{"id":28,"date":"2024-10-16T16:55:45","date_gmt":"2024-10-16T16:55:45","guid":{"rendered":"https:\/\/teams.issibern.ch\/expanding\/?page_id=28"},"modified":"2026-01-27T09:04:09","modified_gmt":"2026-01-27T09:04:09","slug":"publications","status":"publish","type":"page","link":"https:\/\/teams.issibern.ch\/expanding\/publications\/","title":{"rendered":"Publications"},"content":{"rendered":"<p><span style=\"font-family: georgia, palatino, serif;font-size: 12pt\">List of Publications in which the team members were involved (lead-authors or contributors):<\/span><\/p>\n<ol>\n<li>\n<div><span style=\"font-family: georgia, palatino, serif;font-size: 12pt\">H0DN Collaboration, Casertano, S., Anand, G., Anderson, R. I., Beaton, R., <strong>Bhardwaj, A.<\/strong>, et. al (2025), e-prints, arXiv:2510.23823, accepted in A&amp;A<\/span><\/div>\n<div><span id=\"OBJ_PREFIX_DWT581_com_zimbra_url\" class=\"Object\" style=\"font-family: georgia, palatino, serif;font-size: 12pt\" role=\"link\"><span id=\"OBJ_PREFIX_DWT603_com_zimbra_url\" class=\"Object\" role=\"link\"><a href=\"https:\/\/ui.adsabs.harvard.edu\/abs\/2025arXiv251023823H\" target=\"_blank\" rel=\"nofollow noopener noreferrer\">The Local Distance Network: a community consensus report on the measurement of the Hubble constant at 1% precision<\/a><\/span><\/span><\/div>\n<\/li>\n<li>\n<div><span style=\"font-family: georgia, palatino, serif;font-size: 12pt\"><span id=\"OBJ_PREFIX_DWT581_com_zimbra_url\" class=\"Object\" role=\"link\"><span id=\"OBJ_PREFIX_DWT603_com_zimbra_url\" class=\"Object\" role=\"link\"><\/span><\/span>Breuval, L., Anand, G. S., Anderson, R. I., Beaton, R., <strong>Bhardwaj, A.,<\/strong> Casertano, S., et. al (2025), The Astrophysical Journal, 994, 111.<\/span><\/div>\n<div><span id=\"OBJ_PREFIX_DWT582_com_zimbra_url\" class=\"Object\" style=\"font-family: georgia, palatino, serif;font-size: 12pt\" role=\"link\"><span id=\"OBJ_PREFIX_DWT604_com_zimbra_url\" class=\"Object\" role=\"link\"><a href=\"https:\/\/ui.adsabs.harvard.edu\/abs\/2025ApJ...994..111B\" target=\"_blank\" rel=\"nofollow noopener noreferrer\">Converging on the Cepheid Metallicity Dependence: Implications of Nonstandard Gaia Parallax Recalibration on Distance Measures<\/a><\/span><\/span><\/div>\n<\/li>\n<li>\n<div><span style=\"font-family: georgia, palatino, serif;font-size: 12pt\"><strong>Trentin, E.<\/strong>, Catanzaro, G., <strong>Ripepi, V.<\/strong>, Alonso-Santiago, J., Molinaro, R., Storm, J., De Somma, G., <strong>Marconi, M., Bhardwaj, A.<\/strong>, Gatto, M., Musella, I., &amp; Testa, V. (2024), Astronomy and Astrophysics, 690, A246.