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  • Oxford University Press (OUP)  (19)
  • 11
    In: Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP), Vol. 491, No. 3 ( 2020-01-21), p. 3374-3384
    Kurzfassung: Using kinematics from Gaia and the large elemental abundance space of the second data release of the GALAH survey, we identify two new members of the Fimbulthul stellar stream, and chemically tag them to massive, multimetallic globular cluster ω Centauri. Recent analysis of the second data release of Gaia had revealed the Fimbulthul stellar stream in the halo of the Milky Way. It had been proposed that the stream is associated with the ω Cen, but this proposition relied exclusively upon the kinematics and metallicities of the stars to make the association. In this work, we find our two new members of the stream to be metal-poor stars that are enhanced in sodium and aluminium, typical of second population globular cluster stars, but not otherwise seen in field stars. Furthermore, the stars share the s-process abundance pattern seen in ω Cen, which is rare in field stars. Apart from one star within 1.5 deg of ω Cen, we find no other stars observed by GALAH spatially near ω Cen or the Fimbulthul stream that could be kinematically and chemically linked to the cluster. Chemically tagging stars in the Fimbulthul stream to ω Cen confirms the earlier work, and further links this tidal feature in the Milky Way halo to ω Cen.
    Materialart: Online-Ressource
    ISSN: 0035-8711 , 1365-2966
    Sprache: Englisch
    Verlag: Oxford University Press (OUP)
    Publikationsdatum: 2020
    ZDB Id: 2016084-7
    SSG: 16,12
    Standort Signatur Einschränkungen Verfügbarkeit
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  • 12
    In: Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP), Vol. 507, No. 1 ( 2021-08-17), p. 43-54
    Kurzfassung: The European Space Agency (ESA) Gaia mission has enabled the remarkable discovery that a large fraction of the stars near the solar neighbourhood are debris from a single in-falling system, the so-called Gaia-Sausage-Enceladus (GSE). This discovery provides astronomers for the first time with a large cohort of easily observable, unevolved stars that formed in a single extragalactic environment. Here we use these stars to investigate the ‘Spite plateau’ – the near-constant lithium abundance observed in unevolved metal-poor stars across a wide range of metallicities (−3 & lt; [Fe/H] & lt; −1). Our aim is to test whether individual galaxies could have different Spite plateaus – e.g. the interstellar medium could be more depleted in lithium in a lower galactic mass system due to it having a smaller reservoir of gas. We identified 93 GSE dwarf stars observed and analysed by the GALactic Archaeology with HERMES (GALAH) survey as part of its Data Release 3 (DR3). Orbital actions were used to select samples of GSE stars, and comparison samples of halo and disc stars. We find that the GSE stars show the same lithium abundance as other likely accreted stars and in situ Milky Way stars. Formation environment leaves no imprint on lithium abundances. This result fits within the growing consensus that the Spite plateau, and more generally the ‘cosmological lithium problem’ – the observed discrepancy between the amount of lithium in warm, metal-poor dwarf stars in our Galaxy, and the amount of lithium predicted to have been produced by big bang nucleosynthesis – is the result of lithium depletion processes within stars.
