1,726,682 research outputs found
MOESM3 of LINC01006 promotes cell proliferation and metastasis in pancreatic cancer via miR-2682-5p/HOXB8 axis
No full textAdditional file 3: Figure S3. (A) Expression profile of HOXB8 and miR-2682-5p from TCGA datasets. (B) Pearson correlation analysis of interrelation among LINC01006, HOXB8 and miR-2682-5p from TCGA datasets. (C) RT-qPCR assayed the expression of miR-2682-5p, HOXB8 and LINC01006 in PC tissues or matched normal samples. (D) The expression correlation among LINC01006, HOXB8 and miR-2682-5p was analyzed via Pearson correlation analysis. **P < 0.01, ***P < 0.00
Other title: Testimony on House Bill 2682; Other title: House Bill 2682; Other title: HB 2682
No full textApplication/pdf.; "February 14, 2012."; Testimony before the Kansas Legislature, House Government Efficiency Committee, presented by Ray Roberts, Secretary, Kansas Department of Corrections.Testimony in support of HB 2682, which "repeals statutes that authorized the secretary of corrections to purchase real estate."
Mandurama photograph collection [2682] [picture] /
No full textAlso available in an electronic version via the Internet at: http://nla.gov.au/nla.pic-an8526486-2682
Extended halo of NGC 2682 (M 67) from Gaia DR2
No full textContext. NGC 2682 is a nearby open cluster that is approximately 3.5 Gyr old. Dynamically, most open clusters are expected to dissolve on shorter timescales of ≈1 Gyr. That it has survived until now means that NGC 2682 was likely much more massive in the past and is bound to have an interesting dynamical history. Aims. We investigate the spatial distribution of the stars in NGC 2682 to constrain dynamical evolution of the cluster. We particularly focus on the marginally bound stars in the cluster outskirts. Methods. We used Gaia DR2 data to identify NGC 2682 members up to a distance of ∼150 pc (10°). The two methods Clusterix and UPMASK were applied to this end. We estimated distances to obtain 3D stellar positions using a Bayesian approach to parallax inversion, with an appropriate prior for star clusters. We calculated the orbit of NGC 2682 using the GRAVPOT16 software. Results. The cluster extends up to 200′ (50 pc), which implies that its size is at least twice as large as previously believed. This exceeds the cluster Hill sphere based on the Galactic potential at the distance of NGC 2682. Conclusion. The extra-tidal stars in NGC 2682 may originate from external perturbations such as disc-shocking or dynamical evaporation from two-body relaxation. The former origin is plausible given the orbit of NGC 2682, which crossed the Galactic disc ≈40 Myr ago
FIGURE 13 in Nephtyidae (Annelida, Polychaeta) from southern Europe 2682
No full textFIGURE 13. Relationships between: A. Number of segments and body length. B. Body length and body width. C. Length of ventral cirri (VC) and dorsal cirri (DC) of chaetiger 1. D. Length of pharynx distalmost subterminal papillae and middorsal papilla. Nephtys caeca. N. ciliata. × N. longosetosa.Published as part of Ravara, Ascensão, Cunha, Marina R. & Pleijel, Fredrik, 2010, Nephtyidae (Annelida, Polychaeta) from southern Europe 2682, pp. 1-68 in Zootaxa 2682 (1) on page 39, DOI: 10.11646/zootaxa.2682.1.1, http://zenodo.org/record/534623
Block Card 2682 Otis Street
No full textThis image was produced by the Auditor's Office in Lucas County, Ohio for tax assessment purposes. Associated dates are approximate. Descriptive terms related to this photograph include: Colonial Revival Style | 2682 Otis Street (Toledo, Ohio) | Dwelling | Parkdale Addition | Auburndale Area (Toledo, Ohio
McKay, Silas Harland, 1807-1884 (SC 2682)
No full textFinding aid and scans (Click on Additional Files below) for Manuscripts Small Collection 2682. Promissory note dated 23 April 1857 of S. H. McKay of Warren County, Kentucky to Samuel Worthington for 1000 was made on the note in 1859 by Joseph Rogers Underwood. Also includes a survey sketch of the land
Going Beyond Counting First Authors in Author Co-citation Analysis
No full textThe present study examines one of the fundamental aspects of author co-citation analysis (ACA) - the way co-citation
counts are defined. Co-citation counting provides the data on which all subsequent statistical analyses and mappings
are based, and we compare ACA results based on two different types of co-citation counting - the traditional type that
only counts the first one among a cited work's authors on the one hand and a non-traditional type that takes into
account the first 5 authors of a cited work on the other hand. Results indicate that the picture produced through this non-traditional author co-citation counting contains more coherent author groups and is therefore considerably clearer. However, this picture represents fewer specialties in the research field being studied than that produced through the traditional first-author co-citation counting when the same number of top-ranked authors is selected and analyzed. Reasons for these effects are discussed
- …
