📄 Astronomical surveys and big data

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Mickaelian, Areg M. et al. (2016) · Baltic Astronomy
Reads: 145 · Citations: 9
DOI: 10.48550/arXiv.1511.07322

🔗 https://ui.adsabs.harvard.edu/abs/2016BaltA..25...75M/abstract

#Astronomy #Astrophysics #Galaxies #RadioAstronomy #AstronomicalDatabasesMiscellaneous

Astronomical surveys and big data

Recent all-sky and large-area astronomical surveys and their catalogued data over the whole range of electromagnetic spectrum, from γ -rays to radio waves, are reviewed, including such as Fermi-GLAST and INTEGRAL in γ -ray, ROSAT, XMM and Chandra in X-ray, GALEX in UV, SDSS and several POSS I and POSS II-based catalogues (APM, MAPS, USNO, GSC) in the optical range, 2MASS in NIR, WISE and AKARI IRC in MIR, IRAS and AKARI FIS in FIR, NVSS and FIRST in radio range, and many others, as well as the most important surveys giving optical images (DSS I and II, SDSS, etc.), proper motions (Tycho, USNO, Gaia), variability (GCVS, NSVS, ASAS, Catalina, Pan-STARRS), and spectroscopic data (FBS, SBS, Case, HQS, HES, SDSS, CALIFA, GAMA). An overall understanding of the coverage along the whole wavelength range and comparisons between various surveys are given: galaxy redshift surveys, QSO/AGN, radio, Galactic structure, and Dark Energy surveys. Astronomy has entered the Big Data era, with Astrophysical Virtual Observatories and Computational Astrophysics playing an important role in using and analyzing big data for new discoveries.

ADS

📄 A KInetic Database for Astrochemistry (KIDA)

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Wakelam, V. et al. (2012) · The Astrophysical Journal Supplement Series
Reads: 460 · Citations: 484
DOI: 10.1088/0067-0049/199/1/21

🔗 https://ui.adsabs.harvard.edu/abs/2012ApJS..199...21W/abstract

#Astronomy #Astrophysics #PlanetaryScience #Astrochemistry #AstronomicalDatabasesMiscellaneous

A KInetic Database for Astrochemistry (KIDA)

We present a novel chemical database for gas-phase astrochemistry. Named the KInetic Database for Astrochemistry (KIDA), this database consists of gas-phase reactions with rate coefficients and uncertainties that will be vetted to the greatest extent possible. Submissions of measured and calculated rate coefficients are welcome, and will be studied by experts before inclusion into the database. Besides providing kinetic information for the interstellar medium, KIDA is planned to contain such data for planetary atmospheres and for circumstellar envelopes. Each year, a subset of the reactions in the database (kida.uva) will be provided as a network for the simulation of the chemistry of dense interstellar clouds with temperatures between 10 K and 300 K. We also provide a code, named Nahoon, to study the time-dependent gas-phase chemistry of zero-dimensional and one-dimensional interstellar sources.

ADS