A New Distance to The Antennae Galaxies (NGC 4038/39) Based on the Type Ia Supernova 2007sr
Francois Schweizer (1), Christopher R. Burns (1), Barry F. Madore (1),, Violet A. Mager (1), M.M. Phillips (2), Wendy L. Freedman (1), Luis Boldt, (2), Carlos Contreras (2), Gaston Folatelli (3), Sergio Gonzalez (2), Mario, Hamuy (3), Wojtek Krzeminski (2), Nidia I. Morrell (2)

TL;DR
This paper presents a new distance measurement to the Antennae Galaxies using Type Ia supernova observations, which aligns well with flow model estimates and challenges previous shorter distance estimates based on TRGB photometry.
Contribution
The study introduces a supernova-based distance estimate that refines previous measurements and addresses issues with TRGB-based distances, providing a more reliable value for the Antennae Galaxies.
Findings
Supernova-based distance: 22.3±2.8 Mpc.
Flow model distance: 22.5±2.8 Mpc.
TRGB distance revised to 20.0±1.6 Mpc.
Abstract
Traditionally, the distance to NGC 4038/39 has been derived from the systemic recession velocity, yielding about 20 Mpc for H_0 = 72 km/s/Mpc. Recently, this widely adopted distance has been challenged based on photometry of the presumed tip of the red giant branch (TRGB), which seems to yield a shorter distance of 13.3+-1.0 Mpc and, with it, nearly 1 mag lower luminosities and smaller radii for objects in this prototypical merger. Here we present a new distance estimate based on observations of the Type Ia supernova (SN) 2007sr in the southern tail, made at Las Campanas Observatory as part of the Carnegie Supernova Project. The resulting distance of D(SN Ia) = 22.3+-2.8 Mpc [(m-M)_0 = 31.74+-0.27 mag] is in good agreement with a refined distance estimate based on the recession velocity and the large-scale flow model developed by Tonry and collaborators, D(flow) = 22.5+-2.8 Mpc. We…
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