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  • 1
    Online-Ressource
    Online-Ressource
    Oxford University Press (OUP) ; 2019
    In:  Monthly Notices of the Royal Astronomical Society Vol. 484, No. 4 ( 2019-04-21), p. 5315-5329
    In: Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP), Vol. 484, No. 4 ( 2019-04-21), p. 5315-5329
    Materialart: Online-Ressource
    ISSN: 0035-8711 , 1365-2966
    Sprache: Englisch
    Verlag: Oxford University Press (OUP)
    Publikationsdatum: 2019
    ZDB Id: 2016084-7
    SSG: 16,12
    Standort Signatur Einschränkungen Verfügbarkeit
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  • 2
    Online-Ressource
    Online-Ressource
    American Astronomical Society ; 2020
    In:  The Astrophysical Journal Supplement Series Vol. 249, No. 2 ( 2020-08-01), p. 22-
    In: The Astrophysical Journal Supplement Series, American Astronomical Society, Vol. 249, No. 2 ( 2020-08-01), p. 22-
    Kurzfassung: Radial velocity (RV) variable stars are important in astrophysics. The Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST) spectroscopic survey has provided ∼6.5 million stellar spectra in its Data Release 4 (DR4). During the survey ∼4.7 million unique sources were targeted and ∼1 million stars observed repeatedly. The probabilities of stars being RV variables are estimated by comparing the observed RV variations with simulated ones. We build a catalog of 80,702 RV variable candidates with probability greater than 0.60 by analyzing the multi-epoch sources covered by LAMOST DR4. Simulations and cross-identifications show that the purity of the catalog is higher than 80%. The catalog consists of 77% binary systems and 7% pulsating stars as well as 16% pollution by single stars. 3138 RV variables are classified through cross-identifications with published results in literatures. By using the 3138 sources common in both LAMOST and a collection of published RV variable catalogs, we are able to analyze LAMOST’s RV variable detection rate. The efficiency of the method adopted in this work relies not only on the sampling frequency of observations but also periods and amplitudes of RV variables. With the progress of LAMOST, Gaia, and other surveys, more and more RV variables will be confirmed and classified. This catalog is valuable for other large-scale surveys, especially for RV variable searches. The catalog will be released according to the LAMOST Data Policy via  http://dr4.lamost.org .
    Materialart: Online-Ressource
    ISSN: 0067-0049 , 1538-4365
    RVK:
    Sprache: Unbekannt
    Verlag: American Astronomical Society
    Publikationsdatum: 2020
    ZDB Id: 2006860-8
    ZDB Id: 2207650-5
    SSG: 16,12
    Standort Signatur Einschränkungen Verfügbarkeit
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  • 3
    Online-Ressource
    Online-Ressource
    American Association for Cancer Research (AACR) ; 2023
    In:  Cancer Research Vol. 83, No. 5_Supplement ( 2023-03-01), p. P1-05-31-P1-05-31
    In: Cancer Research, American Association for Cancer Research (AACR), Vol. 83, No. 5_Supplement ( 2023-03-01), p. P1-05-31-P1-05-31
    Kurzfassung: Introduction: Metaplastic breast cancer (MBC) is a rare breast tumor.WHO histological classification of breast tumors in 2019 divided MBC into the following seven types: low-grade adenosquamous carcinoma, fibromatoid metaplastic carcinoma, squamous cell carcinoma, spindle cell carcinoma, metaplastic carcinoma with mesenchymal differentiation, mixed metaplastic carcinoma and myoepithelial carcinoma. Based on single center data, this study intends to conduct a detailed analysis of the clinicopathological features, treatment and prognostic factors of MBC. Methods:We collected 259 MBCs