Zobrazeno 1 - 10
of 109
pro vyhledávání: '"Andrew J. Monson"'
Autor:
Abigail J. Lee, Andrew J. Monson, Wendy L. Freedman, Barry F. Madore, Kayla A. Owens, Rachael L. Beaton, Coral Espinoza, Tongtian Ren, Yi Ren
Publikováno v:
The Astrophysical Journal, Vol 967, Iss 1, p 22 (2024)
We present near-infrared JHK photometry for the resolved stellar populations in 13 nearby galaxies: NGC 6822, IC 1613, NGC 3109, Sextans B, Sextans A, NGC 300, NGC 55, NGC 7793, NGC 247, NGC 5253, Cen A, NGC 1313, and M83, acquired from the 6.5 m Baa
Externí odkaz:
https://doaj.org/article/2567cdc6e55b4add8900cc4b5061787c
Autor:
Brian D. Metzger, Andrew J. Monson, D. Christopher Martin, Keri Hoadley, Mark Seibert, Ken J. Shen, James D. Neill, Gudmundur Stefansson, Andrew McWilliam, Bradley E. Schaefer
Publikováno v:
Nature. 587:387-391
Stellar mergers are a brief but common phase in the evolution of binary star systems1,2. These events have many astrophysical implications; for example, they may lead to the creation of atypical stars (such as magnetic stars3, blue stragglers4 and ra
Autor:
Radek Poleski, P. Pietrukowicz, Jennifer L. Marshall, S. Kozlowski, Nidia Morrell, Andrew J. Monson, Ian B. Thompson, S. E. Persson, Andrew McWilliam, P. Mróz, Jan Skowron, Wyrzykowski, David J. Osip, Wojciech Pych, Yuri Beletsky, Krzysztof Ulaczyk, M. Rozyczka, G. S. Burley, Aaron Dotter, Andrzej Udalski, Michał K. Szymański, A. Schwarzenberg-Czerny, Igor Soszyński
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 494:846-849
Autor:
Eric B. Ford, Samuel Halverson, Michael Endl, Chad F. Bender, Suvrath Mahadevan, William D. Cochran, Joe P. Ninan, Ryan Terrien, Steven Janowiecki, Fred Hearty, Christian Schwab, Gudmundur Stefansson, Jason T. Wright, Shubham Kanodia, Niv Drory, Lawrence W. Ramsey, Scott A. Diddams, Andrew J. Monson, Arpita Roy, Andrew J. Metcalf, Paul Robertson
The Habitable zone Planet Finder (HPF) is a fiber fed precise radial velocity spectrograph at the 10 m Hobby Eberly Telescope (HET). Due to its fixed altitude design, the HET pupil changes appreciably across a track, leading to significant changes of
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9f241d83fe7cfbfc3c720a8836586968
http://arxiv.org/abs/2103.05148
http://arxiv.org/abs/2103.05148
Autor:
Rae Holcomb, Michael Endl, Arpita Roy, Gudmundur Stefansson, Chad F. Bender, Andrew J. Monson, Fred Hearty, Connor Fredrick, Suvrath Mahadevan, Shubham Kanodia, Alex Wolszczan, Lawrence W. Ramsey, William D. Cochran, Scott A. Diddams, Paul Robertson, Ryan Terrien, Andrew J. Metcalf, Christian Schwab, Samuel Halverson, Joe P. Ninan
The coherent low-frequency radio emission detected by LOFAR from Gliese 1151, a quiescent M4.5 dwarf star, has radio emission properties consistent with theoretical expectations of star-planet interactions for an Earth-sized planet on a 1-5 day orbit
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::39b7e699d057fcac9cb9ad3a3bace088
http://arxiv.org/abs/2102.02233
http://arxiv.org/abs/2102.02233
Autor:
Rachael L. Beaton, Wendy L. Freedman, Barry F. Madore, In Sung Jang, Jillian R. Neeley, Andrew J. Monson, Mark Seibert, Myung Gyoon Lee, Jeffrey A. Rich, Taylor J. Hoyt
The primary goal of the Carnegie Chicago Hubble Program (CCHP) is to calibrate the zero-point of the Type Ia supernova (SN Ia) Hubble Diagram through the use of Population II standard candles. So far, the CCHP has measured direct distances to 11 SNe
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::8befb76baa0a866fce9445c917541496
http://arxiv.org/abs/2101.12232
http://arxiv.org/abs/2101.12232
Autor:
Chad F. Bender, Andrew J. Monson, Cullen H. Blake, Michael W. McElwain, Ryan Terrien, Paul Robertson, Samuel Halverson, Sarah E. Logsdon, Suvrath Mahadevan, Arvind F. Gupta, Gudmundur Stefansson, Arpita Roy, Jacob K. Luhn, Shubham Kanodia, Joe P. Ninan, Eric B. Ford, Fred Hearty, Jason T. Wright, Christian Schwab
NEID is a high-resolution optical spectrograph on the WIYN 3.5-m telescope at Kitt Peak National Observatory and will soon join the new generation of extreme precision radial velocity instruments in operation around the world. We plan to use the inst
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::726f8869eacc9486de4d841dab136f1a
http://arxiv.org/abs/2101.11689
http://arxiv.org/abs/2101.11689
Publikováno v:
X-Ray, Optical, and Infrared Detectors for Astronomy IX.
In the search for exoplanets, the TESS mission shifts much of the focus in transit detection towards observing nearby cool stars.1 Many of the M-dwarf systems identified can be followed up from the ground with meter class telescopes or smaller to con
Autor:
Samuel Halverson, Gudmundur Stefansson, Andrew J. Monson, Joe P. Ninan, Arpita Roy, Chad F. Bender, Shubham Kanodia, Lawrence W. Ramsey, Suvrath Mahadevan, Colin Nitroy, Frederick R. Hearty, Ryan Terrien, Paul Robertson, Christian Schwab, Michael W. McElwain, Daniel J. Stevens, Emily Lubar
Publikováno v:
Ground-based and Airborne Instrumentation for Astronomy VIII.
The NEID spectrograph is a R $\sim$ 120,000 resolution fiber-fed and highly stabilized spectrograph for extreme radial velocity (RV) precision. It is being commissioned at the 3.5 m WIYN telescope in Kitt Peak National Observatory with a desired inst
Autor:
Lawrence W. Ramsey, Samuel Halverson, Chad F. Bender, Joe P. Ninan, Suvrath Mahadevan, Connor Fredrick, Ryan Terrien, Gudmundur Stefansson, Andrew J. Metcalf, Scott A. Diddams, Arpita Roy, Andrew J. Monson
Publikováno v:
X-Ray, Optical, and Infrared Detectors for Astronomy IX.
High precision Doppler spectroscopy hinges on an accurate understanding of the wavelength-to-pixel mapping (wavelength solution) of the spectrograph, including particularly systematics related to the detector. Herein, we describe the uniformity and s