On radio emission of the Geminga pulsar and RBS 1223 at the frequency of 111 MHz
Alexander A. Ershov (Pushchino Radio Astronomy Observatory, ASC, LPI)

TL;DR
This study searched for pulsed radio emissions from the Geminga pulsar and RBS 1223 at 111 MHz but detected none, establishing upper limits on their flux densities.
Contribution
First to set upper limits on pulsed radio emissions from Geminga and RBS 1223 at 111 MHz.
Findings
No pulsed signals detected from either source.
Upper flux density limits established for both pulsars.
Abstract
I have searched for pulsed radio emission from the Geminga pulsar and for the nearby isolated neutron star 1RX J1308.6+2127 (RBS 1223) at the frequency of 111 MHz. No pulsed signals were detected from these sources. Upper limits for mean flux density are 0.4 - 4 mJy for the Geminga pulsar and 1.5 - 15 mJy for RBS 1223 depending on assumed duty cycle (.05 - .5) of the pulsars.
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsRadio Astronomy Observations and Technology · Pulsars and Gravitational Waves Research · Geophysics and Sensor Technology