    Materialart: Online-Ressource
    ISSN: 0035-8711 , 1365-2966
    Sprache: Englisch
    Verlag: Oxford University Press (OUP)
    Publikationsdatum: 2021
    ZDB Id: 2016084-7
    SSG: 16,12
    Standort Signatur Einschränkungen Verfügbarkeit
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  • 13
    Online-Ressource
    Online-Ressource
    Oxford University Press (OUP) ; 2017
    In:  Monthly Notices of the Royal Astronomical Society Vol. 464, No. 2 ( 2017-01-11), p. 1259-1281
    In: Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP), Vol. 464, No. 2 ( 2017-01-11), p. 1259-1281
    Materialart: Online-Ressource
    ISSN: 0035-8711 , 1365-2966
    Sprache: Englisch
    Verlag: Oxford University Press (OUP)
    Publikationsdatum: 2017
    ZDB Id: 2016084-7
    SSG: 16,12
    Standort Signatur Einschränkungen Verfügbarkeit
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  • 14
    In: Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP), Vol. 491, No. 2 ( 2020-01-11), p. 2465-2480
    Kurzfassung: We present the serendipitous discovery of the fastest main-sequence hyper-velocity star (HVS) by the Southern Stellar Stream Spectroscopic Survey (S5). The star S5-HVS1 is a ∼2.35 M⊙ A-type star located at a distance of ∼9 kpc from the Sun and has a heliocentric radial velocity of 1017 ± 2.7 $\mathrm{\, km\, s^{-1}}$ without any signature of velocity variability. The current 3D velocity of the star in the Galactic frame is 1755 ± 50 $\mathrm{\, km\, s^{-1}}$. When integrated backwards in time, the orbit of the star points unambiguously to the Galactic Centre, implying that S5-HVS1 was kicked away from Sgr A* with a velocity of ∼1800 $\mathrm{\, km\, s^{-1}}$ and travelled for 4.8 Myr to its current location. This is so far the only HVS confidently associated with the Galactic Centre. S5-HVS1 is also the first hyper-velocity star to provide constraints on the geometry and kinematics of the Galaxy, such as the Solar motion Vy,⊙ = 246.1 ± 5.3 $\mathrm{\, km\, s^{-1}}$ or position R0 = 8.12 ± 0.23 kpc. The ejection trajectory and transit time of S5-HVS1 coincide with the orbital plane and age of the annular disc of young stars at the Galactic Centre, and thus may be linked to its formation. With the S5-HVS1 ejection velocity being almost twice the velocity of other hyper-velocity stars previously associated with the Galactic Centre, we question whether they have been generated by the same mechanism or whether the ejection velocity distribution has been constant over time.
    Materialart: Online-Ressource
    ISSN: 0035-8711 , 1365-2966
    Sprache: Englisch
    Verlag: Oxford University Press (OUP)
    Publikationsdatum: 2020
    ZDB Id: 2016084-7
    SSG: 16,12
    Standort Signatur Einschränkungen Verfügbarkeit
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  • 15
    In: British Journal of Dermatology, Oxford University Press (OUP), Vol. 188, No. Supplement_2 ( 2023-01-25)
    Kurzfassung: Abrocitinib is an oral Janus kinase 1 inhibitor with demonstrated efficacy in moderate-to-severe atopic dermatitis (AD). To evaluate the long-term safety profile of abrocitinib and provide relevant information for practitioners. Data from patients who received ≥1 dose of abrocitinib 200 mg or 100 mg in the JADE clinical program were pooled in two cohorts. The consistent-dose (CD) cohort comprised patients who received the same abrocitinib dose during the entire exposure time in parent phase 3 studies and/or the long-term extension study JADE EXTEND (NCT03422822). Parent studies were: JADE MONO-1 (NCT03349060), JADE MONO-2 (NCT03575871), JADE TEEN (NCT03796676), JADE COMPARE (NCT03720470), JADE DARE (NCT04345367; 200 mg only) and JADE REGIMEN (NCT03627767); in JADE REGIMEN only patients from the open-label run-in phase (200 mg only) who did not subsequently enter the randomized phase were included. Patients from the phase 2b study (NCT02780167) were also included in the CD cohort. The variable-dose (VD) cohort comprised patients who received different doses of abrocitinib (200 and 100 mg) throughout exposure time in the parent study