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Stock, Johanna
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Stock, Johanna
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Stock, Johanna
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Stock, J.
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2017Journal Article [["dc.bibliographiccitation.firstpage","131"],["dc.bibliographiccitation.issue","1"],["dc.bibliographiccitation.journal","Pediatric Nephrology"],["dc.bibliographiccitation.lastpage","137"],["dc.bibliographiccitation.volume","32"],["dc.contributor.author","Stock, Johanna"],["dc.contributor.author","Kuenanz, Johannes"],["dc.contributor.author","Glonke, Niklas"],["dc.contributor.author","Sonntag, Joseph"],["dc.contributor.author","Frese, Jenny"],["dc.contributor.author","Toenshoff, Burkhard"],["dc.contributor.author","Hoecker, Britta"],["dc.contributor.author","Hoppe, Bernd"],["dc.contributor.author","Feldkoetter, Markus"],["dc.contributor.author","Pape, Lars"],["dc.contributor.author","Lerch, Christian"],["dc.contributor.author","Wygoda, Simone"],["dc.contributor.author","Weber, Manfred"],["dc.contributor.author","Mueller, Gerhard-Anton"],["dc.contributor.author","Gross, Oliver"],["dc.date.accessioned","2018-11-07T10:29:37Z"],["dc.date.available","2018-11-07T10:29:37Z"],["dc.date.issued","2017"],["dc.description.abstract","Patients with autosomal or X-linked Alport syndrome (AS) with heterozygous mutations in type IV collagen genes have a 1-20 % risk of progressing to end-stage renal disease during their lifetime. We evaluated the long-term renal outcome of patients at risk of progressive disease (chronic kidney disease stages 1-4) with/without nephroprotective therapy. This was a prospective, non-interventional, observational study which included data from a 4-year follow-up of AS patients with heterozygous mutations whose datasets had been included in an analysis of the 2010 database of the European Alport Registry. Using Kaplan-Meier estimates and logrank tests, we prospectively analyzed the updated datasets of 52 of these patients and 13 new datasets (patients added to the Registry after 2011). The effects of therapy, extrarenal symptoms and inheritance pattern on renal outcome were analyzed. The mean prospective follow-up was 46 +/- 10 months, and the mean time on therapy was 8.4 +/- 4.4 (median 7; range 2-18) years. The time from the appearance of the first symptom to diagnosis was 8.1 +/- 14.2 (range 0-52) years. At the time of starting therapy, 5.4 % of patients had an estimated glomerular filtration rate of < 60 ml/min, 67.6 % had proteinuria and 27.0 % had microalbuminuria. Therapeutic strategies included angiotensin-converting enzymer inhibitors (97.1 %), angiotensin receptor antagonists (1 patient), dual therapy (11.8 %) and statins (8.8 %). Among patients included in the prospective dataset, prevented the need for dialysis. Among new patients, no patient at risk for renal failure progressed to the next disease stage after 4 years follow-up; three patients even regressed to a lower stage during therapy. Treatment with blockers of the renin-angiotensin-aldosterone system prevents progressive renal failure in AS patients with heterozygous mutations in the genes causing AS. Considerable numbers of aging AS patients on dialysis may have heterozygous mutations in these genes (present in 1 % of total population) as underlying disease. Hence, greater alertness towards timely diagnosis and therapy has the potential to prevent progressive renal failure in most-if not all-AS patients with heterozygous mutations in the causal genes."],["dc.identifier.doi","10.1007/s00467-016-3452-z"],["dc.identifier.isi","000388976400015"],["dc.identifier.pmid","27402170"],["dc.identifier.uri","https://resolver.sub.uni-goettingen.de/purl?gro-2/43676"],["dc.notes.status","zu