-
crossref
Anonymous
2020-03-16T19:34:32Z
置信度 0.70
-
crossref
Ron Cowen
2014-04-30T17:24:38Z
置信度 0.70
-
crossref
2019-11-01T09:02:01Z
置信度 0.70
-
The atmospheres of close-in, low-mass exoplanets are extremely vulnerable to the effects of stellar UV to X-ray radiation. Photoevaporation can significantly ablate planetary atmospheres or even strip them entirely, potentially rendering a planet inhabitable. …
crossref
Laura Harbach, James Owen, Subhanjoy Mohanty
2020-10-08T11:51:28Z
置信度 0.70
-
TOI-6894 b, the largest exoplanet relative to its host star yet seen, doesn’t fit the most widely accepted formation model for giant worlds.
crossref
Damond Benningfield
2025-07-01T07:00:21Z
置信度 0.70
-
ExoClock Unlocked, an initiative of the ExoClock project team, aims to democratize the field of exoplanet research by enabling public participation in support of ESA’s Ariel space mission. The project has been running for two years and participants g…
crossref
Georgia Pantelidou, Anastasia Kokori
2024-07-03T11:09:04Z
置信度 0.70
-
We can hope that, in a near future, external occulter systems, called Starshade will allow the detection of exo-Earth type exoplanets, but as unresolved points.  The telescopes used will be of a few meters.To get real multi-pixels images of  …
crossref
Claude Aime, Céline Theys, Simon Prunet
2024-07-03T12:38:20Z
置信度 0.70
-
crossref
Natalie Hinkel
2025-08-25T23:12:17Z
置信度 0.70
-
<p>The field of exoplanets is one of the most rapidly growing, with more than 5000 planets discovered to date. Follow-up observations of Exoplanets is one of the few fields of astronomy that small telescopes can still contribute to ongoing resear…
crossref
Angelos Tsiaras
2022-09-23T12:06:09Z
置信度 0.70
-
crossref
Charles Day
2026-02-24T16:00:58Z
置信度 0.70
-
Transmission spectroscopy has been integral to the atmospheric characterisation of transiting exoplanets – constraining their chemical abundances and temperature profiles. However, transit spectra are often interpreted using 1D models of the atmosphe…
crossref
Joost Wardenier, Vivien Parmentier
2021-07-21T14:54:19Z
置信度 0.70
-
crossref
2011-06-29T21:47:46Z
置信度 0.70
-
crossref
2019-11-01T09:02:01Z
置信度 0.70
-
crossref
2020-05-09T01:08:46Z
置信度 0.70
-
crossref
2019-11-01T09:02:01Z
置信度 0.70
-
crossref
2017-01-31T11:26:00Z
置信度 0.70
-
Laser-driven experiments on silica help scientists learn more about planetary formation and evolution.
crossref
JoAnna Wendel
2015-03-03T19:37:27Z
置信度 0.70
-
crossref
2019-05-11T17:02:34Z
置信度 0.70
-
The exoplanet’s host star blasts it with so much radiation that it will someday evaporate.
crossref
JoAnna Wendel
2017-06-06T07:00:08Z
置信度 0.70
-
crossref
2017-01-31T11:52:57Z
置信度 0.70
-
crossref
2019-05-11T17:02:34Z
置信度 0.70
-
crossref
Gregory D. Allen
2021-05-10T17:10:59Z
置信度 0.70
-
<p>I this talk I will present the process to get observations on a Europlanet network telescope for an exoplanet transit.  The steps of obtaining and also analysing the exoplanet transit light curve will be described. These data are …
crossref
Florence Libotte, Mercè Correa
2022-09-23T12:06:09Z
置信度 0.70
-
crossref
2017-01-31T11:25:24Z
置信度 0.70
-
crossref
Rachel Berkowitz
2022-10-06T17:10:58Z
置信度 0.70
-
crossref
2019-05-11T17:02:34Z
置信度 0.70
-
crossref
Aparna Bhattacharya
2025-04-28T17:48:32Z
置信度 0.70
-
crossref
2015-09-18T14:14:22Z
置信度 0.70
-
crossref
2017-01-31T11:51:09Z
置信度 0.70
-
crossref
2019-02-23T16:27:53Z
置信度 0.70
-
Exoplanetary science is now pushing to constrain the atmospheric compositions of exoplanets. This quest will be further aided by the next generation of facilities, such as the JWST and ground-based ELTs. Linking the observed composition of exoplanet atmosphere…
crossref
Christian Eistrup
2020-10-08T09:23:31Z
置信度 0.70
-
crossref
Roberta Kwok
2009-01-31T15:10:09Z
置信度 0.70
-
Taurus Hill Observatory (THO) [1], observatory code A95, is an amateur observatory located in Varkaus, Finland. The observatory is maintained by the local astronomical association Warkauden Kassiopeia. THO research team has observed and measured various stella…
crossref
Harri Haukka, Veli-Pekka Hentunen, Markku Nissinen, Tuomo Salmi 等
2021-07-21T10:46:47Z
置信度 0.70
-
NASA's low-cost space telescope opened up a universe of possibilities for scientists who scour space in search of planets—and possibly life.
