{"id":7,"date":"2021-09-30T12:52:32","date_gmt":"2021-09-30T12:52:32","guid":{"rendered":"https:\/\/teams.issibern.ch\/solarandstellarvariabilities\/?page_id=7"},"modified":"2021-11-04T08:24:39","modified_gmt":"2021-11-04T08:24:39","slug":"publications","status":"publish","type":"page","link":"https:\/\/teams.issibern.ch\/solarandstellarvariabilities\/publications\/","title":{"rendered":"Publications"},"content":{"rendered":"<ul>\n<li style=\"margin-bottom: 0.3cm\">Johnson, L. J., Norris, C. M., Unruh, Y. C., Solanki, S. K., Krivova, N., Witzke, V., &amp; Shapiro, A. I.,<em> Forward modelling of Kepler-band variability due to faculae and spots<\/em>, MNRAS, 504, 4751, 2021, (<a href=\"https:\/\/ui.adsabs.harvard.edu\/abs\/2021MNRAS.504.4751J\/abstract\">ADS link<\/a>);<\/li>\n<li style=\"margin-bottom: 0.3cm\">Sowmya, K., Shapiro, A. I., Witzke, V., N\u00e8mec, N.-E., Chatzistergos, T., Yeo, K. L., Krivova, N. A., &amp; Solanki, S. K., <em>Modeling Stellar Ca II H and K Emission Variations. I. Effect of Inclination on the S-index<\/em>, The Astrophysical Journal, 914, 21, 2021, (<a href=\"https:\/\/ui.adsabs.harvard.edu\/abs\/2021ApJ...914...21S\/abstract\">ADS link<\/a>);<\/li>\n<li style=\"margin-bottom: 0.3cm\">Reinhold, T., Shapiro, A. I., Witzke, V., N\u00e8mec, N.-E., I\u015f\u0131k, E., &amp; Solanki, S. K. , <em>Where Have All the Solar-like Stars Gone? Rotation Period Detectability at Various Inclinations and Metallicities<\/em>, The\u00a0Astrophysical Journal Letters, 908, L21, 2021, (<a href=\"https:\/\/ui.adsabs.harvard.edu\/abs\/2021ApJ...908L..21R\/abstract\">ADS link<\/a>);<\/li>\n<li style=\"margin-bottom: 0.3cm\">Shapiro, A. I., Solanki, S. K., &amp; Krivova, N. A. , Predictions of Astrometric Jitter for Sun-like Stars. I. The Model and Its Application to the Sun as Seen from the Ecliptic, The Astrophysical Journal, 908, 223, 2021, (<a href=\"https:\/\/ui.adsabs.harvard.edu\/abs\/2021ApJ...908..223S\/abstract\">ADS link<\/a>);<\/li>\n<li style=\"margin-bottom: 0.3cm\">Amazo-G\u00f3mez, E. M., Shapiro, A. I., Solanki, S. K., Kopp, G., Oshagh, M., Reinhold, T., &amp; Reiners, A. , <em>Inflection point in the power spectrum of stellar brightness variations. III. Facular versus spot dominance on stars with known rotation periods<\/em>, Astronomy&amp;Astrophysics, 642, A225, 2020, (<a href=\"https:\/\/ui.adsabs.harvard.edu\/abs\/2020A%26A...642A.225A\/abstract\">ADS link<\/a>);<\/li>\n<li style=\"margin-bottom: 0.3cm\">I\u015f\u0131k, E., Shapiro, A. I., Solanki, S. K., &amp; Krivova, N. A. , Amplification of Brightness Variability by Active-region Nesting in Solar-like Stars, The\u00a0Astrophysical Journal Letters,, 901, L12, 2020, (<a href=\"https:\/\/ui.adsabs.harvard.edu\/abs\/2020ApJ...901L..12I\/abstract\">ADS link<\/a>);<\/li>\n<li style=\"margin-bottom: 0.3cm\">Reinhold, T., Shapiro, A. I., Solanki, S. K., Montet, B. T., Krivova, N. A., Cameron, R. H., &amp; Amazo-G\u00f3mez, E. M. , The Sun is less active than other solar-like stars, Science, 368, 518, 2020, (<a href=\"https:\/\/ui.adsabs.harvard.edu\/abs\/2020Sci...368..518R\/abstract\">ADS link<\/a>);<\/li>\n<li style=\"margin-bottom: 0.3cm\">Amazo-G\u00f3mez, E. M., Shapiro, A. I., Solanki, S. K., Krivova, N. A., Kopp, G., Reinhold, T., Oshagh, M., &amp; Reiners, A. , Inflection point in the power spectrum of stellar brightness variations. II. The Sun, Astronomy&amp;Astrophysics, 636, A69, 2020, (<a href=\"https:\/\/ui.adsabs.harvard.edu\/abs\/2020A%26A...636A..69A\/abstract\">ADS link<\/a>);<\/li>\n<li style=\"margin-bottom: 0.3cm\">N\u00e8mec, N.