prüfen"],["dc.notes.submitter","PUB_WoS_Import"],["dc.publisher","Springer"],["dc.relation.issn","1432-198X"],["dc.relation.issn","0931-041X"],["dc.title","Prospective study on the potential of RAAS blockade to halt renal disease in Alport syndrome patients with heterozygous mutations"],["dc.type","journal_article"],["dc.type.internalPublication","yes"],["dc.type.peerReviewed","yes"],["dc.type.status","published"],["dspace.entity.type","Publication"]]Details DOI PMID PMC WOS2018Journal Article [["dc.bibliographiccitation.firstpage","921"],["dc.bibliographiccitation.journal","Frontiers in Physiology"],["dc.bibliographiccitation.volume","9"],["dc.contributor.author","Bajerski, Felizitas"],["dc.contributor.author","Stock, Johanna"],["dc.contributor.author","Hanf, Benjamin"],["dc.contributor.author","Darienko, Tatyana"],["dc.contributor.author","Heine-Dobbernack, Elke"],["dc.contributor.author","Lorenz, Maike"],["dc.contributor.author","Naujox, Lisa"],["dc.contributor.author","Keller, E. R. J."],["dc.contributor.author","Schumacher, H. M."],["dc.contributor.author","Friedl, Thomas"],["dc.contributor.author","Eberth, Sonja"],["dc.contributor.author","Mock, Hans-Peter"],["dc.contributor.author","Kniemeyer, Olaf"],["dc.contributor.author","Overmann, Jörg"],["dc.date.accessioned","2019-07-22T14:46:42Z"],["dc.date.available","2019-07-22T14:46:42Z"],["dc.date.issued","2018"],["dc.description.abstract","In many natural environments, organisms get exposed to low temperature and/or to strong temperature shifts. Also, standard preservation protocols for live cells or tissues involve ultradeep freezing in or above liquid nitrogen (-196°C or -150°C, respectively). To which extent these conditions cause cold- or cryostress has rarely been investigated systematically. Using ATP content as an indicator of the physiological state of cells, we found that representatives of bacteria, fungi, algae, plant tissue, as well as plant and human cell lines exhibited similar responses during freezing and thawing. Compared to optimum growth conditions, the cellular ATP content of most model organisms decreased significantly upon treatment with cryoprotectant and cooling to up to -196°C. After thawing and a longer period of regeneration, the initial ATP content was restored or even exceeded the initial ATP levels. To assess the implications of cellular ATP concentration for the physiology of cryostress, cell viability was determined in parallel using independent approaches. A significantly positive correlation of ATP content and viability was detected only in the cryosensitive algae Chlamydomonas reinhardtii SAG 11-32b and Chlorella variabilis NC64A, and in plant cell lines of Solanum tuberosum. When comparing mesophilic with psychrophilic bacteria of the same genera, and cryosensitive with cryotolerant algae, ATP levels of actively growing cells were generally higher in the psychrophilic and cryotolerant representatives. During exposure to ultralow temperatures, however, psychrophilic and cryotolerant species showed a decline in ATP content similar to their mesophilic or cryosensitive counterparts. Nevertheless, psychrophilic and cryotolerant species attained better culturability after freezing. Cellular ATP concentrations and viability measurements thus monitor different features of live cells during their exposure to ultralow temperatures and cryostress."],["dc.identifier.doi","10.3389/fphys.2018.00921"],["dc.identifier.pmid","30065659"],["dc.identifier.uri","https://resolver.sub.uni-goettingen.de/purl?gro-2/61835"],["dc.language.iso","en"],["dc.notes.intern","DeepGreen Import"],["dc.publisher","Frontiers Media