VVV DR1: The first data release of the Milky Way bulge and southern plane from the near-infrared ESO public survey VISTA variables in the Vía Láctea
Context. The ESO public survey VISTA variables in the Vía Láctea (VVV) started in 2010.
VVV targets 562 sq. deg in the Galactic bulge and an adjacent plane region and is expected …
VVV targets 562 sq. deg in the Galactic bulge and an adjacent plane region and is expected …
The Spitzer Survey of Stellar Structure in Galaxies ()
ABSTRACT The Spitzer Survey of Stellar Structure in Galaxies () is an Exploration Science
Legacy Program approved for the Spitzer post–cryogenic mission. It is a volume-, magnitude …
Legacy Program approved for the Spitzer post–cryogenic mission. It is a volume-, magnitude …
Quantifying Variability of Young Stellar Objects in the Mid-infrared Over 6 Years with the Near-Earth Object Wide-field Infrared Survey Explorer
W Park, JE Lee, CC Peña, D Johnstone… - The Astrophysical …, 2021 - iopscience.iop.org
Variability in young stellar objects (YSOs) can be caused by various time-dependent
phenomena associated with star formation, including accretion rates, geometric changes in …
phenomena associated with star formation, including accretion rates, geometric changes in …
The WFCAM science archive
NC Hambly, RS Collins, NJG Cross… - Monthly Notices of …, 2008 - academic.oup.com
We describe the WFCAM Science Archive, which is the primary point of access for users of
data from the wide-field infrared camera WFCAM on the United Kingdom Infrared Telescope …
data from the wide-field infrared camera WFCAM on the United Kingdom Infrared Telescope …
All-sky Co-moving Recovery Of Nearby Young Members (ACRONYM). II. The β Pictoris Moving Group∗
We confirm 66 low-mass stellar and brown dwarf systems (K7–M9) plus 19 visual or
spectroscopic companions of the β Pictoris moving group (BPMG). Of these, 41 are new …
spectroscopic companions of the β Pictoris moving group (BPMG). Of these, 41 are new …
A STELLAR CENSUS OF THE TUCANA–HOROLOGIUM MOVING GROUP
We report the selection and spectroscopic confirmation of 129 new late-type (SpT= K3–M6)
members of the Tucana–Horologium moving group, a nearby (d∼ 40 pc), young (τ∼ 40 …
members of the Tucana–Horologium moving group, a nearby (d∼ 40 pc), young (τ∼ 40 …
Meeting the cool neighbors. X. Ultracool dwarfs from the 2MASS all-sky data release
IN Reid, KL Cruz, JD Kirkpatrick, PR Allen… - The Astronomical …, 2008 - iopscience.iop.org
Using data from the 2 Micron All Sky Survey All-Sky Point Source Catalogue, we have
extended our census of nearby ultracool dwarfs to cover the full celestial sphere above …
extended our census of nearby ultracool dwarfs to cover the full celestial sphere above …
The Gaia alerted fading of the FUor-type star Gaia21elv
Z Nagy, S Park, P Ábrahám, Á Kóspál… - Monthly Notices of …, 2023 - academic.oup.com
ABSTRACT FU Orionis objects (FUors) are eruptive young stars, which exhibit outbursts that
last from decades to a century. Due to the duration of their outbursts, and to the fact that only …
last from decades to a century. Due to the duration of their outbursts, and to the fact that only …
[图书][B] Handbook of infrared astronomy
IS Glass - 1999 - books.google.com
Infrared astronomy is a dynamic area of current research. It has been revolutionized in the
past few years by the advent of large, sensitive, infrared arrays, and the success of several …
past few years by the advent of large, sensitive, infrared arrays, and the success of several …
The Asiago Database on Photometric Systems (ADPS)-II. Band and reddening parameters
M Fiorucci, U Munari - Astronomy & Astrophysics, 2003 - aanda.org
The Asiago Database on Photometric Systems (ADPS) is a compilation of basic information
and reference data on 201 photometric systems (both ground-based and space-born) …
and reference data on 201 photometric systems (both ground-based and space-born) …