treated in our center from 2006 to 2022. The patient’s age, histological type, image feature, tumor size, lymph node metastasis, tumor stage, immunohistochemical information, surgical plan and systemic adjuvant therapy were summarized and considered to explore the factors affecting the overall survival rate (OS) and disease-free survival rate (DFS). T-test and chi-square test were performed on the data. P & lt; 0.05 showed that the difference was statistically significant. Kaplan-Meier survival was used to analyze the long-term efficacy. Results: The incidence rate of MBC in breast cancer patients in our center is about 0.5%. They included 105 cases of squamous cell carcinoma (40.5%), 49 cases of mixed metaplastic carcinoma (18.9%), 41 cases of spindle cell carcinoma (15.8%), 27 cases of metaplasia carcinoma secreting matrix (10.4%), 6 cases of metaplastic carcinoma with mesenchymal differentiation (2.3%), 6 cases of myoepithelial carcinoma (2.3%), 3 cases of low-grade adenosquamous carcinoma (1.2%), 1 case of fibromatoid metaplasia carcinoma (0.4%) and 21 cases of unknown (8.1%). MBC were mainly three negative subtypes, which were 204 cases (78.8%), 41 cases (15.8%) luminal subtypes and 14 cases (5.4%) HER2 positive subtypes. There was no significant difference in the distribution of breast cancer subtypes among different histological types of MBC. There were 63 cases (24.3%) in clinical stage I, 171 cases (66.0%) in stage II, 23 cases (8.9%) in stage III and 2 cases (0.8%) in stage IV. 58 patients underwent core needle biopsy, of which only 7 (12.1%) reported histological types consistent with MBC. Among 154 patients with molybdenum target reports, 59 of them (38.3%) had malignant calcifications. The diagnostic coincidence rates of MRI, ultrasound and molybdenum target were 90.0%, 85.1% and 74.7% respectively. 258 cases of MBC received surgical treatment, including 183 cases of total mastectomy (70.9%), 53 cases of breast conserving surgery (20.5%) and 22 cases of quadrant resection (8.5%); 132 patients (51.2%) underwent axillary lymph node dissection and 93 patients (36.0%) underwent sentinel lymph node biopsy. 24 patients (9.3%) received neoadjuvant chemotherapy, of which only 2 (8.3%) achieved pathological complete remission. 56 patients (21.6%) received adjuvant radiotherapy, with a median of 25 times. 167 patients (64.5%) received adjuvant chemotherapy, and anthracycline sequential paclitaxel was the most commonly used regimen. The median follow-up was 31 months. The five-year DFS was 82.0%, and the five-year OS was 89.4%. Through Cox regression analysis, it was found that patients’ N stage (P=0.036) and receiving anthracycline sequential paclitaxel adjuvant chemotherapy (P=0.004) were independent prognostic factors. Conclusion: The histological types of MBC are complex. MRI is of high value in diagnosis. Conventional CNB is difficult to meet the needs of pathological tissue classification. Patients without lymph node metastasis and receiving anthracycline sequential paclitaxel adjuvant chemotherapy are associated with better prognosis. Through multidisciplinary standardized diagnosis and treatment, there is no significant difference between the prognosis of MBC and the common types of breast cancer. Keyword: metaplastic breast cancer; pathological characteristics; imaging; treatment; prognosis. Citation Format: Douwaner Liu, Jiajian Chen, Shuang Hao, Bingqiu Xiu, Qi Zhang, Liyi Zhang, Guangyu Liu, Zhimin Shao, Jiong Wu. A single center retrospective analysis of 259 cases of metaplastic breast cancer [abstract]. In: Proceedings of the 2022 San Antonio Breast Cancer Symposium; 2022 Dec 6-10; San Antonio, TX. Philadelphia (PA): AACR; Cancer Res 2023;83(5 Suppl):Abstract nr P1-05-31.