S.A."],["dc.relation.eissn","1664-042X"],["dc.relation.issn","1664-042X"],["dc.rights","http://creativecommons.org/licenses/by/4.0/"],["dc.title","ATP Content and Cell Viability as Indicators for Cryostress Across the Diversity of Life"],["dc.type","journal_article"],["dc.type.internalPublication","yes"],["dspace.entity.type","Publication"]]Details DOI PMID PMC2021Journal Article [["dc.bibliographiccitation.firstpage","A78"],["dc.bibliographiccitation.journal","Astronomy and Astrophysics"],["dc.bibliographiccitation.volume","650"],["dc.contributor.author","Bluhm, P."],["dc.contributor.author","Pallé, E."],["dc.contributor.author","Molaverdikhani, K."],["dc.contributor.author","Kemmer, J."],["dc.contributor.author","Hatzes, A. P."],["dc.contributor.author","Kossakowski, D."],["dc.contributor.author","Stock, S."],["dc.contributor.author","Caballero, J. A."],["dc.contributor.author","Lillo-Box, J."],["dc.contributor.author","Zapatero Osorio, M. R."],["dc.date.accessioned","2021-08-12T07:45:05Z"],["dc.date.available","2021-08-12T07:45:05Z"],["dc.date.issued","2021"],["dc.description.abstract","Dynamical histories of planetary systems, as well as the atmospheric evolution of highly irradiated planets, can be studied by characterizing the ultra-short-period planet population, which the TESS mission is particularly well suited to discover. Here, we report on the follow-up of a transit signal detected in the TESS sector 19 photometric time series of the M3.0 V star TOI-1685 (2MASS J04342248+4302148). We confirm the planetary nature of the transit signal, which has a period of P b = 0.6691403 −0.0000021 +0.0000023 d, using precise radial velocity measurements taken with the CARMENES spectrograph. From the joint photometry and radial velocity analysis, we estimate the following parameters for TOI-1685 b: a mass of M b = 3.78 −0.63 +0.63 M ⊕ , a radius of R b = 1.70 −0.07 +0.07 R ⊕ , which together result in a bulk density of ρ b = 4.21 −0.82 +0.95 g cm −3 , and an equilibrium temperature of T eq = 1069 −16 +16 K. TOI-1685 b is the least dense ultra-short-period planet around an M dwarf known to date. TOI-1685 b is also one of the hottest transiting super-Earth planets with accurate dynamical mass measurements, which makes it a particularly attractive target for thermal emission spectroscopy. Additionally, we report with moderate evidence an additional non-transiting planet candidate in the system, TOI-1685 [c], which has an orbital period of P c = 9.02 −0.12 +0.10 d."],["dc.identifier.doi","10.1051/0004-6361/202140688"],["dc.identifier.pii","aa40688-21"],["dc.identifier.uri","https://resolver.sub.uni-goettingen.de/purl?gro-2/88366"],["dc.notes.intern","DOI Import GROB-448"],["dc.relation.eissn","1432-0746"],["dc.relation.issn","0004-6361"],["dc.title","An ultra-short-period transiting super-Earth orbiting the M3 dwarf TOI-1685"],["dc.type","journal_article"],["dc.type.internalPublication","yes"],["dspace.entity.type","Publication"]]Details DOI2020Journal Article [["dc.bibliographiccitation.firstpage","A236"],["dc.bibliographiccitation.journal","Astronomy and Astrophysics"],["dc.bibliographiccitation.volume","642"],["dc.contributor.author","Kemmer, J."],["dc.contributor.author","Stock, S."],["dc.contributor.author","Kossakowski, D."],["dc.contributor.author","Kaminski, A."],["dc.contributor.author","Molaverdikhani, K."],["dc.contributor.author","Schlecker, M."],["dc.contributor.author","Caballero, J. A."],["dc.contributor.author","Amado, P. J."],["dc.contributor.author","Astudillo-Defru, N."],["dc.contributor.author","Zechmeister, M."],["dc.date.accessioned","2021-04-14T09:58:48Z"],["dc.date.available","2021-04-14T09:58:48Z"],["dc.date.issued","2020"],["dc.identifier.uri","https://resolver.sub.uni-goettingen.de/purl?gro-2/84192"],["dc.notes.intern","DOI