Related papers: The ALMA2030 Wideband Sensitivity Upgrade

Future prospects in observational galaxy evolution: towards increased resolution

Future prospects in observational galaxy evolution are reviewed from a personal perspective. New insights will especially come from high-redshift integral field kinematic data and similar low-redshift observations in very large and…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-12 Karl Glazebrook

Sustaining ALMA Science Through 2030 A North American Perspective

ALMA will sustain its transformational science through 2030 via an aggressive series of upgrades, for which an overview is provided.

Instrumentation and Methods for Astrophysics · Physics 2017-09-22 Henry Alwyn Wootten

BlueMUSE: Project Overview and Science Cases

We present the concept of BlueMUSE, a blue-optimised, medium spectral resolution, panoramic integral field spectrograph based on the MUSE concept and proposed for the Very Large Telescope. With an optimised transmission down to 350 nm, a…

Instrumentation and Methods for Astrophysics · Physics 2021-11-11 Johan Richard , Roland Bacon , Jérémy Blaizot , Samuel Boissier , Alessandro Boselli , NicolasBouché , Jarle Brinchmann , Norberto Castro , Laure Ciesla , Paul Crowther , Emanuele Daddi , Stefan Dreizler , Pierre-Alain Duc , David Elbaz , Benoit Epinat , Chris Evans , Matteo Fossati , Michele Fumagalli , Miriam Garcia , Thibault Garel , Matthew Hayes , Angela Adamo , Artemio Herrero , Emmanuel Hugot , Andrew Humphrey , Pascale Jablonka , Sebastian Kamann , Lex Kaper , Andreas Kelz , Jean-Paul Kneib , Alex de Koter , Davor Krajnović , Rolf-Peter Kudritzki , Norbert Langer , Carmela Lardo , Floriane Leclercq , Danny Lennon , Guillaume Mahler , Fabrice Martins , Richard Massey , Peter Mitchell , Ana Monreal-Ibero , Paco Najarro , Cyrielle Opitom , Polychronis Papaderos , Céline Péroux , Yves Revaz , Martin M. Roth , Philippe Rousselot , Andreas Sander , Charlotte Simmonds Wagemann , Ian Smail , Anthony Mark Swinbank , Frank Tramper , Tanya Urrutia , Anne Verhamme , Jorick Vink , Jeremy Walsh , Peter Weilbacher , Martin Wendt , Lutz Wisotzki , Bin Yang

A Characterization of the ALMA Phasing System at 345 GHz

The development of the Atacama Large Millimeter/submillimeter Array (ALMA) phasing system (APS) has allowed ALMA to function as an extraordinarily sensitive station for very long baseline interferometry (VLBI) at frequencies of up to 230…

Instrumentation and Methods for Astrophysics · Physics 2023-03-15 G. B. Crew , C. Goddi , L. D. Matthews , H. Rottmann , A. Saez , I. Marti-Vidal

The ALMA archive and its place in the astronomy of the future

The Atacama Large Millimeter/submillimeter Array (ALMA), an international partnership of Europe, North America and East Asia in cooperation with the Republic of Chile, is the largest astronomical project in existence. While ALMA's…

Instrumentation and Methods for Astrophysics · Physics 2015-04-29 Felix Stoehr , Mark Lacy , Stéphane Leon , Erik Muller , Alisdair Manning , Christophe Moins , Dustin Jenkins

Expanded Very Large Array

The Very Large Array is undergoing a major upgrade that will attain an order of magnitude improvement in continuum sensitivity across 1 to 50 GHz with instantaneous bandwidths up to 8 GHz in both polarizations. The new WIDAR correlator…

Instrumentation and Methods for Astrophysics · Physics 2010-11-04 Sean M. Dougherty , Rick Perley

High-redshift star formation in the ALMA era

The Atacama Large Millimetre/submillimetre Array (ALMA) is currently in the process of transforming our view of star-forming galaxies in the distant ($z\gtrsim1$) universe. Before ALMA, most of what we knew about dust-obscured star…

Astrophysics of Galaxies · Physics 2021-01-18 Jacqueline A. Hodge , Elisabete da Cunha

Adaptive Real Time Imaging Synthesis Telescopes

The digital revolution is transforming astronomy from a data-starved to a data-submerged science. Instruments such as the Atacama Large Millimeter Array (ALMA), the Large Synoptic Survey Telescope (LSST), and the Square Kilometer Array…

