---
DOAJ_listed: '1'
OA_place: publisher
OA_type: gold
PlanS_conform: '1'
_id: '21760'
abstract:
- lang: eng
text: 3I/ATLAS is the third interstellar object discovered to date, following 1I/‘Oumuamua
and 2I/Borisov. Its unusually high excess velocity and active cometary nature
make it a key probe of the Galactic population of icy planetesimals. Understanding
its origin requires its past trajectory through the Galaxy to be traced and the
possible role of stellar encounters to be assessed, both as a potential origin
and a perturber to its orbit. We integrated the orbit of 3I/ATLAS backward in
time for 10 Myr, together with a sample of Gaia DR3 stars with high-quality astrometry
and radial velocities, to identify close passages within 2 pc. We identify 93
nominal encounters, 62 of which are significant at the 2σ level. However, none
of these encounters produced any meaningful perturbation. The strongest perturber
Gaia DR3 6863591389529611264 at 0.30 pc and with a relative velocity of 35 km
s−1, imparted only a velocity change of ∣Δv∣ ≃ 5 × 10−4 km s−1 to the orbit
of 3I/ATLAS. Our results indicate that no stellar flybys within the past 10 Myr
and 500 pc contained in Gaia DR3 can account for the present trajectory of 3I/ATLAS
or be associated with its origin. We further show that 3I/ATLAS is kinematically
consistent with a thin-disk population, despite its large peculiar velocity.
acknowledgement: We thank the anonymous referee for a careful reading of the manuscript
and for constructive comments that improved the paper. X.P.C. and S.T. thank J.L.
Gragera-Más and Ylva Götberg for their valuable feedback and comments. X.P.C. acknowledges
financial support from the Spanish National Programme for the Promotion of Talent
and its Employability grant PRE2022-104959 cofunded by the European Social Fund.
S.T. acknowledges the funding from the European Union’s Horizon 2020 research and
innovation program under the Marie Skłodowska-Curie grant agreement No. 101034413.
E.V. acknowledges support from the DISCOBOLO project funded by the Spanish Ministerio
de Ciencia, Innovación y Universidades under grant PID2021-127289NB-I00. A.J.M.
acknowledges support from the Swedish National Space Agency (Career grant 2023-00146).
X.P.C. and M.M. acknowledge support from the Spanish Ministerio de Ciencia, Innovaciòn
y Universidades under grants PID2021122842OB-C22 and PID2024-157964OB-C22; from
the Xunta de Galicia and the European Union (FEDER Galicia 2021-2027 Program) Ref.
ED431B 2024/21, ED431B 2024/02, and CITIC ED431G 2023/01. This work has made use
of data from the European Space Agency (ESA) Gaia mission and processed by the Gaia
Data Processing and Analysis Consortium (DPAC). Funding for the DPAC has been provided
by national institutions, particularly the institutions participating in the Gaia
Multilateral Agreement.
article_number: '146'
article_processing_charge: Yes
article_type: original
arxiv: 1
author:
- first_name: X.
full_name: Pérez-Couto, X.
last_name: Pérez-Couto
- first_name: Santiago
full_name: Torres Rodriguez, Santiago
id: a8df4360-4328-11ee-8f1a-e502d0c83fc2
last_name: Torres Rodriguez
orcid: 0000-0002-3150-8988
- first_name: E.
full_name: Villaver, E.
last_name: Villaver
- first_name: A. J.
full_name: Mustill, A. J.
last_name: Mustill
- first_name: M.
full_name: Manteiga, M.
last_name: Manteiga
citation:
ama: 'Pérez-Couto X, Torres Rodriguez S, Villaver E, Mustill AJ, Manteiga M. 3I/ATLAS:
In search of the witnesses to its voyage. The Astrophysical Journal. 2026;1001(2).
