Tracing the mass-dependent star formation history of late-type galaxies using X-ray emission : results from the Chandra Deep Fields

Lehmer, B.D.; Brandt, W.N.; Alexander, D.M.; Bell, E.F.; Hornschemeier, A.E.; McIntosh, D.H.; Bauer, F.E.; Gilli, R.; Mainieri, V.; Schneider, D.P.; Silverman, J.D.; Steffen, A.T.; Tozzi, P.; Wolf, C.

Abstract

We report on the X-ray evolution over the last ~9 Gyr of cosmic history (i.e., since z=1.4) of late-type galaxy populations in the Chandra Deep Field-North and Extended Chandra Deep Field-South (CDF-N and E-CDF-S, respectively; jointly CDFs) survey fields. Our late-type galaxy sample consists of 2568 galaxies, which were identified using rest-frame optical colors and HST morphologies. We utilized X-ray stacking analyses to investigate the X-ray emission from these galaxies, emphasizing the contributions from normal galaxies that are not dominated by active galactic nuclei (AGNs). Over this redshift range, we find significant increases (factors of ~5-10) in the X-ray-to-optical mean luminosity ratio (LX/LB) and the X-ray-to-stellar mass mean ratio (LX/M*) for galaxy populations selected by LB and M*, respectively. When analyzing galaxy samples selected via SFR, we find that the mean X-ray-to-SFR ratio (LX/SFR) is consistent with being constant over the entire redshift range for galaxies with SFR = 1-100 Msolar yr-1, thus demonstrating that X-ray emission can be used as a robust indicator of star formation activity out to z~1.4. We find that the star formation activity (as traced by X-ray luminosity) per unit stellar mass in a given redshift bin increases with decreasing stellar mass over the redshift range z = 0.2-1, which is consistent with previous studies of how star formation activity depends on stellar mass. Finally, we extend our X-ray analyses to Lyman break galaxies at z~3 and estimate that LX/LB at z~3 is similar to its value at z=1.4.

Citation

Lehmer, B., Brandt, W., Alexander, D., Bell, E., Hornschemeier, A., McIntosh, D., …Wolf, C. (2008). Tracing the mass-dependent star formation history of late-type galaxies using X-ray emission : results from the Chandra Deep Fields. Astrophysical Journal, 681(2), 1163-1182. https://doi.org/10.1086/588459

• Journal Article Type: Article
• Publication Date: Jul 1, 2008
• Deposit Date: Apr 8, 2013
• Publicly Available Date: Sep 5, 2013
• Journal: Astrophysical Journal
• Print ISSN: 0004-637X
• Electronic ISSN: 1538-4357
• Publisher: American Astronomical Society
• Peer Reviewed: Peer Reviewed
• Volume: 681
• Issue: 2
• Pages: 1163-1182
• DOI: https://doi.org/10.1086/588459
• Keywords: Cosmology, Observations, Galaxies, Active, Spiral, Stars, Formation, Surveys, X-rays.
• Public URL: https://durham-repository.worktribe.com/output/1478972