    Materialart: Online-Ressource
    ISSN: 1538-7445
    Sprache: Englisch
    Verlag: American Association for Cancer Research (AACR)
    Publikationsdatum: 2023
    ZDB Id: 2036785-5
    ZDB Id: 1432-1
    ZDB Id: 410466-3
    Standort Signatur Einschränkungen Verfügbarkeit
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  • 4
    In: Astronomy & Astrophysics, EDP Sciences, Vol. 658 ( 2022-02), p. A51-
    Kurzfassung: Context. Identification of new star cluster candidates in M 31 is fundamental for the study of the M 31 stellar cluster system. The machine-learning method convolutional neural network (CNN) is an efficient algorithm for searching for new M 31 star cluster candidates from tens of millions of images from wide-field photometric surveys. Aims. We search for new M 31 cluster candidates from the high-quality g - and i -band images of 21 245 632 sources obtained from the Pan-Andromeda Archaeological Survey (PAndAS) through a CNN. Methods. We collected confirmed M 31 clusters and noncluster objects from the literature as our training sample. Accurate double-channel CNNs were constructed and trained using the training samples. We applied the CNN classification models to the PAndAS g - and i -band images of over 21 million sources to search new M 31 cluster candidates. The CNN predictions were finally checked by five experienced human inspectors to obtain high-confidence M 31 star cluster candidates. Results. After the inspection, we identified a catalogue of 117 new M 31 cluster candidates. Most of the new candidates are young clusters that are located in the M 31 disk. Their morphology, colours, and magnitudes are similar to those of the confirmed young disk clusters. We also identified eight globular cluster candidates that are located in the M 31 halo and exhibit features similar to those of confirmed halo globular clusters. The projected distances to the M 31 centre for three of them are larger than 100 kpc.
    Materialart: Online-Ressource
    ISSN: 0004-6361 , 1432-0746
    RVK:
    RVK:
    Sprache: Englisch
    Verlag: EDP Sciences
    Publikationsdatum: 2022
    ZDB Id: 1458466-9
    SSG: 16,12
    Standort Signatur Einschränkungen Verfügbarkeit
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  • 5
    Online-Ressource
    Online-Ressource
    Elsevier BV ; 2016
    In:  Archives of Medical Research Vol. 47, No. 4 ( 2016-05), p. 315-320
    In: Archives of Medical Research, Elsevier BV, Vol. 47, No. 4 ( 2016-05), p. 315-320
    Materialart: Online-Ressource
    ISSN: 0188-4409
    Sprache: Englisch
    Verlag: Elsevier BV
    Publikationsdatum: 2016
    ZDB Id: 2010312-8
    Standort Signatur Einschränkungen Verfügbarkeit
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  • 6
    In: The Astronomical Journal, American Astronomical Society, Vol. 152, No. 2 ( 2016-08-03), p. 45-
    Materialart: Online-Ressource
    ISSN: 1538-3881
    Sprache: Unbekannt
    Verlag: American Astronomical Society
    Publikationsdatum: 2016
    ZDB Id: 2207625-6
    ZDB Id: 2003104-X
    Standort Signatur Einschränkungen Verfügbarkeit
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  • 7
    Online-Ressource
    Online-Ressource
    Springer Science and Business Media LLC ; 2021
    In:  Langenbeck's Archives of Surgery Vol. 406, No. 2 ( 2021-03), p. 283-299
    In: Langenbeck's Archives of Surgery, Springer Science and Business Media LLC, Vol. 406, No. 2 ( 2021-03), p. 283-299
    Materialart: Online-Ressource
    ISSN: 1435-2443 , 1435-2451
    RVK:
    Sprache: Englisch
    Verlag: Springer Science and Business Media LLC
    Publikationsdatum: 2021
    ZDB Id: 1459390-7
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  • 8
    In: Astronomy & Astrophysics, EDP Sciences, Vol. 676 ( 2023-08), p. A84-
