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Alveolar Soft Part Sarcoma

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Author Manuscript Published OnlineFirst on July 17, 2018; DOI: 10.1158/2326-6066.CIR-18-0037<br />

Author manuscripts have been peer reviewed and accepted for publication but have not yet been edited.<br />

To determine if the sustained response of ASPS patients to immunotherapy could be<br />

attributed to a high mutational load, exomic mutation burden was calculated. As<br />

expected for tumors lacking a matched-­‐‐normal control, approximately 60 germline<br />

variants per exome were detected. Tumor mutation burden was calculated from all<br />

exonic mutations with a variant allele fraction >0.1 called from a minimum coverage<br />

of 30X in the tumor. In order to control for the lack of a matched normal, we<br />

performed the same tumor-­‐‐only analysis on the fusion driven Ewing sarcoma. We<br />

additionally performed the analysis with a matched normal for Ewing sarcoma and<br />

synovial sarcoma (defined by SS18-­‐‐SSX fusion). In cases where whole exome<br />

sequencing was conducted, no excess mutation burden in ASPS was identified when<br />

compared to tumor-­‐‐only Ewing sarcoma. When analyzed with a matched normal,<br />

both Ewing and synovial sarcoma had low mutation burdens (Supplementary Fig.<br />

S1). This data suggests that ASPS mutation burden is similar to other fusion-­‐‐driven<br />

sarcomas.<br />

Mutational signature analysis<br />

Mutational signatures via COSMIC were identified in the mismatch repair (MMR)<br />

deficiency pathway in 5 of 7 cases (Patient 1: S6, S15; Patient 2: S26; Patient 3: S6,<br />

S26; Patient 4: S6, S26; Patient 5: S6, S26) of which 2 of had partial responses to<br />

immunotherapy (Patients 1 and 2; Fig. 3). The other patients were not treated with<br />

immunotherapy. Patient 1 also underwent whole genome sequencing, which<br />

confirmed a COSMIC signature in the MMR deficiency pathway.<br />

Downloaded from cancerimmunolres.aacrjournals.org on July 19, 2018. © 2018 American Association for Cancer Research.

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