pith. sign in

arxiv: 0707.0467 · v1 · submitted 2007-07-03 · 🌌 astro-ph

Star Formation Rate Determinations

Daniela Calzetti (Dept of Astronomy , UMass) This is my paper
classification 🌌 astro-ph
keywords determinationsformationgalaxiesmid-infraredspitzerstarcapabilitiescombining
0
0 comments X
read the original abstract

I review determinations of star formation rates (SFR) from the ultraviolet to the infrared, in the context of their use for galaxies and galaxy surveys. The mid-infrared SFR indicators have garnered interest in recent years thanks to the Spitzer capabilities and the opportunities offered by the upcoming Herschel Space Telescope. I discuss what we have learned in the mid-infrared from studies of local galaxies combining Spitzer with HST and other data.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.

Forward citations

Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. First Results from the TNG50 Simulation: Galactic outflows driven by supernovae and black hole feedback

    astro-ph.GA 2019-02 unverdicted novelty 6.0

    TNG50 shows galactic outflow mass loading is non-monotonic with stellar mass, rising rapidly above 10^10.5 Msun due to black hole feedback, and produces fast multi-phase outflows with emergent collimation.

  2. Clumpy Disk, Interloper, or Merger? Nature of a Distant Galaxy Pair at 5 kpc Projected Separation

    astro-ph.GA 2026-06 conditional novelty 4.0

    Multi-band imaging and Keck spectroscopy identify a z=0.92 galaxy pair as a physical merger at ~5 kpc projected separation with merger-induced star formation.