crossref
Jack Lissauer
2015-09-16T02:58:23Z
置信度 0.70
-
crossref
2019-02-23T16:27:53Z
置信度 0.70
-
Détection des exoplanètes autour de naines M par spectroscopie proche infra-rouge et visible L'exoplanètologie commence à s’intéresser aux naines M afin de détecter et caractériser des planètes. Ces étoiles sont les plus communes; leur petite taille facilite l…
crossref
Mélissa J. Hobson
2026-04-03T20:50:03Z
置信度 0.70
-
The newly discovered planet balances precariously in orbit within the star system, puzzling scientists.
crossref
JoAnna Wendel
2016-07-08T03:00:17Z
置信度 0.70
-
crossref
Eric Hand
2012-11-16T21:32:51Z
置信度 0.70
-
crossref
2017-01-31T11:22:33Z
置信度 0.70
-
crossref
Jessie Christiansen
2018-05-24T06:01:07Z
置信度 0.70
-
crossref
2018-03-04T15:16:02Z
置信度 0.70
-
crossref
Daniel Huber
2025-08-26T10:33:19Z
置信度 0.70
-
The planet is also shaped like a football (the American kind).
crossref
Kimberly Cartier
2019-08-06T07:00:18Z
置信度 0.70
-
crossref
M. Mugrauer, R. Neuhäuser
2008-12-04T15:15:53Z
置信度 0.70
-
As next generation observation facilities become available for the characterisation of Exoplanet atmospheres, the capacity to move beyond the assumption of molecules existing in local thermodynamic equilibrium becomes more pressing. While atmospheric retrieval…
crossref
Sam Wright, Sergey Yurchenko
2021-07-21T08:42:53Z
置信度 0.70
-
crossref
Tyler D. Robinson
2025-12-31T03:11:40Z
置信度 0.70
-
crossref
2018-03-04T15:16:02Z
置信度 0.70
-
Abstract Both direct and indirect methods of exoplanet detection rely upon detailed knowledge of the potential host stars. Such stellar characterization allows for accurate extraction of planetary properties, as well as contributing to our overall understandin…
crossref
Emilie R. Simpson, Tara Fetherolf, Stephen R. Kane, Joshua Pepper 等
2023-07-20T16:59:47Z
置信度 0.70
-
crossref
Therese Encrenaz
2011-06-29T21:19:58Z
置信度 0.70
-
Abstract In this study, we treat Earth as an exoplanet and investigate our home planet by means of a potential future mid-infrared space mission called the Large Interferometer For Exoplanets (LIFE). We combine thermal spectra from an empirical data set of dis…
crossref
Jean-Noël Mettler, Björn S. Konrad, Sascha P. Quanz, Ravit Helled
2024-02-26T10:30:06Z
置信度 0.70
-
crossref
Ryan Cloutier
2024-06-29T17:59:52Z
置信度 0.70
-
crossref
Hannu Parviainen
2024-11-07T08:47:15Z
置信度 0.70
-
crossref
2019-02-23T16:27:53Z
置信度 0.70
-
Der præsenteres en nyhed fra exoplanetforskningen: opdagelsen af planeten Gliese 581 g, der muligvis befinder sig i sin stjernes beboelige zone. Planeten kredser om en rød dværgstjerne blot 20 lysår fra Jorden og har en masse omkring tre gange Jordens. Artikle…
crossref
John Rosendal Nielsen
2026-06-18T00:05:30Z
置信度 0.70
-
Clouds form and dissipate on a gas giant orbiting a Sun-like star.