JADE REGIMEN and in JADE EXTEND, if enrolled. Patients included in the VD cohort completed the open-label period of JADE REGIMEN (abrocitinib 200 mg only) and entered the randomized phase (abrocitinib 200 mg, abrocitinib 100 mg or placebo); some patients subsequently entered the JADE REGIMEN rescue phase (abrocitinib 200 mg) and/or JADE EXTEND (abrocitinib 200 or 100 mg). The data cutoff was 16 April 2021. A Cox regression analysis evaluated risk factors for specific events of interest. Data from 3582 patients (4313.4 patient-years) were analysed: 2784 patients in the CD cohort (abrocitinib 200 mg, n = 1761, abrocitinib 100 mg, n = 1023) and 798 patients in the VD cohort. Duration of exposure was ≥48 weeks in 43.6%, 66.9% and 86.1% and ≥96 weeks in 18.0%, 23.2% and 45.4% of patients in the CD 200 mg, 100 mg and VD cohorts, respectively. In the CD and VD cohorts, the median age was 30.0 and 29.0 years; 490 (17.6%) and 145 patients (18.2%) were adolescents, and 143 (5.1%) and 30 patients (3.8%) were aged ≥65 years at screening, respectively. Incidence rates (IRs; unique patients with events per 100 patient-years) of serious adverse events (SAEs), deaths, and treatment-emergent adverse events of special interest are shown in Table 1. IRs for SAEs were consistent across abrocitinib doses but were higher in patients aged ≥65 years vs. younger patients. Serious infections were the most frequent SAEs; frequency was not dose related. Herpes zoster (HZ), herpes simplex and pneumonia were the most frequent serious infections. From a Cox regression analysis, potential risk factors for treatment-emergent HZ included abrocitinib dose, baseline age, medical history of HZ, absolute lymphocyte count & lt;1000 mm−3 prior to infection and region. Most (95%) adjudicated opportunistic HZ infections were cutaneous; 2 (5%) were extracutaneous (one serious disseminated varicella-zoster virus infection, one serious HZ meningitis). IRs for nonmelanoma skin cancer, malignancy (excluding nonmelanoma skin cancer), thrombocytopenia and lymphopenia were higher in patients aged ≥65 years vs. younger patients but were not dose related. Abrocitinib has an acceptable long-term safety profile in this large analysis of patients with moderate-to-severe AD. Risk of SAEs, HZ infection, malignancies and hematologic abnormalities increased with older age; HZ risk was also related to dose and prior HZ infection.
    Materialart: Online-Ressource
    ISSN: 0007-0963 , 1365-2133
    Sprache: Englisch
    Verlag: Oxford University Press (OUP)
    Publikationsdatum: 2023
    ZDB Id: 2004086-6
    Standort Signatur Einschränkungen Verfügbarkeit
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  • 16
    Online-Ressource
    Online-Ressource
    Oxford University Press (OUP) ; 2000
    In:  American Journal of Clinical Pathology Vol. 113, No. 4 ( 2000-04-01), p. 541-545
    In: American Journal of Clinical Pathology, Oxford University Press (OUP), Vol. 113, No. 4 ( 2000-04-01), p. 541-545
    Materialart: Online-Ressource
    ISSN: 1943-7722 , 0002-9173
    RVK:
    RVK:
    Sprache: Englisch
    Verlag: Oxford University Press (OUP)
    Publikationsdatum: 2000
    ZDB Id: 2039921-2
    Standort Signatur Einschränkungen Verfügbarkeit
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  • 17
    Online-Ressource
    Online-Ressource
    Oxford University Press (OUP) ; 2000
    In:  American Journal of Clinical Pathology Vol. 113, No. 2 ( 2000-02-01), p. 288-294
    In: American Journal of Clinical Pathology, Oxford University Press (OUP), Vol. 113, No. 2 ( 2000-02-01), p. 288-294
    Materialart: Online-Ressource
    ISSN: 1943-7722 , 0002-9173
    RVK:
    RVK:
    Sprache: Englisch
    Verlag: Oxford University Press (OUP)
    Publikationsdatum: 2000
    ZDB Id: 2039921-2
    Standort Signatur Einschränkungen Verfügbarkeit
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  • 18
    In: Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP), Vol. 481, No. 2 ( 2018-12-01), p. 2666-2684
    Materialart: Online-Ressource
    ISSN: 0035-8711 , 1365-2966
    Sprache: Englisch
