Search Publications

Magnetosphere-Ionosphere Drivers of Transient-Large-Amplitude Geomagnetic Disturbances: Statistical Analysis and Event Study
DOI: 10.1029/2023JA031587 Bibcode: 2023JGRA..12831587M

Nishimura, Yukitoshi; Moldwin, Mark B.; Weygand, James M. +2 more

We present a comprehensive statistical analysis of high-frequency transient-large-amplitude (TLA) magnetic perturbation events that occurred at 12 high-latitude ground magnetometer stations throughout Solar Cycle 24 from 2009 to 2019. TLA signatures are defined as one or more second-timescale dB/dt interval with magnitude ≥6 nT/s within an hour ev…

2023 Journal of Geophysical Research (Space Physics)
Cluster 3
Fabry-Pérot etalons in solar astronomy. A review
DOI: 10.1007/s10509-023-04212-3 Bibcode: 2023Ap&SS.368...55B

del Toro Iniesta, J. C.; Orozco Suárez, D.; Bailén, F. J.

During the last decades, the use of Fabry-Pérot etalons as filtergraphs has become frequent in solar instruments. The main reason is that they stand out for offering quasi-monochromatic, two-dimensional fields of view much higher than those provided by conventional slit-based spectrographs in a given time interval. Unfortunately, they also present…

2023 Astrophysics and Space Science
SolarOrbiter 3
Dissecting Earth's Magnetosphere: 3D Energy Transport in a Simulation of a Real Storm Event
DOI: 10.1029/2023JA031899 Bibcode: 2023JGRA..12831899B

Toth, G.; Pulkkinen, T. I.; Brenner, A. +1 more

We present new analysis methods of 3D MHD output data from the Space Weather Modeling Framework during a simulated storm event. Earth's magnetosphere is identified in the simulation domain and divided based on magnetic topology and the bounding magnetopause definition. Volume energy contents and surface energy fluxes are analyzed for each subregio…

2023 Journal of Geophysical Research (Space Physics)
Cluster 3
A reduction procedure and pipeline for the detection of trans-Neptunian objects using occultations
DOI: 10.1093/rasti/rzad040 Bibcode: 2023RASTI...2..567N

Ofek, Eran O.; Nir, Guy; Zackay, Barak

Kuiper belt objects smaller than a few kilometres are difficult to observe directly. They can be detected when they randomly occult a background star. Close to the ecliptic plane, each star is occulted once every tens of thousands of hours, and occultations typically last for less than a second. We present an algorithm, and companion pipeline, for…

2023 RAS Techniques and Instruments
Gaia 3
The galaxy counterpart and environment of the dusty damped Lyman-α absorber at z = 2.226 towards Q 1218+0832
DOI: 10.1051/0004-6361/202347403 Bibcode: 2023A&A...679A..30F

Östlin, G.; Milvang-Jensen, B.; Fynbo, J. P. U. +8 more

We report on further observations of the field of the quasar Q 1218+0832. Geier et al. (2019, A&A, 625, L9) presented the discovery of the quasar resulting from a search for quasars reddened and dimmed by dust in foreground damped Lyman-α absorbers (DLAs). The DLA is remarkable by having a very large H I column density close to 1022

2023 Astronomy and Astrophysics
eHST 3
Confirmation of Color-dependent Centroid Shift Measured After 1.8 Years with HST
DOI: 10.3847/1538-3881/acc85e Bibcode: 2023AJ....165..206B

Lu, Jessica R.; Cole, Andrew A.; Fukui, Akihiko +10 more

We measured the precise masses of the host and planet in the OGLE-2003-BLG-235 system, when the lens and source were resolving, with 2018 Keck high resolution images. This measurement is in agreement with the observation taken in 2005 with the Hubble Space Telescope (HST). In the 2005 data, the lens and sources were not resolved and the measuremen…

2023 The Astronomical Journal
eHST 3
Centre-to-limb variations in coronal hole and quiet sun regions obtained with IRIS spectroscopic observations
DOI: 10.1093/mnras/stad2761 Bibcode: 2023MNRAS.526..383K

Young, Peter R.; Kayshap, Pradeep

The centre-to-limb variations (CLV) of Gaussian fit parameters of the transition region Si IV 1402.77 Å spectral line in quiet Sun (QS) and coronal hole (CH) regions are presented. The results are derived from a full-disc mosaic scan obtained by the Interface Region Imaging Spectrograph on 2017 September 24. The CLV for a CH transition region line…

2023 Monthly Notices of the Royal Astronomical Society
IRIS SOHO 3
Search for Planets in Hot Jupiter Systems with Multi-Sector TESS Photometry. III. A Study of Ten Systems Enhanced with New Ground-Based Photometry
DOI: 10.32023/0001-5237/73.1.4 Bibcode: 2023AcA....73...57M

Amado, P. J.; Mugrauer, M.; Fernández, M. +12 more

The loneliness of hot Jupiters supports the high-eccentricity migration as a primary path leading to the formation of systems with those planets stripped of any close-in planetary companions. Here we present the null results of searches for low-mass planets close to hot Jupiters in 10 planetary systems: HAT-P-4, HAT-P-10, HAT-P-12, HAT-P-17, HAT-P…

2023 Acta Astronomica
Gaia 3
Accretion-modified Stars in Accretion Disks of Active Galactic Nuclei: The Low-luminosity Cases and an Application to Sgr A*
DOI: 10.3847/2041-8213/ad0bd9 Bibcode: 2023ApJ...958L..40W

Ho, Luis C.; Wang, Jian-Min; Li, Yan-Rong +3 more

In this paper, we investigate the astrophysical processes of stellar-mass black holes (sMBHs) embedded in advection-dominated accretion flows (ADAFs) of supermassive black holes (SMBHs) in low-luminosity active galactic nuclei. The sMBH is undergoing Bondi accretion at a rate lower than the SMBH. Outflows from the sMBH-ADAF dynamically interact wi…

2023 The Astrophysical Journal
INTEGRAL 3
The X-ray point source population hosted by globular clusters in the elliptical galaxy NGC 4261
DOI: 10.1093/mnras/stad1927 Bibcode: 2023MNRAS.524.3662N

Kundu, Arunav; Dage, Kristen C.; Zepf, Stephen E. +4 more

Utilizing archival Chandra X-ray Observatory data and Hubble Space Telescope globular cluster catalogues, we probe the time-domain properties of the low mass X-ray binary population in the elliptical galaxy NGC 4261. Of the 98 unique X-ray sources identified in this study, 62 sources are within the optical field of view and, of those, 33 per cent …

2023 Monthly Notices of the Royal Astronomical Society
eHST 3