Search Publications

BOWIE-ALIGN: A JWST comparative survey of aligned versus misaligned hot Jupiters to test the dependence of atmospheric composition on migration history
DOI: 10.1093/rasti/rzae043 Bibcode: 2024RASTI...3..691K

Owen, James E.; Kirk, James; López-Morales, Mercedes +20 more

A primary objective of exoplanet atmosphere characterization is to learn about planet formation and evolution, however, this is challenged by degeneracies. To determine whether differences in atmospheric composition can be reliably traced to differences in evolution, we are undertaking a transmission spectroscopy survey with JWST to compare the co…

2024 RAS Techniques and Instruments
Gaia JWST 5
PYSSED: an automated method of collating and fitting stellar spectral energy distributions
DOI: 10.1093/rasti/rzae005 Bibcode: 2024RASTI...3...89M

McDonald, Iain; Zijlstra, Albert A.; Cox, Nick L. J. +4 more

Stellar atmosphere modelling predicts the luminosity and temperature of a star, together with parameters such as the effective gravity and the metallicity, by reproducing the observed spectral energy distribution. Most observational data come from photometric surveys, using a variety of passbands. We herein present the Python Stellar Spectral Ener…

2024 RAS Techniques and Instruments
Gaia 4
Microchannel plate response to solar energetic particles and consequences for solar-wind measurements on ESA's Vigil mission
DOI: 10.1093/rasti/rzae053 Bibcode: 2024RASTI...3..844P

Owen, C. J.; Nicolaou, G.; Verscharen, D. +1 more

Space weather forecasting aims at predicting the impacts of the Sun, interplanetary space, and the planetary environment on biological and technological systems. To monitor space weather, the European Space Agency is developing the Vigil mission. Vigil will carry the Plasma Analyser (PLA) instrument. We investigate the expected impact of Solar Ene…

2024 RAS Techniques and Instruments
SolarOrbiter 0
On the nature of apparent transient sources on the National Geographic Society-Palomar Observatory Sky Survey glass copy plates
DOI: 10.1093/rasti/rzae004 Bibcode: 2024RASTI...3...73H

Hambly, N. C.; Blair, A.

We examine critically recent claims for the presence of above-atmosphere optical transients in publicly available digitized scans of Schmidt telescope photographic plate material derived from the National Geographic Society-Palomar Observatory Sky Survey. We employ the publicly available SuperCOSMOS Sky Survey catalogues to examine statistically t…

2024 RAS Techniques and Instruments
Gaia 0
Statistical properties of Hipparcos 2, caveats on its use, and a recalibration of the intermediate astrometric data
DOI: 10.1093/rasti/rzad011 Bibcode: 2023RASTI...2..218B

Brandt, Timothy D.; Brandt, G. Mirek; Michalik, Daniel

We revisit the Hipparcos 2007 re-reduction and find improvements to the catalogue by leveraging Gaia EDR3. We show that including a constant residual offset and additional dispersion (two free parameters in total) in the Hipparcos 2007 Intermediate Astrometric Data (IAD) creates a new catalogue with significantly better agreement with Gaia EDR3. T…

2023 RAS Techniques and Instruments
Gaia Hipparcos 4
Searching for quasi-periodic eruptions using machine learning
DOI: 10.1093/rasti/rzad015 Bibcode: 2023RASTI...2..238W

Young, A. J.; Webbe, Robbie

Quasi-periodic eruption (QPE) is a rare phenomenon in which the X-ray emission from the nuclei of galaxies shows a series of large amplitude flares. Only a handful of QPEs have been observed but the possibility remains that there are as yet undetected sources in archival data. Given the volume of data available a manual search is not feasible, and…

2023 RAS Techniques and Instruments
XMM-Newton 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
Overcoming separation between counterparts due to unknown proper motions in catalogue cross-matching
DOI: 10.1093/rasti/rzac009 Bibcode: 2023RASTI...2....1W

Wilson, Tom J.

To perform precise and accurate photometric catalogue cross-matches - assigning counterparts between two separate data sets - we need to describe all possible sources of uncertainty in object position. With ever-increasing time baselines between observations, like 2MASS in 2001 and the next generation of surveys, such as the Vera C. Rubin Observat…

2023 RAS Techniques and Instruments
Gaia 0
Extending time-series models for irregular observational gaps with a moving average structure for astronomical sequences
DOI: 10.1093/rasti/rzac011 Bibcode: 2023RASTI...2...33O

Elorrieta, F.; Eyheramendy, S.; Palma, W. +1 more

In this study, we introduce a novel moving-average model for analyzing stationary time-series observed irregularly in time. The process is strictly stationary and ergodic under normality and weakly stationary when normality is not assumed. Maximum likelihood (ML) estimation can be efficiently carried out through a Kalman algorithm obtained from th…

2023 RAS Techniques and Instruments
Hipparcos 0
An investigation into the effect of exposing XMM-Newton's Optical Monitor to the light of Jupiter
DOI: 10.1093/rasti/rzad048 Bibcode: 2023RASTI...2..673S

Sullivan, S; Page, M J; Breeveld, A A +2 more

After nearly 18 yr of successful and safe operations, on 2017 July 17 and 18, XMM-Newton's Optical Monitor (OM) observed Jupiter - an object 10 magnitudes brighter than safe brightness limits - in its visual (V) filter. The object was exposed 40 arcsec from the nominal European Photon Imaging Cameras pn boresight in the negative Y direction, creat…

2023 RAS Techniques and Instruments
XMM-Newton 0