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The Hubble Arp Galaxy Survey

  • Authors: Julianne J. Dalcanton, Meredith J. Durbin, Benjamin F. Williams

Julianne J. Dalcanton et al 2026 The Astrophysical Journal Supplement Series 283 .

  • Provider: AAS Journals

Caption: Figure 23.

(a) Thumbnails of systems containing at least one galaxy with strong, red, central WISE W3+W4 point-source emission. All have detectable VLASS emission aligned with the WISE source if observed (δ > −40°), with the exception of Arp 82, AM1421-282, and AM2350-302, which were observed but had no visible radio emission in VLASS. Systems shown are ARP15; ARP18; ARP49; ARP72; ARP82; ARP86; ARP91; ARP97; ARP107; ARP126; ARP143; ARP144; ARP145; ARP158; ARP163; ARP195; ARP200; ARP204; ARP205; ARP216; ARP219; ARP221; ARP241; ARP245; ARP248; ARP251; ARP255; ARP278; ARP283; ARP293; ARP300; ARP301; ARP314; ARP321; ARP322; AM0018-485. (b) Thumbnails of systems containing at least one galaxy with strong, red, central WISE W3+W4 point-source emission. All have detectable VLASS emission aligned with the WISE source if observed (δ > −40°), with the exception of Arp 82, AM1421-282, and AM2350-302, which were observed but had no visible radio emission in VLASS. Systems shown are AM0135-650; AM0223-403; AM0313-545; AM0052-321; AM0459-340; AM0558-335; AM0642-801; AM0658-590; AM1214-255; AM1229-512; AM1255-430; AM1421-282; AM1440-241; AM1546-284; AM1957-471; AM2031-440; AM2038-382; AM2048-571; AM2105-332; AM2105-632; AM2159-320; AM2222-275; AM2258-595; AM2303-305; AM2339-661; AM2350-302; AM2350-410.

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