<\/span><\/div>\n<div><span id=\"OBJ_PREFIX_DWT583_com_zimbra_url\" class=\"Object\" style=\"font-family: georgia, palatino, serif;font-size: 12pt\" role=\"link\"><span id=\"OBJ_PREFIX_DWT605_com_zimbra_url\" class=\"Object\" role=\"link\"><a href=\"https:\/\/ui.adsabs.harvard.edu\/abs\/2024A&amp;A...690A.246T%20%E2%80%8B\" target=\"_blank\" rel=\"nofollow noopener noreferrer\">Cepheid Metallicity in the Leavitt Law (C-MetaLL) survey: VI. Radial abundance gradients of 29 chemical species in the Milky Way disc,\u00a0<\/a><\/span><\/span><\/div>\n<\/li>\n<li>\n<div><span style=\"font-family: georgia, palatino, serif;font-size: 12pt\"><span id=\"OBJ_PREFIX_DWT583_com_zimbra_url\" class=\"Object\" role=\"link\"><span id=\"OBJ_PREFIX_DWT605_com_zimbra_url\" class=\"Object\" role=\"link\"><\/span><\/span><strong>Bhardwaj, A., Matsunaga, N.,<\/strong> Huang, C. D., Riess, A. G., &amp; <strong>Rejkuba, M.<\/strong> (2025), The Astrophysical Journal, 990, 63.<\/span><\/div>\n<div><span id=\"OBJ_PREFIX_DWT584_com_zimbra_url\" class=\"Object\" style=\"font-family: georgia, palatino, serif;font-size: 12pt\" role=\"link\"><span id=\"OBJ_PREFIX_DWT606_com_zimbra_url\" class=\"Object\" role=\"link\"><a href=\"https:\/\/ui.adsabs.harvard.edu\/abs\/2025ApJ...990...63B%20%E2%80%8B\" target=\"_blank\" rel=\"nofollow noopener noreferrer\">Absolute Calibration of Cluster Mira Variables to Provide a New Anchor for the Hubble Constant Determination,\u00a0<\/a><\/span><\/span><\/div>\n<div><strong><span style=\"font-family: georgia, palatino, serif;font-size: 12pt;color: #993366\">IUCAA press release &#8212; <a style=\"color: #993366\" href=\"https:\/\/web.iucaa.in\/news\/WCMAIRCE\/\">https:\/\/web.iucaa.in\/news\/WCMAIRCE\/<\/a><\/span><\/strong><\/div>\n<\/li>\n<li>\n<div><span style=\"font-family: georgia, palatino, serif;font-size: 12pt\">Sicignano, T., <strong>Ripepi, V., Rejkuba, M.<\/strong>, Romaniello, M., <strong>Marconi, M.<\/strong>, Molinaro, R., <strong>Bhardwaj, A.,<\/strong> De Somma, G., Cioni, M.-R. L., et. al (2025), Astronomy and Astrophysics, 699, A370.<\/span><\/div>\n<div><span id=\"OBJ_PREFIX_DWT585_com_zimbra_url\" class=\"Object\" style=\"font-family: georgia, palatino, serif;font-size: 12pt\" role=\"link\"><span id=\"OBJ_PREFIX_DWT607_com_zimbra_url\" class=\"Object\" role=\"link\"><a href=\"https:\/\/ui.adsabs.harvard.edu\/abs\/2025A&amp;A...699A.370S\" target=\"_blank\" rel=\"nofollow noopener noreferrer\">The VMC Survey: LIII. Anomalous Cepheids in the Magellanic Clouds: Period-luminosity relations in the near-infrared bands,\u00a0<\/a><\/span><\/span><\/div>\n<\/li>\n<li>\n<div><span style=\"font-family: georgia, palatino, serif;font-size: 12pt\"><span id=\"OBJ_PREFIX_DWT585_com_zimbra_url\" class=\"Object\" role=\"link\"><span id=\"OBJ_PREFIX_DWT607_com_zimbra_url\" class=\"Object\" role=\"link\"><\/span><\/span>Catanzaro, G., <strong>Bhardwaj, A., Ripepi, V., Trentin, E., Marconi, M.<\/strong>, Romaniello, M., <strong>Matsunaga, N.