Zobrazeno 1 - 10
of 1 171
pro vyhledávání: '"H. Blake"'
Publikováno v:
BMC Musculoskeletal Disorders, Vol 23, Iss 1, Pp 1-9 (2022)
Abstract Background Self-management (SM) is a key recommended strategy for managing chronic low back pain (CLBP). However, SM programmes generate small to moderate benefits for reducing pain and disability in patients with CLBP. The benefits of the S
Externí odkaz:
https://doaj.org/article/5e6b8b501bc042399da74434c0079364
Autor:
H. Blake, S. Carlisle, L. Fothergill, J. Hassard, A. Favier, J. Corner, J. K. Ball, C. Denning
Publikováno v:
BMC Public Health, Vol 22, Iss 1, Pp 1-26 (2022)
Abstract Background Regular testing for Severe Acute Respiratory Syndrome Coronavirus 2 (SARS-CoV-2) is an important strategy for controlling virus outbreaks on university campuses during the COVID-19 pandemic but testing participation rates can be l
Externí odkaz:
https://doaj.org/article/d937225310354669bcd270014610c8dc
Publikováno v:
BMC Public Health, Vol 16, Iss 1, Pp 1-16 (2016)
Abstract Background HIV-related mHealth interventions have demonstrable efficacy in supporting treatment adherence, although the evidence base for promoting HIV testing is inconclusive. Progress is constrained by a limited understanding of processes
Externí odkaz:
https://doaj.org/article/e54dd53d8d55431885cabb3fe30e409d
Publikováno v:
BMC Public Health, Vol 16, Iss 1, Pp 1-1 (2016)
Externí odkaz:
https://doaj.org/article/3ea09d4d080f45c1a8d857bb40c8d904
Autor:
Chih-Chun Hsu, Adam J. Burgasser, Christopher A. Theissen, Jessica L. Birky, Christian Aganze, Roman Gerasimov, Sarah J. Schmidt, Cullen H. Blake, Kevin R. Covey, Elizabeth Moreno-Hilario, Christopher R. Gelino, Javier Serna, Joel R. Brownstein, Katia Cunha
Publikováno v:
The Astrophysical Journal Supplement Series, Vol 274, Iss 2, p 40 (2024)
We present precise measurements of radial (RV) and projected rotational ( $v\sin i$ ) velocities of a sample of 258 M6 to L2 dwarfs with multiepoch, high-resolution ( λ /Δ λ = 22,500), near-infrared (1.514–1.696 μ m) spectroscopic observations
Externí odkaz:
https://doaj.org/article/2d566a9a22f047eda558d614d6083c55
Autor:
Jared C. Siegel, Samuel Halverson, Jacob K. Luhn, Lily L. Zhao, Khaled Al Moulla, Paul Robertson, Chad F. Bender, Ryan C. Terrien, Arpita Roy, Suvrath Mahadevan, Fred Hearty, Joe P. Ninan, Jason T. Wright, Eric B. Ford, Christian Schwab, Guðmundur Stefánsson, Cullen H. Blake, Michael W. McElwain
Publikováno v:
The Astronomical Journal, Vol 168, Iss 4, p 158 (2024)
For solar-type stars, spots and their associated magnetic regions induce radial velocity perturbations through the Doppler rotation signal and the suppression of convective blueshift, collectively known as rotation modulation. We developed the Rotati
Externí odkaz:
https://doaj.org/article/78fc79b471624736bddad7eb31f2d1f9
Autor:
Corey Beard, Paul Robertson, Mark R. Giovinazzi, Joseph M. Akana Murphy, Eric B. Ford, Samuel Halverson, Te Han, Rae Holcomb, Jack Lubin, Rafael Luque, Pranav Premnath, Chad F. Bender, Cullen H. Blake, Qian Gong, Howard Isaacson, Shubham Kanodia, Dan Li, Andrea S. J. Lin, Sarah E. Logsdon, Emily Lubar, Michael W. McElwain, Andrew Monson, Joe P. Ninan, Jayadev Rajagopal, Arpita Roy, Christian Schwab, Gudmundur Stefansson, Ryan C. Terrien, Jason T. Wright
