Астрономические данные
Инфографика и код в репозитории на GitHub,
коллекции астрономических объектов
- Сверхновые, транзиенты и болиды: видео,
статистика и инфографика,
код
- Потенциально опасные астероиды: видео
- Солнечная система: видео,
статья,
код
- Статистика Солнечной системы: видео,
статистика, инфографика,
код
- Переменность звезд и планет: видео,
код
- Гамма-всплески: статистика и инфографика,
код
- Метеориты (инфографика), база данных метеоритов,
база данных импактных структур на Земле
Статистика космоса: обзоры
Статьи
Наблюдательная астрономия
Данные космонавтики
Ссылки
Код
Наблюдательная астрономия
Космонавтика
Солнечная система
Звезды
- List of smallest stars
- List of stars with proplyds
- A catalog of collected debris disks: properties, classifications and correlations between disks and stars/planets
- A compilation of optical polarization catalogs
- Двойные звезды: The Washington Visual Double Star Catalog,
CDS: B/wds, >156557 двойных
- Спектроскопические двойные
- Гиперскоростные звёзды:
Hyper-runaway and hypervelocity white dwarf candidates in Gaia Data Release 3: Possible remnants from Ia/Iax supernova explosions or dynamical encounters,
The fastest stars in the Galaxy.
- The Toruń catalogue of Galactic post-AGB and related objects (Version: 13 Mar 2010),
An evolutionary catalogue of galactic post-AGB and related objects (2007),
The second release of the Toruń catalogue of Galactic post-AGB objects: New classification scheme (2011),
Variability in Proto-planetary Nebulae. I. Light Curve Studies of 12 Carbon-rich Objects (2010),
Variability in Protoplanetary Nebulae. X. Multiyear Periods as an Indicator of Potential Binaries (2024),
New light on Galactic post-asymptotic giant branch stars - I. First distance catalogue (2015),
A census of post-AGB stars in Gaia DR3: evidence for a substantial population of Galactic post-RGB stars (2022)
- Catalogue of the central stars of planetary nebulae. Expanded edition (2020),
New catalog of distances to planetary nebulae based on Gaia parallaxes and statistical distances (2024)
- Звездные остатки
- White Dwarf Catalog (14294 total WD's),
A Catalog of Spectroscopically Identified White Dwarfs;
ReadMe
- Initial-final mass relation from white dwarfs within 40 pc;
The 40 pc sample of white dwarfs from Gaia.
Our DR3 sample contains 1076 spectroscopically confirmed white dwarfs, with just five candidates within the volume remaining unconfirmed (>99 per cent spectroscopic completeness). Our sample is likely to be incomplete until systematic spectroscopic, photometric and astrometric variability searches are performed for all ≈20000 main-sequence stars within 40 pc.
- Pulsar mass measurements and tests of general relativity
- The Australia Telescope National Facility Pulsar Catalogue,
ATNF Pulsar Catalogue (3473 sources, 2024-01-20)
- Catalog of the Galactic Population of X-Ray Pulsars in High-mass X-Ray Binary Systems (82 confirmed sources: 18 persistent and 64 transient pulsars)
- BlackCAT: A Catalog of Stellar-Mass Black Holes in X-ray Binaries,
2016A&A...587A..61C
- WATCHDOG: A Comprehensive All-sky Database of Galactic Black Hole X-ray Binaries
- Masses in the Stellar Graveyard:
LIGO-Virgo-KAGRA Discoveries Over Time.
Интерактивный график
- An Overview of Compact Star Populations and Some of Its Open Problems. we now count on more than 150 known Galactic neutron stars and black hole masses, as well as another 180 objects from binary mergers detected from gravitational-waves by the Ligo-Virgo-KAGRA Collaboration. We focus on Galactic black holes, and offer an updated catalog of 35 black hole masses and orbital parameters.
- A Systematic View of Ten New Black Hole Spins
- GWTC-3, a third catalog of gravitational wave detections,
Population of Merging Compact Binaries Inferred Using Gravitational Waves through GWTC-3
- List of supernova remnants;
A revised catalogue of 294 Galactic supernova remnants,
A Catalogue of Galactic Supernova Remnants (updated version)
- Сверхновые
- Гамма-всплески
Переменные звезды
- List of stars that have unusual dimming periods
- Новые
- Компактные двойные
- Catalogue of cataclysmic binaries, low-mass X-ray binaries and related objects (Seventh edition),
Cataclysmic Binaries (1429), LMXBs, and related objects (Ritter+, 2004) (7th Edition, Release 7.24, February 2017)
- A catalogue of cataclysmic variables from 20 yr of the Sloan Digital Sky Survey with new classifications, periods, trends, and oddities (2023): 507 CVs observed in SDSS I to IV including 70 new classifications collated from multiple archival data sets.
- A Volume-limited Sample of Cataclysmic Variables from Gaia DR2: Space Density and Population Properties (2020): 42 CVs within 150 pc, including two new systems discovered using the Gaia data, and is (77±10) per cent complete.