<\/strong>, De Somma, G., Sicignano, T., Musella, I., &amp; Soung-Chul, Y. (2025), e-prints, arXiv:2511.06264, A&amp;A in press<\/span><\/div>\n<div><span id=\"OBJ_PREFIX_DWT586_com_zimbra_url\" class=\"Object\" style=\"font-family: georgia, palatino, serif;font-size: 12pt\" role=\"link\"><span id=\"OBJ_PREFIX_DWT608_com_zimbra_url\" class=\"Object\" role=\"link\"><a href=\"https:\/\/ui.adsabs.harvard.edu\/abs\/2025arXiv251106264C\" target=\"_blank\" rel=\"nofollow noopener noreferrer\">Cepheid Metallicity in the Leavitt Law (C&#8211;MetaLL) survey: VIII. High-Resolution IGRINS Spectroscopy of 23 Classical Cepheids: Validating NIR Abundances,\u00a0<\/a><\/span><\/span><\/div>\n<\/li>\n<li>\n<div><span style=\"font-family: georgia, palatino, serif;font-size: 12pt\"><strong>Trentin, E.<\/strong>, Catanzaro, G., Ripepi, V., Luongo, E., <strong>Marconi, M.<\/strong>, Musella, I., Cusano, F., Storm, J., <strong>Bhardwaj, A.,<\/strong> De Somma, G., Sicignano, T., &amp; Molinaro, R. (2025), e-prints, arXiv:2511.04269, A&amp;A, in review<\/span><\/div>\n<div><span style=\"font-family: georgia, palatino, serif;font-size: 12pt\">Cepheid Metallicity in the Leavitt Law (C- MetaLL) survey: IX: Spectroscopic detection of rare earth Dysprosium, Erbium, Lutetium and Thorium in Classical Cepheids,<\/span><\/div>\n<\/li>\n<li>\n<div><span style=\"font-family: georgia, palatino, serif;font-size: 12pt\"><strong>Ripepi, V., Trentin, E.<\/strong>, Catanzaro, G., <strong>Marconi, M., Bhardwaj, A.<\/strong>, Clementini, G., Cusano, F., De Somma, G., Molinaro, R., Sicignano, T., &amp; Storm, J. (2025),\u00a0 e-prints, arXiv:2508.17447.<\/span><\/div>\n<div><span id=\"OBJ_PREFIX_DWT587_com_zimbra_url\" class=\"Object\" style=\"font-family: georgia, palatino, serif;font-size: 12pt\" role=\"link\"><span id=\"OBJ_PREFIX_DWT609_com_zimbra_url\" class=\"Object\" role=\"link\"><a href=\"https:\/\/ui.adsabs.harvard.edu\/abs\/2025arXiv250817447R\" target=\"_blank\" rel=\"nofollow noopener noreferrer\">Cepheid Metallicity in the Leavitt Law (C-MetaLL) survey: VII. Metallicity dependence of Period-Wesenheit relations based on a homogeneous spectroscopic sample,\u00a0<\/a><\/span><\/span><\/div>\n<\/li>\n<li>\n<div><span style=\"font-family: georgia, palatino, serif;font-size: 12pt\"><span id=\"OBJ_PREFIX_DWT587_com_zimbra_url\" class=\"Object\" role=\"link\"><span id=\"OBJ_PREFIX_DWT609_com_zimbra_url\" class=\"Object\" role=\"link\"><\/span><\/span><strong>Deka, M., Marconi, M.<\/strong>, Molinaro, R., De Somma, G., <strong>Bhardwaj, A., Trentin, E.<\/strong>, Deb, S., Sicignano, T., Musella, I., Ripepi, V., Luongo, E., &amp; Kanbur, S. M. (2025), e-prints, arXiv:2510.26385.<\/span><\/div>\n<div><span id=\"OBJ_PREFIX_DWT588_com_zimbra_url\" class=\"Object\" style=\"font-family: georgia, palatino, serif;font-size: 12pt\" role=\"link\"><span id=\"OBJ_PREFIX_DWT610_com_zimbra_url\" class=\"Object\" role=\"link\"><a href=\"https:\/\/ui.adsabs.harvard.edu\/abs\/2025arXiv251026385D\" target=\"_blank\" rel=\"nofollow noopener noreferrer\">The light curve model fitting of LMC Cepheids: MESA-RSP versus Stellingwerf&#8217;s code predictions,\u00a0<\/a><\/span><\/span><\/div>\n<\/li>\n<li>\n<div><span style=\"font-family: georgia, palatino, serif;font-size: 12pt\"><span id=\"OBJ_PREFIX_DWT588_com_zimbra_url\" class=\"Object\" role=\"link\"><span id=\"OBJ_PREFIX_DWT610_com_zimbra_url\" class=\"Object\" role=\"link\"><\/span><\/span><strong>Das, S., Bhardwaj, A., &amp; Marconi, M.