3 research outputs found
Automated digitization of radial charts
Radial charts were commonly used in the industry to allow retrospective assessment of technological parameters. Today it is relevant to digitize the obtained data in order to simplify the automation of technological processes. Digitization of radial charts by means of standard methods is carried out with the help of human labor at significant time costs. The article proposes an automated method for digitizing radial charts using software, developed in the LabVIEW programming environment. The results of processing radial charts are displayed on the screen in numerical and graphical form, and can also be exported to a file (for example, to Notepad or MSÂ Excel). The presented technique can be applied to images obtained on a color or black-and-white scanner, which minimizes geometric distortions, associated with the conversion of a paper document into electronic form, and ensures recognition quality of the clear plot line with an average relative error of up to 3Â %. In case of ink fading or perspective photos of the diagram, the value of relative error can reach 8Â %, as a result of which additional manual correction of the data will be required
Amido Ca and Yb(II) Complexes Coordinated by Amidine-Amidopyridinate Ligands for Catalytic Intermolecular Olefin Hydrophosphination
A series
of amido Ca and YbÂ(II) complexes LMÂ[NÂ(SiMe<sub>3</sub>)<sub>2</sub>]Â(THF) (<b>1Yb</b>, <b>1–4Ca</b>) coordinated
by amidine-amidopyridinate ligands <b>L</b><sup><b>1</b>–<b>4</b></sup> were synthesized via a transamination
reaction between proligands <b>L</b><sup><b>1</b>–<b>4</b></sup><b>H</b> and bisamido complexes MÂ[NÂ(SiMe<sub>3</sub>)<sub>2</sub>]<sub>2</sub>Â(THF)<sub>2</sub> (M = Yb,
Ca). The reactions of YbÂ[NÂ(SiMe<sub>3</sub>)<sub>2</sub>]<sub>2</sub>Â(THF)<sub>2</sub> with proligands <b>L</b><sup><b>2</b></sup><b>H</b>-<b>L</b><sup><b>4</b></sup><b>H</b> containing CF<sub>3</sub> and C<sub>6</sub>H<sub>4</sub>F fragments do not allow for preparing the target YbÂ(II) complexes,
while the Ca analogues were synthesized in good yields. Complexes <b>1Yb</b> and <b>1</b>–<b>4Ca</b> were evaluated
as precatalysts for hydrophosphination of styrene, <i>p</i>-substituted styrenes, α-Me-styrene, and 2,3-dimethylbutadiene
with various primary and secondary phosphines (PhPH<sub>2</sub>, 2,4,6-Me<sub>3</sub>C<sub>6</sub>H<sub>2</sub>PH<sub>2</sub>, 2-C<sub>5</sub>NH<sub>4</sub>PH<sub>2</sub>, Ph<sub>2</sub>PH, Cy<sub>2</sub>PH). Complexes <b>1Yb</b>, <b>1</b>–<b>4Ca</b> performed high
catalytic activities in styrene hydrophosphination with PhPH<sub>2</sub> and Ph<sub>2</sub>PH and demonstrated high regioselectivity affording
exclusively the anti-Markovnikov addition products. For primary PhPH<sub>2</sub> the reactions (1:1 molar ratio of substrates) catalyzed by <b>1Yb</b>, <b>1Ca</b>, and <b>2Ca</b> proved to be highly
chemoselective affording the secondary phosphine PhÂ(PhCH<sub>2</sub>CH<sub>2</sub>)ÂPH; however, complexes <b>3Ca</b> and <b>4Ca</b> led to the formation of both secondary and tertiary phosphines
in 80:20 and 86:14 ratios. Styrene hydrophosphinations with 2,4,6-Me<sub>3</sub>C<sub>6</sub>H<sub>2</sub>PH<sub>2</sub> and 2-pyridylphosphine
for all complexes <b>1Yb</b> and <b>1–4Ca</b> proceeded
much more slowly compared to PhPH<sub>2</sub>. Addition of 2-C<sub>5</sub>NH<sub>4</sub>PH<sub>2</sub> to styrene catalyzed by complex <b>1Yb</b> turned out to be non-regioselective and led to the formation
of a mixture of Markovnikov and anti-Markovnikov addition products,
while all Ca complexes enabled regioselective anti-Markovnikov addition.
Complexes <b>1Ca</b> and <b>1Yb</b> containing catalytic
centers featuring similar ionic radii performed different catalytic
activity: the ytterbium analogue proved to be a more active catalyst
for intermolecular hydrophosphination of styrene with Cy<sub>2</sub>PH, 2-C<sub>5</sub>NH<sub>4</sub>PH<sub>2</sub>, and PhPH<sub>2</sub>, but less active with sterically demanding 2,4,6-Me<sub>3</sub>C<sub>6</sub>H<sub>2</sub>PH<sub>2</sub>. Styrenes containing in <i>p</i>-position electron-donating groups (Me, tBu, OMe) performed
with noticeably lower rates in the reactions with PhPH<sub>2</sub> compared to styrene. Complexes <b>1Yb</b>, <b>1Ca</b>, <b>2Ca</b>, <b>3Ca</b>, and <b>4Ca</b> enabled
addition of PhPH<sub>2</sub> toward the double Cî—»C bond of
α-Me-styrene, and the reaction rate for this substrate is noticeably
lower; however quantitative conversions were reached in ∼40
h. Complexes <b>1Ca</b> and <b>2Ca</b> promoted 1,2-addition
of PhPH<sub>2</sub> to 2,3-dimethyl butadiene with excellent regio-
and chemoselectivity to afford linear secondary phosphines. Hydrophosphination
of inert 1-nonene with Ph<sub>2</sub>PH with 40% conversion becomes
possible due to the application of complex <b>2Ca</b> (40 h,
70 °C). The rate law for the hydrophosphination of styrene with
Ph<sub>2</sub>PH catalyzed by <b>1Ca</b> was found to agree
with the idealized equation: <i>v</i> = <i>k</i>[styrene]<sup>1</sup>[<b>1Ca</b>]<sup>1</sup>
TOI 564 b and TOI 905 b: grazing and fully transiting hot Jupiters discovered by TESS
We report the discovery and confirmation of two new hot Jupiters discovered by the Transiting Exoplanet Survey Satellite (TESS): TOI 564 b and TOI 905 b. The transits of these two planets were initially observed by TESS with orbital periods of 1.651 and 3.739 days, respectively. We conducted follow-up observations of each system from the ground, including photometry in multiple filters, speckle interferometry, and radial velocity measurements. For TOI 564 b, our global fitting revealed a classical hot Jupiter with a mass of MJ and a radius of RJ. Also a classical hot Jupiter, TOI 905 b has a mass of MJ and radius of RJ. Both planets orbit Sun-like, moderately bright, mid-G dwarf stars with V ∼ 11. While TOI 905 b fully transits its star, we found that TOI 564 b has a very high transit impact parameter of , making it one of only ∼20 known systems to exhibit a grazing transit and one of the brightest host stars among them. Therefore, TOI 564 b is one of the most attractive systems to search for additional nontransiting, smaller planets by exploiting the sensitivity of grazing transits to small changes in inclination and transit duration over a timescale of several years