    Verlag: Oxford University Press (OUP)
    Publikationsdatum: 2018
    ZDB Id: 2016084-7
    SSG: 16,12
    Standort Signatur Einschränkungen Verfügbarkeit
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  • 19
    In: British Journal of Dermatology, Oxford University Press (OUP), Vol. 188, No. Supplement_2 ( 2023-01-25)
    Kurzfassung: Abrocitinib, an oral, once-daily Janus kinase 1-selective inhibitor, had a superior efficacy vs. dupilumab in head-to-head randomized trials in moderate-to-severe atopic dermatitis (AD). Data on patients who switched from dupilumab to abrocitinib have been limited. To evaluate abrocitinib response in patients with moderate-to-severe AD who were responders or nonresponders to dupilumab. Dupilumab-treated patients from the JADE DARE trial (NCT04345367), which was designed to compare the efficacy and safety of 26-week abrocitinib (200 mg daily) vs. dupilumab (300 mg bi-weekly) in patients receiving topical medicated therapy, had the option to switch to abrocitinib 200 mg by enrolling to an open-label JADE EXTEND trial (NCT03422822). In this analysis, we evaluated the response to abrocitinib 200 mg at week 12 of JADE EXTEND of responders and nonresponders to dupilumab at week 26 of JADE DARE. Response and nonresponse were defined as patients’ achievement and nonachievement, respectively, of ≥50%, ≥ 75% or ≥90% improvement from the JADE DARE baseline in Eczema Area and Severity Index (EASI-50, EASI-75 or EASI-90), ≥ 4-point improvement from JADE DARE baseline in Peak Pruritus Numerical Rating Scale (PP-NRS4), and PP-NRS score of 0 or 1 (PP-NRS 0/1) at week 26 of JADE DARE. In addition, changes in individual EASI and PP-NRS scores were evaluated in dupilumab-treated patients with significant skin lesions (EASI ≥16) or itch burden (PP-NRS ≥7) at week 26 of JADE DARE. Patients who withdrew from JADE EXTEND were considered nonresponders after withdrawal. Additionally, adverse events (AEs) of dupilumab-treated patients from JADE DARE occurring during JADE EXTEND were assessed. Out of 365 dupilumab-treated patients in JADE DARE, 312 received treatment in JADE EXTEND. After 12 weeks of switching to abrocitinib, EASI-50 response was maintained in 98% of patients (277/282) who had attained EASI-50 after 26 weeks of dupilumab. Those values were 95% (232/245) for EASI-75, 88% (143/162) for EASI-90, 91% (192/210) for PP-NRS4 and 79% (86/109) for PP-NRS 0/1. Conversely, among patients who did not attain EASI-50 after 26 weeks of dupilumab, switching to abrocitinib for 12 weeks resulted in 75% (12/16) of patients attaining this level of response. Those values were 77% (41/53) for EASI-75, 62% (85/136) for EASI-90, 51% (46/90) for PP-NRS4 and 45% (86/192) for PP-NRS 0/1. Among dupilumab-treated patients with EASI ≥16 at week 26 of JADE DARE, 91% (10/11) experienced improvements (i.e. EASI & lt;16), after switching to abrocitinib for 12 weeks; in two such patients, score changes were consistent with ≥97% improvement in EASI from JADE DARE week 26 to JADE EXTEND week 12 (from 45.5 to 0 and from 42.3 to 1.4). Among patients with PP-NRS ≥7 at JADE DARE week 26, 75% (12/16) showed an improvement (i.e. PP-NRS score & lt;7), 12 weeks after switching to abrocitinib; three such patients achieved a PP-NRS score of 0 or 1. During JADE EXTEND, 57% (178/312) of patients who previously received dupilumab experienced AEs and 3% (9/312) experienced serious AEs. Most patients with moderate-to-severe AD who switched from dupilumab to abrocitinib after 26 weeks maintained their response, while a great proportion of the nonresponders achieved clinically relevant efficacy outcomes 12 weeks after the switch. The safety profile of abrocitinib after switching from dupilumab was consistent with that of previous safety analyses; serious AEs were relatively rare.
    Materialart: Online-Ressource
    ISSN: 0007-0963 , 1365-2133
    Sprache: Englisch
    Verlag: Oxford University Press (OUP)
    Publikationsdatum: 2023
    ZDB Id: 2004086-6
    Standort Signatur Einschränkungen Verfügbarkeit
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