crossref
Nola Redd
2020-03-12T07:00:22Z
置信度 0.70
-
crossref
Tyler D. Robinson
2018-01-09T15:29:01Z
置信度 0.70
-
europepmc
2026
置信度 0.80
-
Abstract Spectral retrieval is a key computational tool for interpreting spectroscopic observations of exoplanets. As data quality has dramatically improved with the launch of JWST, so the complexity of retrieval models has also increased. Due to the lack of g…
europepmc
Joanna K. Barstow, Luis Welbanks
2026
置信度 0.80
-
europepmc
2026
置信度 0.80
-
europepmc
2026
置信度 0.80
-
europepmc
2026
置信度 0.80
-
crossref
E. Korpela, D. Werthimer, D. Anderson, J. Cobb 等
2002-08-24T18:17:23Z
置信度 0.70
-
crossref
Iván Almár
2009-10-14T15:00:36Z
置信度 0.70
-
We propose a novel instrument design to greatly expand the current optical and near-infrared SETI search parameter space by monitoring the entire observable sky during all observable time. This instrument is aimed to search for technosignatures by means of det…
arxiv
Jérôme Maire, Shelley A. Wright, Maren Cosens, Franklin Antonio 等
2018-08-17T06:49:44Z
置信度 0.78
astro-ph.IM
-
SETI@home, a search for signals from extraterrestrial intelligence, has been recording data at the Arecibo radio telescope since 1999. These data are sent via the Internet to the personal computers of volunteers who have donated their computers' idle time towa…
arxiv
Eric J. Korpela, Jeff Cobb, Matt Lebofsky, Andrew Siemion 等
2011-09-07T22:32:09Z
置信度 0.78
astro-ph.IM
-
Optical SETI (Search for Extraterrestrial Intelligence) instruments that can explore the very fast time domain, especially with large sky coverage, offer an opportunity for new discoveries that can complement multimessenger and time domain astrophysics. The Pa…
arxiv
Jérôme Maire, Shelley A. Wright, Jamie Holder, David Anderson 等
2022-10-04T03:50:46Z
置信度 0.78
astro-ph.IM
-
If the signals that are being sought in SETI programs do exist but are very brief, for example because they are produced intermittently to conserve energy, then it is essential to know when these signals will arrive at the Earth. Different types of synchroniza…
arxiv
Robin H. D. Corbet
2002-08-06T15:39:27Z
置信度 0.78
astro-ph
-
A Search for Extraterrestrial Life (SETI), based on the possibility of interstellar communication via laser signals, is being designed to extend the search into the near-infrared spectral region (Wright et al, this conference). The dedicated near-infrared (900…
arxiv
Jérôme Maire, Shelley A. Wright, Dan Werthimer, Richard R. Treffers 等
2014-07-09T20:00:32Z
置信度 0.78
astro-ph.IM
-
As a major approach to looking for life beyond the Earth, the search for extraterrestrial intelligence (SETI) is committed to detecting technosignatures such as engineered radio signals that are indicative of technologically capable life. In this paper, we rep…
arxiv
Zhen-Zhao Tao, Hai-Chen Zhao, Tong-Jie Zhang, Vishal Gajjar 等
2022-08-04T03:13:29Z
置信度 0.78
astro-ph.EPastro-ph.IM
-
Narrowband radio search for extraterrestrial intelligence (SETI) in the 21st century suffers severely from radio frequency interference (RFI), resulting in a high number of false positives, and it could be the major reason why we have not yet received any mess…
arxiv
Bo-Lun Huang, Zhen-Zhao Tao, Tong-Jie Zhang
2023-07-21T05:42:30Z
置信度 0.78
astro-ph.IMastro-ph.EP
-
We consider interstellar scintillations as a cause of intermittency in radio signals from extraterrestrial intelligence (ETI). We demonstrate that scintillations are very likely to allow initial detections of narrowband signals from distant sources (> 100 p…
