![]() Durkee, Kurt Nielsen, Elisabeth Öström, Colin O'Dowd, Michael H. Gasparovic, and Ian BrooksĪ Case Study of Ship Track Formation in a Polluted Marine Boundary Layer, Kevin J. Hudson, Robert Pockalny, Lieve De Bock, René E. HellerĪ Case Study of Self-Checking Circuits Reliability, Jien-Chung LoĪ Case Study of Ships Forming and Not Forming Tracks in Moderately Polluted Clouds, Kevin J. Iaea, Januka Budhathoki-Uprety, Nina Pipalia, Abigail S. Randolph WatssĪbuse or Be Abused: Traumatic Memory, Sex Inequality, and Millennium as a Socio-Literary Device, Kate RoseĪcademic Standards and Calendar Committee Report #, University of Rhode Island Faculty SenateĪcademic Standards and Calendar Committee Report # is, University of Rhode Island Faculty SenateĪcademic Standards and Calendar Committee Report #, University Manual Section 8.33.31, University of Rhode Island Faculty SenateĪcademic Standards and Calendar Committee Report #, Accelerated Online Program Calendar AY 23-24, and Revisions to University Manual Section Chapter 8 and Appendix F, Transfer Policies, University of Rhode Island Faculty SenateĪcademic Standards and Calendar Committee Report #, Report on request concerning Columbus Day, University of Rhode Island Faculty SenateĪ Carbon Nanotube Optical Reporter Maps Endolysosomal Lipid Flux, Jena V. Donohue, Erin Firing, and Shuiming ChenĪbsolute Transports of Mass and Temperature for the North Atlantic Current– Subpolar Front System, Paula Pérez-Brunius, Tom Rossby, and D. ≤1 mas yr−1 for R>17, and are no larger than ∼10 mas yr−1 for R<17 mas yr−1.3D Printing Applications in the Business World, Dennis ZhitkovichĪ Bayesian Method for Detecting Pairwise Associations in Compositional Data, Emma Schwager, Himel Mallick, Steffen Ventz, and Curtis HuttenhowerĪBCC3 as a marker for multidrug resistance in non-small cell lung cancer, Yanbin Zhao, Hailing Lu, An Yan, Yanmei Yang, Qingwei Meng, Lichun Sun, Hui Pang, Chunhong Li, Xiaoqun Dong, and Li CaiĪbsolute geostrophic velocity within the Subantarctic Front in the Pacific Ocean, Kathleen A. We show that the zero-point errors in the proper motions are Measurements are shown to be accurate to typically ☑0 mas yr−1 at J,R∼19,18, rising to ±50 mas yr−1 at J,R∼22,21, and are tied to zero using the extragalactic reference frame. celestial coordinates, which are tied to the International Celestial Reference Frame via the Tycho–2 referenceĬatalogue, are accurate to better than ☐.2 arcsec at J,R∼19,18, rising to ☐.3 arcsec at J,R∼22,21, with positional-dependent systematic effects from bright to faint magnitudes at the ∼0.1-arcsec level. ![]() Their accuracies by comparison with external data sets using the first release of data, the South Galactic Cap survey. We describe the algorithms employed in the derivation of the astrometric parameters of the data, and demonstrate In this, the third in a series of three papers concerning the SuperCOSMOS Sky Survey, we describe the astrometric properties This supports cold mode accretion where filament galaxies with a large gravitational potential can draw gas from the large-scale structure. We suggest that this is evidence for massive galaxies accreting cold gas from the intrafilament medium that can replenish some HI gas. The HI fraction is measured for different stellar masses and fifth nearest neighbour projected densities ($\Sigma_$. HI spectral stacking of HI Parkes all sky survey observations yields the HI fraction for filament galaxies and a field control sample. This work uses the 6 degree Field Galaxy Survey and the Discrete Persistent Structures Extractor to define the filamentary structure of the local cosmic web. We examine the HI-to-stellar mass ratio (HI fraction) for galaxies near filament backbones within the nearby Universe ($d <$ 181 Mpc). We show that the zeropoint errors in the proper motions are 17 and are no larger than 10 mas/yr for R < 17 mas/yr. The proper motion measurements are shown to be accurate to typically /- 10 mas/yr at J,R=19,18 rising to /- 50 mas/yr at J,R=22,21 and are tied to zero using the extragalactic reference frame. We show that the celestial coordinates, which are tied to the International Celestial Reference Frame via the Tycho-2 reference catalogue, are accurate to better than /- 0.2 arcsec at J,R=19,18 rising to /- 0.3 arcsec at J,R=22,21 with positional dependent systematic effects from bright to faint magnitudes at the /- 0.1 arcsec level. We describe the algorithms employed in the derivation of the astrometric parameters of the data, and demonstrate their accuracies by comparison with external datasets using the first release of data, the South Galactic Cap survey. In this, the third in a series of three papers concerning the SuperCOSMOS Sky Survey, we describe the astrometric properties of the database.
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