Recent developments in the P y SCF program package

Sun, Qiming  (ORCID:0000000305286186); Zhang, Xing  (ORCID:0000000218921380); Banerjee, Samragni; Bao, Peng; Barbry, Marc  (ORCID:0000000151977944); Blunt, Nick S.  (ORCID:0000000222846969); Bogdanov, Nikolay A.; Booth, George H.  (ORCID:0000000325034904); Chen, Jia  (ORCID:0000000273103196); Cui, Zhi-Hao  (ORCID:0000000273894063); Eriksen, Janus J.  (ORCID:0000000185833842); Gao, Yang  (ORCID:0000000323202839); Guo, Sheng  (ORCID:0000000210831882); Hermann, Jan  (ORCID:0000000227790749); Hermes, Matthew R.; Koh, Kevin  (ORCID:0000000204124516); Koval, Peter  (ORCID:0000000254612278); Lehtola, Susi  (ORCID:0000000162968103); Li, Zhendong  (ORCID:0000000206836293); Liu, Junzi; Mardirossian, Narbe; McClain, James D.; Motta, Mario  (ORCID:0000000316479864); Mussard, Bastien  (ORCID:0000000208264719); Pham, Hung Q.  (ORCID:0000000336081298); Pulkin, Artem  (ORCID:0000000293641653); Purwanto, Wirawan  (ORCID:0000000221244552); Robinson, Paul J.  (ORCID:0000000304654979); Ronca, Enrico  (ORCID:0000000304945506); Sayfutyarova, Elvira R.  (ORCID:0000000184035013); Scheurer, Maximilian  (ORCID:0000000305923464); Schurkus, Henry F.  (ORCID:0000000232105929); Smith, James E. T.  (ORCID:0000000251308633); Sun, Chong  (ORCID:0000000282999094); Sun, Shi-Ning; Upadhyay, Shiv  (ORCID:0000000285010501); Wagner, Lucas K.  (ORCID:000000023755044X); Wang, Xiao  (ORCID:0000000314027522); White, Alec  (ORCID:0000000297431469); Whitfield, James Daniel  (ORCID:0000000328730622); Williamson, Mark J.  (ORCID:0000000252957811); Wouters, Sebastian; Yang, Jun  (ORCID:0000000187019297); Yu, Jason M.  (ORCID:0000000222706798); Zhu, Tianyu  (ORCID:0000000320613237); Berkelbach, Timothy C.  (ORCID:0000000274452136); Sharma, Sandeep; Sokolov, Alexander Yu.  (ORCID:0000000326374134); Chan, Garnet Kin-Lic  (ORCID:0000000180096038)

doi:10.1063/5.0006074

Abstract

We present differential Strömgrenuvbyobservations from the Four College Automated Photometric Telescope (FCAPT) in Washington Camp, AZ of eight magnetic Chemically Peculiar (mCP) stars: HD 32966, HD 35298, HD 68292, HD 93226, HD 171247, HD 217833, HD 220147, and HD 223358. We use multiple period‐finding algorithms and incorporate data from the ESA Hipparcos catalogue to study the amplitudes, periods, and asymmetries in the light curves. No previous FCAPT data have been published for HD 68292. For the seven other stars, these studies substantially extend the analyses of published FCAPT datasets.

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