Publications

Haystack publications across all research areas: astronomy, geodesy, geospace and atmospheric science, and space technology. Publications listed here each include at least one Haystack author.

3087 Results found

Asymmetric distributions of H2O and SiO masers towards V627 Cas. Monthly Notices of the Royal Astronomical Society. (2020). DOI: https://doi.org/10.1093/mnras/staa1206

Detection of Periodicity in SiO Maser Intensity and Velocity Shift of the Symbiotic Star CH Cyg. The Astrophysical Journal Letters. (2020).

Monitoring the Morphology of M87* in 2009–2017 with the Event Horizon Telescope. The Astrophysical Journal. (2020).

SYMBA: An end-to-end VLBI synthetic data generation pipeline-Simulating Event Horizon Telescope observations of M 87. Astronomy & Astrophysics. (2020).

Monitoring the Morphology of M87* in 2009–2017 with the Event Horizon Telescope. The Astrophysical Journal. (2020). DOI: https://doi.org/10.3847/1538-4357/abac0d

Radio observations of HD 80606 near planetary periastron. Astronomy & Astrophysics. (2020). DOI: https://doi.org/10.1051/0004-6361/202038746

First Results of the Event Horizon Telescope. Butsuri. (2020). DOI: https://doi.org/10.11316/butsuri.75.1_4

A jet-bases emission model of the EHT 2017 image of M87. Arxiv. (2020). DOI: https://doi.org/10.48550/arxiv.2009.08641

Monitoring the morphology of M87∗ in 2009–2017 with the Event Horizon Telescope. Arxiv. (2020). DOI: https://doi.org/10.48550/arxiv.2009.11842

Polarization imaging of M87 jets by general relativistic radiative transfer calculation based on GRMHD simulations. Arxiv. (2020). DOI: https://doi.org/10.48550/arxiv.2002.00954

SYMBA: An end-to-end VLBI synthetic data generation pipeline Simulating Event Horizon Telescope observations of M87. Arxiv. (2020). DOI: https://doi.org/10.48550/arxiv.2004.01161

SYMBA: An end-to-end VLBI synthetic data generation pipeline: Simulating Event Horizon Telescope observations of M 87. Astronomy and Astrophysics. (2020). DOI: https://doi.org/10.1051/0004-6361/201936622

Micro-arcsecond structure of Sagittarius A∗ revealed by high-sensitivity 86 GHz VLBI observations. Astronomy and Astrophysics. (2019). DOI: https://doi.org/10.1051/0004-6361/201834148

The CARMA-NRO Orion Survey. Filamentary structure as seen in C18O emission. Astronomy and Astrophysics. (2019). DOI: https://doi.org/10.1051/0004-6361/201834049

Radio Occultation Observations of the Solar Corona Over 1.60-1.86 R☉: Faraday Rotation and Frequency Shift Analysis. Journal of Geophysical Research (Space Physics). (2019). DOI: https://doi.org/10.1029/2019JA026937

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