Publikováno v:
The Astronomical Journal, Vol 168, Iss 4, p 149 (2024)
We present a new analysis of Kepler-21, the brightest ( V = 8.5) Kepler system with a known transiting exoplanet, Kepler-21 b. Kepler-21 b is a radius valley planet ( R = 1.6 ± 0.2 R _⊕ ) with an Earth-like composition (8.38 ± 1.62 g cm ^–3 ),
Externí odkaz:
https://doaj.org/article/9e8d36f492f74b37afd276b4f75a7811
Autor:
Mark R. Giovinazzi, Bryson Cale, Jason D. Eastman, Joseph E. Rodriguez, Cullen H. Blake, Keivan G. Stassun, Andrew Vanderburg, Michelle Kunimoto, Adam L. Kraus, Joseph Twicken, Thomas G. Beatty, Cayla M. Dedrick, Jonathan Horner, John A. Johnson, Samson A. Johnson, Nate McCrady, Peter Plavchan, David H. Sliski, Maurice L. Wilson, Robert A. Wittenmyer, Jason T. Wright, Marshall C. Johnson, Mark E. Rose, Matthew Cornachione
Publikováno v:
The Astronomical Journal, Vol 168, Iss 3, p 118 (2024)
We present a new analysis of the KELT-24 system, comprising a well-aligned hot Jupiter, KELT-24 b, and a bright ( V = 8.3), nearby ( d = 96.9 pc) F-type host star. KELT-24 b was independently discovered by two groups in 2019, with each reporting best
Externí odkaz:
https://doaj.org/article/e5f27cec64154aa4925458370eb7cda3
Autor:
Abigail Burrows, Samuel Halverson, Jared C. Siegel, Christian Gilbertson, Jacob Luhn, Jennifer Burt, Chad F. Bender, Arpita Roy, Ryan C. Terrien, Selma Vangstein, Suvrath Mahadevan, Jason T. Wright, Paul Robertson, Eric B. Ford, Gumundur Stefánsson, Joe P. Ninan, Cullen H. Blake, Michael W. McElwain, Christian Schwab, Jinglin Zhao
Publikováno v:
The Astronomical Journal, Vol 167, Iss 5, p 243 (2024)
We revisit the long-studied radial velocity (RV) target HD 26965 using recent observations from the NASA-NSF “NEID” precision Doppler facility. Leveraging a suite of classical activity indicators, combined with line-by-line RV analyses, we demons
Externí odkaz:
https://doaj.org/article/d86e74c21cd149b9869c8f5ea556f3b4
The Extreme Stellar-signals Project. III. Combining Solar Data from HARPS, HARPS-N, EXPRES, and NEID
Autor:
Lily L. Zhao, Xavier Dumusque, Eric B. Ford, Joe Llama, Annelies Mortier, Megan Bedell, Khaled Al Moulla, Chad F. Bender, Cullen H. Blake, John M. Brewer, Andrew Collier Cameron, Rosario Cosentino, Pedro Figueira, Debra A. Fischer, Adriano Ghedina, Manuel Gonzalez, Samuel Halverson, Shubham Kanodia, David W. Latham, Andrea S. J. Lin, Gaspare Lo Curto, Marcello Lodi, Sarah E. Logsdon, Christophe Lovis, Suvrath Mahadevan, Andrew Monson, Joe P. Ninan, Francesco Pepe, Rachael M. Roettenbacher, Arpita Roy, Nuno C. Santos, Christian Schwab, Guđmundur Stefánsson, Andrew E. Szymkowiak, Ryan C. Terrien, Stephane Udry, Sam A. Weiss, François Wildi, Thibault Wildi, Jason T. Wright
Publikováno v:
The Astronomical Journal, Vol 166, Iss 4, p 173 (2023)
We present an analysis of Sun-as-a-star observations from four different high-resolution, stabilized spectrographs—HARPS, HARPS-N, EXPRES, and NEID. With simultaneous observations of the Sun from four different instruments, we are able to gain insi
Externí odkaz:
https://doaj.org/article/887e68b95d464a76bbb643318247a2b8