    Kurzfassung: The mass-loss rate (MLR) is one of the most important parameters in astrophysics, because it impacts many areas of astronomy, such as ionizing radiation, wind feedback, star-formation rates, initial mass functions, stellar remnants, supernovae, and so on. However, the most important modes of mass loss are also the most uncertain, as the dominant physical mechanisms that lead to this phenomenon are stull largely unknown. Here we assemble the most complete and clean red supergiant (RSG) sample (2121 targets) so far in the Small Magellanic Cloud (SMC) with 53 different bands of data to study the MLR of RSGs. In order to match the observed spectral energy distributions (SEDs), we created a theoretical grid of 17 820 oxygen-rich models (“normal” and “dusty” grids are half-and-half) using the radiatively driven wind model of the DUSTY code, covering a wide range of dust parameters. We select the best model for each target by calculating the minimal modified chi-square and visual inspection. The resulting MLRs from DUSTY are converted to real MLRs based on the scaling relation, for which a total MLR of 6.16 × 10 −3   M ⊙ yr −1 is measured (corresponding to a dust-production rate of ∼6 × 10 −6   M ⊙ yr −1 ), with a typical MLR of ∼10 −6   M ⊙ yr −1 for the general population of the RSGs. The complexity of mass-loss estimations based on the SED is fully discussed for the first time, and our results indicate large uncertainties based on the photometric data (potentially up to one order of magnitude or more). The Hertzsprung-Russell (HR) and luminosity versus median-absolute-deviation (MAD) diagrams of the sample indicate the positive relation between luminosity and MLR. Meanwhile, the luminosity versus MLR diagrams show a “knee-like” shape with enhanced mass loss occurring above log 10 ( L / L ⊙ )≈4.6, which may be due to the degeneracy of luminosity, pulsation, low surface gravity, convection, and other factors. We derive our MLR relation using a third-order polynomial to fit the sample and compare our results with previous empirical MLR prescriptions. Given that our MLR prescription is based on a much larger sample than previous determinations, it provides a more accurate relation at the cool and luminous region of the HR diagram at low metallicity compared to previous studies. Finally, nine targets in our sample were detected in the UV, which could be an indicator of OB-type companions of binary RSGs.
    Materialart: Online-Ressource
    ISSN: 0004-6361 , 1432-0746
    RVK:
    RVK:
    Sprache: Englisch
    Verlag: EDP Sciences
    Publikationsdatum: 2023
    ZDB Id: 1458466-9
    SSG: 16,12
    Standort Signatur Einschränkungen Verfügbarkeit
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  • 9
    In: Journal of Materials Chemistry A, Royal Society of Chemistry (RSC), Vol. 8, No. 21 ( 2020), p. 10885-10890
    Materialart: Online-Ressource
    ISSN: 2050-7488 , 2050-7496
    Sprache: Englisch
    Verlag: Royal Society of Chemistry (RSC)
    Publikationsdatum: 2020
    ZDB Id: 2702232-8
    Standort Signatur Einschränkungen Verfügbarkeit
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  • 10
    In: Advanced Energy Materials, Wiley
    Kurzfassung: With the rapidly increasing demand for grid‐scale energy storage systems, rechargeable aqueous zinc ion batteries (ZIBs) are capturing attention as a highly promising technology with low cost and high safety. Nevertheless, rampant dendrite growth, hydrogen evolution reaction (HER), and corrosion of the zinc anode have dramatically impacted their practical application. Here, a self‐supported modified layer with ultrafine high‐entropy nanoparticles (2 nm) as the zincophilic sites is realized to modify the Zn anode for the first time. High‐entropy materials with unique continuously distributed potential gaps significantly reduce the activation energy of multi‐electron reactions and modulate ion transport during zinc deposition. Moreover, thanks to the hydrophobic properties and effective desolventizing ability of the ultrafine high‐entropy nanomaterial, the unfavorable side reactions of the zinc anode are prevented to promote the zinc deposition process. As a result, stable cycling of 3500 h at 1 mA cm −2 and 600 h at a high current density of 10 mA cm −2 is achieved. Coin cells and flexible pouch cells assembled with KMO and NH 4 V 4 O 10 cathodes also demonstrate promoted electrochemical performance. The dual effects of accelerating and homogenizing mechanisms in high‐entropy materials provide a new strategy for stabilizing zinc metal anodes.
    Materialart: Online-Ressource
    ISSN: 1614-6832 , 1614-6840
    Sprache: Englisch
    Verlag: Wiley
    Publikationsdatum: 2023
    ZDB Id: 2594556-7
    Standort Signatur Einschränkungen Verfügbarkeit
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