MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY

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MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY Journal

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Beyond the merger-quasar-quench paradigm I: mergers are neither necessary nor sufficient to quench central galaxies inspaceillustrisTNG. 548. 2026
Environmental versus intrinsic quenching at cosmic noon: predictions from cosmological hydrodynamical simulations for VLT-MOONRISE. 543:2006-2034. 2025
Different regulation of stellar metallicities between star-forming and quiescent galaxies - insights into galaxy quenching. 534:30-38. 2024
EPOCHS Paper V. The dependence of galaxy formation on galaxy structure at z < 7 from JWST observations. 531:4857-4875. 2024
The role of environment and AGN feedback in quenching local galaxies: comparing cosmological hydrodynamical simulations to the SDSS. 528:4891-4921. 2024
The ALMaQUEST Survey XI: a strong but non-linear relationship between star formation and dynamical equilibrium pressure. 527:10201-10220. 2024
Different higher order kinematics between star-forming and quiescent galaxies based on the SAMI, MAGPI, and LEGA-C surveys. 525:2765-2788. 2023
Evolution in the orbital structure of quiescent galaxies from MAGPI, LEGA-C, and SAMI surveys: direct evidence for merger-driven growth over the last 7 Gyr. 525:2789-2805. 2023
The metallicity's fundamental dependence on both local and global galactic quantities. 519:1149-1170. 2023
The molecular gas main sequence and Schmidt-Kennicutt relation are fundamental, the star-forming main sequence is a (useful) byproduct. 518:4767-4781. 2023
The ALMaQUEST Survey X: what powers merger induced star formation?. 516:1462-1480. 2022
Host galaxy magnitude of OJ 287 from its colours at minimum light. 514:3017-3023. 2022
Rapid X-ray variability in Mkn 421 during a multiwavelength campaign. 513:1662-1679. 2022
On the quenching of star formation in observed and simulated central galaxies: evidence for the role of integrated AGN feedback. 512:1052-1090. 2022
The ALMaQUEST survey IX: the nature of the resolved star forming main sequence. 510:3622-3628. 2022
Nebular-phase spectra of Type Ia supernovae from the Las Cumbres Observatory Global Supernova Project. 511:3682-3707. 2022
What drives galaxy quenching? A deep connection between galaxy kinematics and quenching in the local Universe. 511:1913-1941. 2022
OzDES reverberation mapping program: Lag recovery reliability for 6-yr C iv analysis. 509:4008-4023. 2022
Galaxy morphological classification catalogue of the Dark Energy Survey Year 3 data with convolutional neural networks. 507:4425-4444. 2021
Towards robust determination of non-parametric morphologies in marginal astronomical data: resolving uncertainties with cosmological hydrodynamical simulations. 507:886-903. 2021
Understanding the extreme luminosity of DES14X2fna. 505:3950-3967. 2021
Spatially resolved star formation and fuelling in galaxy interactions. 503:3113-3133. 2021
Time delay lens modelling challenge. 503:1096-1123. 2021
A machine learning approach to galaxy properties: joint redshift-stellar mass probability distributions with Random Forest. 502:2770-2786. 2021
The ALMaQUEST Survey - V. The non-universality of kpc-scale star formation relations and the factors that drive them. 501:4777-4797. 2021
The ALMaQUEST survey - VI. The molecular gas main sequence of 'retired' regions in galaxies. 502:L6-L10. 2021
The effect of environment on Type Ia supernovae in the Dark Energy Survey three-year cosmological sample. 501:4861-4876. 2021
How do central and satellite galaxies quench? - Insights from spatially resolved spectroscopy in the MaNGA survey. 499:230-268. 2020
OzDES multi-object fibre spectroscopy for the Dark Energy Survey: results and second data release. 496:19-35. 2020
Optimizing automatic morphological classification of galaxies with machine learning and deep learning using Dark Energy Survey imaging. 493:4209-4228. 2020
The ALMaQUEST Survey II. What drives central starbursts at z ti 0?. 492:6027-6041. 2020
The ALMaQUEST survey - III. Scatter in the resolved star-forming main sequence is primarily due to variations in star formation efficiency. 493:L39-L43. 2020
Are galactic star formation and quenching governed by local, global, or environmental phenomena?. 492:96-139. 2020
Towards a deeper understanding of the physics driving galaxy quenching - inferring trends in the gas content via extinction. 492:L6-L11. 2020
C IV black hole mass measurements with the Australian Dark Energy Survey (OzDES). 487:3650-3663. 2019
First cosmological results using Type Ia supernovae from the Dark Energy Survey: measurement of the Hubble constant. 486:2184-2196. 2019
First cosmology results using Type Ia supernova from the Dark Energy Survey: simulations to correct supernova distance biases. 485:1171-1187. 2019
Interacting galaxies on FIRE-2: the connection between enhanced star formation and interstellar gas content. 485:1320-1338. 2019
The origin of the mass scales for maximal star formation efficiency and quenching: the critical role of supernovae. 485:3446-3456. 2019
