text:
\section{Introduction}

How will the Sun evolve in the future?  In the case of stellar rotation, thanks to seminal works in the past \citep[e.g.][]{skumanich72, barnes03}, we now have a fundamental tool that traces many astrophysical effects \citep[e.g., magnetic fields, interaction with close planets, structural evolution;][]{vidotto14,ferrazmello15} and, as a byproduct of all these correlations with time, stellar rotation can be used as an elegant and straightforward chronometer \citep{barnes07, mamajek08}.

However, stellar rotation as a predictive tool still lacks strong observational constraints in critical regions of its parameter space, for example, old stars with global properties similar to those of the Sun ($\gtrsim$4 Gyr, $\sim$ 1 $M_\odot$, \feh$\sim$ 0.00). Therefore, due to this scarcity, after this age, different theoretical assumptions of radius dependence \citep{reiners12}, angular momentum loss \citep{matt15}, magnetic field topology \citep{see19}, stellar differential rotation profile \citep{benomar18}, for example, might significantly affect the predictions for rotational evolution of the Sun  \citep[][the latter referred hereafter as LO19]{barnes07,donascimento13,donascimento14,lorenzo19}. As suggested by \cite{vansaders16} (hereafter VS16), around solar age or a critical value of Rossby number $\sim$ 2 \citep[Ro $\equiv$ \Prot/$\tau_{\rm conv}$, where $\tau_{\rm conv}$ is the convective turnover time;][]{noyes84} the efficiency of magnetic braking may be significantly reduced, leading to a dramatically different rotational evolution scenario for the Sun. Therefore, it is crucial to constrain this age interval with new observations. To solve this burning conflict, and assess how solar-mass \& solar-metallicity stars cease to slow down after solar age, we provide unique constraints to unveil the rotational fate of our Sun towards the end of the main-sequence through an extensive activity analysis of the ancient solar twin HIP 102152.
\begin{table}
\caption{Main stellar parameters derived for HIP 102152. [1] \citet{gaia18}; [2] \citet{spina17}; [3] \citet{lorenzo18}; [4] LO19; [5]
\citet{lorenzo16};
[6] This work; [7] \citet{barnes10}; [8] \citet{mittag13}; [9] \citet{carlos19}}
\begin{center}
\begin{tabular}{c c c}
\hline
Parameter & Value & Reference \\
\hline
\hline
\textit{Alias} &  & \\
Gaia DR2 & 6799090223510802176 & [1] \\
HD & 197027 & $--$ \\
TIC & 212354618 & $--$\\
\hline
\textit{Atmospheric parameters} &  & \\
\Teff [K] & $5718 \pm 4$ & [2] \\
\feh & $-0.016 \pm 0.003$ & [2]\\
\logg & $4.325 \pm 0.011$ & [2]\\
\hline
\textit{HR diagram} &  & \\
mass [M$\odot$] & $0.97 \pm 0.03$ & [4] \\
radius [R$\odot$] & $1.07 \pm 0.02$ & [4]\\
\hline
\textit{Stellar Activity} &  & \\
$<S_{\rm MW}>$ & $0.159 \pm 0.001$ & [6] \\
\ensuremath{\log R^\prime_{\rm HK} ({\rm B-V})} & $-5.01 \pm 0.02$  & [6] \\
\ensuremath{\log R^\prime_{\rm HK} (T_{\rm eff})} & $-5.12 \pm 0.02$ & [6] \\
$\log R^+_{\rm HK}$ & $-5.2$ & [6][8] \\
\hline
\textit{Stellar Rotation} &  & \\
\Psini [d] & $34.8 \pm 4.7$ & [4] \\
\Prot (\tess) [d] & $>27$  & [6] \\
$P_{\rm rot , TESS, P/\sin i}$ [d] & $34.4_{-6.2}^{+ 6.9}$  & [6] \\
\Prot  [d] (adopted) [d] & $35.7 \pm 1.4$ & [6] \\
\hline
\textit{Stellar Age} &  & \\
$t_{\rm iso}$ [Gyr] & $8.0_{-0.4}^{+0.3}$ & [4]\\
$t_{\rm HK~1}$ [Gyr] & $7.6 \pm 1.0$ & [3][6] \\
$t_{\rm HK~2}$ [Gyr] & $6.6^{+2.5}_{-1.8}$ & [5][6] \\
$t_{\rm Gyro}$ [Gyr] & $7.6\pm0.6$ & [6][7] \\
$t_{\rm Li}$ [Gyr] & $9.1 \pm 1.1$ & [6][9] \\
$<t_{\rm Chem}>$ [Gyr] & $7.2 \pm 1.0$ & [2][6] \\
\hline
\hline

\end{tabular}
\end{center}

\label{table:id}
\end{table}
\section{Observations, Parameters and Activity Indicators}

The star HIP 102152, located at $\sim$ 78.4 parsecs from us, is one of the most interesting solar twins ever discovered \citep[][hereafter M13]{monroe13}. Its macroscopic characteristics are nearly indistinguishable from what we would expect for the ancient Sun. Considering its isochronal age, mass and metallicity ($t_{\rm iso}$ = $8.0_{-0.4}^{+0.3}$ Gyr, 0.97$\pm$0.03 M$_\odot$, \feh = $-$0.016$\pm$0.003 dex, LO19), HIP102152 is placed at almost the end of the main-sequence. From a chemical point of view, it has the same level of deficiency of refractory elements as the Sun, which could be a hint about the formation of eventual terrestrial planets (M13). Additionally, empiric age indicators such as chromospheric activity \citep{lorenzo16a, lorenzo18}, Li abundances \citep{carlos19}, [Y/Mg], and [Y/Al] \citep{spina17} also yield ages ranging from 7 to 9 Gyr, which agrees with the estimates from \citet{lorenzo19}. In Table \ref{table:id} we summarize the main stellar parameters derived for HIP 102152.

The observations were carried out for \textit{exactly} 10 years, between 05-22-2009 and 05-22-2019 (MJD=54973.9$-$58625.8), with the HARPS spectrograph \citep{mayor03} fed by the 3.6 m telescope at La Silla Observatory, under the programs 183.D-0729 (PI: Bazot, M.), 292.C-5004 (PI: Mel\'endez, J.), 188.C-0265 (PI: Mel\'endez, J.), 0100.D-0444 (Lorenzo-Oliveira, D.), and 0103.D-0445 (Lorenzo-Oliveira, D.).