doi:10.3847/1538-4357/ae56ff'
apa: 'Pérez-Couto, X., Torres Rodriguez, S., Villaver, E., Mustill, A. J., &
Manteiga, M. (2026). 3I/ATLAS: In search of the witnesses to its voyage. The
Astrophysical Journal. IOP Publishing. https://doi.org/10.3847/1538-4357/ae56ff'
chicago: 'Pérez-Couto, X., Santiago Torres Rodriguez, E. Villaver, A. J. Mustill,
and M. Manteiga. “3I/ATLAS: In Search of the Witnesses to Its Voyage.” The
Astrophysical Journal. IOP Publishing, 2026. https://doi.org/10.3847/1538-4357/ae56ff.'
ieee: 'X. Pérez-Couto, S. Torres Rodriguez, E. Villaver, A. J. Mustill, and M. Manteiga,
“3I/ATLAS: In search of the witnesses to its voyage,” The Astrophysical Journal,
vol. 1001, no. 2. IOP Publishing, 2026.'
ista: 'Pérez-Couto X, Torres Rodriguez S, Villaver E, Mustill AJ, Manteiga M. 2026.
3I/ATLAS: In search of the witnesses to its voyage. The Astrophysical Journal.
1001(2), 146.'
mla: 'Pérez-Couto, X., et al. “3I/ATLAS: In Search of the Witnesses to Its Voyage.”
The Astrophysical Journal, vol. 1001, no. 2, 146, IOP Publishing, 2026,
doi:10.3847/1538-4357/ae56ff.'
short: X. Pérez-Couto, S. Torres Rodriguez, E. Villaver, A.J. Mustill, M. Manteiga,
The Astrophysical Journal 1001 (2026).
date_created: 2026-04-26T22:01:46Z
date_published: 2026-04-20T00:00:00Z
date_updated: 2026-04-28T13:08:39Z
day: '20'
ddc:
- '520'
department:
- _id: LiBu
doi: 10.3847/1538-4357/ae56ff
ec_funded: 1
external_id:
arxiv:
- '2509.07678'
file:
- access_level: open_access
checksum: c3daf49261a9933c079854c38eec316f
content_type: application/pdf
creator: dernst
date_created: 2026-04-28T13:06:00Z
date_updated: 2026-04-28T13:06:00Z
file_id: '21773'
file_name: 2026_AstrophysicalJournal_PerezCouto.pdf
file_size: 2905627
relation: main_file
success: 1
file_date_updated: 2026-04-28T13:06:00Z
has_accepted_license: '1'
intvolume: ' 1001'
issue: '2'
language:
- iso: eng
month: '04'
oa: 1
oa_version: Published Version
project:
- _id: fc2ed2f7-9c52-11eb-aca3-c01059dda49c
call_identifier: H2020
grant_number: '101034413'
name: 'IST-BRIDGE: International postdoctoral program'
publication: The Astrophysical Journal
publication_identifier:
eissn:
- 1538-4357
issn:
- 0004-637X
publication_status: published
publisher: IOP Publishing
quality_controlled: '1'
scopus_import: '1'
status: public
title: '3I/ATLAS: In search of the witnesses to its voyage'
tmp:
image: /images/cc_by.png
legal_code_url: https://creativecommons.org/licenses/by/4.0/legalcode
name: Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)
short: CC BY (4.0)
type: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 1001
year: '2026'
...
---
DOAJ_listed: '1'
OA_place: publisher
OA_type: diamond
PlanS_conform: '1'
_id: '20930'
abstract:
- lang: eng
text: "Context. Beta Pictoris is an A-type star that hosts a complex planetary system
with two massive gas giants and a prominent debris disc. Variable absorption lines
in its stellar spectrum have been interpreted as signatures of exocomets – comet-like
bodies transiting the star. Stellar flybys can gravitationally perturb objects
in the outer comet reservoir, altering their orbits and potentially injecting
them into the inner system, thereby triggering exocomet showers.\r\nAims. We assessed
the contribution of stellar flybys to the observed exocomet activity by reconstructing
the stellar encounter history of β Pictoris in the past and future.\r\nMethods.
