1,723 research outputs found

    Star Formation Rate Distributions: Inadequacy of the Schechter Function

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    In this paper we posit that galaxy luminosity functions (LFs) come in two fundamentally different types depending on whether the luminosity traces galaxy stellar mass or its current star formation rate (SFR). Mass function types reflect the older stars and therefore the stellar mass distribution, while SFR function types arise from the young stars and hence the distribution of SFRs. Optical and near-infrared LFs are of the mass function type, and are well fit by a Schechter function (power law with an exponential cutoff at the bright end). In contrast, LFs of the SFR function type are of a different form, one that cannot be adequately described by a Schechter function. We demonstrate this difference by generating SFR distributions for mock samples of galaxies drawn from a Schechter stellar mass distribution along with established empirical relations between the SFR and stellar mass. Compared with the Schechter function, SFR distributions have a shallower decline at the bright end, which can be traced to the large intrinsic scatter of SFRs at any given stellar mass. A superior description of SFR distributions is given by the "Saunders" function, which combines a power law with a Gaussian at the high end. We show that the Schechter-like appearance of UV and H alpha LFs, although they are LFs of SFR function type, results when luminosities are not corrected for dust, or when average statistical corrections are used because individual attenuation measurements are not available. We thus infer that the non-Schechter form of the far-IR LFs is a true reflection of the underlying SFR distribution, rather than the purported artifact of AGN contamination.Comment: Revised after a referee report. Submitted to ApJ. Compatible with B/W printers. Comments are welcom

    Dust Attenuation Curves in the Local Universe: Demographics and New Laws for Star-forming Galaxies and High-redshift Analogs

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    We study dust attenuation curves of 230,000 individual galaxies in the local universe, ranging from quiescent to intensely star-forming systems, using GALEX, SDSS, and WISE photometry calibrated on Herschel-ATLAS. We use a new method of constraining SED fits with infrared luminosity (SED+LIR fitting), and parameterized attenuation curves determined with the CIGALE SED fitting code. Attenuation curve slopes and UV bump strengths are reasonably well constrained independently from one another. We find that Aλ/AVA_{\lambda}/A_V attenuation curves exhibit a very wide range of slopes that are on average as steep as the SMC curve slope. The slope is a strong function of optical opacity. Opaque galaxies have shallower curves - in agreement with recent radiate transfer models. The dependence of slopes on the opacity produces an apparent dependence on stellar mass: more massive galaxies having shallower slopes. Attenuation curves exhibit a wide range of UV bump amplitudes, from none to MW-like; with an average strength 1/3 of the MW bump. Notably, local analogs of high-redshift galaxies have an average curve that is somewhat steeper than the SMC curve, with a modest UV bump that can be to first order ignored, as its effect on the near-UV magnitude is 0.1 mag. Neither the slopes nor the strengths of the UV bump depend on gas-phase metallicity. Functional forms for attenuation laws are presented for normal star-forming galaxies, high-z analogs and quiescent galaxies. We release the catalog of associated SFRs and stellar masses (GSWLC-2).Comment: Accepted to ApJ. GSWLC-2 catalog of SED+LIR SFRs and M* to be released Jun 1 at http://pages.iu.edu/~salims/gswlc

    Uncomfortable Comfort Women: Examining shame culture and the internal conflict between Japanese-Americans and Korean-Americans regarding the comfort women issue

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    Women\u27s rights are human rights that should be emphasized across the globe. The sexual slavery system that the Japanese Imperial army put in place during World War II, commonly known as \u27comfort women,\u27 is now getting international attention. 50 years after the war ended, survivors and former \u27comfort women\u27 are now raising their voice and telling their stories. This research paper focuses on the issue of shame culture and how it drives the internal conflict between Japanese-Americans and Korean-Americans today and how this long conflict effects generations today

    On the Mass-Metallicity-Star Formation Rate Relation for Galaxies at z∌2z\sim 2

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    Recent studies have shown that the local mass-metallicity (M-Z) relation depends on the specific star formation rate (SSFR). Whether such a dependence exists at higher redshifts, and whether the resulting M-Z-SFR relation is redshift invariant, is debated. We re-examine these issues by applying the non-parametric techniques of Salim et al. (2014) to ~130 z∌2.3z\sim2.3 galaxies with N2 and O3 measurements from KBSS (Steidel et al. 2014). We find that the KBSS M-Z relation depends on SSFR at intermediate masses, where such dependence exists locally. KBSS and SDSS galaxies of the same mass and SSFR ("local analogs") are similarly offset in the BPT diagram relative to the bulk of local star-forming galaxies, and thus we posit that metallicities can be compared self-consistently at different redshifts as long as the masses and SSFRs of the galaxies are similar. We find that the M-Z-SFR relation of z∌2z\sim2 galaxies is consistent with the local one at log⁥M∗<10\log M_*<10, but is offset up to -0.25 dex at higher masses, so it is altogether not redshift invariant. This high-mass offset could arise from a bias that high-redshift spectroscopic surveys have against high-metallicity galaxies, but additional evidence disfavors this possibility. We identify three causes for the reported discrepancy between N2 and O3N2 metallicities at z∌2z\sim2: (1) a smaller offset that is also present for SDSS galaxies, which we remove with new N2 calibration, (2) a genuine offset due to differing ISM condition, which is also present in local analogs, (3) an additional offset due to unrecognized AGN contamination.Comment: ApJ accepted. 14 pages. Comments welcom

    An analysis of the implementation of the Indian Studies Law of 1973.

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    Examining the Relationship Between Preschool Teachers’ Use of Social and Emotional Teaching Strategies and Children’s Challenging Behavior and Social Skills

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    Because there are immediate and long-term implications when preschool children exhibit challenging behavior in the classroom, it is crucial to prevent and address challenging behavior as early as possible. Social and emotional teaching strategies have been shown to reduce challenging behavior of preschoolers and increase social and emotional skills. The purpose of this quantitative study was to examine if social and emotional teaching strategies correlated with changes in the challenging behavior and social skills of preschoolers with persistent challenging behavior. Data were obtained from an archival data set of a randomized controlled trial (RCT) efficacy study of an intervention for preschoolers with persistent challenging behavior. The data set included baseline measures of teaching practices in classrooms as measured by the Teaching Pyramid Observation Tool (TPOT) and changes in preschooler’s challenging behavior and social skills using the Social Skills Improvement System (SSIS) collected at pre- and post-test of study participation (spanning 4 months). Pearson correlations of the teaching practices and children’s change scores for challenging behavior and social skills were analyzed for possible statistical significance. Results showed that teaching behavior expectations and teaching problem solving were associated with statistically significant reductions in preschoolers’ challenging behavior for children who participated in the intervention group of the original RCT. No statistically significant relationships were identified for teaching social and emotional competencies, friendship skills, or expressing emotions. Implications for persistent challenging behavior in preschool classrooms are discussed
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