4 research outputs found

    Floppy aortic graft reconstruction for germ cell tumor invasion of the infrarenal aorta

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    AbstractSignificant aortic invasion by metastatic nonseminomatous germ cell tumors can present difficult problems intraoperatively in attempted curative retroperitoneal lymph node dissection. Aortic replacement with Dacron graft has been a successful method of dealing with this predicament. We describe a new approach of intraoperative floppy aortic graft reconstruction in a young patient with testicular germ cell cancer in whom a 14 cm pseudoaneurysm involving the infrarenal aorta developed after four courses of preoperative chemotherapy. This technique prevents significant lower extremity and pelvic ischemia during resection of the aorta and retroperitoneal tumor while providing the urologic surgeon with excellent exposure and minimal interference from the aortic graft. (J Vasc Surg 2003;37:889-91.

    UBVRI Light Curves of 44 Type Ia Supernovae

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    We present UBVRI photometry of 44 type-Ia supernovae (SN Ia) observed from 1997 to 2001 as part of a continuing monitoring campaign at the Fred Lawrence Whipple Observatory of the Harvard-Smithsonian Center for Astrophysics. The data set comprises 2190 observations and is the largest homogeneously observed and reduced sample of SN Ia to date, nearly doubling the number of well-observed, nearby SN Ia with published multicolor CCD light curves. The large sample of U-band photometry is a unique addition, with important connections to SN Ia observed at high redshift. The decline rate of SN Ia U-band light curves correlates well with the decline rate in other bands, as does the U-B color at maximum light. However, the U-band peak magnitudes show an increased dispersion relative to other bands even after accounting for extinction and decline rate, amounting to an additional ~40% intrinsic scatter compared to B-band.Comment: 84 authors, 71 pages, 51 tables, 10 figures. Accepted for publication in the Astronomical Journal. Version with high-res figures and electronic data at http://astron.berkeley.edu/~saurabh/cfa2snIa
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