2,459 research outputs found
Clinical aspects of cervical insufficiency
Fetal loss is a painful experience. A history of second or early third trimester fetal loss, after painless dilatation of the cervix, prolapse or rupture of the membranes, and expulsion of a live fetus despite minimal uterine activity, is characteristic for cervical insufficiency. In such cases the risk of recurrence is high, and a policy of prophylactic cerclage may be safer than one of serial cervical length measurements followed by cerclage, tocolysis and bed rest in case of cervical shortening or dilatation. In low risk cases, however, prophylactic cerclage is not useful. There is a need for more basic knowledge of cervical ripening, objective assessment of cervical visco-elastic properties, and randomized controlled trials of technical aspects of cervical cerclage (e.g. suturing technique)
How many black holes fit on the head of a pin?
The Bekenstein-Hawking entropy of certain black holes can be computed
microscopically in string theory by mapping the elusive problem of counting
microstates of a strongly gravitating black hole to the tractable problem of
counting microstates of a weakly coupled D-brane system, which has no event
horizon, and indeed comfortably fits on the head of a pin. We show here that,
contrary to widely held beliefs, the entropy of spherically symmetric black
holes can easily be dwarfed by that of stationary multi-black-hole
``molecules'' of the same total charge and energy. Thus, the corresponding
pin-sized D-brane systems do not even approximately count the microstates of a
single black hole, but rather those of a zoo of entropically dominant
multicentered configurations.Comment: 4 pages, fourth prize in the Gravity Research Foundation Essay
competition 200
The Panchromatic High-Resolution Spectroscopic Survey of Local Group Star Clusters - I. General Data Reduction Procedures for the VLT/X-shooter UVB and VIS arm
Our dataset contains spectroscopic observations of 29 globular clusters in
the Magellanic Clouds and the Milky Way performed with VLT/X-shooter. Here we
present detailed data reduction procedures for the VLT/X-shooter UVB and VIS
arm. These are not restricted to our particular dataset, but are generally
applicable to different kinds of X-shooter data without major limitation on the
astronomical object of interest. ESO's X-shooter pipeline (v1.5.0) performs
well and reliably for the wavelength calibration and the associated
rectification procedure, yet we find several weaknesses in the reduction
cascade that are addressed with additional calibration steps, such as bad pixel
interpolation, flat fielding, and slit illumination corrections. Furthermore,
the instrumental PSF is analytically modeled and used to reconstruct flux
losses at slit transit and for optimally extracting point sources. Regular
observations of spectrophotometric standard stars allow us to detect
instrumental variability, which needs to be understood if a reliable absolute
flux calibration is desired. A cascade of additional custom calibration steps
is presented that allows for an absolute flux calibration uncertainty of less
than ten percent under virtually every observational setup provided that the
signal-to-noise ratio is sufficiently high. The optimal extraction increases
the signal-to-noise ratio typically by a factor of 1.5, while simultaneously
correcting for resulting flux losses. The wavelength calibration is found to be
accurate to an uncertainty level of approximately 0.02 Angstrom. We find that
most of the X-shooter systematics can be reliably modeled and corrected for.
This offers the possibility of comparing observations on different nights and
with different telescope pointings and instrumental setups, thereby
facilitating a robust statistical analysis of large datasets.Comment: 22 pages, 18 figures, Accepted for publication in Astronomy &
Astrophysics; V2 contains a minor change in the abstract. We note that we did
not test X-shooter pipeline versions 2.0 or later. V3 contains an updated
referenc
Analisis Pengaruh Perilaku Masyarakat Terhadap Kualitas Air Baku dan Air Minum PDAM Tirta Handayani Gunung Kidul
PDAM Tirta Handayani merupakan perusahaan penyedia dan penyalur air pada masyarakat yangterletak di Gunung Kidul.. Kualitas air baku diketahui dengan membandingkan nilai yang ditetapkan PeraturanPemerintah Nomor 22 tahun 2021dan kualitas air minum berdasarkan nilai dari Peraturan Menteri KesehatanNo 492 tahun 2010. Hasil uji air baku untuk IPA Baron dan Bribin semua parameternya masuk kelas I yangperuntukannya sebagai air baku air minum. Hasil Uji kualitas air minum IPA Baron dan Bribin menunjukkanbahwa parameter fisik dan mikrobiologi melebihi kadar yang seharusnya yaitu nilai E.Coli dan Total Coliform0 pada daerah yang diuji nilai tertinggi mencapai 1200. Perilaku masyarakat sangat berpengaruh pada kualitasair baku dimana warga Gunung kidul sering mengubur jasad hewan dalam tanah sehingga bakteri dari hewanyang dikubur itu bisa mempengaruhi kualitas tanah sekitarnya. Air PDAM yang diterima masyarakat masihberbau amis sehingga mereka memasak airnya lagi untuk menghilangkan bau untuk dikonsumsi tiap hari
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