Import GROB-399"],["dc.relation.eissn","1432-0746"],["dc.relation.issn","0004-6361"],["dc.title","Discovery of a hot, transiting, Earth-sized planet and a second temperate, non-transiting planet around the M4 dwarf GJ 3473 (TOI-488)"],["dc.type","journal_article"],["dc.type.internalPublication","yes"],["dspace.entity.type","Publication"]]Details2022Journal Article [["dc.bibliographiccitation.firstpage","A17"],["dc.bibliographiccitation.journal","Astronomy & Astrophysics"],["dc.bibliographiccitation.volume","659"],["dc.contributor.author","Kemmer, J."],["dc.contributor.author","Dreizler, S."],["dc.contributor.author","Kossakowski, D."],["dc.contributor.author","Stock, S."],["dc.contributor.author","Quirrenbach, A."],["dc.contributor.author","Caballero, J. A."],["dc.contributor.author","Amado, P. J."],["dc.contributor.author","Collins, K. A."],["dc.contributor.author","Espinoza, N."],["dc.contributor.author","Herrero, E."],["dc.contributor.author","Zechmeister, M."],["dc.date.accessioned","2022-04-01T10:00:42Z"],["dc.date.available","2022-04-01T10:00:42Z"],["dc.date.issued","2022"],["dc.description.abstract","We report the discovery of GJ 3929 b, a hot Earth-sized planet orbiting the nearby M3.5 V dwarf star, GJ 3929 (G 180-18, TOI-2013). Joint modelling of photometric observations from TESS sectors 24 and 25 together with 73 spectroscopic observations from CARMENES and follow-up transit observations from SAINT-EX, LCOGT, and OSN yields a planet radius of R b = 1.150 ± 0.040 R ⊕ , a mass of M b = 1.21 ± 0.42 M ⊕ , and an orbital period of P b = 2.6162745 ± 0.0000030 d . The resulting density of ρ b = 4.4 ± 1.6 g cm −3 is compatible with the Earth’s mean density of about 5.5 g cm −3 . Due to the apparent brightness of the host star ( J = 8.7 mag) and its small size, GJ 3929 b is a promising target for atmospheric characterisation with the JWST. Additionally, the radial velocity data show evidence for another planet candidate with P [c] = 14.303 ± 0.035 d, which is likely unrelated to the stellar rotation period, P rot = 122 ± 13 d, which we determined from archival HATNet and ASAS-SN photometry combined with newly obtained TJO data."],["dc.identifier.doi","10.1051/0004-6361/202142653"],["dc.identifier.pii","aa42653-21"],["dc.identifier.uri","https://resolver.sub.uni-goettingen.de/purl?gro-2/105493"],["dc.notes.intern","DOI-Import GROB-530"],["dc.relation.eissn","1432-0746"],["dc.relation.issn","0004-6361"],["dc.title","Discovery and mass measurement of the hot, transiting, Earth-sized planet, GJ 3929 b"],["dc.type","journal_article"],["dc.type.internalPublication","yes"],["dspace.entity.type","Publication"]]Details DOI2019Journal Article [["dc.bibliographiccitation.firstpage","e0222102"],["dc.bibliographiccitation.issue","9"],["dc.bibliographiccitation.journal","PLoS One"],["dc.bibliographiccitation.volume","14"],["dc.contributor.author","Grupp, Clemens"],["dc.contributor.author","Troche-Polzien, Ilka"],["dc.contributor.author","Stock, Johanna"],["dc.contributor.author","Bramlage, Carsten"],["dc.contributor.author","Müller, Gerhard A."],["dc.contributor.author","Koziolek, Michael"],["dc.contributor.editor","Gonzalez Suarez, Maria Lourdes"],["dc.date.accessioned","2020-12-10T18:42:10Z"],["dc.date.available","2020-12-10T18:42:10Z"],["dc.date.issued","2019"],["dc.identifier.doi","10.1371/journal.pone.0222102"],["dc.identifier.eissn","1932-6203"],["dc.identifier.purl","https://resolver.sub.uni-goettingen.de/purl?gs-1/16604"],["dc.identifier.uri","https://resolver.sub.uni-goettingen.de/purl?gro-2/77833"],["dc.language.iso","en"],["dc.notes.intern","DOI Import GROB-354"],["dc.notes.intern","Merged from goescholar"],["dc.rights","CC BY 