To perform the activity analysis, we selected only observations with a signal-to-noise ratio greater than 30 around the Ca II lines and constrained our sample to those observations with angular separation greater than 15 degrees away from the Moon to avoid excessive contamination of scattered light. Our sample is composed of 52 spectra, of which 34 were taken at high cadence during a short observational window over $\sim$4 months (MJD=56484.69$-$56625.50). Different activity indicators were used in this work such as \ion{Ca}{II} H (3933.663$\pm$0.595 \AA) and K (3968.469$\pm$0.595 \AA) lines; Balmer lines H$\alpha$ (6562.8$\pm$0.5 \AA), H$\beta$ (4861.32$\pm$0.5 \AA), H$\gamma$ (4340.46$\pm$0.4\AA), H$\delta$ (4101.76$\pm$0.25 \AA), and H$\epsilon$ (3970.07$\pm$0.3\AA); \ion{Na}{I} lines (5889.95$\pm$0.25 \AA, 5895.92$\pm$0.25 \AA). We defined their respective pseudo-continuum regions based on \cite{maldonado19} and \cite{giribaldi19}, albeit with slight modifications: 3901.07 and 4001.07 \AA\ ($\Delta\lambda$ = 20 \AA; \ion{Ca}{II} and H$\epsilon$), 6500.625 and 6625.55 \AA\ ($\Delta\lambda$ = 5 \AA; H$\alpha$), 4845.0 and 4880.0 \AA\ ($\Delta\lambda$ = 10 \AA; H$\beta$), 4318 and 4366 \AA\ ($\Delta\lambda$ = 10 \AA; H$\gamma$), 4085 and 4120 \AA\ ($\Delta\lambda$ = 20 \AA; H$\delta$), 5845.0 and 5940 \AA\ ($\Delta\lambda$ = 5 \AA; \ion{Na}{I}). Instrumental activity indices are given by the ratio between the sum of the line fluxes and their respective continuum regions. Internal errors are estimated propagating the typical photonic errors in each HARPS spectral order analyzed. In the case of \ion{Ca}{II} lines, we also use the S index converted into the Mount Wilson scale \citep[see][]{lorenzo18}. To calculate the activity indices, we resampled the spectra using linear interpolation, assuming constant steps of 0.01 \AA. Then, for a given spectral region (defined by each chromospheric indicator), we build a master spectrum based on a combination of all available observations and, subsequently, normalize each one of the observations in comparison to its master spectrum, to correct minor continuum variations from one observation to another. Spectra taken within a 1-day interval were combined to improve the S/N.

\section{Rotational period of HIP102152}

We started the calculation of the most likely rotational period of HIP 102152 using the \ion{Ca}{II} S index, which is well-known to be strongly correlated to stellar rotation \citep{mamajek08}. The star is very inactive and shows a low level of chromospheric variability over 10 years of monitoring, possibly indicating a rotation level around 30$-$40 days, according to the \citet{mamajek08} rotation$-$activity calibration. As a starting point, we analyzed the activity time series of HIP 102152 during the highest cadence dates (MJD = 56484.70$-$56625.51). We use \textit{Generalized Lomb-Scargle} periodogram (GLS) analysis to detect a clear peak around $\sim$36 days. From this initial guess, we refined our analysis by using the Gaussian Process regression fit to deal with quasi-periodic (QP) trends in the activity time series \citep{haywood15}. For a given chromospheric indicator \textit{i}, we define an appropriate combination of covariance functions relating to different epochs ($t$ and $t'$) of observations to build our QP activity model:
\begin{equation}
    k(t,t')\equiv \mathcal{I}_{\rm const}+\mathcal{A}\exp\left(-\frac{||t-t'||}{2 \ell^2} -\Gamma\sin^2\left[\frac{\pi}{ P_{\rm rot}}||t-t'||\right] \right)+\sigma^2\delta_{t,t'},
\end{equation}
where $\mathcal{I}_{\rm const}$ gives a constant scale to match the observed mean activity level of the star, $\mathcal{A}$ is the amplitude of rotation signal, $\ell$ is commonly interpreted as the timescale of rising and decay of active regions. The harmonic nature of the time series is represented by $\Gamma$, and the white noise term is $\sigma^2\delta_{t,t'}$. We adopted log-normal prior distribution for the hyperparameters: $\mathcal{I}_{\rm const}$ ($\mu = {\rm <i>}$,$\sigma = \sigma_{\rm <i>}$), \Prot ($\mu = P_{\rm rot, GLS}$,$\sigma = 0.2\times P_{\rm rot, GLS}$), and $\ln\Gamma$ \citep[$\mu = -2.3$, $\sigma = 1.4$, as in][]{angus18}. For the other hyperparameters, we adopted Jeffrey's prior. To find the optimal solution and the associated errors for the stellar rotation GP model, we use the \textit{emcee} \citep{foremanmackey13} \textit{Python} implementation of the affine-invariant ensemble sampler for \textit{Markov Chain Monte Carlo} method (MCMC) following \citet{angus18}. In brief, we start the MCMC process with 100 walkers spread around an optimal solution obtained by maximum likelihood optimization. Then, we evaluate the convergence of chains every 100 steps, checking the chain autocorrelation timescale ($\tau_{\rm chain}$) and the consistency of walkers solutions through Gelman$-$Rubin statistics (\^R).  We define as a convergence criterion when  $\tau_{\rm chain}$ is less than 10\% of the total chain length, $\tau_{\rm chain}$ is stable concerning the previous chain evaluation within 1\%, and \^R less than 1.03. We then discard the initial iterations (3$\times$ $\tau_{\rm chain}$) and randomly resample 5000 samples to represent our final estimate of posteriori probability distribution.

We found for the \ion{Ca}{II} S index a rotational period of 36.1$_{- 3.3}^{+ 3.8}$ days. Alternatively, we built another GP model composed of only the constant kernel $\mathcal{I}_{\rm const}$ that relates the mean activity level in order to assess its statistical relevance over the QP model. In Fig. \ref{fig:S} (upper left panel), we show the rotational behavior found for the S index. The blue shaded area is our $\pm2\sigma$ QP model prediction. The probability distribution of \Prot is shown in the right panel. The red dashed line is the gyrochronology prediction for 8 Gyr-old solar mass star using \citet{barnes10} relations. The ratio between MCMC QP and Constant model posterior probabilities ($\log p_{\rm QP}/p_{\rm Const}\equiv\log B_{\rm factor}$) gives us an idea about which model is more suitable to describe the data. The greater the $B_{\rm factor}$, the greater the probability that we should favor the QP model. According to \citet{kass95}, $\log B_{\rm factor}\geq2$ has a \textit{decisive} probability favoring QP model. For the S index, we found a value of $\log B_{\rm factor}\sim60$. The same result is obtained by analyzing each \ion{Ca}{II} line, now adopting as a \Prot\ prior the S index $p_{\rm QP}$ distribution. As seen in Fig. \ref{fig:S} (panel immediately below the S index one), the modulation of the \ion{Ca}{II} K line is even more significant than those obtained for the S index, reaching $\log~B_{\rm factor}\geq70$ for \Prot = $36.1_{-2.0}^{+2.6}$ days. Although the lower $B_{\rm factor}$ compared with \ion{Ca}{II} K line and S index, \ion{Ca}{II} H shows consistent rotational period. For the other indicators, we repeat the same strategy used for the S index. In the lower panel of Fig. \ref{fig:S}, we also show the H$\epsilon$ line performance.
\begin{figure}
\centering
  \begin{minipage}[t]{0.49 \linewidth}
\centering
    \resizebox{\hsize}{!}{\includegraphics{FIGURES/FIGURE1.pdf}}
  \end{minipage}
  \begin{minipage}[t]{0.49 \linewidth}
\centering
    \resizebox{\hsize}{!}{\includegraphics{FIGURES/FIGURE1b.pdf}}
  \end{minipage}
  \caption{\textit{Left panel:} Rotational signal detected in S index, \ion{Ca}{II} K, and H$\epsilon$ lines (upper, middle, and lower panels, respectively). Solid lines and shaded blue regions are QP model and 2$\sigma$ predictions. The error bars are given by the quadratic propagation of white noise and spectroscopic index errors. \textit{Right panel:} \Prot pdf for the same activity indicators. Red dashed lines is the gyrochronology prediction from \citet{barnes10}.}
\label{fig:S}
\end{figure}
In Table \ref{table:prots}, we show the best indicators: \ion{Ca}{II} K line, \ion{Ca}{II} S index (H+K), \ion{Ca}{II} H line, and H$\epsilon$. The remaining set of indicators that show $\log B_{\rm factor} < 2$ are followed by H$\gamma$, H$\alpha$, \ion{Na}{I} D2 and D1 lines, H$\delta$, and H$\beta$. As we decrease $B_{\rm factor}$, the results begin to spread out over a wider range of \Prot possibilities (with some of them yielding multimodal \Prot estimates), but still within a given range (\Prot = $31.1_{-3.2}^{+4.6}$ days) that is statistically indistinguishable from the values provided by the best indicators (\Prot = $35.7$ $\pm$ $1.4$ days). Therefore, we interpret that, as we consider more reliable estimates of \Prot, the rotational signal of HIP 102152 becomes progressively stronger, converging into a sharp distribution of possibilities that peak at $\sim$36 days.

