171,081 research outputs found
Babinkamtibmas dalam penanganan penyalahgunaan narkoba di Desa Binong Kecamatan Curug Kabupaten Tangerang / oleh Manda Adistha
No full textabstrak (A) Manda Adistha (NIM: 205000033) (B) Judul Skripsi: ?Peran Babinkamtibmas Dalam Penanganan Penyalahgunaan Narkoba Di Desa Binong Kecamatan Curug Kabupaten Tangerang? (C) Halaman vi + 70 + 2007 (D) Kata Kunci : Peran Babinkamtibmas (E) Isi: Peredaran gelap dan penyalahgunaan narkoba di wilayah indonesia sudah sangat meresahkan, bukan lagi berada di kota-kota besar tetapi sudah sampai ke daerah-daerah terpencil. Untuk mengetahu hal tersebut digunakan metode penelitian hukum empiris/sosiologis. Dalam penanganan penyalahgunaan dan peredaran gelap narkoba, khususnya di Desa Binong Kecamatan Curug Kabupaten Tangerang, maka peran Babinkamtimas menjadi unsur yang paling inti, dalam penanganan penyalahgunaan dan peredaran gelap narkoba. Diharapkan kinerja pihak Babinkamtibmas dapat memperkecil ruang gerak jaringan sindikat narkoba. (F) Daftar acuan : 23 (1987-2006) (G) Dosen Pembimbing : Yuwono Prianto, S.H, M.H (H) Penulis : Manda Adisth
C iv emission-line properties and systematic trends in quasar black hole mass estimates
No full textBlack hole masses are crucial to understanding the physics of the connection between quasars and their host galaxies and measuring cosmic black hole-growth. At high redshift, z ≳ 2.1, black hole masses are normally derived using the velocity width of the C iv1548, 1550 broad emission line, based on the assumption that the observed velocity widths arise from virial-induced motions. In many quasars, the C iv emission line exhibits significant blue asymmetries (‘blueshifts’) with the line centroid displaced by up to thousands of km s−1 to the blue. These blueshifts almost certainly signal the presence of strong outflows, most likely originating in a disc wind. We have obtained near-infrared spectra, including the Hα 6565 emission line, for 19 luminous (LBol = 46.5–47.5 erg s−1) Sloan Digital Sky Survey quasars, at redshifts 2 2000 km s−1, the velocity widths appear to be dominated by non-virial motions. Black hole masses, based on the full width at half-maximum of the C iv emission line, can be overestimated by a factor of 5 at large blueshifts. A larger sample of quasar spectra with both C iv and H β, or Hα, emission lines will allow quantitative corrections to C iv-based black hole masses as a function of blueshift to be derived. We find that quasars with large C iv blueshifts possess high Eddington luminosity ratios and that the fraction of high-blueshift quasars in a flux-limited sample is enhanced by a factor of approximately 4 relative to a sample limited by black hole mass
Pemberian Rehabilitasi Tersangka Narkotika Ditinjau Dari Undang-Undang Nomor 35 Tahun 2009 Tentang Narkotika / oleh Dede Manda Putri Doenggio
No full textabstrak (A)Nama : Dede Manda Putri Doenggio (B) Judul Skripsi : Pemberian Rehabilitasi Tersangka Narkotika Ditinjau Dari Undang-Undang Nomor 35 Tahun 2009 Tentang Narkotika.(C)Halaman : vii+75+25+2013 (D)Kata Kunci : Rehabilitasi Narkotika (E)Isi : Penyalahgunaan narkotika sudah sangat memprihatinkan. Penyalahguna narkoba yang tertangkap tangan saat terjadi penggerebekan oleh penyidik berdasarkan Undang-Undang Narkotika dapat diputus atau ditetapkan untuk menjalani rehabilitasi. Akan tetapi pemberian rehabilitasi tersangka narkotika yang diberikan oleh penyidik BNN kepada RA yang ditangkap dikediamannya sudah bertentangan dengan UU Narkotika. RA yang berstatus tersangka menjalani rehabilitasi narkotika di Lido tersebut pada saat kasusnya belum diputus oleh pengadilan. Disinilah timbul permasalahan dikarenakan pemberian rehabilitasi tersebut bertentangan dengan UU Narkotika. Dalam penelitian ini Penulis menggunakan metode penelitian normatif yang memfokuskan penelitian dengan menggunakan bahan pustaka. Penulis juga melengkapi bahan penelitian dengan melakukan wawancara kepada beberapa narasumber. Pemberian rehabilitasi tersangka narkotika pada saat proses kasusnya masih berjalan dan belum mempunyai putusan pengadilan yang tetap jelas bertentangan dengan UU Narkotika khususnya Pasal 103. Pemberian rehabilitasi tersebut juga menimbulkan permasalahan baru pada saat pembuktian dipengadilan karena status tersangka bukan lagi pecandu akibat telah menjalani rehabilitasi.(F)Acuan : 26 (1977-2011) (G) Pembimbing Soetan Budhi Satria S., S.H., M.H. (H) Penulis Dede Manda Putri Doenggi