4.0"],["dc.rights.uri","https://creativecommons.org/licenses/by/4.0"],["dc.title","Thrombophilic risk factors in hemodialysis: Association with early vascular access occlusion and patient survival in long-term follow-up"],["dc.type","journal_article"],["dc.type.internalPublication","yes"],["dc.type.version","published_version"],["dspace.entity.type","Publication"]]Details DOI2019Journal Article [["dc.bibliographiccitation.firstpage","A39"],["dc.bibliographiccitation.journal","Astronomy and Astrophysics"],["dc.bibliographiccitation.volume","628"],["dc.contributor.author","Luque, R."],["dc.contributor.author","Pallé, E."],["dc.contributor.author","Kossakowski, D."],["dc.contributor.author","Dreizler, S."],["dc.contributor.author","Kemmer, J."],["dc.contributor.author","Espinoza, N."],["dc.contributor.author","Burt, J."],["dc.contributor.author","Anglada-Escudé, G."],["dc.contributor.author","Béjar, V. J. S."],["dc.contributor.author","Caballero, J. A."],["dc.contributor.author","Collins, K. A."],["dc.contributor.author","Collins, K. I."],["dc.contributor.author","Cortés-Contreras, M."],["dc.contributor.author","Díez-Alonso, E."],["dc.contributor.author","Feng, F."],["dc.contributor.author","Hatzes, A."],["dc.contributor.author","Hellier, C."],["dc.contributor.author","Henning, T."],["dc.contributor.author","Jeffers, S. V."],["dc.contributor.author","Kaltenegger, L."],["dc.contributor.author","Kürster, M."],["dc.contributor.author","Madden, J."],["dc.contributor.author","Molaverdikhani, K."],["dc.contributor.author","Montes, D."],["dc.contributor.author","Narita, N."],["dc.contributor.author","Nowak, G."],["dc.contributor.author","Ofir, A."],["dc.contributor.author","Oshagh, M."],["dc.contributor.author","Parviainen, H."],["dc.contributor.author","Quirrenbach, A."],["dc.contributor.author","Reffert, S."],["dc.contributor.author","Reiners, A."],["dc.contributor.author","Rodríguez-López, C."],["dc.contributor.author","Schlecker, M."],["dc.contributor.author","Stock, S."],["dc.contributor.author","Trifonov, T."],["dc.contributor.author","Winn, J. N."],["dc.contributor.author","Zapatero Osorio, M. R."],["dc.contributor.author","Zechmeister, M."],["dc.contributor.author","Amado, P. J."],["dc.contributor.author","Anderson, D. R."],["dc.contributor.author","Batalha, N. E."],["dc.contributor.author","Bauer, F. F."],["dc.contributor.author","Bluhm, P."],["dc.contributor.author","Burke, C. J."],["dc.contributor.author","Butler, R. P."],["dc.contributor.author","Caldwell, D. A."],["dc.contributor.author","Chen, G."],["dc.contributor.author","Crane, J. D."],["dc.contributor.author","Dragomir, D."],["dc.contributor.author","Dressing, C. D."],["dc.contributor.author","Dynes, S."],["dc.contributor.author","Jenkins, J. M."],["dc.contributor.author","Kaminski, A."],["dc.contributor.author","Klahr, H."],["dc.contributor.author","Kotani, T."],["dc.contributor.author","Lafarga, M."],["dc.contributor.author","Latham, D. W."],["dc.contributor.author","Lewin, P."],["dc.contributor.author","McDermott, S."],["dc.contributor.author","Montañés-Rodríguez, P."],["dc.contributor.author","Morales, J. C."],["dc.contributor.author","Murgas, F."],["dc.contributor.author","Nagel, E."],["dc.contributor.author","Pedraz, S."],["dc.contributor.author","Ribas, I."],["dc.contributor.author","Ricker, G. R."],["dc.contributor.author","Rowden, P."],["dc.contributor.author","Seager, S."],["dc.contributor.author","Shectman, S. A."],["dc.contributor.author","Tamura, M."],["dc.contributor.author","Teske, J."],["dc.contributor.author","Twicken, J. D."],["dc.contributor.author","Vanderspeck, R."],["dc.contributor.author","Wang, S. X."],["dc.contributor.author","Wohler, B."],["dc.date.accessioned","2020-12-10T18:11:50Z"],["dc.date.available","2020-12-10T18:11:50Z"],["dc.date.issued","2019"],["dc.identifier.doi","10.1051/0004-6361/201935801"],["dc.identifier.eissn","1432-0746"],["dc.identifier.issn","0004-6361"],["dc.identifier.uri","https://resolver.sub.uni-goettingen.de/purl?gro-2/74158"],["dc.notes.intern","DOI