Broadband near-infrared astronomical spectrometer calibration and on-sky validation with an electro-optic laser frequency comb.

The quest for extrasolar planets and their characterization as well as studies of fundamental physics on cosmological scales rely on capabilities of high-resolution astronomical spectroscopy. A central requirement is a precise wavelength calibration of astronomical spectrographs allowing for extraction of subtle wavelength shifts from the spectra of stars and quasars. Here, we present an all-fiber, 400 nm wide near-infrared frequency comb based on electro-optic modulation with 14.5 GHz comb line spacing. Tests on the high-resolution, near-infrared spectrometer GIANO-B show a photon-noise limited calibration precision of < 10 cms as required for Earth-like planet detection. Moreover, the presented comb provides detailed insight into particularities of the spectrograph such as detector inhomogeneities and differential spectrograph drifts. The system is validated in on-sky observations of a radial velocity standard star (HD221354) and telluric atmospheric absorption features. The advantages of the system include simplicity, robustness and turn-key operation, features that are valuable at the observation sites.

[Comparative evaluation of indicators of local, humoral immunity and nonspecific resistance in patients with different pathology of the cervix].

A comparative evaluation of some indicators of immune system and analysis of the dependence of these parameters (correlation) are carried out to identify interrelated mechanisms. The observed changes in the concentrations of indicators of immune system and the correlation between cytokines, humoral immunity and nonspecific resistance in cervical mucus in patients with cervical pathology demonstrate the complex, interrelated and changing interactions of the local immune system at various stages of development of the pathological process of the cervix.

Deletions of the transcription factor Ikaros in myeloproliferative neoplasms.

Transformation to acute leukemia is a major complication of myeloproliferative neoplasms (MPNs), however, the genetic changes leading to transformation remain largely unknown. We screened nine patients with post-MPN leukemia for chromosomal aberrations using microarray karyotyping. Deletions on the short arm of chromosome 7 (del7p) emerged as a recurrent defect. We mapped the common deleted region to the IKZF1 gene, which encodes the transcription factor Ikaros. We further examined the frequency of IKZF1 deletions in a total of 29 post-MPN leukemia and 526 MPN patients without transformation and observed a strong association of IKZF1 deletions with post-MPN leukemia in two independent cohorts. Patients with IKZF1 loss showed complex karyotypes, and del7p was a late event in the genetic evolution of the MPN clone. IKZF1 deletions were observed in both undifferentiated and differentiated myeloid cell types, indicating that IKZF1 loss does not cause differentiation arrest but rather renders progenitors susceptible to transformation, most likely through chromosomal instability. Induced Ikzf1 haploinsufficiency in primary murine progenitors resulted in elevated Stat5 phosphorylation and increased cytokine-dependent growth, suggesting that reduced expression of IKZF1 is sufficient to perturb growth regulation. Thus, IKZF1 loss is an important step in the leukemic transformation of a subpopulation of MPN patients.

Patrilocality and recent migrations have little impact on shaping patterns of genetic structure of the Armenian population.

In general, genetic distances between human populations (also within one ethnic group) are larger for the Y chromosome markers than for the mtDNA. It is usually explained by higher rate of female versus male migration due to the cultural practice of patrilocality, when women move to their husbands' residence after marriage. Recently found a reversed picture for the genetic variation in some ethno-territorial groups confirm the strict role of cultural traditions in shaping patterns of populations' genetic structure. To test the role of patrilocality for the genetic structure of the Armenian population, we compared the Y chromosome and the mtDNA haplotype variations among and between geographical groups identified according to paternal (maternal) grandparental place of birth, from one side, and the populations currently living in the same geographical areas, from the other side. The results demonstrate that the Armenian population is regionally more structured for the Y chromosome than for the mtDNA. Additionally, in spite of expressed directivity of migration processes (caused by the phenomenon of patrilocality as well), the patterns of genetic variations for the populations of the same geographic areas remain without any significant changes during the last three generations.

A low-energy core-collapse supernova without a hydrogen envelope.

The final fate of massive stars depends on many factors. Theory suggests that some with initial masses greater than 25 to 30 solar masses end up as Wolf-Rayet stars, which are deficient in hydrogen in their outer layers because of mass loss through strong stellar winds. The most massive of these stars have cores which may form a black hole and theory predicts that the resulting explosion of some of them produces ejecta of low kinetic energy, a faint optical luminosity and a small mass fraction of radioactive nickel. An alternative origin for low-energy supernovae is the collapse of the oxygen-neon core of a star of 7-9 solar masses. No weak, hydrogen-deficient, core-collapse supernovae have hitherto been seen. Here we report that SN 2008ha is a faint hydrogen-poor supernova. We propose that other similar events have been observed but have been misclassified as peculiar thermonuclear supernovae (sometimes labelled SN 2002cx-like events). This discovery could link these faint supernovae to some long-duration gamma-ray bursts, because extremely faint, hydrogen-stripped core-collapse supernovae have been proposed to produce such long gamma-ray bursts, the afterglows of which do not show evidence of associated supernovae.

Reduced carbon solubility in Fe nanoclusters and implications for the growth of single-walled carbon nanotubes.

Fe nanoclusters are becoming the standard catalysts for growing single-walled carbon nanotubes via chemical vapor decomposition. Contrary to the Gibbs-Thompson model, we find that the reduction of the catalyst size requires an increase of the minimum temperature necessary for the growth. We address this phenomenon in terms of solubility of C in Fe nanoclusters and, by using first-principles calculations, we devise a simple model to predict the behavior of the phases competing for stability in Fe-C nanoclusters at low temperature. We show that, as a function of particle size, there are three scenarios compatible with steady state growth, limited growth, and no growth of single-walled carbon nanotubes, corresponding to unaffected, reduced, and no solubility of C in the particles.

A giant outburst two years before the core-collapse of a massive star.

The death of massive stars produces a variety of supernovae, which are linked to the structure of the exploding stars. The detection of several precursor stars of type II supernovae has been reported (see, for example, ref. 3), but we do not yet have direct information on the progenitors of the hydrogen-deficient type Ib and Ic supernovae. Here we report that the peculiar type Ib supernova SN 2006jc is spatially coincident with a bright optical transient that occurred in 2004. Spectroscopic and photometric monitoring of the supernova leads us to suggest that the progenitor was a carbon-oxygen Wolf-Rayet star embedded within a helium-rich circumstellar medium. There are different possible explanations for this pre-explosion transient. It appears similar to the giant outbursts of luminous blue variable stars (LBVs) of 60-100 solar masses, but the progenitor of SN 2006jc was helium- and hydrogen-deficient (unlike LBVs). An LBV-like outburst of a Wolf-Rayet star could be invoked, but this would be the first observational evidence of such a phenomenon. Alternatively, a massive binary system composed of an LBV that erupted in 2004, and a Wolf-Rayet star exploding as SN 2006jc, could explain the observations.