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We present the first results from our Red Optical Planet Survey (ROPS) to search for low mass planets orbiting late type dwarfs (M5.5V - M9V) in their habitable zones (HZ). Our observations, with the red arm of the MIKE spectrograph (0.5 -…

Earth and Planetary Astrophysics · Physics 2015-06-04 J. R. Barnes , J. S. Jenkins , H. R. A. Jones , P. Rojo , P. Arriagada , A. Jordan , D. Minniti , M. Tuomi , S. V. Jeffers , D. Pinfield

We presented a comprehensive multi-epoch timing and multiwavelength analysis of the accreting millisecond X-ray pulsar MAXI J1957+032, covering two major outbursts in 2022 and 2025. By reanalyzing the 2022 outburst data from the Neutron…

A new meteor shower $\lambda$-Sculptorids produced by the comet 46P/Wirtanen was forecast for December 12, 2023. The predicted activity was highly uncertain, but generally considered to be low. Observations in Australia, New Zealand, and…

Earth and Planetary Astrophysics · Physics 2024-02-13 D. Vida , J. M. Scott , A. Egal , J. Vaubaillon , Q. -Z. Ye , D. Rollinson , M. Sato , D. E. Moser

We report on the broadband spectral and timing properties of the accreting millisecond X-ray pulsar IGR J17498$-$2921 during its April 2023 outburst using data from NICER (1$-$10 keV), NuSTAR (3$-$79 keV), Insight-HXMT (2$-$150 keV), and…

High Energy Astrophysical Phenomena · Physics 2024-11-06 Zhaosheng Li , L. Kuiper , Y. Y. Pan , M. Falanga , J. Poutanen , Y. P. Chen , R. X. Xu , M. Y. Ge , Y. Huang , L. M. Song , S. Zhang , F. J. Lu , S. N. Zhang

The accreting millisecond X-ray pulsar IGR J17498-2921 went into X-ray outburst on April 13-15, 2023, for the first time since its discovery on August 11, 2011. Here, we report on the first follow-up \nustar{} observation of the source,…

High Energy Astrophysical Phenomena · Physics 2024-09-12 Mahasweta Bhattacharya , Aditya S. Mondal , Mayukh Pahari , Biplab Raychaudhuri , Rohit Ghosh , Gulab C. Dewangan

Comet C/2020 V2 (ZTF) is categorized as a dynamically new long-period comet, making its first approach to the inner Solar system. We have observed this comet for around 32 months (from January 2022 to July 2024) at heliocentric distances…

Earth and Planetary Astrophysics · Physics 2025-10-01 Goldy Ahuja , K. Aravind , Shashikiran Ganesh , Said Hmiddouch , Mathieu Vander Donckt , Emmanuel Jehin , Devendra Sahu , T. Sivarani

In the last decades Near-Earth Objects (NEOs) have become very important targets to study, since they can give us clues to the formation, evolution and composition of the Solar System. In addition, they may represent either a threat to…

Earth and Planetary Astrophysics · Physics 2014-09-24 S. Ieva , E. Dotto , D. Perna , M. A. Barucci , F. Bernardi , S. Fornasier , F. De Luise , E. Perozzi , A. Rossi , J. R. Brucato

Context. Characterizing mission-accessible asteroids using telescopic observations is fundamental for target-selection and planning for spacecraft missions. Near-Earth asteroids on Earth-like orbits are of particular importance for…

Earth and Planetary Astrophysics · Physics 2024-10-10 Jin Beniyama , Alexey V. Sergeyev , David J. Tholen , Marco Micheli

We present an update to the first white-light detections of a dust trail observed closely following the orbit of asteroid (3200) Phaethon, as seen by the Wide-field Imager for Parker Solar Probe (WISPR) instrument on the NASA Parker Solar…

We present a detailed analysis of three XMM-Newton observations of the black hole low-mass X-ray binary IGR~J17091-3624 taken during its 2016 outburst. Radio observations obtained with the Australia Telescope Compact Array (ATCA) indicate…

High Energy Astrophysical Phenomena · Physics 2020-01-08 E. Gatuzz , M. Díaz Trigo , J. C. A. Miller-Jones , S. Migliari

A fast radio burst (FRB) was recently detected to be associated with a hard X-ray burst from the Galactic magnetar SGR 1935+2154. Scenarios involving magnetars for FRBs are hence highly favored. In this work, we suggest that the impact…

High Energy Astrophysical Phenomena · Physics 2020-08-12 Jin-Jun Geng , Bing Li , Long-Biao Li , Shao-Lin Xiong , Rolf Kuiper , Yong-Feng Huang

We present a physical model and spin-state analysis of the potentially hazardous asteroid (23187) 2000 PN9. As part of a long-term campaign to make direct detections of the YORP effect, we collected optical lightcurves of the asteroid…

We present near-infrared narrow- and broad-band imaging of the field of GRB021004, performed with ISAAC on the UT1 of the ESO Very Large Telescope. The narrow-band filters were chosen to match prominent emission lines at the redshift of the…

Astrophysics · Physics 2009-11-10 P. M. Vreeswijk , P. Moller , J. P. U. Fynbo

On August 17, 2017 at 12:41:04 UTC the Advanced LIGO and Advanced Virgo gravitational-wave detectors made their first observation of a binary neutron star inspiral. The signal, GW170817, was detected with a combined signal-to-noise ratio of…

General Relativity and Quantum Cosmology · Physics 2017-10-17 The LIGO Scientific Collaboration , The Virgo Collaboration

We report the broadband timing and spectral properties of the neutron star low-mass X-ray binary Aql X-1 during the 2024 outburst with NICER, NuSTAR, and Swift observatories. We detected six thermonuclear X-ray bursts during the NICER and…

High Energy Astrophysical Phenomena · Physics 2025-04-25 Manoj Mandal , Sabyasachi Pal , G. K. Jaisawal , Anne Lohfink , Sachindra Naik , Jaiverdhan Chauhan

The Aguas Zarcas (Costa Rica) CM2 carbonaceous chondrite fell during night time in April 2019. Security and dashboard camera video of the meteor were analyzed to provide a trajectory, lightcurve, and orbit of the meteoroid. The trajectory…

We present the prospects for the early (pre-merger) detection and localization of compact-binary coalescences using gravitational waves over the next 10 years. Early warning can enable the direct observation of the prompt and early…

High Energy Astrophysical Phenomena · Physics 2020-10-20 Alexander H. Nitz , Marlin Schäfer , Tito Dal Canton

We present the discovery of AT 2024wpp ("Whippet"), a fast and luminous 18cow-like transient. At a redshift of z=0.0868, revealed by Keck Cosmic Web Imager spectroscopy of its faint star-forming host, it is the fourth-nearest example of its…

The Rapid Burster (MXB 1730-335) is a unique object, showing both type I and type II X-ray bursts. A type I burst of the Rapid Burster was observed with Swift/XRT on 2009 March 5, showing photospheric radius expansion for the first time in…

High Energy Astrophysical Phenomena · Physics 2015-06-04 Gloria Sala , Frank Haberl , Jordi Jose , Anuj Parikh , Richard Longland , Luis Carlos Pardo , Morten Andersen

We report on optical and NIR observations obtained during and after the 2004 December discovery outburst of the X-ray transient and accretion-powered millisecond pulsar IGR J00291+5934. Our observations monitored the evolution of the…