arxiv
James M. Cordes, T. Joseph W. Lazio, Carl Sagan
1997-07-02T23:13:32Z
置信度 0.78
astro-ph
-
The transmission rate of communication between radio telescopes on Earth and extraterrestrial intelligence (ETI) is here calculated up to distances of 1000 light years. Both phase-shift-keying (PSK) and frequency-shift keying (FSK) modulation schemes are consi…
arxiv
P. A. Fridman
2011-02-15T16:36:51Z
置信度 0.78
astro-ph.IM
-
Many hypotheses have been raised to explain the famous Fermi paradox. One of them is that self-replicating probes could have explored the whole Galaxy, including our Solar System, and that they are still to be detected. In this scenario, it is proposed here th…
arxiv
M. Gillon
2013-09-29T12:30:55Z
置信度 0.78
physics.pop-phastro-ph.EPastro-ph.IM
-
The search for extraterrestrial intelligence (SETI) commensal surveys aim to scan the sky to detect technosignatures from extraterrestrial life. A major challenge in SETI is the effective mitigation of radio frequency interference (RFI), a critical step that i…
arxiv
Li-Li Zhao, Xiao-Hang Luan, Xin Chao, Yu-Chen Wang 等
2025-12-17T09:32:45Z
置信度 0.78
astro-ph.IM
-
Spatiotemporal techniques for signal coordination with actively transmitting extraterrestrial civilizations, without the need for prior communication, can constrain technosignature searches to a significantly smaller coordinate space. With the variable star ca…
arxiv
Andy Nilipour, James R. A. Davenport, Steve Croft, Andrew P. V. Siemion
2023-07-31T18:37:20Z
置信度 0.78
astro-ph.IM
-
С момента окончания формирования такого научного направления как связь с внеземными цивилизациями, обобщённого как СЕТИ, SETI прошло достаточно лет, чтобы внести в существующую научную парадигму заметные изменения. Отказ от радиотехнических средств связи (приё…
crossref
О.Б. Хаврошкин, В.В. Цыплаков
2024-09-03T10:56:30Z
置信度 0.70
-
crossref
Claudio Maccone
2021-02-26T10:10:14Z
置信度 0.70
-
crossref
Jill C. Tarter
2003-11-19T21:02:25Z
置信度 0.70
-
crossref
Lukman O. Olasunkanmi, Oladoyin G. Famutimi, Idris O. Raimi, Olumide O. Omoboye 等
2025-12-08T04:58:49Z
置信度 0.70
-
crossref
Claudio Maccone
2021-02-26T10:10:14Z
置信度 0.70
-
crossref
Claudio Maccone
2021-02-26T10:10:14Z
置信度 0.70
-
crossref
Peter J. Brand
2021-10-24T22:02:51Z
置信度 0.70
-
crossref
Claudio Maccone
2021-02-26T10:10:14Z
置信度 0.70
-
Abstract The standard search-for-extraterrestrial-intelligence (SETI) observational protocol, examining individual stars or groups of stars for ten minutes each, has failed. It is argued that persistently and directly transmitting signals with high power to Ea…
crossref
John Gertz
2025-06-09T15:42:58Z
置信度 0.70
-
crossref
Peter J. Brand
2021-10-24T22:02:51Z
置信度 0.70
-
crossref
Stephen Baxter
2011-02-14T09:55:06Z
置信度 0.70
-
crossref
Claudio Maccone
2021-02-26T10:10:14Z
置信度 0.70
-
crossref
Claudio Maccone
2021-02-26T10:10:14Z
置信度 0.70
-
crossref
Claudio Maccone
2021-02-26T10:10:14Z
置信度 0.70
-
crossref
Claudio Maccone
2021-02-26T10:10:14Z
置信度 0.70
-
europepmc
2026
置信度 0.80
-
crossref
Claudio Maccone
2021-02-26T10:10:14Z
置信度 0.70
-
crossref
Louisa Mason
2025-01-31T21:08:46Z
置信度 0.70
-
crossref
Claudio Maccone
2021-02-26T10:10:14Z
置信度 0.70
-
crossref
Richard Factor
2011-02-14T09:55:06Z
置信度 0.70
-
crossref
M. Mitchell Waldrop
2011-07-27T09:26:02Z
置信度 0.70
-
crossref
Alvin D. Harvey, Danielle Wood
2026-01-16T14:18:27Z
置信度 0.70
-
crossref
Claudio Maccone
2021-02-26T10:10:14Z
置信度 0.70
-
crossref
Kenneth Houston
2025-01-31T21:08:46Z
置信度 0.70
-
crossref
William H. Edmondson
2010-03-08T02:38:57Z
置信度 0.70