We used Gaia DR3 data, supplemented with radial velocities from complementary
spectroscopic surveys, to compile a catalogue of stars currently within 80 pc
of β Pictoris. Their orbits were integrated backwards and forwards in time in
an axisymmetric Galactic potential (via the GALA package) to identify encounters
within 2 pc of the system.\r\nResults. We identified 99 416 stars currently within
80 pc of β Pictoris with resolved kinematics. Among these, 49 stars (including
the eight components of five binaries) encounter β Pictoris within 2 pc between
–1.5 Myr and +2 Myr. For four of the binaries, the centre-of-mass trajectories
also pass within 2 pc. We estimated the sample to be more than 60% complete within
0.5 Myr of today.\r\nConclusions. Despite β Pictoris being the eponym of its famous
moving group, none of the identified encounters involved its moving group members;
all are unrelated field stars. We found no encounter capable of shaping the observed
disc structures, although stellar flybys may contribute to the long-term evolution
of an Oort Cloud-like structure. Our catalogue constitutes the most complete reconstruction
of the β Pictoris encounter history to date and provides a robust foundation for
future dynamical simulations."
acknowledgement: We thank the referee for their suggestions and comments, which helped
us improve the quality and clarity of the paper. JLGM and EV acknowledge the support
from the Spanish Ministry of Science and Innovation/State Agency of Research (MCIN/AEI)
under the grant PID2021-127289-NB-I00. ST acknowledges the funding from the European
Union’s Horizon 2020 research and innovation program under the Marie Skłodowska-Curie
grant agreement No. 101034413. AJM acknowledges support from the Swedish National
Space Agency (Career Grant 2023-00146) and from the Swedish Research Council (Project
Grant 2022-04043). JLGM also sincerely thanks AMP for his careful final reading
of this manuscript. This work has made use of data from the European Space Agency
(ESA) mission Gaia (https://www.cosmos.esa.int/gaia), processed by the Gaia Data
Processing and Analysis Consortium (DPAC). Funding for the DPAC has been provided
by national institutions, in particular the institutions participating in the Gaia
Multilateral Agreement. We acknowledge the use of the public data products from
RAVE (https://www.rave-survey.org), GALAH (https://galah-survey.org), APOGEE ((https://www.sdss.org)
and LAMOST (http://www.lamost.org) surveys. This research has also made use of the
SIMBAD database and the VizieR catalogue access tool, operated at CDS, Strasbourg,
France, as well as the NASA Astrophysics Data System Bibliographic Services and
the arXiv pre-print server operated by Cornell University. Computational analyses
in this work relied extensively on the NumPy and SciPy libraries for numerical computing,
matplotlib and seaborn for data visualization, and the Gala package for Galactic
dynamics. This work also made use of Astropy, a community-developed core PYTHON
package and an ecosystem of tools and resources for astronomy. We thank the developers
and maintainers of these open-source resources for their invaluable contributions
to the astronomical community.
article_number: A237
article_processing_charge: No
article_type: original
arxiv: 1
author:
- first_name: J. L.
full_name: Gragera-Más, J. L.
last_name: Gragera-Más
- first_name: Santiago
full_name: Torres Rodriguez, Santiago
id: a8df4360-4328-11ee-8f1a-e502d0c83fc2
last_name: Torres Rodriguez
orcid: 0000-0002-3150-8988
- first_name: A. J.
full_name: Mustill, A. J.
last_name: Mustill
- first_name: E.
full_name: Villaver, E.
last_name: Villaver
citation:
ama: Gragera-Más JL, Torres Rodriguez S, Mustill AJ, Villaver E. A kinematic history
of stellar encounters with Beta Pictoris. Astronomy & Astrophysics.