In Fig. \ref{fig:rot_indicators}, left panel, we show the $p_{\rm QP}$ of chromospheric indicators. Three scenarios were analyzed: the first one (in blue), we combined the $p_{\rm QP}$ of the best indicators ($\log B_{\rm factor} > 2$). The second one (in red) is given by the combination of all indicators used in this work. The last scenario (in black) is  based on the weakest rotation indicators derived for HIP 102152 ($\log B_{\rm factor} \leq 2$). In Fig. \ref{fig:rot_indicators} (right panel), we summarize the results found for each indicator. The mode of each posterior distribution gives the centroid of the error bars, and the width of the same distribution represents the error bars at 60\% of its height. The red shaded region shows the 95\% confidence interval for \Prot estimates using the best indicators (\Prot = 35.7 $\pm$ 2.8 days, $\pm2\sigma$).
\begin{table}
\caption{Rotation periods derived for \ion{Ca}{II} lines and H$\epsilon$ according to the QP model. $B_{\rm factor}$ is given by the ratio between QP and Constant model posteriors.}
\begin{center}
\begin{tabular}{c c c}
\hline
 Indicator & \Prot & $\log B_{\rm factor}$\\
\hline
 \ion{Ca}{II} K & 36.1$_{- 3.3}^{+ 3.8}$  & $+$70.91 \\
 \ion{Ca}{II} S (H+K) & 36.1$_{- 2.0}^{+ 2.6}$  & $+62.54$ \\
 \ion{Ca}{II} H & 36.1$_{- 3.1}^{+ 4.6}$  & $+58.63$ \\
H$\epsilon$ & 34.3$_{- 2.5}^{+ 2.5}$  & $+6.94$\\
\hline
\end{tabular}
\end{center}
\label{table:prots}
\end{table}
\begin{figure}

  \begin{minipage}[t]{1 \linewidth}
\centering
    \resizebox{\hsize}{!}{\includegraphics{FIGURES/PROT_INDICATORS1.pdf}}
  \end{minipage}
  \begin{minipage}[t]{1 \linewidth}
\centering
    \resizebox{\hsize}{!}{\includegraphics{FIGURES/PROT_INDICATORS2.pdf}}
  \end{minipage}
  \caption{\textit{Left panel:} joint \Prot probability distribution for 3 combinations of indicators: best (in blue), all (red), and weakest (black) indicators. \textit{Right panel:} \Prot mode and errors for each one of the best indicator as a function of its QP model statistical significance in comparison to Constant model. The red shaded region is the 2$\sigma$ region around 35.7 days.}
\label{fig:rot_indicators}
\end{figure}
The star HIP 102152 was monitored photometrically in short cadence mode (2 minutes) by \tess\ mission along with its sector 1 (camera 1, CCD 4, between MJD = 58325.3 and 58353.2 days). We extracted the light curve from target pixel files using the \textit{lightkurve} python package \citep{lightkurve18} and corrected the long-term pointing jitter using \textit{Pixel-Level Decorrelation} method \citep[PLD,][]{luger16}. Because of the restricted time span of 27 days, we could only assign an upper limit for HIP 102152 variability, which is $>$ 27 days. Still, it is possible to go one step further, bracketing the photometric information from one side and the \Psini from the other (see Table \ref{table:id}). To do so, the corrected light curve was binned in chunks of 10 h and then, we applied our QP model, now with an additional \Prot prior given by the Survival function $\mathcal{S}$($\mu \equiv$\Psini$=34.8$ and $\sigma = 4.7$ days) resulting in $P_{\rm rot , TESS, P/\sin i} =  34.4_{-6.2}^{+ 6.9}
$ days ($\log B_{\rm factor} = 21$).

\section{Future of the Sun: HIP 102152 in the context of magneto-rotational evolution}

With $\sim$36 days of rotational period and $\sim$8 Gyr, HIP 102152 lies at a critical region, where the evolutionary speed increases and the physical effects accumulated over the entire stellar lifetime become more relevant, such as radius dependence \citep{reiners12}, mass loss rate \citep{fionnagain18}, magnetic field geometry \citep{petit08}, and metallicity \citep{lorenzo16,amard20}. Therefore, it is possible to constrain rotational models better and start to unveil the solar evolutionary path within $\sim$3.5 Gyr from now.

After the solar age, solar mass stars become very inactive and with their surfaces dominated by plages \citep[unlike the younger counterparts dominated by spots,][]{hall09}. The balance between plages and spots can introduce different signatures in the light curves as we vary the stellar metallicity \citep{witzke20}. Besides the possible systematic trends in light curve extraction techniques \citep{cui19}, this spot/plage balance hampers the \textit{true} \Prot detection \citep{reinhold19} and also makes the interpretation of the light curves not straightforward, requiring sophisticated approaches \citep[e.g.][]{amazogomez20}. On the other hand, spectroscopy as a benchmark technique is a good alternative because it carries a wealth of important physical information \citep{strassmeier18}, as a large number of activity tracers throughout the optical to near-infrared spectral regions. In the case of \ion{Ca}{II} lines, for example, they are collisionally controlled set of lines formed in the lower chromosphere. Besides, its response to the increase of plage coverage \citep{meunier09} makes it an interesting rotational discriminator for \textit{plage-dominated} old stars.

