alphaFeedback
astro-ph.GAastro-ph.EPastro-ph.IMastro-ph.SRastro-ph.HEgr-qc

On Valency

published · living versions
W_nfz7nj75·v1 · currentpublished
Keck Observations of the Galactic Center Source G2: Gas Cloud or Star?
with K. Phifer, T. Do, L. Meyer, A. M. Ghez +6
1 version

Preprints & journals

23 papers in the corpus · 2012–2025
L 363-38 b: a planet newly discovered with ESPRESSO orbiting a nearby M dwarf star2210.12710v1 · Lia F. Sartori, Christophe Lovis, Jean-Baptiste Delisle et al.2022 · 3 citationsA&A 670, A42 (2023)
Vector-apodizing phase plate coronagraph: design, current performance, and future development [Invited].34263828 · Doelman, D S, Snik, F, Por, E H et al.2021 · 30 citationsApplied optics. 2021;60(19):D52-D72
A Spatially-Resolved Survey of Distant Quasar Host Galaxies: I. Dynamics of galactic outflows2106.08337v1 · Andrey Vayner, Shelley A. Wright, Norman Murray et al.2021 · 30 citationsarXiv
Molecular mapping of the PDS70 system: No molecular absorption signatures from the forming planet PDS70 b2106.03615v1 · G. Cugno, P. Patapis, T. Stolker et al.2021 · 38 citationsA&A 653, A12 (2021)
Constraints on the nearby exoplanet ϵ\epsilon Ind Ab from deep near/mid-infrared imaging limits2105.09773v1 · Gayathri Viswanath, Markus Janson, Carl-Henrik Dahlqvist et al.2021 · 12 citationsA&A 651, A89 (2021)
Author Correction: Imaging low-mass planets within the habitable zone of α Centauri.33953194 · Wagner, K, Boehle, A, Pathak, P et al.2021 · 2 citationsNature communications. 2021;12(1):2651
High contrast imaging at 10 microns, a search for exoplanets around: Eps Indi A, Eps Eri, Tau Ceti, Sirius A and Sirius B2104.13032v1 · P. Pathak, D. J. M. Petit dit de la Roche, M. Kasper et al.2021 · 30 citationsA&A 652, A121 (2021)
Imaging low-mass planets within the habitable zone of α Centauri.33568657 · Wagner, K, Boehle, A, Pathak, P et al.2021 · 54 citationsNature communications. 2021;12(1):922
A Spatially-Resolved Survey of Distant Quasar Host Galaxies: II. Photoionization and Kinematics of the ISM2101.08291v1 · Andrey Vayner, Shelley A. Wright, Norman Murray et al.2021 · 11 citationsarXiv
Combining high contrast imaging and radial velocities to constrain the planetary architecture of nearby stars1907.04334v1 · A. Boehle, S. P. Quanz, C. Lovis et al.2019 · 11 citationsA&A 630, A50 (2019)
Characterizing and Improving the Data Reduction Pipeline for the Keck OSIRIS Integral Field Spectrograph1812.02053v1 · Kelly E. Lockhart, Tuan Do, James E. Larkin et al.2018 · 29 citationsarXiv
PynPoint: a modular pipeline architecture for processing and analysis of high-contrast imaging data1811.03336v2 · Tomas Stolker, Markus J. Bonse, Sascha P. Quanz et al.2018 · 70 citationsA&A 621, A59 (2019)
ERIS: revitalising an adaptive optics instrument for the VLT1807.05089v1 · Richard Davies, Simone Esposito, Hans Martin Schmid et al.2018 · 28 citationsarXiv
Testing General Relativity with Stellar Orbits around the Supermassive Black Hole in Our Galactic Center.28598651 · Hees, A, Do, T, Ghez, A M et al.2018 · 265 citationsPhysical review letters. 2017;118(21):211101
An Improved Distance and Mass Estimate for Sgr A* from a Multistar Orbit Analysis1607.05726v1 · A. Boehle, A. M. Ghez, R. Schodel et al.2016 · 351 citationsarXiv
Detection of Galactic Center source G2 at 3.8 μ\mum during periapse passage1410.1884v2 · Gunther Witzel, Andrea M. Ghez, Mark R. Morris et al.2014 · 108 citationsarXiv
The Keplerian orbit of G21312.1715v1 · L. Meyer, A. M. Ghez, G. Witzel et al.2013 · 9 citationsarXiv
Keck Observations of the Galactic Center Source G2: Gas Cloud or Star?1304.5280v2 · K. Phifer, T. Do, L. Meyer et al.2013 · 98 citationsarXivon Valency
The shortest-known-period star orbiting our Galaxy's supermassive black hole.23042888 · Meyer, L, Ghez, A M, Schödel, R et al.2012 · 227 citationsScience (New York, N.Y.). 2012;338(6103):84-7
Career total: 56 works. 23 are in this corpus.

Profile built from the corpus for this byline.

Author records are still filling in while the Hub is in alpha. If this is your page, you'll be able to claim it soon. Spot a mistake? Tell us.