2025;704. doi:10.1051/0004-6361/202555940
apa: Gragera-Más, J. L., Torres Rodriguez, S., Mustill, A. J., & Villaver, E.
(2025). A kinematic history of stellar encounters with Beta Pictoris. Astronomy
& Astrophysics. EDP Sciences. https://doi.org/10.1051/0004-6361/202555940
chicago: Gragera-Más, J. L., Santiago Torres Rodriguez, A. J. Mustill, and E. Villaver.
“A Kinematic History of Stellar Encounters with Beta Pictoris.” Astronomy &
Astrophysics. EDP Sciences, 2025. https://doi.org/10.1051/0004-6361/202555940.
ieee: J. L. Gragera-Más, S. Torres Rodriguez, A. J. Mustill, and E. Villaver, “A
kinematic history of stellar encounters with Beta Pictoris,” Astronomy &
Astrophysics, vol. 704. EDP Sciences, 2025.
ista: Gragera-Más JL, Torres Rodriguez S, Mustill AJ, Villaver E. 2025. A kinematic
history of stellar encounters with Beta Pictoris. Astronomy & Astrophysics.
704, A237.
mla: Gragera-Más, J. L., et al. “A Kinematic History of Stellar Encounters with
Beta Pictoris.” Astronomy & Astrophysics, vol. 704, A237, EDP Sciences,
2025, doi:10.1051/0004-6361/202555940.
short: J.L. Gragera-Más, S. Torres Rodriguez, A.J. Mustill, E. Villaver, Astronomy
& Astrophysics 704 (2025).
date_created: 2026-01-04T23:01:34Z
date_published: 2025-12-01T00:00:00Z
date_updated: 2026-02-16T12:15:07Z
day: '01'
ddc:
- '520'
department:
- _id: LiBu
doi: 10.1051/0004-6361/202555940
ec_funded: 1
external_id:
arxiv:
- '2510.02509'
file:
- access_level: open_access
checksum: 2fb4d5a1603043aa7931a31f2c180877
content_type: application/pdf
creator: dernst
date_created: 2026-01-05T11:06:16Z
date_updated: 2026-01-05T11:06:16Z
file_id: '20942'
file_name: 2025_AstronomyAstrophysics_GrageraMas.pdf
file_size: 11021467
relation: main_file
success: 1
file_date_updated: 2026-01-05T11:06:16Z
has_accepted_license: '1'
intvolume: ' 704'
language:
- iso: eng
month: '12'
oa: 1
oa_version: Published Version
project:
- _id: fc2ed2f7-9c52-11eb-aca3-c01059dda49c
call_identifier: H2020
grant_number: '101034413'
name: 'IST-BRIDGE: International postdoctoral program'
publication: Astronomy & Astrophysics
publication_identifier:
eissn:
- 1432-0746
issn:
- 0004-6361
publication_status: published
publisher: EDP Sciences
quality_controlled: '1'
scopus_import: '1'
status: public
title: A kinematic history of stellar encounters with Beta Pictoris
tmp:
image: /images/cc_by.png
legal_code_url: https://creativecommons.org/licenses/by/4.0/legalcode
name: Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)
short: CC BY (4.0)
type: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 704
year: '2025'
...
---
DOAJ_listed: '1'
OA_place: publisher
OA_type: gold
PlanS_conform: '1'
_id: '18984'
abstract:
- lang: eng
text: Although planets have been found orbiting binary systems, whether they can
survive binary interactions is debated. While the tightest-orbit binaries should
host the most dynamically stable and long-lived circumbinary planetary systems,
they are also the systems that are expected to experience mass transfer, common
envelope evolution, or stellar mergers. In this study, we explore the effect of
stable non-conservative mass transfer on the dynamical evolution of circumbinary
planets. We present a new script that seamlessly integrates binary evolution data
from the 1D binary stellar evolution code MESA into the N-body simulation code
REBOUND. This integration framework enables a comprehensive examination of the
dynamical evolution of circumbinary planets orbiting mass-transferring binaries,
while simultaneously accounting for the detailed stellar structure evolution.