<\/strong> (2025), arXiv e-prints, arXiv:2511.16118.<\/span><\/div>\n<div><span id=\"OBJ_PREFIX_DWT589_com_zimbra_url\" class=\"Object\" style=\"font-family: georgia, palatino, serif;font-size: 12pt\" role=\"link\"><span id=\"OBJ_PREFIX_DWT611_com_zimbra_url\" class=\"Object\" role=\"link\"><a href=\"https:\/\/ui.adsabs.harvard.edu\/abs\/2025arXiv251116118D%20%E2%80%8B\" target=\"_blank\" rel=\"nofollow noopener noreferrer\">Type II Cepheids: Period-Luminosity-Metallicity relations for the Population II distance scale,\u00a0<\/a><\/span><\/span><\/div>\n<\/li>\n<li>\n<div><span style=\"font-family: georgia, palatino, serif;font-size: 12pt\"><span id=\"OBJ_PREFIX_DWT589_com_zimbra_url\" class=\"Object\" role=\"link\"><span id=\"OBJ_PREFIX_DWT611_com_zimbra_url\" class=\"Object\" role=\"link\"><\/span><\/span>Ngeow, C.-C., &amp; <strong>Bhardwaj, A.<\/strong> (2025), The Astronomical Journal, 169, 156.<\/span><\/div>\n<div><span id=\"OBJ_PREFIX_DWT590_com_zimbra_url\" class=\"Object\" style=\"font-family: georgia, palatino, serif;font-size: 12pt\" role=\"link\"><span id=\"OBJ_PREFIX_DWT612_com_zimbra_url\" class=\"Object\" role=\"link\"><a href=\"https:\/\/ui.adsabs.harvard.edu\/abs\/2025AJ....169..156N\" target=\"_blank\" rel=\"nofollow noopener noreferrer\">Candidate RR Lyrae Associated with the Ultrafaint Dwarf Galaxy Aquarius III,\u00a0<\/a><\/span><\/span><\/div>\n<\/li>\n<li>\n<div><span style=\"font-family: georgia, palatino, serif;font-size: 12pt\"><span id=\"OBJ_PREFIX_DWT590_com_zimbra_url\" class=\"Object\" role=\"link\"><span id=\"OBJ_PREFIX_DWT612_com_zimbra_url\" class=\"Object\" role=\"link\"><\/span><\/span><strong>Das, S.<\/strong>, Moln\u00e1r, L., Kov\u00e1cs, G. B., Smolec, R., Joyce, M., <strong>Kanbur, S. M<\/strong>., Szklen\u00e1r, T., <strong>Bhardwaj, A.,<\/strong> Singh, H. P., <strong>Marconi, M., &amp; Ripepi, V.<\/strong> (2025), Astronomy and Astrophysics, 694, A255.<\/span><\/div>\n<div><span id=\"OBJ_PREFIX_DWT591_com_zimbra_url\" class=\"Object\" style=\"font-family: georgia, palatino, serif;font-size: 12pt\" role=\"link\"><span id=\"OBJ_PREFIX_DWT613_com_zimbra_url\" class=\"Object\" role=\"link\"><a href=\"https:\/\/ui.adsabs.harvard.edu\/abs\/2025A&amp;A...694A.255D\" target=\"_blank\" rel=\"nofollow noopener noreferrer\">A theoretical framework for BL Her stars: III. A case study: Robust light curve optimization in the Large Magellanic Cloud,\u00a0<\/a><\/span><\/span><\/div>\n<\/li>\n<li>\n<div><span style=\"font-family: georgia, palatino, serif;font-size: 12pt\"><span id=\"OBJ_PREFIX_DWT591_com_zimbra_url\" class=\"Object\" role=\"link\"><span id=\"OBJ_PREFIX_DWT613_com_zimbra_url\" class=\"Object\" role=\"link\"><\/span><\/span>Kurbah, K., <strong>Kanbur, S. M.