More Like this

1. Neogene sloth assemblages ( M ammalia, P ilosa) of the C ocinetas B asin ( L a G uajira, C olombia): implications for the G reat A merican B iotic I nterchange

   https://doi.org/10.1111/pala.12244  

   Amson, Eli ; Carrillo, Juan D. ; Jaramillo, Carlos ; O'Regan, ed., Hannah ( June 2016 , Palaeontology)
2. Metabolic Oscillations in Co-Cultures of Hepatocytes and Mesenchymal Stem Cells: Effects of Seeding Arrangement and Culture Mixing: S EEDING A RRANGEMENT E FFECTS ON C o -C ULTURE S YSTEMS

   https://doi.org/10.1002/jcb.25962  

   Alzebdeh, Dalia Abdelrahim ; Matthew, Howard William ( September 2017 , Journal of Cellular Biochemistry)
3. The changes in plant and soil C pools and their C : N stoichiometry control grassland N retention under elevated N inputs

   https://doi.org/10.1002/eap.2517  

   Yang, Sen ; Liu, Weixing ; Guo, Lulu ; Wang, Chengzhang ; Deng, Meifeng ; Peng, Ziyang ; Liu, Lingli ( March 2022 , Ecological Applications)
4. Evaluating hydrological processes in the C ommunity A tmosphere M odel V ersion 5 ( C AM5) using stable isotope ratios of water

   https://doi.org/10.1002/2016MS000839  

   Nusbaumer, Jesse ; Wong, Tony E. ; Bardeen, Charles ; Noone, David ( April 2017 , Journal of Advances in Modeling Earth Systems)
5. The ALPINE-ALMA [C  ii ] survey: Investigation of 10 galaxies at z ∼ 4.5 with [O  ii ] and [C  ii ] line emission − ISM properties and [O  ii ]−SFR relation

   https://doi.org/10.1093/mnras/stac071  

   Vanderhoof, Brittany N. ; Faisst, A. L. ; Shen, L. ; Lemaux, B. C. ; Béthermin, M. ; Capak, P. L. ; Cassata, P. ; Le Fèvre, O. ; Schaerer, D. ; Silverman, J. ; et al ( January 2022 , Monthly Notices of the Royal Astronomical Society)

   We present 10 main-sequence ALPINE galaxies (log (M/M⊙) = 9.2−11.1 and ${\rm SFR}=23-190\, {\rm M_{\odot }\, yr^{-1}}$) at z ∼ 4.5 with optical [O ii] measurements from Keck/MOSFIRE spectroscopy and Subaru/MOIRCS narrow-band imaging. This is the largest such multiwavelength sample at these redshifts, combining various measurements in the ultraviolet, optical, and far-infrared including [C ii]158 $\mu$m line emission and dust continuum from ALMA and H α emission from Spitzer photometry. For the first time, this unique sample allows us to analyse the relation between [O ii] and total star-formation rate (SFR) and the interstellar medium (ISM) properties via [O ii]/[C ii] and [O ii]/H α luminosity ratios at z ∼ 4.5. The [O ii]−SFR relation at z ∼ 4.5 cannot be described using standard local descriptions, but is consistent with a metal-dependent relation assuming metallicities around $50{{\ \rm per\ cent}}$ solar. To explain the measured dust-corrected luminosity ratios of $\log (L_{\rm [OII]}/L_{\rm [CII]}) \sim 0.98^{+0.21}_{-0.22}$ and $\log (L_{\rm [OII]}/L_{\rm H\alpha }) \sim -0.22^{+0.13}_{-0.15}$ for our sample, ionization parameters log (U) < −2 and electron densities $\log (\rm n_e / {\rm [cm^{-3}]}) \sim 2.5-3$ are required. The former is consistent with galaxies at z ∼ 2−3, however lower than at z > 6. The latter may be slightly higher than expected given the galaxies’ specific SFR. The analysis of this pilot sample suggests that typical log (M/M⊙) > 9 galaxies at z ∼ 4.5 to have broadly similar ISM properties as their descendants at z ∼ 2 and suggest a strong evolution of ISM properties since the epoch of reionization at z > 6.

    

   more » « less