In addition, we introduce a recalibration method to mitigate numerical errors
from updates of binary properties during the system's dynamical evolution. We
construct a reference binary model in which a 2.21M⊙ star loses its hydrogen-rich
envelope through non-conservative mass transfer to the 1.76M⊙ companion star,
creating a 0.38M⊙ subdwarf. We find the tightest stable orbital separation for
circumbinary planets to be ≃2.5 times the binary separation after mass transfer.
Accounting for tides by using the interior stellar structure, we find that tidal
effects become apparent after the rapid mass transfer phase and start to fade
away during the latter stage of the slow mass transfer phase. Our research provides
a new framework for exploring circumbinary planet dynamics in interacting binary
systems.
acknowledgement: We thank the participants of the 2023 Kavli Summer Program in Astrophysics,
hosted by the Max Planck Institute for Astrophysics and funded by the Kavli Foundation.
In particular, Holly Preece, Selma de Mink, and Stephen Justham for their feedback
and comments on our work. ZX acknowledges support from the China Scholarship Council
(CSC). ST acknowledges the funding from the European Union’s Horizon 2020 research
and innovation programme under the Marie Skłodowska-Curie grant agreement No. 101034413.
AAT acknowledges support from the Horizon Europe research and innovation programmes
under the Marie Skłodowska-Curie grant agreement no. 101103134.
article_processing_charge: Yes
article_type: original
arxiv: 1
author:
- first_name: Zepei
full_name: Xing, Zepei
last_name: Xing
- first_name: Santiago
full_name: Torres Rodriguez, Santiago
id: a8df4360-4328-11ee-8f1a-e502d0c83fc2
last_name: Torres Rodriguez
orcid: 0000-0002-3150-8988
- first_name: Ylva Louise Linsdotter
full_name: Götberg, Ylva Louise Linsdotter
id: d0648d0c-0f64-11ee-a2e0-dd0faa2e4f7d
last_name: Götberg
orcid: 0000-0002-6960-6911
- first_name: Alessandro A.
full_name: Trani, Alessandro A.
last_name: Trani
- first_name: Valeriya
full_name: Korol, Valeriya
last_name: Korol
- first_name: Jorge
full_name: Cuadra, Jorge
last_name: Cuadra
citation:
ama: 'Xing Z, Torres Rodriguez S, Götberg YLL, Trani AA, Korol V, Cuadra J. Combining
REBOUND and MESA: Dynamical evolution of planets orbiting interacting binaries.
Monthly Notices of the Royal Astronomical Society. 2025;537(1):285-292.
doi:10.1093/mnras/stae2820'
apa: 'Xing, Z., Torres Rodriguez, S., Götberg, Y. L. L., Trani, A. A., Korol, V.,
& Cuadra, J. (2025). Combining REBOUND and MESA: Dynamical evolution of planets
orbiting interacting binaries. Monthly Notices of the Royal Astronomical Society.
Oxford University Press. https://doi.org/10.1093/mnras/stae2820'
chicago: 'Xing, Zepei, Santiago Torres Rodriguez, Ylva Louise Linsdotter Götberg,
Alessandro A. Trani, Valeriya Korol, and Jorge Cuadra. “Combining REBOUND and
MESA: Dynamical Evolution of Planets Orbiting Interacting Binaries.” Monthly
Notices of the Royal Astronomical Society. Oxford University Press, 2025.
https://doi.org/10.1093/mnras/stae2820.'
ieee: 'Z. Xing, S. Torres Rodriguez, Y. L. L. Götberg, A. A. Trani, V. Korol, and
J. Cuadra, “Combining REBOUND and MESA: Dynamical evolution of planets orbiting
interacting binaries,” Monthly Notices of the Royal Astronomical Society,
vol. 537, no. 1. Oxford University Press, pp. 285–292, 2025.'
ista: 'Xing Z, Torres Rodriguez S, Götberg YLL, Trani AA, Korol V, Cuadra J. 2025.