<\/strong>, Deb, S., <strong>Bhardwaj, A., Deka, M., Das, S.<\/strong>, &amp; Bhuyan, G. (2025), Monthly Notices of the Royal Astronomical Society, 541, 2594.<\/span><\/div>\n<div><span id=\"OBJ_PREFIX_DWT592_com_zimbra_url\" class=\"Object\" style=\"font-family: georgia, palatino, serif;font-size: 12pt\" role=\"link\"><span id=\"OBJ_PREFIX_DWT614_com_zimbra_url\" class=\"Object\" role=\"link\"><a href=\"https:\/\/ui.adsabs.harvard.edu\/abs\/2025MNRAS.541.2594K\" target=\"_blank\" rel=\"nofollow noopener noreferrer\">Multiwavelength study of observed and predicted pulsation properties of first overtone Cepheids in the Magellanic Clouds,\u00a0<\/a><\/span><\/span><\/div>\n<\/li>\n<li>\n<div><span style=\"font-family: georgia, palatino, serif;font-size: 12pt\"><span id=\"OBJ_PREFIX_DWT592_com_zimbra_url\" class=\"Object\" role=\"link\"><span id=\"OBJ_PREFIX_DWT614_com_zimbra_url\" class=\"Object\" role=\"link\"><\/span><\/span><strong>Das, S.,<\/strong> Moln\u00e1r, L., Szab\u00f3, R., Singh, H. P., <strong>Kanbur, S. M., Bhardwaj, A., Marconi, M.<\/strong>, &amp; Smolec, R. (2025), Astronomy and Astrophysics, 695, A38.<\/span><\/div>\n<div><span id=\"OBJ_PREFIX_DWT593_com_zimbra_url\" class=\"Object\" style=\"font-family: georgia, palatino, serif;font-size: 12pt\" role=\"link\"><span id=\"OBJ_PREFIX_DWT615_com_zimbra_url\" class=\"Object\" role=\"link\"><a href=\"https:\/\/ui.adsabs.harvard.edu\/abs\/2025A&amp;A...695A..38D%20%E2%80%8B\" target=\"_blank\" rel=\"nofollow noopener noreferrer\">A theoretical framework for BL Her stars: IV. New period-luminosity relations in the Rubin-LSST filters,<\/a><\/span><\/span><\/div>\n<\/li>\n<li>\n<div><span style=\"font-family: georgia, palatino, serif;font-size: 12pt\"><span id=\"OBJ_PREFIX_DWT593_com_zimbra_url\" class=\"Object\" role=\"link\"><span id=\"OBJ_PREFIX_DWT615_com_zimbra_url\" class=\"Object\" role=\"link\"><\/span><\/span>Ngeow, C.-C., &amp; <strong>Bhardwaj, A.<\/strong> (2025), The Astronomical Journal, 169, 68.<\/span><\/div>\n<div><span id=\"OBJ_PREFIX_DWT594_com_zimbra_url\" class=\"Object\" style=\"font-family: georgia, palatino, serif;font-size: 12pt\" role=\"link\"><span id=\"OBJ_PREFIX_DWT616_com_zimbra_url\" class=\"Object\" role=\"link\"><a href=\"https:\/\/ui.adsabs.harvard.edu\/abs\/2025AJ....169...68N%20%E2%80%8B\" target=\"_blank\" rel=\"nofollow noopener noreferrer\">The Lack of RR Lyrae Variables in Ultrafaint Dwarf Galaxy Sextans II,\u00a0<\/a><\/span><\/span><\/div>\n<\/li>\n<li>\n<div><span style=\"font-family: georgia, palatino, serif;font-size: 12pt\"><span id=\"OBJ_PREFIX_DWT594_com_zimbra_url\" class=\"Object\" role=\"link\"><span id=\"OBJ_PREFIX_DWT616_com_zimbra_url\" class=\"Object\" role=\"link\"><\/span><\/span>Kumar, N., Singh, H. P., Malkov, O., Joshi, S., Tan, K., Prugniel, P., &amp; <strong>Bhardwaj, A.