Kinematics of C iv and [O iii] emission in luminous high-redshift quasars
No full textWe characterize ionized gas outflows using a large sample of ≃330 high-luminosity [45.5 < log(Lbol/erg s−1) < 49.0], high-redshift (1.5 ≲ z ≲ 4.0) quasars via their [O III]λλ4960,5008 emission. The median velocity width of the [O III] emission line is 1540 kms−1, increasing with increasing quasar luminosity. Broad, blue-shifted wings are seen in the [O III] profiles of ≃42 per cent of the sample. Rest-frame ultraviolet spectra with well-characterized C IVλ1550 emission-line properties are available for more than 210 quasars, allowing an investigation of the relationship between the broad-line region (BLR) and narrow-line region (NLR) emission properties. The [O III] blueshift is correlated with C IV blueshift, even when the dependence of both quantities on quasar luminosity has been taken into account. A strong anticorrelation between the [O III] equivalent width (EW) and C IV blueshift also exists. Furthermore, [O III] is very weak, with EW < 1 Å in ≃10 per cent of the sample, a factor of 10 higher compared to quasars at lower luminosities and redshifts. If the [O III] emission originates in an extended NLR, the observations suggest that quasar-driven winds are capable of influencing the host-galaxy environment out to kilo-parsec scales. The mean kinetic power of the ionized gas outflows is then 1044.7 erg s−1, which is ≃0.15 per cent of the bolometric luminosity of the quasar. These outflow efficiencies are broadly consistent with those invoked in current active galactic nuclei feedback models
Exploring the link between C IV outflow kinematics and sublimation-temperature dust in quasars
No full textUsing data from SDSS, UKIDSS, and WISE, we investigate the properties of the high-frequency cutoff to the infrared emission in ≈5000 carefully selected luminous (Lbol ~1047) type 1 quasars. The strength of ≈2 μm emission, corresponding to emission from the hottest (T > 1200K) dust in the sublimation zone surrounding the central continuum source, is observed to correlate with the blueshift of the C iv λ1550 emission line. We therefore find that objects with stronger signatures of nuclear outflows tend to have a larger covering fraction of sublimation-temperature dust. When controlling for the observed outflow strength, the hot dust covering fraction does not vary significantly across our sample as a function of luminosity, black hole mass, or Eddington fraction. The correlation between the hot dust and the C iv line blueshifts, together with the lack of correlation between the hot dust and other parameters, therefore provides evidence of a link between the properties of the broad emission line region and the infrared-emitting dusty regions in quasars.</p
Istruzzione D'Un Padre à Suo Figlio Ch'egli Manda Nell' Academia
No full textISTRUZZIONE D'UN PADRE À SUO FIGLIO CH'EGLI MANDA NELL' ACADEMIA
Istruzzione D'Un Padre à Suo Figlio Ch'egli Manda Nell' Academia ( - )
Cover ( - )
Exlibris: Bibliotheck des Geh. R. u. C. &z Carl Gerds v. Ketelhodt acquirit zum allgemeinen Besten von Ludwig Friedrich Fürsten zu Schwarzbueg Rud. 1804 ( - )
Titelseite ([I])
Avvertimento Del Traduttore. ([III])
Text: Istruzzione D'Un Padre à Suo Figlio Ch'egli Manda Nell' Academia (5
Manda sütü üretiminin ekonomik yönden sürdürülebilirliği üzerine bir araştırma:
No full textAraştırmacılar; Sait Engindeniz, Hakan Adanacıoğlu, Duran GülerAraştırma projesi -- Ege Üniversitesi, 2019Türkiye'de manda yetiştiriciliği son yıllarda giderek önem kazanmıştır. Manda süt ve et yönlü olarak büyükbaş hayvan grubunda yer almakla birlikte mandacılıktan elde edilen ürün sayısı oldukça fazladır. Süt ve süt ürünleri açısından bakıldığında mandanın sütünden afyon kaymağı, lüle (rulo) kaymağı, manda yoğurdu, dondurma, tereyağı, peynir ve özellikle de mozzarella peyniri elde edilirken, etinden de sucuk, salam ve pastırma gibi işlenmiş et ürünleri elde edilmektedir. Manda sütü gerek protein (%4.2), gerekse yağ(%7.9), kalsiyum (264mg/100gr), magnezyum (307mg/100gr) ve C vitamini (6.7 mg/100gr) açısından inek sütüne