We present an interactive IDL program for viewing and analyzing astronomical spectra in the context of modern imaging surveys. SpecPro’s interactive design lets the user simultaneously view spectroscopic, photometric, and imaging data, allowing for rapid object classification and redshift determination. The spectroscopic redshift can be determined with automated cross-correlation against a variety of spectral templates or by manually overlaying common emission and absorption features on the 1-D and 2-D spectra. Stamp images and the spectral energy distribution (SED) of a source can be displayed with the interface, with the positions of prominent photometric features indicated on the SED plot. Results can easily be saved to file from within ...
This article describes a method for making a spectroscope from scrap materials, i.e. a fragment of c...
IDL (Interactive Data Language) is a commercial programming, plotting, and image display language, w...
SpecCal software for the spectral calibration of high-resolution spectrometers is presented in this ...
We present an interactive IDL program for viewing and analyzing astronomical spectra in the context ...
The goal of this project is to develop an attachment for cameras and telescopes which can easily and...
We present an exploration tool for very large spectrum data sets such as the SDSS (Sloan Digital Sky...
With the advancement of chirped-pulse techniques, broadband rotational spectra with a few tens to se...
Spectral data reduction is a crucial step, as so important as the acquisition process. Rigor shall b...
We examined several publicly available spectral analysis software packages looking for one with enou...
With the ever-growing popularity of integral field unit (IFU) spectroscopy, countless observations a...
spectrino is a spectra preparation software utility for the R language and environment for statistic...
We describe a new software package that may be used to determine stellar and atomic parameters by ma...
Spectral energy distributions (SEDs) are useful primary and complementary tools in the analysis of o...
In this activity students construct simple spectrometers and gain experience comparing and contrasti...
We present a convenient, all-in-one framework for the scientific analysis of fully reduced, (integra...
This article describes a method for making a spectroscope from scrap materials, i.e. a fragment of c...
IDL (Interactive Data Language) is a commercial programming, plotting, and image display language, w...
SpecCal software for the spectral calibration of high-resolution spectrometers is presented in this ...
We present an interactive IDL program for viewing and analyzing astronomical spectra in the context ...
The goal of this project is to develop an attachment for cameras and telescopes which can easily and...
We present an exploration tool for very large spectrum data sets such as the SDSS (Sloan Digital Sky...
With the advancement of chirped-pulse techniques, broadband rotational spectra with a few tens to se...
Spectral data reduction is a crucial step, as so important as the acquisition process. Rigor shall b...
We examined several publicly available spectral analysis software packages looking for one with enou...
With the ever-growing popularity of integral field unit (IFU) spectroscopy, countless observations a...
spectrino is a spectra preparation software utility for the R language and environment for statistic...
We describe a new software package that may be used to determine stellar and atomic parameters by ma...
Spectral energy distributions (SEDs) are useful primary and complementary tools in the analysis of o...
In this activity students construct simple spectrometers and gain experience comparing and contrasti...
We present a convenient, all-in-one framework for the scientific analysis of fully reduced, (integra...
This article describes a method for making a spectroscope from scrap materials, i.e. a fragment of c...
IDL (Interactive Data Language) is a commercial programming, plotting, and image display language, w...
SpecCal software for the spectral calibration of high-resolution spectrometers is presented in this ...