Import GROB-354"],["dc.title","Planetary system around the nearby M dwarf GJ 357 including a transiting, hot, Earth-sized planet optimal for atmospheric characterization"],["dc.type","journal_article"],["dc.type.internalPublication","yes"],["dspace.entity.type","Publication"]]Details DOI2022Journal Article [["dc.bibliographiccitation.artnumber","110857"],["dc.bibliographiccitation.journal","Journal of Psychosomatic Research"],["dc.bibliographiccitation.volume","157"],["dc.contributor.author","Herrmann-Lingen, C."],["dc.contributor.author","Zelenak, C."],["dc.contributor.author","Nagel, J."],["dc.contributor.author","Bersch, K."],["dc.contributor.author","Wicker, M."],["dc.contributor.author","Herbeck Belnap, B."],["dc.contributor.author","Friede, T."],["dc.contributor.author","Lühmann, D."],["dc.contributor.author","Ousager, J."],["dc.contributor.author","Stock, S."],["dc.contributor.author","Pedersen, S."],["dc.date.accessioned","2022-09-01T09:49:42Z"],["dc.date.available","2022-09-01T09:49:42Z"],["dc.date.issued","2022"],["dc.identifier.doi","10.1016/j.jpsychores.2022.110857"],["dc.identifier.pii","S0022399922001428"],["dc.identifier.uri","https://resolver.sub.uni-goettingen.de/purl?gro-2/113505"],["dc.language.iso","en"],["dc.notes.intern","DOI-Import GROB-597"],["dc.relation.issn","0022-3999"],["dc.title","Evaluation of a patient-centred biopsychoSocial blended collaborative CAre Pathway for the treatment of multi-morbid Elderly patients – The ESCAPE clinical study"],["dc.type","journal_article"],["dc.type.internalPublication","yes"],["dspace.entity.type","Publication"]]Details DOI2021Journal Article [["dc.bibliographiccitation.firstpage","A124"],["dc.bibliographiccitation.journal","Astronomy & Astrophysics"],["dc.bibliographiccitation.volume","656"],["dc.contributor.author","Kossakowski, D."],["dc.contributor.author","Kemmer, J."],["dc.contributor.author","Bluhm, P."],["dc.contributor.author","Stock, S."],["dc.contributor.author","Caballero, J. A."],["dc.contributor.author","Béjar, V. J. S."],["dc.contributor.author","Guillén, C. Cardona"],["dc.contributor.author","Lodieu, N."],["dc.contributor.author","Collins, K. A."],["dc.contributor.author","Oshagh, M."],["dc.contributor.author","Zechmeister, M."],["dc.date.accessioned","2022-01-11T14:05:46Z"],["dc.date.available","2022-01-11T14:05:46Z"],["dc.date.issued","2021"],["dc.description.abstract","We present the discovery of a transiting mini-Neptune around TOI-1201, a relatively bright and moderately young early M dwarf ( J ≈ 9.5 mag, ~600–800 Myr) in an equal-mass ~8 arcsecond-wide binary system, using data from the Transiting Exoplanet Survey Satellite, along with follow-up transit observations. With an orbital period of 2.49 d, TOI-1201 b is a warm mini-Neptune with a radius of R b = 2.415 ± 0.090 R ⊕ . This signal is also present in the precise radial velocity measurements from CARMENES, confirming the existence of the planet and providing a planetary mass of M b = 6.28 ± 0.88 M ⊕ and, thus, an estimated bulk density of 2.45 −0.42 +0.48 g cm −3 . The spectroscopic observations additionally show evidence of a signal with a period of 19 d and a long periodic variation of undetermined origin. In combination with ground-based photometric monitoring from WASP-South and ASAS-SN, we attribute the 19 d signal to the stellar rotation period ( P rot = 19–23 d), although we cannot rule out that the variation seen in photometry belongs to the visually close binary companion. We calculate