It is expected that close-in massive planets \citep[or engulfed planets,][]{melendez17} can significantly alter the stellar rotational evolution \citep{ferrazmello15} for a considerable amount of time. We investigated these possibilities from planetary engulfment point of view and possible presence close-in massive planets. This star has the same abundance pattern as a function of the condensation temperature in comparison to the Sun (M13), showing no sign of enhanced refractories due to planet engulfment. Nearby massive companions are also unlikely since the radial velocity variations over the time span of observations are less than a few m/s, which excludes the possibility of both binarity and the presence of nearby massive planets.

Therefore, we can consider HIP 102152 as a genuine old \textit{solar proxy} that may give us an exciting chance to understand the future of the Sun in many ways. From the magnetic evolution side, during the 10 years of observations, its low level of activity never reached the solar activity typical level. This corroborates the scenario of activity evolution towards the end of the main-sequence \citep[see][]{lorenzo18}. Possibly, HIP 102152 approached to the basal level of activity. According to \citep[][hereafter M18]{mittag18}, when the star's activity converges into the basal flux level, it is reasonable to expect a change in the dominant components of the stellar dynamo (from a vigorous global magnetic field to small-scale turbulent components). M18 points out that this stage would occur around Ro $\sim$ 1. In other words, the dynamo of stars with slow rotation will no longer be dominated by rotational effects. We use the activity and $\tau_{\rm conv}$ relations found in M18 to be 39 $\pm$ 6.3 days (value close to \Prot = 35.7) and Ro = 0.91 $\pm$ 0.15, respectively for HIP 102152. The chromospheric activity corrected from basal component is $\log R_{\rm HK}^{+}$ $\sim$ $-$5.2 \citep[$\log R_{\rm HK, \odot}^{+}\sim-5.06$,][]{mittag13}. For comparison, this star lies in the lower part of the activity$-$Ro diagram shown in M18. Based on these values, we estimate that HIP 102152 will reach Ro = 1 in less than 0.5 Gyr from now (according to the models used in LO19), a negligible age interval that makes it statistically within the expected region of basal flux dominance. In brief, LO19 built \Prot tracks from modified Kawaler wind-law and  \textrm{YaPSI} models \citep{spada17}. LO19 assumed the dominance of structural effects over magnetic braking terms whenever the star approaches into the turn-off region or a given Rossby number ($Ro_{\rm crit}$), leaving only the moment of inertia to drive the subsequent \Prot evolution.

Alternatively, around $\sim$4 Gyr or a critical value of Ro (Ro$_{\rm crit} \sim2$,  note that the $\tau_{\rm conv}$ here is in a different scale to those obtained by M18), it is hypothesized that stellar rotation will no longer be sufficient to maintain an organized global dipole field, giving preponderance to the higher-order multipole components \citep{metcalfe16}. As these components are not expected to be capable of efficiently draining angular momentum via winds \citep{see19}, in comparison to the global dipole geometry, it is argued that the rotational evolution of solar mass stars older than 4 Gyr would be driven only by structural variations (VS16). As seen in Fig. \ref{fig:rot_age}, HIP 102152 (red cross) fits properly to the scenario of smooth rotational evolution described in LO19 (see their Fig. 2), with no need to introduce any additional degree of freedom to emulate the angular momentum loss inefficiency around 4 Gyr (Ro$_{\rm crit}\sim$2). The shaded region in blue is the prediction band for smooth rotational evolution models of 0.97 $\pm$ 0.06 $M_\odot$ ($\pm2\sigma$). As \feh$\sim$ 0.00, we restricted our analysis to the solar metallicity tracks. LO19 used a sample of solar twins with measured \Prot and determined the most probable age for a magnetic transition, finding $\gtrsim8\, $Gyr or Ro$_{\rm crit}$ = $2.6^{+\infty}_{-0.1}$. These values are in line with M18 prediction. Therefore, stars of $\sim$1 solar mass travel along the main sequence without undergoing any dynamo disruption. For the sake of consistency, if this transition still occurs along the main sequence lifetime, a conservative lower limit within $2\sigma$ was estimated to be Ro$_{\rm crit}\gtrsim$ 2.3 (or $t_{\rm crit}\gtrsim$ 5.3 Gyr). We repeated the same procedure adopted in LO19 to derive the  probability distribution for Ro$_{\rm crit}$ yielding $\gtrsim$2.8 (or $t_{\rm crit}\gtrsim$9 Gyr). The only difference between our procedure and those from LO19 is that we are deriving the probability for a single star instead of a joint probability given by a sample of solar twins.
\begin{figure}
\centering
  \begin{minipage}[t]{1 \linewidth}
\centering
    \resizebox{\hsize}{!}{\includegraphics{FIGURES/AGE_ROTATION.pdf}}
  \end{minipage}
  \caption{Age-Rotation diagram with model predictions for 0.97 M$_\odot$ star using modified Kawaler wind-law and  \textrm{YaPSI} tracks \citep{spada17}. The red cross is HIP 102152, and the Sun is represented by its usual symbol. The shaded region is the 2$\sigma$ prediction band.}
\label{fig:rot_age}
\end{figure}
\section{Conclusions}
We use high cadence HARPS observations to provide constraints to the possible solar magneto-rotational evolutionary path $\sim$ 3.5 Gyr from now when it is near to leave the main sequence. As the chromospheric modulations in old stars are very subtle, we approached this issue in multiple ways to detect the rotational signal. We derived several activity indices throughout the spectral coverage of HARPS and tested their sensitivities against the weak rotational signal of HIP 102152. To do so, quasi-periodic models based on Gaussian processes were used. We found that \ion{Ca}{II} K line stands out as the most sensitive indicator ($B_{\rm factor}\sim10^{70}$), followed by the \ion{Ca}{II} S index (H$+$K), and H$\epsilon$. For the best indicators, it was detected a \Prot of 36 $\pm$ 1.4 days with very high statistical significance. Both \tess\, photometry and projected rotational period (\Psini) are consistent with the spectroscopic indicators. These values are in full agreement with the expected rotation for an 8 Gyr-old, 1 solar mass, and solar metallicity star, in opposition to the weakened magnetic braking scenario from VS16. Thus, HIP 102152 supports the smooth rotational evolution of the Sun and validates the use of gyrochronology \citep{barnes07}.

\section*{Acknowledgements}
We thank the anonymous referee for useful comments that helped improve this manuscript. D.L.O is grateful to the tenacious Brazilian workers and taxpayers, whose effort enabled the existence of this project.
D.L.O. and J.M. thanks support from FAPESP (2016/20667-8; 2018/04055-8). G.P. acknowledges the support from CAPES, FAPESP, and MackPesquisa fundings. J.Y.G. acknowledges the support from CNPq.

