Daniel Reverte

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Beef trimmings from cattle finished on forage or grain were restructured into steaks to enhance palatability. Steaks were treated with propyl gallate with or without a beefy flavoring agent, stored at -29 °C, and analyzed after 0, 1, 3, and 6 months. The strong grassy flavor of forage-finished beef steaks, detected by a sensory panel, was masked by the(More)
We report optical and near-infrared broad band observations of the short-duration GRB 050724 host galaxy, used to construct its spectral energy distribution (SED). Unlike the hosts of long-duration gamma-ray bursts (GRBs), which show younger stellar population, the SED of the GRB 050724 host galaxy is optimally fitted with a synthetic elliptical galaxy(More)
We report on the detection of two Hα-emitting extreme compact objects from deep images of the Abell 634 and Abell 539 clusters of galaxies at z ∼ 0.03. Follow up long slit spectroscopy of these two unresolved sources revealed that they are members of their respective clusters showing Hii type spectra. The luminosity and the extreme equivalent width of(More)
This paper presents the first results of an Hα imaging survey of galaxies in the central regions of the A2151 cluster. A total of 50 sources were detected in Hα, from which 41 were classified as secure members of the cluster and 2 as likely members based on spectroscopic and photometric redshift considerations. The remaining 7 galaxies were classified as(More)
We present multiwavelength observations of a gamma-ray burst detected by INTEGRAL (GRB 030227) between 5.3 hours and∼ 1.7 days after the event. Here we report the discovery of a dim optical afterglow (OA) that would not have been detected by many previous searches due to its faintess (R∼ 23). This OA was seen to decline following a power law decay with(More)
We present multiwavelength observations of a gamma-ray burst detected by INTEGRAL (GRB 030227) between 5.3 hours and ∼1.7 days after the event. Here we report the discovery of a dim optical afterglow (OA) that would not have been detected by many previous searches due to its faintess (R ∼ 23). This OA was seen to decline following a power law decay with(More)
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