precise stellar parameters for both TOI-1201 and its companion. The transiting planet is anexcellent target for atmosphere characterization (the transmission spectroscopy metric is 97 −16 +21 ) with the upcoming James Webb Space Telescope. It is also feasible to measure its spin-orbit alignment via the Rossiter-McLaughlin effect using current state-of-the-art spectrographs with submeter per second radial velocity precision."],["dc.description.abstract","We present the discovery of a transiting mini-Neptune around TOI-1201, a relatively bright and moderately young early M dwarf ( J ≈ 9.5 mag, ~600–800 Myr) in an equal-mass ~8 arcsecond-wide binary system, using data from the Transiting Exoplanet Survey Satellite, along with follow-up transit observations. With an orbital period of 2.49 d, TOI-1201 b is a warm mini-Neptune with a radius of R b = 2.415 ± 0.090 R ⊕ . This signal is also present in the precise radial velocity measurements from CARMENES, confirming the existence of the planet and providing a planetary mass of M b = 6.28 ± 0.88 M ⊕ and, thus, an estimated bulk density of 2.45 −0.42 +0.48 g cm −3 . The spectroscopic observations additionally show evidence of a signal with a period of 19 d and a long periodic variation of undetermined origin. In combination with ground-based photometric monitoring from WASP-South and ASAS-SN, we attribute the 19 d signal to the stellar rotation period ( P rot = 19–23 d), although we cannot rule out that the variation seen in photometry belongs to the visually close binary companion. We calculate precise stellar parameters for both TOI-1201 and its companion. The transiting planet is anexcellent target for atmosphere characterization (the transmission spectroscopy metric is 97 −16 +21 ) with the upcoming James Webb Space Telescope. It is also feasible to measure its spin-orbit alignment via the Rossiter-McLaughlin effect using current state-of-the-art spectrographs with submeter per second radial velocity precision."],["dc.identifier.doi","10.1051/0004-6361/202141587"],["dc.identifier.pii","aa41587-21"],["dc.identifier.uri","https://resolver.sub.uni-goettingen.de/purl?gro-2/97745"],["dc.notes.intern","DOI-Import GROB-507"],["dc.relation.eissn","1432-0746"],["dc.relation.issn","0004-6361"],["dc.rights.uri","https://creativecommons.org/licenses/by/4.0"],["dc.title","TOI-1201 b: A mini-Neptune transiting a bright and moderately young M dwarf"],["dc.type","journal_article"],["dc.type.internalPublication","yes"],["dspace.entity.type","Publication"]]Details DOI2013Journal Article [["dc.bibliographiccitation.firstpage","1012"],["dc.bibliographiccitation.issue","5"],["dc.bibliographiccitation.journal","Nephrology Dialysis Transplantation"],["dc.bibliographiccitation.lastpage","1019"],["dc.bibliographiccitation.volume","29"],["dc.contributor.author","Rubel, D."],["dc.contributor.author","Stock, J."],["dc.contributor.author","Ciner, A."],["dc.contributor.author","Hiller, H."],["dc.contributor.author","Girgert, R."],["dc.contributor.author","Muller, G.-A."],["dc.contributor.author","Gross, O."],["dc.date.accessioned","2021-06-01T10:51:21Z"],["dc.date.available","2021-06-01T10:51:21Z"],["dc.date.issued","2013"],["dc.identifier.doi","10.1093/ndt/gft434"],["dc.identifier.uri","https://resolver.sub.uni-goettingen.de/purl?gro-2/86983"],["dc.language.iso","en"],["dc.notes.intern","DOI-Import GROB-425"],["dc.relation.eissn","1460-2385"],["dc.relation.issn","0931-0509"],["dc.title","Antifibrotic, nephroprotective effects of paricalcitol versus calcitriol on top of ACE-inhibitor therapy in the COL4A3 knockout mouse model for progressive renal fibrosis"],["dc.type","journal_article"],["dc.type.internalPublication","yes"],["dspace.entity.type","Publication"]]Details DOI