\bibliographystyle{mnras}

redpajama_set_name: RedPajamaArXiv


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What's the Deal with 'Survivor: Island of Idols'
By Dustin Rowles | TV | September 11, 2019 |
When you're an adult with three kids with a fairly sizable age-discrepancy, there's not a lot of suitable television you can watch together as a family. I don't think it was until I had kids that I really began to understand the appeal of reality television. At the moment, we have basically four "family shows": Nailed It, Queer Eye, The Amazing Race and Survivor. We've gone back and watched almost every season of The Amazing Race and Survivor (or at least, those seasons in high definition, because pre-HD is like black-and-white to kids). I genuinely love it — it's my favorite 42 minutes of the day, and the twins are so invested in the characters on Survivor that they'll often hide behind the couch during Tribal Council because they hate to see certain players go home. They get deeply into it.
In any respect, the kids have been asking for weeks when the next season of Survivor starts, although they have expressed some reservation about Survivor: Island of the Idols because they do not care for Sandra, because they're not fans of the villainous Survivor players (I was so excited about showing them season 16 when Eric was voted off after giving up the immunity idol — the most boneheaded move in the history of Survivor — but they were hugely disappointed because they thought Eric was a good guy because, you know, he's an "ice cream scooper," and when you're seven years old, that' s a big draw).
In any event, the upcoming season — the 39th, which premieres on September 25th — has an additional twist that I'm not sure I'm keen on, either. Rob Mariano (Boston Rob) and Sandra Diaz Twine (who have 3 wins and 7 seasons between them) are returning to Survivor, not as players but as mentors. The two will set up shop on something akin to Exile Island — they'll build their own shelter together and live out there for presumably the duration. When a player gets sent to the Island of the Idols, they'll have the opportunity to talk about gameplay and learn certain survival skills from Rob and Sandra. The exiled player will also be offered the opportunity to compete in challenges using the skills provided to them by Rob and Sandra. Should they succeed in the challenge, they will win advantages or idols. However, if they lose the challenge, something bad will happen, which could completely upset their game. The exiled players, however, also have the option of not competing in a challenge: No harm, no foul.
From Jeff Probst, via EW:
"For the person who is foolish enough to take the test and fail, they say, 'Here's your other life lesson, you should have never gone up against me. I'm the one who just showed you that. I'm an expert. And now you're in trouble. Here's how you recover.' And if somebody says, "I'm no fool, I don't want to go up against you," [Rob and Sandra] were given the freedom, their own decision, to raise the stakes. So we gave them a cushion and said, you can go from here to here with the advantage. Whatever you want."
Essentially, it's a form of Survivor haggling and betting all rolled into one. "So Sandra could lean in and say, 'What if we make an idol good for three Tribal Councils?'" says Probst. "Now you're interested. And then the player might say yes. And they might still lose. And Rob might say 'Why did you change your mind simply because the advantage got bigger? Your odds didn't.' So that's the basic premise."
Eh. It's not my favorite premise, and I assume by the ninth or tenth day once the audience has gravitated toward certain players, Sandra and Rob will be in the way more than anything. Still, it's better than the clusterf*ck Edge of Extinction, in which almost every eliminated player found themselves living on a separate island vying for an opportunity to return, which might have been more interesting (and fair) if the fate of a player who had been out there for 30+ days did not rest on a single challenge.
The rumor, however, is that season 40 will be an All-Winners season, one in which Boston Rob and Sandra will return again, along with Rob's wife, Amber, and of course the best guy who ever played the game, Yul.
Meanwhile, if you're interested, here's the cast for the upcoming season.
Dustin is the founder and co-owner of Pajiba. You may email him here, follow him on Twitter, or listen to his weekly TV podcast, Podjiba.
Header Image Source: CBS
Jokes Seth Can't Tell: No One Inside a Black Restaurant Has Ever Heard of Seth Meyers
Review: 'The New Pope' Proves There's Still Plenty Of Life After 'The Young Pope'
Review: HBO's 'The Outsider' is Moodily Atmospheric and Tightly Plotted, with a Righteously Good Ensemble Selling the Spooky Stuff
'Underwater' Review: Next Time I Hope Cthulhu Wins
Review: Hopelessly Uninspired 'Like A Boss' Unlikely to Entertain
Review: The Sixth and Final Season of 'Schitt's Creek' Maintains its Delightful Kookiness for a Bittersweet Goodbye
Pete Davidson and Kaia Gerber Spending Time Apart, Probably to Cindy Crawford's Relief
Hugh Grant Says it's 'Such a Relief' to Not Play Nice Guys Anymore
Bravo's 'Below Deck' Kate Chastain is the Queen of Competency Porn

redpajama_set_name: RedPajamaCommonCrawl


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text:
Issue: The verdict is only the beginning of a powerful movement
"George Floyd mattered… he mattered because he was human." –Minnesota Attorney General, Keith Ellison
The world was watching yesterday as the jury delivered the verdict of Derek Chauvin, the police officer that killed George Floyd in May of 2020. Chauvin was found guilty on all accounts for second-degree murder, third-degree murder and second-degree manslaughter.
While this news is a brief reprieve from the year of protests, pain and worry amongst the Black community, there is still work to be done.
Americans have already made their outrage clear, taking to the streets and protesting Floyd's death over the last summer. South Dakotans joined them, with protests occurring in Sioux Falls, Rapid City, Pierre, Mitchell and right here in Brookings. We wanted justice, and yesterday some justice was served.
Floyd should still be alive today, and at the end of the day, this verdict does not bring him back to life.
However, it is a testament to the year's work on anti-racism and the Black Lives Matter movement that went into making Floyd's death a nationwide issue.
This is accountability, but it is only the start.
Chauvin is only the second police officer in Minnesota history that has been convicted of murdering a civilian while on active duty.
Police brutality still runs rampant through the streets in America. Only 10 days ago, Daunte Wright, another Black man from Minnesota, was killed by a female officer who mistook her gun for a taser.
There are too many officers who have killed Black people in this country. Accountability needs to be taken for each and every one of them, starting with J. Alexander Kueng, Thomas Lane and Tou Thao, the officers assisting Chauvin in Floyd's death.
Racism in our law enforcement is not the only place we need to look to for change; our universities must be held accountable when incidents like the racist message found on campus this past January occur.
It's important that we hold everyone —our police officers, government and even university and school officials—accountable, and though this trial will hopefully begin to change things for the better, our fight isn't over yet.
In the end, we can't bring George Floyd back to life. We can only honor his legacy and stand behind the Black community as the fight for justice continues.
The Collegian Editorial Board meets weekly and agrees on the issue of the editorial. The editorial represents the opinion of The Collegian.
Email [email protected]om


text:
Q: PROBLEMA AO CLICAR COM UM ROBÔ USANDO PUPPETEER Eu estou criando este robô para automatizar algumas tarefas do eu dia a dia, eu peço para ele acessar o site, clicar no input, e depois logar. Ele acessa a pagina, Mas ele não está clicando, não consigo achar o problema. este é o código

const puppeteer = require('puppeteer');