Combining REBOUND and MESA: Dynamical evolution of planets orbiting interacting
binaries. Monthly Notices of the Royal Astronomical Society. 537(1), 285–292.'
mla: 'Xing, Zepei, et al. “Combining REBOUND and MESA: Dynamical Evolution of Planets
Orbiting Interacting Binaries.” Monthly Notices of the Royal Astronomical Society,
vol. 537, no. 1, Oxford University Press, 2025, pp. 285–92, doi:10.1093/mnras/stae2820.'
short: Z. Xing, S. Torres Rodriguez, Y.L.L. Götberg, A.A. Trani, V. Korol, J. Cuadra,
Monthly Notices of the Royal Astronomical Society 537 (2025) 285–292.
date_created: 2025-02-02T23:01:53Z
date_published: 2025-02-01T00:00:00Z
date_updated: 2025-12-30T07:25:37Z
day: '01'
ddc:
- '520'
department:
- _id: YlGo
- _id: LiBu
doi: 10.1093/mnras/stae2820
ec_funded: 1
external_id:
arxiv:
- '2410.19695'
isi:
- '001400731500001'
file:
- access_level: open_access
checksum: 49fb4fe69f487d36169ccea60acbeccc
content_type: application/pdf
creator: dernst
date_created: 2025-12-30T07:24:34Z
date_updated: 2025-12-30T07:24:34Z
file_id: '20881'
file_name: 2025_MonthlyNoticesRAS_Xing.pdf
file_size: 2974244
relation: main_file
success: 1
file_date_updated: 2025-12-30T07:24:34Z
has_accepted_license: '1'
intvolume: ' 537'
isi: 1
issue: '1'
language:
- iso: eng
month: '02'
oa: 1
oa_version: Published Version
page: 285-292
project:
- _id: fc2ed2f7-9c52-11eb-aca3-c01059dda49c
call_identifier: H2020
grant_number: '101034413'
name: 'IST-BRIDGE: International postdoctoral program'
publication: Monthly Notices of the Royal Astronomical Society
publication_identifier:
eissn:
- 1365-2966
issn:
- 0035-8711
publication_status: published
publisher: Oxford University Press
quality_controlled: '1'
scopus_import: '1'
status: public
title: 'Combining REBOUND and MESA: Dynamical evolution of planets orbiting interacting
binaries'
tmp:
image: /images/cc_by.png
legal_code_url: https://creativecommons.org/licenses/by/4.0/legalcode
name: Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)
short: CC BY (4.0)
type: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 537
year: '2025'
...
---
DOAJ_listed: '1'
OA_place: publisher
OA_type: gold
_id: '18306'
abstract:
- lang: eng
text: Neutral sodium (Na i) is an alkali metal with a favorable absorption cross
section such that tenuous gases are easily illuminated at select transiting exoplanet
systems. We examine both the time-averaged and time-series alkali spectral flux
individually, over 4 nights at a hot Saturn system on a ∼2.8 day orbit about a
Sun-like star WASP-49 A. Very Large Telescope/ESPRESSO observations are analyzed,
providing new constraints. We recover the previously confirmed residual sodium
flux uniquely when averaged, whereas night-to-night Na i varies by more than an
order of magnitude. On HARPS/3.6 m Epoch II, we report a Doppler redshift at vΓ,NaD
= + 9.7 ± 1.6 km s−1 with respect to the planet's rest frame. Upon examining the
lightcurves, we confirm night-to-night variability, on the order of ∼1%–4% in
NaD, rarely coinciding with exoplanet transit, not readily explained by stellar
activity, starspots, tellurics, or the interstellar medium. Coincident with the
∼+10 km s−1 Doppler redshift, we detect a transient sodium absorption event dFNaD/F⋆
= 3.6% ± 1% at a relative difference of ΔFNaD(t) ∼ 4.4% ± 1%, lasting ΔtNaD ≳
40 minutes. Since exoplanetary alkali signatures are blueshifted due to the natural
vector of radiation pressure, estimated here at roughly ∼−5.7 km s−1, the radial
velocity is rather at +15.4 km s−1, far larger than any known exoplanet system.
