Search Publications

Angular clustering properties of the DESI QSO target selection using DR9 Legacy Imaging Surveys
DOI: 10.1093/mnras/stab3252 Bibcode: 2022MNRAS.509.3904C

Myers, Adam D.; Palanque-Delabrouille, Nathalie; Yèche, Christophe +12 more

The quasar target selection for the upcoming survey of the Dark Energy Spectroscopic Instrument (DESI) will be fixed for the next 5 yr. The aim of this work is to validate the quasar selection by studying the impact of imaging systematics as well as stellar and galactic contaminants, and to develop a procedure to mitigate them. Density fluctuation…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 25
Direct First Parker Solar Probe Observation of the Interaction of Two Successive Interplanetary Coronal Mass Ejections in 2020 November
DOI: 10.3847/1538-4357/ac590b Bibcode: 2022ApJ...930...88N

Reeves, Katharine K.; Hess, Phillip; Nieves-Chinchilla, Teresa +20 more

We investigate the effects of the evolutionary processes in the internal magnetic structure of two interplanetary coronal mass ejections (ICMEs) detected in situ between 2020 November 29 and December 1 by the Parker Solar Probe (PSP). The sources of the ICMEs were observed remotely at the Sun in EUV and subsequently tracked to their coronal counte…

2022 The Astrophysical Journal
SOHO 25
Photometric Observations of the Binary Near-Earth Asteroid (65803) Didymos in 2015-2021 Prior to DART Impact
DOI: 10.3847/PSJ/ac7be1 Bibcode: 2022PSJ.....3..175P

Carry, B.; Souami, D.; Dotto, E. +24 more

We performed photometric observations of the binary near-Earth asteroid (65803) Didymos in support of the Double Asteroid Redirection Test (DART) mission that will test the Kinetic Impactor technology for diverting dangerous asteroids. It will hit the Didymos secondary, called Dimorphos, on 2022 September 26. We observed Didymos with 11 telescopes…

2022 The Planetary Science Journal
Gaia 25
Can tides explain the low dark matter density in Fornax?
DOI: 10.1093/mnras/stab3526 Bibcode: 2022MNRAS.510.2186G

Fattahi, Azadeh; Read, Justin I.; Frenk, Carlos S. +1 more

The low dark matter density in the Fornax dwarf galaxy is often interpreted as being due to the presence of a constant density 'core', but it could also be explained by the effects of Galactic tides. The latter interpretation has been disfavoured because it is apparently inconsistent with the orbital parameters and star formation history of Fornax…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 25
Near-infrared transmission spectrum of TRAPPIST-1 h using Hubble WFC3 G141 observations
DOI: 10.1051/0004-6361/202142140 Bibcode: 2022A&A...658A.133G

Marcq, E.; Charnay, B.; Mori, M. +4 more

Context. The TRAPPIST-1 planetary system is favourable for transmission spectroscopy and offers the unique opportunity to study rocky planets with possibly non-primary envelopes. We present here the transmission spectrum of the seventh planet of the TRAPPIST-1 system, TRAPPIST-1 h (RP = 0.752 R, Teq = 173 K) using…

2022 Astronomy and Astrophysics
eHST 25
Magnetograph Saturation and the Open Flux Problem
DOI: 10.3847/1538-4357/ac4491 Bibcode: 2022ApJ...926..113W

Ulrich, R. K.; Wang, Y. -M.; Harvey, J. W.

Extrapolations of line-of-sight photospheric field measurements predict radial interplanetary magnetic field (IMF) strengths that are factors of ~2-4 too low. To address this open flux problem, we reanalyze the magnetograph measurements from different observatories, with particular focus on those made in the saturation-prone Fe I 525.0 nm line by …

2022 The Astrophysical Journal
SOHO 25
Systematic KMTNet Planetary Anomaly Search. VI. Complete Sample of 2018 Sub-prime-field Planets
DOI: 10.3847/1538-3881/ac9c5c Bibcode: 2022AJ....164..262J

Han, Cheongho; Udalski, Andrzej; Lee, Chung-Uk +31 more

We complete the analysis of all 2018 sub-prime-field microlensing planets identified by the KMTNet AnomalyFinder. Among the 9 previously unpublished events with clear planetary solutions, 6 are clearly planetary (OGLE-2018-BLG-0298, KMT-2018-BLG-0087, KMT-2018-BLG-0247, KMT-2018-BLG-0030, OGLE-2018-BLG-1119, and KMT-2018-BLG-2602), while the remai…

2022 The Astronomical Journal
Gaia 25
A Carbon/Oxygen-dominated Atmosphere Days after Explosion for the "Super-Chandrasekhar" Type Ia SN 2020esm
DOI: 10.3847/1538-4357/ac4780 Bibcode: 2022ApJ...927...78D

Kilpatrick, Charles D.; Izzo, Luca; Coulter, David A. +18 more

Seeing pristine material from the donor star in a type Ia supernova (SN Ia) explosion can reveal the nature of the binary system. In this paper, we present photometric and spectroscopic observations of SN 2020esm, one of the best-studied SNe of the class of "super-Chandrasekhar" SNe Ia (SC SNe Ia), with data obtained -12 to +360 days relative to p…

2022 The Astrophysical Journal
eHST 25
The 3D Kinematics of the Orion Nebula Cluster: NIRSPEC-AO Radial Velocities of the Core Population
DOI: 10.3847/1538-4357/ac3252 Bibcode: 2022ApJ...926..141T

Lu, Jessica R.; Kim, Dongwon; Hsu, Chih-Chun +5 more

The kinematics and dynamics of stellar and substellar populations within young, still-forming clusters provide valuable information for constraining theories of formation mechanisms. Using Keck II NIRSPEC+AO data, we have measured radial velocities for 56 low-mass sources within 4' of the core of the Orion Nebula Cluster (ONC). We also remeasure r…

2022 The Astrophysical Journal
Gaia eHST 25
The Stellar Mass Function in CANDELS and Frontier Fields: The Buildup of Low-mass Passive Galaxies since z 3
DOI: 10.3847/1538-4357/ac9a48 Bibcode: 2022ApJ...940..135S

Santini, Paola; Calabrò, Antonello; Castellano, Marco +8 more

Despite significant efforts in recent years, the physical processes responsible for the formation of passive galaxies through cosmic time remain unclear. The shape and evolution of the stellar mass function (SMF) give an insight into these mechanisms. Taking advantage of the CANDELS and the deep Hubble Frontier Fields (HFF) programs, we estimated …

2022 The Astrophysical Journal
eHST 25