- WZ Sge-type dwarf novae (2015): nearly 100 WZ Sge-type dwarf novae
- A Catalog and Atlas of Cataclysmic Variables, R. Downes et al.
CV Catalog Statistics: 1600 CVs (2006)
- Low-Mass X-ray Binaries (2023)
- XRBcats: Galactic low-mass X-ray binary catalogue (349 LMXBs),
XRBcats: Galactic High Mass X-ray Binary Catalogue (169 HMXBs)
- A catalogue of low-mass X-ray binaries: 150 sources, 31 new low-mass X-ray binaries in addition to the 119 sources listed in van Paradijs' catalogue. (2001)
- An Optical Search for New Outbursting Low Mass X-Ray Binaries (2023). Using Monte Carlo simulations of the Galactic LMXB population, we estimate that 29% of outbursting LMXBs are detectable by ZTF and that 4.4% of LMXBs would be present in the crossmatched X-ray catalogs, giving an estimated Galactic population of 3390.
- Catalogue of high-mass X-ray binaries in the Galaxy (4th edition, 2006)
A catalogue of high-mass X-ray binaries in the Galaxy: from the INTEGRAL to the Gaia era.
Binary rEvolution: live version of catalogue.
We provide a catalogue of 161 HMXBs in the Galaxy with their best known coordinates, the spectral type of the companion star, systemic radial velocities, component masses, orbital period, eccentricity, and spin period when available.
- Accreting Binaries; Nature, formation, and evolution.
Galactic distribution, in Galactic coordinates, of accreting binaries, hosting low-mass (LMXB) and high-mass (HMXB) stars. All accreting binaries known to date are included, based on a catalog of 218 LMXB and 148 HMXB
- Каталоги переменных звезд
- A First Catalog of Variable Stars Measured by the Asteroid Terrestrial-impact Last Alert System (ATLAS) (2018). About 10% (427000 stars) pass extensive tests designed to screen out spurious variability detections: we label these as “probable” variables. Of these, 214 000 receive specific classifications as eclipsing binaries, pulsating, Mira-type, or sinusoidal variables: these are the “classified” variables. New discoveries among the probable variables number 315000, while 141000 of the classified variables are new, including about 10400 pulsating variables, 2060 Mira stars, and 74700 eclipsing binaries.
- The ASAS-SN catalogue of variable stars I: The Serendipitous Survey (2018),
ASAS-SN catalog of variable stars (Jayasinghe+, 2018-2020). In Paper I (Jayasinghe+ 2018MNRAS.477.3145J), we present a catalogue of 66179 bright, new variable stars discovered during our search for supernovae, including 27479 periodic variables and 38700 irregular variables. In paper II (Jayasinghe+ 2019MNRAS.486.1907J), We extracted the ASAS-SN light curves of ~412000 variable stars previously discovered by other surveys and in the VSX catalogue. In paper III (Jayasinghe+ 2019MNRAS.485..961J), we extracted the ASAS-SN light curves of ~1.3 million sources within 18deg of the Southern Ecliptic Pole.
- The value-added catalogue of ASAS-SN eclipsing binaries: parameters of 30 000 detached systems (2022),
The value-added catalogue of ASAS-SN eclipsing binaries - II. Properties of extra-physics systems (2023)
- Wide-field Infrared Survey Explorer (WISE) Catalog of Periodic Variable Stars (2018). Requiring more than 100 detections for a given object, 50 282 carefully and robustly selected periodic variables are discovered, of which 34 769 (69%) are new. Careful classification of the new variables results in a tally of 21 427 new EW-type eclipsing binaries, 5654 EA-type eclipsing binaries, 1312 Cepheids, and 1231 RR Lyrae. By comparison with known variables available in the literature, we estimate that the misclassification rate is 5% and 10% for short- and long-period variables, respectively.
- The Zwicky Transient Facility Catalog of Periodic Variable Stars (2020). We classify 781 602 periodic variables into 11 main types using an improved classification method. Comparison with previously published catalogs shows that 621 702 objects (79.5%) are newly discovered or newly classified, including ~700 Cepheids, ~5000 RR Lyrae stars, ~15000 δ Scuti variables, ~350 000 eclipsing binaries, ~100000 long-period variables, and about 150000 rotational variables.
- The Catalina Surveys Periodic Variable Star Catalog (2014). We present ~47,000 periodic variables found during the analysis of 5.4 million variable star candidates within a 20,000 deg2 region covered by the Catalina Surveys Data Release-1 (CSDR1). Combining these variables with type ab RR Lyrae from our previous work, we produce an online catalog containing periods, amplitudes, and classifications for ~61,000 periodic variables.
- The Catalina Surveys Southern periodic variable star catalogue (2017)
- Gaia Data Release 3. Specific processing and validation of all-sky RR Lyrae and Cepheid stars: The RR Lyrae sample (2023).