göre çok daha zengin bir süttür. Türkiye'de manda varlığının en yoğun olduğu iller sırasıyla Samsun, İstanbul, Diyarbakır, Muş, Bitlis, Afyon, Sivas ve Kayseri illeridir. Ege bölgesinde ise manda yetiştiriciliği ve manda sütü üretimi ağırlıklı olarak Afyonkarahisar, Balıkesir ve Kütahya illerinde gerçekleştirilmektedir. Bu araştırmada manda sütü üretimi açısından Ege bölgesinde ikinci sırada yer alan Balıkesir ili seçilmiştir. Araştırmanın verileri; Balıkesir ilinde manda sayısının yüksek olduğu ve manda sütü üretiminin yoğun olarak yapıldığı Altıeylül ile Gönen ilçelerinde bulunan toplam 102 üreticiden anket yoluyla elde edilmiştir. Araştırmada Balıkesir ili manda yetiştiriciliği yapan işletmelerin mevcut durumu, hangi koşullarda bu üretimi gerçekleştirdikleri incelenmiş, kârlılık düzeyleri, üretici eline geçen fiyatlar, pazarlama kanalları ortaya konularak, üretimde ve pazarlamada karşılaşılan sorunlar ile bu sorunlara yönelik çözüm yolları sunulmuştur. Manda işletmelerinin teknik etkinliği Veri Zarflama Analizi (VZA) kullanılarak gridi ve çıktı yönelimli olarak hesaplanmıştır. 17 işletme etkin olarak bulunmuştur. İşletmelerin girdiye yönelik ortalama etkinlik skoru devlet desteği olması durumunda %58.51, olmaması durumunda ise %58.14 bulunmuştur. Çıktıya yönelik analizde, manda yetiştiriciliği yapılan işletmelerde tam etkinliğin sağlanması için brüt üretim değerinin %37.04 oranında artırılması gerekmektedir. Girdiye yönelik analizde bulunan potansiyel iyileştirme değerleri çıktıya yönelik olanla oldukça benzerlik göstermektedir. Çıktı ve girdilerdeki iyileştirme önerileri brüt üretim değeri haricindeki bütün değişkenler için azaltma yönündedir.;Manda Sütü, Ekonomik Analiz, Etkinlik, Sürdürülebilirlik.;Buffalo Milk, Economical Analysis, Efficiency, Sustainability
Manda meni ryytimaahan Kukkasia poimimahan (3/4 C)
No full textLaulun sanat: Manda meni ryytimaahan Kukkasia poimimahan; Hän poimi kukkasia Hermannill', Vaan Hermannii ei kuulunut, Hän poimi kukkasia Hermannill', Vaan Hermannii ei kuulunut
Modelling type 1 quasar colours in the era of Rubin and Euclid
No full textWe construct a parametric SED model which is able to reproduce the average observed SDSS–UKIDSS–WISE quasar colours to within one-tenth of a magnitude across a wide range of redshift (0 < z < 5) and luminosity (−22 > Mi > −29). This model is shown to provide accurate predictions for the colours of known quasars which are less luminous than those used to calibrate the model parameters, and also those at higher redshifts z > 5. Using a single parameter, the model encapsulates an up-to-date understanding of the intra-population variance in the rest-frame ultraviolet and optical emission lines of luminous quasars. At fixed redshift, there are systematic changes in the average quasar colours with apparent i-band magnitude, which we find to be well explained by the contribution from the host galaxy and our parametrization of the emission-line properties. By including redshift as an additional free parameter, the model could be used to provide photometric redshifts for individual objects. For the population as a whole we find that the average emission line and host-galaxy contributions can be well described by simple functions of luminosity which account for the observed changes in the average quasar colours across 18.1 < iAB < 21.5. We use these trends to provide predictions for quasar colours at the luminosities and redshifts which will be probed by the Rubin Observatory LSST and ESA-Euclid wide survey. The model code is applicable to a wide range of upcoming photometric and spectroscopic surveys, and is made publicly available
QSOGEN: model quasar SEDs
No full textThe QSOGEN collection of Python code models quasar colors, magnitudes and SEDs. It implements an empirically-motivated parametric model to efficiently account for the observed emission-line properties, host-galaxy contribution, dust reddening, hot dust emission, and IGM suppression in the rest-frame 900-30000A wavelength range for quasars with a wide range of redshift and luminosity. The code is packaged with a set of empirically-derived emission-line templates and an empirically-derived quasar dust extinction curve which are publicly released
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