Resumen
We study 87 extremely red objects (EROs), selected both to have color redder than R - [3.6] = 4.0 and to have confirmed spectroscopic redshifts. Together, these two constraints result in this sample populating a fairly narrow redshift range at 0.76 < z < 1.42. The key new ingredient included here is deep Spitzer Space Telescope Infrared Array Camera (IRAC) data. Based on [3.6] - [8.0] color, we demonstrate that it is possible to classify EROs as early-type galaxies, dusty starburst galaxies, or active galactic nuclei (AGNs; power-law types). We present ultraviolet-to-mid-infrared spectral energy distributions (SEDs) and Advanced Camera for Surveys (ACS) images, both of which support our simple IRAC color classification.
| Idioma original | English |
|---|---|
| Páginas (desde-hasta) | L59-L63 |
| Publicación | Astrophysical Journal |
| Volumen | 660 |
| N.º | 1 II |
| DOI | |
| Estado | Published - may 1 2007 |
ASJC Scopus subject areas
- Astronomy and Astrophysics
- Space and Planetary Science
Huella
Profundice en los temas de investigación de 'AEGIS: A panchromatic study of IRAC-selected extremely red objects with confirmed spectroscopic redshifts'. En conjunto forman una huella única.Citar esto
- APA
- Author
- BIBTEX
- Harvard
- Standard
- RIS
- Vancouver