Abstract (paraphrased)¶
Assuming the disk IMF is universal and simple, the authors adopt a single smooth analytic form and constrain its parameters with integral observables (star counts, luminosities). The form approaches a power law at both ends — low-mass () and high-mass () — joined smoothly, which they term the Smoothed Two-Power Law (STPL).
What progenax uses (PDF-verified 2026-07-11)¶
Eq. 1 (p. 2) — the STPL form.
which is exactly progenax’s
TaperedPowerLawPDF up to the slope convention: PMH11 write per unit (their Salpeter is ), progenax’salphais the linear-mass slope (), and PMH11’s taper exponent is the code’sbeta. This convention mapping is a formaldeviationsentry on the tapered_powerlaw model card.Historical attribution (p. 2). The functional form was first proposed by Paresce & De Marchi (2000) for globular-cluster present-day mass functions; PMH11 adopted and calibrated it as a disk IMF (with Hollenbach et al. 2005 an earlier STPL step). Maschberger (2013) lists it as his comparison Eq. 12 — the route by which progenax originally cited it.
Connections in progenax¶
progenax.imf.smooth.TaperedPowerLaw— implements Eq. 1 in the linear-mass convention.Maschberger (2013) — the house-default smooth IMF; the STPL is the closest sibling without a closed-form quantile (Newton ppf), which is why Maschberger remains the production default.
- Parravano, A., McKee, C. F., & Hollenbach, D. J. (2011). An Initial Mass Function for Individual Stars in Galactic Disks. I. Constraining the Shape of the Initial Mass Function. The Astrophysical Journal, 726, 27. 10.1088/0004-637X/726/1/27