Given that the redshift magnitude vΓ is in between the Roche limit and dynamically
stable satellite orbits, the transient sodium may be a putative indication of
a natural satellite orbiting WASP-49 A b.
acknowledgement: The research described in this Letter was carried out in part at
the Jet Propulsion Laboratory, California Institute of Technology, under a contract
with the National Aeronautics Space Administration, © 2024. California Institute
of Technology. Government sponsorship acknowledged. A.V.O. and J.V.S. thank M. Lendl
for constraints and discussions on the mass of WASP-49 A b. S.G.S acknowledges the
support from FCT through Investigador FCT contract nr. CEECIND/00826/2018 and POPH/FSE
(EC).
article_number: L53
article_processing_charge: Yes
article_type: original
arxiv: 1
author:
- first_name: Apurva V.
full_name: Oza, Apurva V.
last_name: Oza
- first_name: Julia V.
full_name: Seidel, Julia V.
last_name: Seidel
- first_name: H. Jens
full_name: Hoeijmakers, H. Jens
last_name: Hoeijmakers
- first_name: Athira
full_name: Unni, Athira
last_name: Unni
- first_name: Aurora Y.
full_name: Kesseli, Aurora Y.
last_name: Kesseli
- first_name: Carl A.
full_name: Schmidt, Carl A.
last_name: Schmidt
- first_name: Thirupathi
full_name: Sivarani, Thirupathi
last_name: Sivarani
- first_name: Aaron
full_name: Bello-Arufe, Aaron
last_name: Bello-Arufe
- first_name: Andrea
full_name: Gebek, Andrea
last_name: Gebek
- first_name: Moritz
full_name: Meyer Zu Westram, Moritz
last_name: Meyer Zu Westram
- first_name: Sérgio G.
full_name: Sousa, Sérgio G.
last_name: Sousa
- first_name: Rosaly M.C.
full_name: Lopes, Rosaly M.C.
last_name: Lopes
- first_name: Renyu
full_name: Hu, Renyu
last_name: Hu
- first_name: Katherine
full_name: De Kleer, Katherine
last_name: De Kleer
- first_name: Chloe
full_name: Fisher, Chloe
last_name: Fisher
- first_name: Sébastien
full_name: Charnoz, Sébastien
last_name: Charnoz
- first_name: Ashley D.
full_name: Baker, Ashley D.
last_name: Baker
- first_name: Samuel P.
full_name: Halverson, Samuel P.
last_name: Halverson
- first_name: Nick M.
full_name: Schneider, Nick M.
last_name: Schneider
- first_name: Angelica
full_name: Psaridi, Angelica
last_name: Psaridi
- first_name: Aurélien
full_name: Wyttenbach, Aurélien
last_name: Wyttenbach
- first_name: Santiago
full_name: Torres Rodriguez, Santiago
id: a8df4360-4328-11ee-8f1a-e502d0c83fc2
last_name: Torres Rodriguez
orcid: 0000-0002-3150-8988
- first_name: Ishita
full_name: Bhatnagar, Ishita
last_name: Bhatnagar
- first_name: Robert E.
full_name: Johnson, Robert E.
