Year: 2025
Type: article
Abstract: Context. The receiver N3AR operating at a frequency range between 67 and 116 GHz was commissioned at the APEX telescope in October 2024. It adds a new low-frequency band for APEX, with the capability of simultaneous dual-frequency observations using a dichroic beamsplitter. The 3 mm receiver also allows APEX to join the existing 3 mm global very long baseline interferometry (VLBI) network. Aims. One of our commissioning goals was to perform simultaneous dual-band VLBI observations at 86 and 258 GHz using receivers with shared optical paths (SOPs) to correct the atmospheric phase fluctuations using the frequency phase transfer (FPT) technique. This was possible together with the IRAM 30 m telescope, which has already developed such a capability. We aimed to verify the expected phase coherence and sensitivity improvement at the higher frequency achievable by applying FPT. Methods. With the dual-band, single baseline data, we applied the FPT method, which uses the lower-frequency data to correct the simultaneously observed higher-frequency data. We evaluated the improvement compared to the conventional single-band observing mode by analyzing the coherence factor in the higher-frequency data. Results. Our results show that the phase fluctuations at the two bands correlate well. After applying FPT, the interferometric phases at the higher frequency vary much less, and the coherence factor is significantly improved. Conclusions. Our analysis confirms the feasibility of applying FPT to frequencies above 250 GHz with SOP receivers. Future observations in this mode could dramatically improve the sensitivity and imaging fidelity of high-frequency VLBI.
Source: Astronomy and Astrophysics
Authors: G.-Y. Zhao, A. L. Roy, J. F. Wagner, E. Donoso, P. Torne, E. Ros, M. Lindqvist, A. P. Lobanov, V. Ramakrishnan, T. P. Krichbaum, H. Rottmann, J. A. Zensus, J. P. Pérez-Beaupuits, B. Klein, K. M. Menten, O. Ricken, N. Reyes, S. Sánchez, I. Ruiz, C. Durán, D. John, J. L. Santaren, M. Sánchez-Portal, M. Bremer, C. Kramer, K. F. Schuster, M. J. Rioja, R. Dodson
Institutions: Max Planck Institute for Radio Astronomy, University of Concepción, Instituto de Radioastronomía Milimétrica, Chalmers University of Technology, Aalto University, Institut de Radioastronomie Millimétrique, University of Turku, The University of Western Australia, Spanish National Observatory, International Centre for Radio Astronomy Research
Language: English
Subfield: Astronomy and Astrophysics
Field: Physics and Astronomy
Domain: Physical Sciences
Open Access status: gold
Estimated APC paid: $1,865
OpenAlex ID: W4413125117