(async () =>{
    const browser = await puppeteer.launch({ headless: false });
    const site = 'http://www.goolsystem.com.br';
    const page = await browser.newPage();
    await page.goto('http://www.goolsystem.com.br/4/Login.aspx?ReturnUrl=%2f4');
    await page.waitFor('#ucTrocarModulo_btnIconeUrbano > input');
    await page.click('#ucTrocarModulo_btnIconeUrbano > input');
    await page.type('input[name="ucLogarUsuario$txtLogin"]','@@@@@', {delay: 100});
    await page.type('input[name="ucLogarUsuario$txtSenha"]', '@@@@@', {delay: 100});
    await page.keyboard.press('Enter');

    await browser.close();
})();

quando eu executo mostra o seguinte erro: "(node:5920) UnhandledPromiseRejectionWarning: Unhandled promise rejection. This error originated either by throwing inside of an async function without a catch block, or by rejecting a promise which was not handled with .catch(). To terminate the node process on unhandled promise rejection, use the CLI flag --unhandled-rejections=strict (see https://nodejs.org/api/cli.html#cli_unhandled_rejections_mode). (rejection id: 1)
(node:5920) [DEP0018] DeprecationWarning: Unhandled promise rejections are deprecated. In the future, promise rejections that are not handled will
terminate the Node.js process with a non-zero exit code."

A: O seletor do input que deseja clicar esta errado, o id do seletor pai é ucTrocarModulo_moduloUrbano e você esta utilizando o id do seletor filho que é ucTrocarModulo_btnIconeUrbano (o input) e tentando buscar um input dentro do mesmo, ou seja, você esta tentando clicar um input dentro do input que você quer clicar, como não existe ele apresenta o erro.
Opções corretas:
1 - #ucTrocarModulo_moduloUrbano > input
2 - #ucTrocarModulo_moduloUrbano #ucTrocarModulo_btnIconeUrbano
3 - #ucTrocarModulo_btnIconeUrbano
Você pode utilizar o ID do elemento diretamente (como na opção 3). Tente isso:
const puppeteer = require('puppeteer');

(async () =>{
    const browser = await puppeteer.launch({ headless: false });
    const site = 'http://www.goolsystem.com.br';
    const page = await browser.newPage();
    await page.goto('http://www.goolsystem.com.br/4/Login.aspx?ReturnUrl=%2f4');
    await page.waitFor('#ucTrocarModulo_btnIconeUrbano'); // ID do input
    await page.click('#ucTrocarModulo_btnIconeUrbano'); // ID do input
    await page.waitFor('#ucLogarUsuario_txtLogin');
    await page.type('#ucLogarUsuario_txtLogin','@@@@@', {delay: 100}); // ID do input Login
    await page.type('#ucLogarUsuario_txtSenha', '@@@@@', {delay: 100}); // ID do senha
    await page.keyboard.press('Enter');

    await browser.close();
})();

redpajama_set_name: RedPajamaStackExchange


text:
Home News Local Manitoulin Arts and Culture Council celebrates first anniversary
Manitoulin Arts and Culture Council celebrates first anniversary
Michael Erskine
KAGAWONG—The Manitoulin Arts and Cultural Council (MACC) has passed a seminal milestone and will be marking its first anniversary with a celebratory meeting at the Kagawong Park Centre.
"This month marks the first anniversary of the MACC," noted organizer author Kate Thompson. "To make our monthly meeting special, we're going to hold it at the Kagawong Park Centre from 1:30 to 3:30 pm."
Spokesperson Alex Baran of Providence Bay noted that MACC grew out of an initiative of LAMBAC two years ago that sought to bring a profitable coherence to the arts and artistic community on Manitoulin.
"Out of that first conference at the Manitoulin Hotel and Conference Centre we held a day of action at the Kagawong Park Centre," noted Mr. Baran. "About 40 people came out and the decision was made to try and give birth to something," he said. Four committees came from that meeting, dealing with structure, communication, innovations/ideas and programming. "Two committees eventually merged," he said. "One of the things that happened out of that final meeting was that we said 'let's try to have something come out of this that represents the thinking that has gone on to date'," said Mr. Baran. Throughout the intervening months the MACC, made up of a number of local artists and interested people, met either in person at Mr. Baran's home in Providence Bay or, more innovatively, by SKYPE. "It's been great," he said of the technological meeting space. "Instead of having to brave the winter roads in January and February we were able to get together in the warmth and safety of our own homes."
The meeting at the Kagawong Park Centre taking place this Sunday, June 21 will provide an opportunity for those who attended the original meeting to be briefed on what has been accomplished to date, as well as to learn about a couple of important possibilities for Manitoulin.
As part of the celebrations, LAMBAC's Maureen Strickland will speak to the meeting about the new Artist Investment Program (an extremely useful and reasonable loans program) being offered by the community investment corporation. Ms. Strickland will also be exploring the topic of 'Cooperatives for Creative Communities.'
"Cooperatives are really Maureen's lifelong area of expertise," noted Mr. Baran. "We are really hoping she will opine on how that model could provide an untapped opportunity that exists here where no other model will work."
"We'll have a quick review of what we've done this past year and what projects we have on our calendar," added Ms. Thompson. "We invite you to bring one or two samples of your work to exhibit, for everyone to enjoy for the day. We hope to raffle off a very special item – a surprise."
MACC is inviting the original attendees and anyone involved or interested in promoting the arts on Manitoulin Island to "come and reconnect with the Manitoulin's creative community; we look forward to seeing you!"
The anniversary meeting will take place Sunday, June 21 from 1:30 to 3:30 pm at the Kagawong Park Centre.
Arts and Cultural Council celebrates first anniversary
New abattoir owners to Cattlemen: come on down
SPRING BAY - One of the new owners of the Manitoulin abattoir, George McGaffin of Limestone Island Abattoir, joined Birgit Martin of...