-E., Shapiro, A. I., Krivova, N. A., Solanki, S. K., Tagirov, R. V., Cameron, R. H., &amp; Dreizler, S. , Power spectra of solar brightness variations at various inclinations, Astronomy&amp;Astrophysics, 636, A43, 2020, (<a href=\"https:\/\/ui.adsabs.harvard.edu\/abs\/2020A%26A...636A..43N\/abstract\">ADS link<\/a>);<\/li>\n<li style=\"margin-bottom: 0.3cm\">Witzke, V., Reinhold, T., Shapiro, A. I., Krivova, N. A., &amp; Solanki, S. K. , Effect of metallicity on the detectability of rotational periods in solar-like stars, Astronomy&amp;Astrophysics, 634, L9, 2020, (<a href=\"https:\/\/ui.adsabs.harvard.edu\/abs\/2020A%26A...634L...9W\/abstract\">ADS link<\/a>);<\/li>\n<li style=\"margin-bottom: 0.3cm\">Shapiro, A. I., Amazo-G\u00f3mez, E. M., Krivova, N. A., &amp; Solanki, S. K. , Inflection point in the power spectrum of stellar brightness variations. I. The model, Astronomy&amp;Astrophysics, 633, A32, 2020, (<a href=\"https:\/\/ui.adsabs.harvard.edu\/abs\/2020A%26A...633A..32S\/abstract\">ADS link<\/a>);<\/li>\n<\/ul>\n","protected":false},"excerpt":{"rendered":"<p>Johnson, L. J., Norris, C. M., Unruh, Y. C., Solanki, S. K., Krivova, N., Witzke, V., &amp; Shapiro, A. I., Forward modelling of Kepler-band variability due to faculae and spots, MNRAS, 504, 4751, 2021, (ADS link); Sowmya, K., Shapiro, A. I., Witzke, V., N\u00e8mec, N.-E., Chatzistergos, T., Yeo, K. L., Krivova, N. A., &amp; Solanki, [&hellip;]<\/p>\n","protected":false},"author":15,"featured_media":0,"parent":0,"menu_order":2,"comment_status":"closed","ping_status":"closed","template":"","meta":{"footnotes":""},"class_list":["post-7","page","type-page","status-publish","hentry"],"_links":{"self":[{"href":"https:\/\/teams.issibern.ch\/solarandstellarvariabilities\/wp-json\/wp\/v2\/pages\/7","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/teams.issibern.ch\/solarandstellarvariabilities\/wp-json\/wp\/v2\/pages"}],"about":[{"href":"https:\/\/teams.issibern.ch\/solarandstellarvariabilities\/wp-json\/wp\/v2\/types\/page"}],"author":[{"embeddable":true,"href":"https:\/\/teams.issibern.ch\/solarandstellarvariabilities\/wp-json\/wp\/v2\/users\/15"}],"replies":[{"embeddable":true,"href":"https:\/\/teams.issibern.ch\/solarandstellarvariabilities\/wp-json\/wp\/v2\/comments?post=7"}],"version-history":[{"count":14,"href":"https:\/\/teams.issibern.ch\/solarandstellarvariabilities\/wp-json\/wp\/v2\/pages\/7\/revisions"}],"predecessor-version":[{"id":28,"href":"https:\/\/teams.issibern.ch\/solarandstellarvariabilities\/wp-json\/wp\/v2\/pages\/7\/revisions\/28"}],"wp:attachment":[{"href":"https:\/\/teams.issibern.ch\/solarandstellarvariabilities\/wp-json\/wp\/v2\/media?parent=7"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}