9 research outputs found
Observation of the TeV gamma-ray source MGRO J1908+06 with ARGO-YBJ
The extended gamma ray source MGRO J1908+06, discovered by the Milagro air
shower detector in 2007, has been observed for about 4 years by the ARGO-YBJ
experiment at TeV energies, with a statistical significance of 6.2 standard
deviations. The peak of the signal is found at a position consistent with the
pulsar PSR J1907+0602. Parametrizing the source shape with a two-dimensional
Gauss function we estimate an extension \sigma = 0.49 \pm 0.22 degrees,
consistent with a previous measurement by the Cherenkov Array H.E.S.S.. The
observed energy spectrum is dN/dE = 6.1 \pm 1.4 \times 10^-13 (E/4 TeV)^{-2.54
\pm 0.36} photons cm^-2 s^-1 TeV^-1, in the energy range 1-20 TeV. The measured
gamma ray flux is consistent with the results of the Milagro detector, but is
2-3 times larger than the flux previously derived by H.E.S.S. at energies of a
few TeV. The continuity of the Milagro and ARGO-YBJ observations and the stable
excess rate observed by ARGO-YBJ along 4 years of data taking support the
identification of MGRO J1908+06 as the steady powerful TeV pulsar wind nebula
of PSR J1907+0602, with an integrated luminosity above 1 TeV about 1.8 times
the Crab Nebula luminosity.Comment: 6 pages, accepted for pubblication by ApJ. Replaced to correct the
author lis
Long-term Monitoring on Mrk 501 for Its VHE gamma Emission and a Flare in October 2011
As one of the brightest active blazars in both X-ray and very high energy
-ray bands, Mrk 501 is very useful for physics associated with jets
from AGNs. The ARGO-YBJ experiment is monitoring it for -rays above 0.3
TeV since November 2007. Starting from October 2011 the largest flare since
2005 is observed, which lasts to about April 2012. In this paper, a detailed
analysis is reported. During the brightest -rays flaring episodes from
October 17 to November 22, 2011, an excess of the event rate over 6 is
detected by ARGO-YBJ in the direction of Mrk 501, corresponding to an increase
of the -ray flux above 1 TeV by a factor of 6.62.2 from its steady
emission. In particular, the -ray flux above 8 TeV is detected with a
significance better than 4 . Based on time-dependent synchrotron
self-Compton (SSC) processes, the broad-band energy spectrum is interpreted as
the emission from an electron energy distribution parameterized with a single
power-law function with an exponential cutoff at its high energy end. The
average spectral energy distribution for the steady emission is well described
by this simple one-zone SSC model. However, the detection of -rays
above 8 TeV during the flare challenges this model due to the hardness of the
spectra. Correlations between X-rays and -rays are also investigated.Comment: have been accepted for publication at Ap
Sequence and expression pattern of the Drosophila melanogaster mitochondrial porin gene: evidence of a conserved protein domain between fly and mouse
We have recently cloned a cDNA encoding mitochondrial porin in Drosophila melanogaster and shown its chromosomal localization (Messina et al., FEBS Lett. (1996) 384, 9-13). Such cDNA was used as a probe for screening a genomic library. We thus cloned and sequenced a 4494-bp genomic region which contained the whole gene for the mitochondrial porin or VDAC. It was found that this D. melanogaster porin gene contains five exons, numbered IA (115 bp), IB (123 bp), II (320 bp), III (228 bp) and IV (752 bp). The exons II, III and IV contain the protein coding sequence and the 3' untranslated sequence (3'-UTR). The first base in exon II precisely corresponds to the first base of the starting ATG codon. Exon IA corresponds to the 5'-UTR sequence reported in the published cDNA sequence. Exon IB corresponds to an alternative 5'-UTR sequence, demonstrated to be transcribed by 5'-RACE experiments. The exon-intron splicing borders and the length of the exon III perfectly match a homologous internal exon detected in the mouse genes. Such exon encodes a protein domain predicted by sequence transmembrane arrangement models to contain major hydrophilic loops and it is thus suspected to have a conserved distinct function. In situ hybridization experiments confirmed the localization of the genomic clone on the chromosome 2L at region 32B3-4. Together with genomic Southern blotting at various stringencies, the same experiment did not confirm the presence of a second genetic locus on D. melanogaster chromosomes. Northern blots demonstrated that the porin gene is a housekeeping one: three messages of approx. 1.2-1.6 kbp are transcribed in every fly developmental stage that was studied. They were shown to derive by an alternative usage of different promoters and polyadenylation sites
OBSERVATION OF TeV GAMMA RAYS FROM THE UNIDENTIFIED SOURCE HESS J1841â055 WITH THE ARGO-YBJ EXPERIMENT
We report the observation of a very high energy Îł -ray source whose position is coincident with HESS J1841â055.
This source has been observed for 4.5 years by the ARGO-YBJ experiment from 2007 November to 2012 July.
Its emission is detected with a statistical significance of 5.3 standard deviations. Parameterizing the source shape
with a two-dimensional Gaussian function, we estimate an extension Ï = (0.40+0.32
â0.22)âŠ, which is consistent with
the HESS measurement. The observed energy spectrum is dN/dE = (9.0 ± 1.6) Ă 10â13(E/5 TeV)â2.32±0.23
photons cmâ2 sâ1 TeVâ1, in the energy range 0.9â50 TeV. The integral Îł -ray flux above 1 TeV is 1.3 ± 0.4 Crab,
which is 3.2 ± 1.0 times the flux derived by HESS. The differences in the flux determination between HESS and
ARGO-YBJ and possible counterparts at other wavelengths are discussed