20 Aug 2018 / 21:15 H.
THERE is little sense in grading a new government on its performance in its first 100 days in office especially if it has just replaced the world's longest running coalition in power, which had degenerated into a notorious kleptocracy in its last phase.
The Pakatan Harapan (PH) itself had set the stage for this evaluation by pledging to fulfil 10 promises within 100 days in its election manifesto.
The 100 days idea is nothing more than a political fad that originated with the Franklin Roosevelt presidency in the US. It is totally inappropriate in our context when the momentous change that occurred on the May 9 and the monumental challenges that have unfolded since then require an appraisal that is continuous and comprehensive.
It is that sort of appraisal that society should provide as feedback to the PH government. It should be non-partisan and as fair and unbiased as possible. The aim would be to encourage the positive dimensions in the PH's governance and to caution against negative aspects of its performance.
Since corruption and abuse of power associated with the previous Barisan Nasional government was a major factor in its downfall, the PH leadership is doing the right thing in exposing the terrible wrongdoings related to the 1MDB scandal and other financial shenanigans. Understandably, the focus has been upon the former prime minister, Datuk Sri Mohd Najib Abdul Razak and upon the handbags, jewellery and other expensive acquisitions of his wife, Datin Sri Rosmah Mansor.
In the course of these revelations, the Malaysian public has become acutely aware of the massive debts that the government had accumulated in recent years. In order to reduce these debts, mammoth projects undertaken with Chinese companies and the Singapore government have had to be cancelled or postponed.
For the people, especially those who were once unquestioningly loyal to Najib, the realisation that a leader that they revered had betrayed their well-being could be a traumatic experience. Nonetheless, one hopes that coming to grips with the truth in this painful manner will, at the collective level, lead to a catharsis – a catharsis of the Malaysian soul that will fortify us, all of us, against the scourge of corruption.
Apart from baring the ugly face of corruption and its consequences, the PH government has also sought to address some of the woes of the people as expressed during the election campaign. It has abolished the unpopular goods and services tax; stabilised the price of petrol and introduced targeted petrol subsidies; eliminated unnecessary debts imposed upon Felda settlers; and postponed the repayment of PTPTN loans for graduates whose salaries are below RM 4,000 per month.
The government has also acted against two institutions related directly or indirectly to national unity. It has abolished the Biro Tata Negara (BTN), which many felt did not conduce towards the promotion of better ethnic relations. And it has also dismantled the National Service Programme, which earlier studies had shown made very limited contribution to the integration of young adults.
While these are among the many positive measures, one should not ignore the gross errors and outright fumbles committed by the new government and entities associated with it.
I shall highlight just one. For a short while in July, Malaysia found itself in an embarrassing situation with two chief justices. It arose partly because in hastening a transition of authority in the Judiciary, respect for the independence and integrity of the institution was set aside.
In spite of this and other flaws, the PH government continues to enjoy the trust and confidence of the vast majority of the people as reflected in a number of surveys.
It is perceived as sincere in its endeavour to rectify the shortcomings of the previous government. Prime Minister Tun Dr Mahathir Mohamad's pivotal role in ousting Najib and the commitment displayed by this 93 year-old leader in planning and executing important changes since May 9, explains in part the high level of public trust in the government of the day.
Nonetheless, Tun and his government will be facing monumental challenges in the days ahead. Even in combating corruption – the first of seven challenges – it has yet to present to Parliament a Bill to regulate political financing and to make electoral funding transparent.
The declaration of the assets and liabilities of Ministers and Deputy Ministers at the federal level to the public through the Malaysian Anti-Corruption Commission is awaiting implementation. Other proposals on barring close relatives of power-holders from bidding for Federal or state government contracts and projects or on minimising and eliminating the role of "middle-men" and proxies in procurement exercises involving Federal and state entities have not been pursued with vigour.
Strengthening democracy has been largely about rescinding laws such as the Sedition Act, and Sosma, among others. But even this remains an unfulfilled promise. However, enhancing human rights must mean more than rescinding authoritarian laws. Some of the vile and vicious excesses of the social media have convinced a lot of human rights advocates of the importance of integrating rights with responsibilities. A more profound commitment to responsibilities at all levels could help develop a deeper attachment to the principle of Amanah (Trust), which in turn will reinforce the spiritual-moral foundation of life and society.
An equally crucial challenge confronting the PH government is the situation of the relatively poor and disadvantaged. Increasing and equalising the minimum wage nationally is one of the prominent PH pledges. The government is also very much aware of why improving the quality of public housing, public education, public health-care, public transportation, and public amenities in general will impact positively upon the life of the poor.
But relative deprivation in a society like ours cannot be overcome unless one also regulates the huge salaries, bonuses and perks that the affluent minority regard as their privilege. There is no sign to suggest that the PH is moving in that direction in a concerted manner.
A fourth fundamental challenge revolves around ethnic relations. Remarks and demands made within and without the PH by different individuals and parties in the first 100 days reveal ethnic and religious fault lines that the coalition has not dealt with as a grouping.
For instance, the uneasiness among some Malays caused by certain senior government appointments indicates not only a lack of appreciation of the Constitution but also points to a superficial understanding of what citizenship in a modern society entails.
Similarly, grossly inaccurate views about the ethnicity of ancient communities in the region, the flow of peoples within Nusantara and the reality of colonial migration and its adverse impact upon contemporary ethnic relations, shows how much ignorance prevails even among top political leaders in PH.
Indeed, one gets the impression that the PH has not really imbued its leadership and membership with knowledge and understanding of how the Malaysian nation-state evolved essentially from Malay Sultanates shaped by the colonial experience and the non-Malay presence.
Without such understanding, it will be difficult to navigate ethnic relations in the country.
PH has also got to deal with the rising crescendo of calls for greater autonomy from the citizens of Sarawak and Sabah. Enforcing the Malaysia Agreement of 1963 is a PH promise though very little appears to have been done in concrete terms. Genuine autonomy for the two states will require a re-appraisal of the federal structure itself.
Forging a foreign policy of dignity that safeguards Malaysia's independence and sovereignty has become a much greater challenge today than it was when Mahathir first became Prime Minister in 1981. The US' negative response to the rise of China in recent decades has transformed Asean into a potential cockpit of conflict. To minimise tension and to avert serious friction, Malaysia together with its Asean neighbours will have to engage not just the US and China but also other states in Asia such as Japan, the Koreas, India and Pakistan in constructive dialogue.
Finally, in order to handle all these challenges, a seventh challenge centred upon PH itself. While we acknowledge that it is a new coalition of four parties, we realise that because it is in power and forced to grapple with monumental challenges, it has no choice but to demonstrate a high degree of cohesion and unity. On many issues of governance it has already achieved an appreciable measure of consensus.
However, the same cannot be said for issues of identity related to ethnicity and religion. For coalitions linked to ethnic and religious communities, directly or indirectly, the politics of identity would be as critical as the ethics of governance.
To evolve a viable understanding on the politics of identity, PH's leading personalities from all the parties will have a decisive role to play. One hopes that heart-to-heart communication among them will lead to greater empathy across ethnic and religious boundaries. It is such empathy – and such empathy alone – that will sustain PH in the years to come.


LSU Ag Center, September 2006. 16 pages.
This report addresses concerns of the proper use and management of poultry litter and how poultry growers have developed "environmentally friendly" alternatives to conventional litter management. Produced by Louisiana State University. The report focuses on the Louisiana broiler industry, where poultry production is the largest animal agricultural industry, seconded only to forestry production.


