Search Publications

Cool white dwarfs as standards for infrared observations
DOI: 10.1093/mnras/stz2984 Bibcode: 2020MNRAS.491.3613G

Bohlin, Ralph C.; Gentile Fusillo, Nicola Pietro; Kalirai, Jason S. +2 more

In the era of modern digital sky surveys, uncertainties in the flux of stellar standards are commonly the dominant systematic error in photometric calibration and can often affect the results of higher level experiments. The Hubble Space Telescope (HST) spectrophotometry, which is based on computed model atmospheres for three hot (Teff

2020 Monthly Notices of the Royal Astronomical Society
Gaia eHST 21
Entropy-driven winds: Outflows and fountains lifted gently by buoyancy
DOI: 10.1093/mnras/staa380 Bibcode: 2020MNRAS.493.2149K

Kruijssen, J. M. Diederik; Keller, Benjamin W.; Wadsley, James W.

We present a new theoretical framework for using entropy to understand how outflows driven by supernovae are launched from disc galaxies: via continuous, buoyant acceleration through the circumgalactic medium (CGM). When young star clusters detonate supernovae in the interstellar medium (ISM) of a galaxy, they generate hot, diffuse bubbles that pu…

2020 Monthly Notices of the Royal Astronomical Society
eHST 21
GeV γ-Ray Emission from M33 and Arp 299
DOI: 10.3847/1538-4357/aba043 Bibcode: 2020ApJ...901..158X

Liu, Ruo-Yu; Zhang, Hai-Ming; Wang, Xiang-Yu +1 more

Star-forming galaxies are huge reservoirs of cosmic rays (CRs) and these CRs convert a significant fraction of their energy into γ-rays by colliding with the interstellar medium (ISM). Several nearby star-forming galaxies have been detected in GeV-TeV γ-rays. It is also found that the γ-ray luminosities in 0.1-100 GeV correlate well with indicator…

2020 The Astrophysical Journal
Herschel 21
MAXIMASK and MAXITRACK: Two new tools for identifying contaminants in astronomical images using convolutional neural networks
DOI: 10.1051/0004-6361/201936345 Bibcode: 2020A&A...634A..48P

Bertin, E.; Bouy, H.; Paillassa, M.

In this work, we propose two convolutional neural network classifiers for detecting contaminants in astronomical images. Once trained, our classifiers are able to identify various contaminants, such as cosmic rays, hot and bad pixels, persistence effects, satellite or plane trails, residual fringe patterns, nebulous features, saturated pixels, dif…

2020 Astronomy and Astrophysics
Herschel 21
The evolution of neutral hydrogen over the past 11 Gyr via H I 21 cm absorption
DOI: 10.1093/mnras/staa2521 Bibcode: 2020MNRAS.498..883G

Bolatto, Alberto D.; Leroy, Adam K.; Grasha, Kathryn +1 more

We present the results of a blind search for intervening H I 21 cm absorption towards 260 radio sources in the redshift range 0 < z < 2.74 with the Green Bank Telescope. The survey has the sensitivity to detect sub-damped Ly α (DLA) systems for H I spin temperatures Ts/f = 100 K, and despite the successful re-detection of 10 known…

2020 Monthly Notices of the Royal Astronomical Society
eHST 21
Two Wolf-Rayet stars at the heart of colliding-wind binary Apep
DOI: 10.1093/mnras/staa1244 Bibcode: 2020MNRAS.495.3323C

Callingham, J. R.; Crowther, P. A.; Marcote, B. +4 more

Infrared imaging of the colliding-wind binary Apep has revealed a spectacular dust plume with complicated internal dynamics that challenges standard colliding-wind binary physics. Such challenges can be potentially resolved if a rapidly rotating Wolf-Rayet star is located at the heart of the system, implicating Apep as a Galactic progenitor system…

2020 Monthly Notices of the Royal Astronomical Society
Gaia 21
Modelling solar irradiance from ground-based photometric observations
DOI: 10.1051/swsc/2020047 Bibcode: 2020JSWSC..10...45C

Chatzistergos, Theodosios; Ermolli, Ilaria; Giorgi, Fabrizio +2 more

Total solar irradiance (TSI) has been monitored from space since 1978, i.e. for about four solar cycles. The measurements show a prominent variability in phase with the solar cycle, as well as fluctuations on timescales shorter than a few days. However, the measurements were done by multiple and usually relatively short-lived missions. The differe…

2020 Journal of Space Weather and Space Climate
SOHO 21
Angular Expansion of Nova Shells
DOI: 10.3847/1538-4357/ab76c5 Bibcode: 2020ApJ...892...60S

Guerrero, M. A.; Toalá, J. A.; Santamaría, E. +4 more

Nova shells can provide important information on their distance, their interactions with circumstellar and interstellar media, and the evolution in morphology of the ejecta. We have obtained narrowband images of a sample of five nova shells, namely DQ Her, FH Ser, T Aur, V476 Cyg, and V533 Her, with ages ranging from 50 to 130 yr. These images hav…

2020 The Astrophysical Journal
Gaia eHST 21
The First Extensive Spectroscopic Study of Young Stars in the North America and Pelican Nebulae
DOI: 10.3847/1538-4357/abba84 Bibcode: 2020ApJ...904..146F

Fang, Min; Herczeg, Gregory J.; Wang, Hongchi +5 more

We present a spectroscopic survey of over 3400 potential members in the North America and Pelican Nebulae (NAP) using several low-resolution (R ≈ 1300-2000) spectrographs: Palomar/Norris, WIYN/Hydra, Keck/DEep Imaging Multi-Object Spectrograph (DEIMOS), and the Multiple Mirror Telescope (MMT)/Hectospec. We identify 580 young stars as likely member…

2020 The Astrophysical Journal
Gaia 21
A New Likely Redback Millisecond Pulsar Binary with a Massive Neutron Star: 4FGL J2333.1-5527
DOI: 10.3847/1538-4357/ab77ba Bibcode: 2020ApJ...892...21S

Strader, Jay; Dage, Kristen C.; Chomiuk, Laura +7 more

We present the discovery of a likely new redback millisecond pulsar (MSP) binary associated with the Fermi γ-ray source 4FGL J2333.1-5527. Using optical photometric and spectroscopic observations from the Southern Astrophysical Research telescope, we identify a low-mass, main-sequence-like companion in a 6.9 hr, highly inclined orbit around a susp…

2020 The Astrophysical Journal
XMM-Newton 21