Precipitation Phenomena in CMOS Technology

Fábián, István; Kormàny, T.; Erdélyi, Katalin; Pál, Edit

doi:10.4028/www.scientific.net/msf.38-41.189

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Cited by 4 publications

(2 citation statements)

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“…In our earlier work [7] the effects of crystal defects on the threshold voltage of MOS transistors were investigated. The transistors were in test chips located in matrix form on the wafers, but during processing the wafers had suffered severe warpage.…”

Section: Experlmental Detailsmentioning

confidence: 99%

Equivalence and characteristic connections of the Monge-Ampere equations

Туницкий¹

1997

Sb. Math.

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Section: Experlmental Detailsmentioning

confidence: 99%

Equivalence and characteristic connections of the Monge-Ampere equations

Туницкий¹

1997

Sb. Math.

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“…This is probably not seen in lower redshift targets because the central activity tends to be a smaller fraction of the total luminosity than in high redshift sources. Among the proposed explanations are that the emission lines arise from shock induced star formation (De Young 1989, Rees 1989 or that it is scattered light originating from the central nucleus (Fabian 1991). This is a crucial question in our understanding of how and when most star formation occured in giant elliptical galaxies and in clusters in general.…”

Section: Introductionmentioning

confidence: 99%

Discovery of an Obscured Broad-Line Region in the High-Redshift Radio Galaxy MRC 2025−218

Larkin¹,

McLean²,

Graham³

et al. 2000

The Astrophysical Journal

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This Letter presents infrared spectra taken with the newly commissioned near-infrared spectrometer (NIRSPEC) on the Keck II telescope of the high-redshift radio galaxy MRC 2025-218 (z=2.63). These observations represent the deepest infrared spectra of a radio galaxy to date and have allowed for the detection of Hbeta, [O iii] lambdalambda4959, 5007, [O i] lambda6300, Halpha, [N ii] lambdalambda6548, 6583, and [S ii] lambdalambda6716, 6713. The Halpha emission is very broad (FWHM=9300 km s-1) and luminous (2.6x1044 ergs s-1), and it is very comparable to the line widths and strengths of radio-loud quasars at the same redshift. This strongly supports active galactic nucleus unification models linking radio galaxies and quasars, although we discuss some of the outstanding differences. The line [O iii] lambda5007 is extremely strong and has extended emission with large relative velocities toward the nucleus. We also derive that if the extended emission is due to star formation, each knot has a star formation rate comparable to a Lyman-break galaxy at the same redshift.

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DiGiacomo

1993

Microelectronics Manufacturing Diagnostics Handbook

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Precipitation Phenomena in CMOS Technology

Cited by 4 publications

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Equivalence and characteristic connections of the Monge-Ampere equations

Equivalence and characteristic connections of the Monge-Ampere equations

Discovery of an Obscured Broad-Line Region in the High-Redshift Radio Galaxy MRC 2025−218

Reliability/Defect Severity

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