Hi, welcome to our poster, I'm Nymis Tifanos, I would like to share with you our detection of emission of netrion on the design of Wastry 3P. So the modification of this work is that the Tarenmox side was suggested to be responsible uh, species for creating stratosphere or thermal information in the atmosphere of HOTGIPETER. But the problem is that the Tarenmox side has only been detected into HOTGIPETER WAPS 19 and WAPS 3P. So that got us thinking whether the Tarenmox side can really be the main cause for the thermal information in HOTGIPETER. So Lotteringer Errol 2018 suggests that natural iron in a gas phase can also be the responsible uh, agent to create a thermal infarction by absorbing the shot wave radiations from the star and heat up the atmosphere. Therefore we search for the natural iron signature under the design of Wastry 3P using our old datasets. This dataset is the same datasets that we used to detect Tarenmox side in 2017. The data cover the planetary orbital phase of 0.2 until 0.538. We obtain the data using Subaru Telescope and hide dispersion spell graph. To see the detail on the data reduction you can read our old paper NUGRO Errol 2017. Shortly we remove the telegraph and serial lines using the strand and then we cross-code the resolals with the double-shifted natural iron template for various abundance of natural iron. And then we stack the cross-coction function into two dimensional array with the x-axis as the RV and the y-axis as the orbital phase of time. As you can see here because Wastry 3P is a delta-scu-d star so there's a positions. The position can be seen right here. This can lead us to a false positive notation so we want to avoid that. We can also see a duct stripes here as the hour candidate for planetary signals. But to be sure we sum up the cross-coction function at the planetary rest frame assuming various values of orbital velocity or kp and systemic velocity and for various log VMR or the abundance of natural iron. After that we did the likelihood analysis and this is the result. We detected neutral iron emission at the expected planetary velocity. We also found that the data is actually 1.3 stronger than our template. And then we were also able to constrain the abundance of neutral iron but this is only correct for the atmospheric modeling that we use. So is it really true that the stratosphere in Wastry 3P at least is caused by the Tadenokseid or Neutriger? So that's still a question that we want to answer in our future project. So if you want to read the details of our work you can visit our poster or even download our paper and read it. So thank you so much. Have a good day. Bye!