<\/strong> (2025), Universe, 11, 207.<\/span><\/div>\n<div><span id=\"OBJ_PREFIX_DWT595_com_zimbra_url\" class=\"Object\" style=\"font-family: georgia, palatino, serif;font-size: 12pt\" role=\"link\"><span id=\"OBJ_PREFIX_DWT617_com_zimbra_url\" class=\"Object\" role=\"link\"><a href=\"https:\/\/ui.adsabs.harvard.edu\/abs\/2025Univ...11..207K\" target=\"_blank\" rel=\"nofollow noopener noreferrer\">Extraction of Physical Parameters of RRab Variables Using Neural Network Based Interpolator,\u00a0<\/a><\/span><\/span><\/div>\n<\/li>\n<\/ol>\n<p><span style=\"font-family: georgia, palatino, serif;font-size: 12pt\">The following acknowledgment was added to all the publications resulting through collaborations among the team members &#8212;<\/span><\/p>\n<p><span style=\"color: #0000ff;font-family: georgia, palatino, serif;font-size: 12pt\"><span style=\"font-weight: 400\">&#8220;This research was supported by the International Space Science Institute (ISSI) in Bern\/Beijing through ISSI\/ISSI-BJ International Team project ID #24-603 &#8211; \u201c<\/span><i><span style=\"font-weight: 400\">EXPANDING Universe\u201d<\/span><\/i><span style=\"font-weight: 400\"> (EXploiting Precision AstroNomical Distance INdicators in the Gaia Universe).&#8221;<\/span><\/span><\/p>\n","protected":false},"excerpt":{"rendered":"<p>List of Publications in which the team members were involved (lead-authors or contributors): H0DN Collaboration, Casertano, S., Anand, G., Anderson, R. I., Beaton, R., Bhardwaj, A., et. al (2025), e-prints, arXiv:2510.23823, accepted in A&amp;A The Local Distance Network: a community consensus report on the measurement of the Hubble constant at 1% precision Breuval, L., Anand, [&hellip;]<\/p>\n","protected":false},"author":141,"featured_media":0,"parent":0,"menu_order":0,"comment_status":"closed","ping_status":"closed","template":"","meta":{"footnotes":""},"class_list":["post-28","page","type-page","status-publish","hentry"],"_links":{"self":[{"href":"https:\/\/teams.issibern.ch\/expanding\/wp-json\/wp\/v2\/pages\/28","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/teams.issibern.ch\/expanding\/wp-json\/wp\/v2\/pages"}],"about":[{"href":"https:\/\/teams.issibern.ch\/expanding\/wp-json\/wp\/v2\/types\/page"}],"author":[{"embeddable":true,"href":"https:\/\/teams.issibern.ch\/expanding\/wp-json\/wp\/v2\/users\/141"}],"replies":[{"embeddable":true,"href":"https:\/\/teams.issibern.ch\/expanding\/wp-json\/wp\/v2\/comments?post=28"}],"version-history":[{"count":12,"href":"https:\/\/teams.issibern.ch\/expanding\/wp-json\/wp\/v2\/pages\/28\/revisions"}],"predecessor-version":[{"id":61,"href":"https:\/\/teams.issibern.ch\/expanding\/wp-json\/wp\/v2\/pages\/28\/revisions\/61"}],"wp:attachment":[{"href":"https:\/\/teams.issibern.ch\/expanding\/wp-json\/wp\/v2\/media?parent=28"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}