capture spectra from various objects simultaneously.
- Questions arise regarding the installation and usage of Ghostview on Unix systems, with participants providing commands and troubleshooting tips.
Areas of Agreement / Disagreement
Participants generally agree on the basic definitions and processes related to 1D and 2D spectra, but there are unresolved questions regarding software usage and installation on Unix systems. The discussion includes multiple perspectives on the complexity of different types of 2D spectra.
Contextual Notes
Some participants express uncertainty about accessing specific file types and the software required to view them. There are also mentions of varying experiences with different software packages, indicating a lack of consensus on the best tools for processing spectra.
Who May Find This Useful
This discussion may be useful for individuals interested in astronomical data analysis, particularly those working with spectrographs and seeking to understand the differences between 1D and 2D spectra.