What shapes a galaxy? - unraveling the role of mass, environment, and star formation in forming galactic structure. 485:666-696. 2019
A catalogue of structural and morphological measurements for DES Y1. 481:2018-2040. 2018
Rapidly evolving transients in the Dark Energy Survey. 481:894-917. 2018
X-ray/UV/optical variability of NGC 4593 with Swift: reprocessing of X-rays by an extended reprocessor. 480:2881-2897. 2018
Polarimetric and spectroscopic study of radio-quiet weak emission line quasars. 479:5075-5082. 2018
Dark Energy Survey Year 1 Results: redshift distributions of the weak-lensing source galaxies. 478:592-610. 2018
Dark Energy Survey Year 1 results: cross-correlation redshifts - methods and systematics characterization. 477:1651-1669. 2018
On the incidence of MgII absorbers along the blazar sightlines. 473:5154-5164. 2018
OzDES multifibre spectroscopy for the Dark Energy Survey: 3-yr results and first data release. 472:273-288. 2017
Multi-epoch intranight optical monitoring of eight radio-quiet BL Lac candidates. 471:606-616. 2017
Intraday optical variability of BL Lacertae. 469:3588-3596. 2017
Radio and optical intra-day variability observations of five blazars. 469:2457-2463. 2017
Discovery of a z=0.65 post-starburst BAL quasar in the DES supernova fields. 468:3682-3688. 2017
The relationship between star formation activity and galaxy structural properties in CANDELS and a semi-analytic model. 465:619-640. 2017
Optical intra-day variability in 3C 66A: A decade of observations. 469:2305-2312. 2017
The impact of galactic properties and environment on the quenching of central and satellite galaxies: a comparison between SDSS, Illustris and L-Galaxies. 462:2559-2586. 2016
Galaxy pairs in the Sloan Digital Sky Survey - XI. A new method for measuring the influence of the closest companion out to wide separations. 461:2589-2604. 2016
redMaGiC: selecting luminous red galaxies from the DES Science Verification data. 461:1431-1450. 2016
Stellar mass functions of galaxies, discs and spheroids at z ∼ 0.1. 459:44-69. 2016
An artificial neural network approach for ranking quenching parameters in central galaxies. 457:2086-2106. 2016
OzDES multifibre spectroscopy for the Dark Energy Survey: first-year operation and results. 452:3047-3063. 2015
Mapping galaxy encounters in numerical simulations: the spatial extent of induced star formation. 448:1107-1117. 2015
Combining Dark Energy Survey Science Verification data with near-infrared data from the ESO VISTA Hemisphere Survey. 446:2523-2539. 2015
Photometric redshift analysis in the Dark Energy Survey Science Verification data. 445:1482-1506. 2014
Galaxy formation as a cosmological tool - I. The galaxy merger history as a measure of cosmological parameters. 444:1125-1143. 2014
Bulge mass is king: the dominant role of the bulge in determining the fraction of passive galaxies in the Sloan Digital Sky Survey. 441:599-629. 2014
The dynamics of galaxy pairs in a cosmological setting. 436:1765-1786. 2013
The redshift and mass dependence on the formation of the Hubble sequence at z > 1 from CANDELS/UDS. 433:1185-1201. 2013
Gas accretion as a dominant formation mode in massive galaxies from the GOODS NICMOS Survey. 430:1051-1060. 2013
Multiwavelength intraday variability of the BL Lacertae S5 0716+714. 425:1357-1370. 2012
The relationship between star formation rates, local density and stellar mass up to z ∼ 3 in the GOODS NICMOS Survey. 418:938-948. 2011
The tumultuous formation of the Hubble sequence at z>1 examined with HST/Wide-Field Camera-3 observations of the Hubble Ultra Deep Field. 417:2770-2788. 2011
Star formation in a stellar mass-selected sample of galaxies to z=3 from the GOODS-NICMOS Survey. 417:289-303. 2011
A deep probe of the galaxy stellar mass functions at z ∼ 1-3 with the GOODS NICMOS Survey. 413:2845-2859. 2011
The Hubble Space Telescope GOODS NICMOS Survey: overview and the evolution of massive galaxies at 1.5<z<3. 413:80-100. 2011
Galaxy properties in different environments up to z ∼ 3 in the GOODS NICMOS Survey. 412:2361-2375. 2011
On the co-evolution of supermassive black holes and their host galaxies since z=3. 410:1174-1196. 2011
The structures of distant galaxies - III. The merger history of over 20 000 massive galaxies at z < 1.2. 394:1956-1972. 2009
A surprisingly high pair fraction for extremely massive galaxies at z ∼ 3 in the GOODS NICMOS survey. 394:L51-L55. 2009
The density structure around quasars from optical depth statistics. 361:1015-1029. 2005
Periodicities and regulatory mechanisms in β Lyrae. 303:736-754. 1999
LIGHT-CURVE SOLUTIONS FOR S-CANCRI AND TT-HYDRAE WITH RAPID ROTATION. 262:220-230. 1993
THE SPECTRAL SHAPE AND VARIABILITY OF THE BLAZAR 3C-446. 219:671-686. 1986
The role of environment and AGN feedback in quenching local galaxies: comparing cosmological hydrodynamical simulations to the SDSS (vol 528, pg 4891, 2024) 2024

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ASTRONOMY & ASTROPHYSICS Category

International Standard Serial Number (ISSN)

0035-8711