last_name: Johnson
citation:
ama: Oza AV, Seidel JV, Hoeijmakers HJ, et al. Redshifted sodium transient near
exoplanet transit. Astrophysical Journal Letters. 2024;973(2). doi:10.3847/2041-8213/ad6b29
apa: Oza, A. V., Seidel, J. V., Hoeijmakers, H. J., Unni, A., Kesseli, A. Y., Schmidt,
C. A., … Johnson, R. E. (2024). Redshifted sodium transient near exoplanet transit.
Astrophysical Journal Letters. IOP Publishing. https://doi.org/10.3847/2041-8213/ad6b29
chicago: Oza, Apurva V., Julia V. Seidel, H. Jens Hoeijmakers, Athira Unni, Aurora
Y. Kesseli, Carl A. Schmidt, Thirupathi Sivarani, et al. “Redshifted Sodium Transient
near Exoplanet Transit.” Astrophysical Journal Letters. IOP Publishing,
2024. https://doi.org/10.3847/2041-8213/ad6b29.
ieee: A. V. Oza et al., “Redshifted sodium transient near exoplanet transit,”
Astrophysical Journal Letters, vol. 973, no. 2. IOP Publishing, 2024.
ista: Oza AV, Seidel JV, Hoeijmakers HJ, Unni A, Kesseli AY, Schmidt CA, Sivarani
T, Bello-Arufe A, Gebek A, Meyer Zu Westram M, Sousa SG, Lopes RMC, Hu R, De Kleer
K, Fisher C, Charnoz S, Baker AD, Halverson SP, Schneider NM, Psaridi A, Wyttenbach
A, Torres Rodriguez S, Bhatnagar I, Johnson RE. 2024. Redshifted sodium transient
near exoplanet transit. Astrophysical Journal Letters. 973(2), L53.
mla: Oza, Apurva V., et al. “Redshifted Sodium Transient near Exoplanet Transit.”
Astrophysical Journal Letters, vol. 973, no. 2, L53, IOP Publishing, 2024,
doi:10.3847/2041-8213/ad6b29.
short: A.V. Oza, J.V. Seidel, H.J. Hoeijmakers, A. Unni, A.Y. Kesseli, C.A. Schmidt,
T. Sivarani, A. Bello-Arufe, A. Gebek, M. Meyer Zu Westram, S.G. Sousa, R.M.C.
Lopes, R. Hu, K. De Kleer, C. Fisher, S. Charnoz, A.D. Baker, S.P. Halverson,
N.M. Schneider, A. Psaridi, A. Wyttenbach, S. Torres Rodriguez, I. Bhatnagar,
R.E. Johnson, Astrophysical Journal Letters 973 (2024).
date_created: 2024-10-13T22:01:49Z
date_published: 2024-10-01T00:00:00Z
date_updated: 2025-09-08T14:18:18Z
day: '01'
ddc:
- '520'
department:
- _id: LiBu
doi: 10.3847/2041-8213/ad6b29
external_id:
arxiv:
- '2409.19844'
isi:
- '001322169500001'
file:
- access_level: open_access
checksum: 23eea2a6a0519694a84998957ad7b7fb
content_type: application/pdf
creator: dernst
date_created: 2024-10-21T11:05:11Z
date_updated: 2024-10-21T11:05:11Z
file_id: '18456'
file_name: 2024_AstrophysicalJourn_Oza.pdf
file_size: 1249747
relation: main_file
success: 1
file_date_updated: 2024-10-21T11:05:11Z
has_accepted_license: '1'
intvolume: ' 973'
isi: 1
issue: '2'
language:
- iso: eng
month: '10'
oa: 1
oa_version: Published Version
publication: Astrophysical Journal Letters
publication_identifier:
eissn:
- 2041-8213
issn:
- 2041-8205
publication_status: published
publisher: IOP Publishing
quality_controlled: '1'
scopus_import: '1'
status: public
title: Redshifted sodium transient near exoplanet transit
tmp:
image: /images/cc_by.png
legal_code_url: https://creativecommons.org/licenses/by/4.0/legalcode
name: Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)
short: CC BY (4.0)
type: journal_article
user_id: 317138e5-6ab7-11ef-aa6d-ffef3953e345
volume: 973
year: '2024'
...