The DR3 RR Lyrae catalogue along with known RR Lyrae stars confirmed with the SOS pipeline, but for which the SOS periods differ from the literature periods (see Sect. 3.1), increases the census of RR Lyrae stars in our Galaxy and its close companions to about 370 000 within the limiting magnitude of Gaia.
- Gaia Data Release 3. Summary of the variability processing and analysis (2023). In total, 10.5 million objects are identified as variable in Gaia DR3 and have associated time series in G, GBP, and GRP and, in some cases, radial velocity time series. The DR3 variable sources subdivide into 9.5 million variable stars and 1 million active galactic nuclei or `quasars'. In addition, supervised classification identified 2.5 million galaxies thanks to spurious variability induced by the extent of these objects.
- Gaia Data Release 3. Cross-match of Gaia sources with variable objects from the literature. Our catalogue gathers 7 841 723 Gaia sources, 1.2 million of which are non-variable objects and 1.7 million are galaxies, in addition to 4.9 million variable sources. This represents over 100 variability (sub)types. In total, 152 different input catalogues from the literature were cross-matched with Gaia DR3 in order to find the counterpart sources. See table A.1. Input catalogues.
- Gaia collaboration; et al., 2022, Gaia Data Release 3 (Gaia DR3) Part 4 Variability. Variability analysis, together with the underlying epoch photometry, for 10.5 million sources. Apart from classification into 24 variability classes, detailed variability results are provided in separate tables for the following candidates (EAS presentation L. Eyer): Cepheids (15,021 objects); Compact companions (6306 objects); Eclipsing binaries (2,184,477 objects); Long-period variables (1,720,588 objects); Microlensing events (363 objects); Planetary transits (214 objects); RR Lyrae stars (271,779 objects); Short-timescale variables (471,679 objects); Solar-like rotational modulation variables (474,026 objects); Upper-main-sequence oscillators (54,476 objects); Active galactic nuclei (872,228 objects).
- 15 000 ellipsoidal binary candidates in TESS: Orbital periods, binary fraction, and tertiary companions (2023). We present a homogeneously selected sample of 15 779 candidate binary systems with main sequence primary stars and orbital periods shorter than 5 d. The targets were selected from TESS full-frame image light curves on the basis of their tidally induced ellipsoidal modulation. Spectroscopic follow-up suggests a sample purity of 83±13 per cent.
- Затменные двойные
- Переменные в данных космических обсерваторий: Kepler, TESS, CoRoT и т.д.
- Kepler Data Search & Retrieval
- Space-Based Photometry of Binary Stars: From Voyager to TESS (2021)
- Kepler Eclipsing Binary Catalog. Last update: Aug. 8, 2019.
The KEBC contains Kepler observations on 2907 unique identified eclipsing binary systems in 2920 entries.
Kepler Eclipsing Binary Stars. VII. The Catalog of Eclipsing Binaries Found in the Entire Kepler Data Set (2016). The total number of identified eclipsing and ellipsoidal binary systems in the Kepler field of view has increased to 2878, 1.3% of all observed Kepler targets.
Kepler Eclipsing Binary Stars. VIII. Identification of False Positive Eclipsing Binaries and Re-extraction of New Light Curves (2016)
- Automated eccentricity measurement from raw eclipsing binary light curves with intrinsic variability (2024),
Eclipsing binary parameters (IJspeert+, 2024)
- Discovery and characterisation of long-period eclipsing binary stars from Kepler K2 campaigns 1, 2, and 3 (2018)
- The Stars Kepler Missed: Investigating the Kepler Target Selection Function Using Gaia DR2 (2021),
VizieR Online Data Catalog: A list of ~330000 stars Kepler missed (Wolniewicz+, 2021). We started with a subset of 2.4 million targets within the KIC that are located in the Kepler field of view
- Kepler Bonus: Light Curves of Kepler Background Sources (2023)
- Exploring a "Flow" of Highly Eccentric Binaries with Kepler (2013).
Light curves for the three longest-period eclipsing binaries in our sample.
- Orbital Parameters of the Eclipsing Detached Kepler Binaries with Eccentric Orbits (2017). We present precise values of the eccentricity and periastron angle of 529 detached, eccentric, eclipsing stars from the Kepler Eclipsing Binary catalog
- TESS Eclipsing Binary Stars. I. Short-cadence Observations of 4584 Eclipsing Binaries in Sectors 1-26 (2022)
- Characteristics of Kepler Eclipsing Binaries Displaying a Significant O'Connell Effect (2022)
- Planets, candidates, and binaries from the CoRoT/Exoplanet programme. The CoRoT transit catalogue (2018). The CoRoT space mission observed 163 665 stars over 26 stellar fields in the faint star channel. The exoplanet teams detected a total of 4123 transit-like features in the 177 454 light curves. From the initial list of transit-like features, we identified and separated 824 false alarms of various kind, 2269 eclipsing binaries among which 616 are contact binaries and 1653 are detached ones, 37 planets and brown dwarfs, and 557 planet candidates.
Коричневые карлики
Экзопланеты
Галактики
Космология