adsabs/AstroCLIMB huggingface dataset:
Paper: An Empirical Framework Characterizing the Metallicity and Star-formation History Dependence of X-Ray Binary Population Formation and Emission in Galaxies
Authors: Bret D. Lehmer, Erik B. Monson, Rafael T. Eufrasio, Amirnezam Amiri, Keith Doore, Antara Basu-Zych, Kristen Garofali, Lidia Oskinova, Jeff J. Andrews, Vallia Antoniou, Robel Geda, Jenny E. Greene, Konstantinos Kovlakas, Margaret Lazzarini, Chris T. Richardson
Figure caption: (a) SFR vs. M ⋆ for the galaxy sample used in our study with 1σ uncertainties shown. Different symbol types correspond to sources with metallicity measurements based on strong-line calibrations (black-filled circles), direct-method calibration (filled green stars), and the M ⋆–Z relation (open orange squares). The gray-shaded region represents the galaxy main sequence, as defined by J. Aird et al. (2019), and lines of constant sSFR have been overlaid for reference (red-dashed lines). Our galaxy sample spans a relatively broad range of SFHs, ranging from massive elliptical galaxies (sSFR ≲ 0.01 Gyr−1) to starburst galaxies (sSFR ≳ 1 Gyr−1). (b) Gas-phase metallicity, Z vs. M ⋆ for our sample galaxies. The M ⋆–Z relation from Table 2 of L. J. Kewley & S. L. Ellison (2008) and its 1σ scatter are displayed as a dotted curve and gray-shaded region, respectively.