A girl, Camryn Nicole Plaxco, was born on June 25, 2007, to Curt Plaxco of Wichita Falls and Heather Plaxco of Fort Worth at Harris Methodist Erath County Hospital.
She weighed 8 pounds and 11 ounces and was 20 inches long.
Welcoming her home are a sister, Jessica Plaxco, 15; and a brother, Parker Plaxco, 3.
Grandparents are Dorothy and Robert Hamblin, Mark and Lisa Lockwood, Jim and Carol Taylor, and Gaines and Jo Ann Plaxco.
Great-grandparents are Terry and Angie Lockwood, Ed Hulvey, Marguerite Hamblin, and Frog and Margie Streit.
Twin girls, Jasmine and Anita Prasittipol, were born on April 24, 2007, to Amita Cheersomsuk and Pakpoom Prasittipol of Thailand at the Palo Pinto Hospital.
Jasmine weighed 3 pounds and 15.6 ounces and was 17 inches long. Anita was 4 pounds and .04 ounces and was 17 1/2 inches long.
Grandparents are Aksorn and Somchai Cheersomsuk from Bangkok, Thailand; and Samruam and Tipawan Prasittipol from Chantaburi, Thailand.
A girl, Oaisia Kay Watson, was born on July 12, 2007, to Jessica Roberts and Shannon Watson at Harris Methodist Erath County Hospital.
She weighed 6 pounds and 13 ounces and was 20 1/2 inches long.
Grandparents are Jeanie and Ken Watson and Laura and Floyd Dennis.
Great-grandparents are Dimple Watson, Herold Welch, and Alva Walton.
Other special family members include aunts, Jennifer Watson and Crystal Roberts.
A girl, Charity Rose Lesa Taylor, was born on June 14, 2007, to Ty and Cherry Taylor of Comanche at Harris Methodist Erath County Hospital.
She weighed 7 pounds and 14.8 ounces and was 20 inches long.
Welcoming her home are sisters, Natalie Hope Derrick, 26, and Joanna Faith, 7; and brother, Trice III, 5.
Grandparents are the late Trice Taylor, Peggy Jo Taylor of Nederland, and Cosme Batalla and Agrifina Batalla both of the Philippines.
Great-grandparents are the late Garett and the late Lucille Rauwerda, the late Edgar and the late Catherine Taylor, Alfonso Batalla and wife, the late Teodora.
Aunts and uncles are Tom and Shelly Glynn and Charlie and Joann Mingming.
Cousins are Angie, Anneliesa, Mandy, Michael, Allison, Ellaine Joy, and Ellis Jordan.


text:
Jenny Milam
Jenny Milam is a writer, editor, motion designer, and wearer-of-many-other-hats living in Atlanta. She's a pop culture junkie, astrology geek, fair to middling gamer, and collector of Funko Pops and tarot decks. When she's not writing you may find her talking someone's ear off about Game of Thrones (yes, still) or beating her husband's ass at Magic: The Gathering.
Everything Coming to Netflix in October
Spooky season is in full effect as new content starts arriving on Netflix in October! But when will we finally get to see the Netflix Original series 'Wednesday'?
Jenny Milam September 30, 2022
Everything Coming to Netflix in September
For the month of September, expect to see tons of new content from Netflix.
Jenny Milam September 1, 2022
Samantha's Fate Revealed in 'And Just Like That' Premiere
We've got all the details of what to expect from 'And Just Like That…" the next chapter of the Sex and the City universe.
Jenny Milam December 9, 2021
Written in the Stars or Destined to Fail? What Astrology Has to Say About Tom Holland and Zendaya
Want to know what astrology has to say about your celebrity couple crush? We're breaking down the birth charts of Tom Holland and Zendaya, and finding out if this duo is written in the stars.
What Your Disney Generation Says About You
There's no question our childhoods were all influenced by Disney. But have you thought about how different that influence might be depending on when you were born?
Jenny Milam June 18, 2021
The Critics Choice Super Awards: Finally, An Awards Show for the Spookier, Geekier Side
Nominations for the inaugural Critics Choice Super Awards have been announced. And we're thrilled to see our favorite genres finally getting the critical acclaim they deserve. The Critics Choice Awards has historically focused on both film and television accolades. But it's created spinoffs for more niche areas of entertainment in
Jenny Milam November 19, 2020
Here's Everything We Know About the Upcoming 'Fresh Prince' Reunion
Now, this is the story all about how… an entire generation of humans can finish that line. It's been stuck in our heads for these last couple of months, as we've been teased with news of our favorite Bel-Air family's return to TV. First, there was the viral video of
These Bachelor Nation Stars Say They Were Manipulated by Producers
On Tuesday, Trista Sutter—the first-ever Bachelorette—made an appearance on the LadyGang podcast and opened up about how her fairytale wedding to Ryan Sutter was in many ways orchestrated by the show's producers behind the scenes. For one, the show dictated that runner-up Charlie Maher serve as emcee for the evening.
CBS Rolls Out Diversity Targets for Unscripted Programming
CBS is making serious strides to improve its diversity both on- and off-camera. On Tuesday, the broadcast network announced its representation targets for unscripted content in the 2021/2022 season. These include an edict that 50% of reality show casts must be Black, Indigenous, or People of Color (BIPOC). They've also
Hilarie Burton and Jeffrey Dean Morgan Are Bringing Their Real-Life Chemistry to 'The Walking Dead'
We finally get to meet the inspiration behind the infamous Lucille on The Walking Dead. According to reports, and the actress herself, Hilarie Burton will be joining real-life husband Jeffrey Dean Morgan on the long-running show during at least one of the bonus episodes slated for season 10. "Been pretty
Jenny Milam November 5, 2020


Fixed an error under DotNetNuke 5.5.x where the ModuleTitle field was no longer accessible from the Modules table. This caused SQL errors on install and when trying to get to the settings page.
Fixed an error under DotNetNuke 5.5.x where the SendToFriend functionality was throwing an error because the call be used for sending email that had previously been deprecated was no longer available.


I admit that I am a John Corey fan, firstly because he is a great detective character who does it his way and secondly for the really funny and mostly obnoxious quips that he makes along the way.
Asad Khalil (aka "The Lion"), is a ruthless Libyan terrorist who menaced ex-NYPD cop John Corey and his wife, FBI agent Kate Mayfield, and planned a major US catastrophe in "The Lion's Game". At the end of that book Khalil told Corey "I just wanted to say good-bye and to remind you that I will be back....I will kill you and kill that whore you are with, if it takes me all of my life." This time Khalil is back in the US planning to avenge those who killed his entire family in a bombing run over Gaddafi's compound in Libya, and everyone who stopped his plans last time.
Kate and Corey are both with the federal Anti-Terrorist Task Force. To destress they go sky-diving together (Corey reluctantly). This book has a fantastic adrenaline filled description of a sky dive gone wrong - sabotaged by Khalil . The book is worth reading for these scenes alone.
Corey then gets caught up in a chase to find Khalil before he can kill again and carry out another catastrophic attack. The chase is a very personal one with both Khalil and Corey tracking one another, but the Lion seems to have the upper hand most of the time.
I really enjoyed this page-turning and exciting John Corey adventure. Corey still had plenty of obnoxious quips, mainly pretty racial ones about Khalil involving camels and towel-heads, and about Khalil's mothers affair with Gaddafi. IMO they weren't up to the standard of those in previous and later books in the series.
This was a revisit as I had read this book when it was published a few years ago. It didn't disappoint.


text:
module PhaseDurationsHelper
end

redpajama_set_name: RedPajamaGithub