Instrumentation and Methods for Astrophysics · Physics 2012-09-25 Melvyn Wright

The Simons Observatory: Science Goals and Forecasts for the Enhanced Large Aperture Telescope

We describe updated scientific goals for the wide-field, millimeter-wave survey that will be produced by the Simons Observatory (SO). Significant upgrades to the 6-meter SO Large Aperture Telescope (LAT) are expected to be complete by 2028,…

Instrumentation and Methods for Astrophysics · Physics 2025-08-11 The Simons Observatory Collaboration , M. Abitbol , I. Abril-Cabezas , S. Adachi , P. Ade , A. E. Adler , P. Agrawal , J. Aguirre , Z. Ahmed , S. Aiola , T. Alford , A. Ali , D. Alonso , M. A. Alvarez , R. An , K. Arnold , P. Ashton , Z. Atkins , J. Austermann , S. Azzoni , C. Baccigalupi , A. Baleato Lizancos , D. Barron , P. Barry , J. Bartlett , N. Battaglia , R. Battye , E. Baxter , A. Bazarko , J. A. Beall , R. Bean , D. Beck , S. Beckman , J. Begin , A. Beheshti , B. Beringue , T. Bhandarkar , S. Bhimani , F. Bianchini , E. Biermann , S. Biquard , B. Bixler , S. Boada , D. Boettger , B. Bolliet , J. R. Bond , J. Borrill , J. Borrow , C. Braithwaite , T. L. R. Brien , M. L. Brown , S. M. Bruno , S. Bryan , R. Bustos , H. Cai , E. Calabrese , V. Calafut , F. M. Carl , A. Carones , J. Carron , A. Challinor , P. Chanial , N. Chen , K. Cheung , B. Chiang , Y. Chinone , J. Chluba , H. S. Cho , S. K. Choi , M. Chu , J. Clancy , S. E. Clark , P. Clarke , J. Cleary , D. L. Clements , J. Connors , C. Contaldi , G. Coppi , L. Corbett , N. F. Cothard , W. Coulton , K. D. Crowley , K. T. Crowley , A. Cukierman , J. M. D'Ewart , K. Dachlythra , R. Datta , S. Day-Weiss , T. de Haan , M. Devlin , L. Di Mascolo , S. Dicker , B. Dober , C. Doux , P. Dow , S. Doyle , C. J. Duell , S. M. Duff , A. J. Duivenvoorden , J. Dunkley , D. Dutcher , R. Dünner , M. Edenton , H. El Bouhargani , J. Errard , G. Fabbian , V. Fanfani , G. S. Farren , J. Fergusson , S. Ferraro , R. Flauger , A. Foster , K. Freese , J. C. Frisch , A. Frolov , G. Fuller , N. Galitzki , P. A. Gallardo , J. T. Galvez Ghersi , K. Ganga , J. Gao , X. Garrido , E. Gawiser , M. Gerbino , R. Gerras , S. Giardiello , A. Gill , V. Gilles , U. Giri , E. Gleave , V. Gluscevic , N. Goeckner-Wald , J. E. Golec , S. Gordon , M. Gralla , S. Gratton , D. Green , J. C. Groh , C. Groppi , Y. Guan , N. Gupta , J. E. Guðmundsson , S. Hagstotz , P. Hargrave , S. Haridas , K. Harrington , I. Harrison , M. Hasegawa , M. Hasselfield , V. Haynes , M. Hazumi , A. He , E. Healy , S. W. Henderson , B. S. Hensley , E. Hertig , C. Hervías-Caimapo , M. Higuchi , C. A. Hill , J. C. Hill , G. Hilton , M. Hilton , A. D. Hincks , G. Hinshaw , R. Hložek , A. Y. Q. Ho , S. Ho , S. P. Ho , T. D. Hoang , J. Hoh , E. Hornecker , A. L. Hornsby , S. C. Hotinli , Z. Huang , Z. B. Huber , J. Hubmayr , K. Huffenberger , J. P. Hughes , A. Idicherian Lonappan , M. Ikape , K. Irwin , J. Iuliano , A. H. Jaffe , B. Jain , H. T. Jense , O. Jeong , A. Johnson , B. R. Johnson , M. Johnson , M. Jones , B. Jost , D. Kaneko , E. D. Karpel , Y. Kasai , N. Katayama , B. Keating , B. Keller , R. Keskitalo , J. Kim , T. Kisner , K. Kiuchi , J. Klein , K. Knowles , A. M. Kofman , B. J. Koopman , A. Kosowsky , R. Kou , N. Krachmalnicoff , D. Kramer , A. Krishak , A. Krolewski , A. Kusaka , A. Kusiak , P. La Plante , A. La Posta , A. Laguë , J. Lashner , M. Lattanzi , A. Lee , E. Lee , J. Leech , C. Lessler , J. S. Leung , A. Lewis , Y. Li , Z. Li , M. Limon , L. Lin , M. Link , J. Liu , Y. Liu , J. Lonergan , T. Louis , T. Lucas , M. Ludlam , M. Lungu , M. Lyons , N. MacCrann , A. MacInnis , M. Madhavacheril , D. Mak , F. Maldonado , M. Mallaby-Kay , A. Manduca , A. Mangu , H. Mani , A. S. Maniyar , G. A. Marques , J. Mates , T. Matsumura , P. Mauskopf , A. May , N. McCallum , H. McCarrick , F. McCarthy , M. McCulloch , J. McMahon , P. D. Meerburg , Y. Mehta , J. Melin , J. Meyers , A. Middleton , A. Miller , M. Mirmelstein , K. Moodley , J. Moore , M. Morshed , T. Morton , E. Moser , T. Mroczkowski , M. Murata , M. Münchmeyer , S. Naess , H. Nakata , T. Namikawa , M. Nashimoto , F. Nati , P. Natoli , M. Negrello , S. K. Nerval , L. Newburgh , D. V. Nguyen , A. Nicola , M. D. Niemack , H. Nishino , Y. Nishinomiya , A. Orlando , J. Orlowski-Scherer , L. Pagano , L. A. Page , S. Pandey , A. Papageorgiou , I. Paraskevakos , B. Partridge , R. Patki , M. Peel , K. Perez Sarmiento , F. Perrotta , P. Phakathi , L. Piccirillo , E. Pierpaoli , T. Pinsonneault-Marotte , G. Pisano , D. Poletti , R. Puddu , G. Puglisi , F. J. Qu , M. J. Randall , C. Ranucci , C. Raum , R. Reeves , C. L. Reichardt , M. Remazeilles , Y. Rephaeli , D. Riechers , J. Robe , M. F. Robertson , N. Robertson , K. Rogers , F. Rojas , A. Romero , E. Rosenberg , A. Rotti , S. Rowe , A. Roy , S. Sadeh , N. Sailer , K. Sakaguri , T. Sakuma , Y. Sakurai , M. Salatino , G. H. Sanders , D. Sasaki , M. Sathyanarayana Rao , T. P. Satterthwaite , L. Saunders , L. Scalcinati , E. Schaan , B. Schmitt , M. Schmittfull , N. Sehgal , J. Seibert , Y. Seino , U. Seljak , S. Shaikh , E. Shaw , P. Shellard , B. Sherwin , M. Shimon , J. E. Shroyer , C. Sierra , J. Sievers , C. Sifón , P. Sikhosana , M. Silva-Feaver , S. M. Simon , A. Sinclair , K. Smith , W. Sohn , X. Song , R. F. Sonka , D. Spergel , J. Spisak , S. T. Staggs , G. Stein , J. R. Stevens , R. Stompor , E. Storer , R. Sudiwala , J. Sugiyama , K. M. Surrao , S. Sutariya , A. Suzuki , J. Suzuki , O. Tajima , S. Takakura , A. Takeuchi , I. Tansieri , A. C. Taylor , G. Teply , T. Terasaki , A. Thomas , D. B. Thomas , R. Thornton , H. Trac , T. Tsan , E. Tsang King Sang , C. Tucker , J. Ullom , L. Vacher , L. Vale , A. van Engelen , J. Van Lanen , J. van Marrewijk , D. D. Van Winkle , C. Vargas , E. M. Vavagiakis , I. Veenendaal , C. Vergès , M. Vissers , M. Viña , K. Wagoner , S. Walker , L. Walters , Y. Wang , B. Westbrook , J. Williams , P. Williams , H. Winch , E. J. Wollack , K. Wolz , J. Wong , Z. Xu , K. Yamada , E. Young , B. Yu , C. Yu , M. Zannoni , K. Zheng , N. Zhu , A. Zonca , I. Zubeldia

Prospects for doubling the range of Advanced LIGO

In the coming years, the gravitational wave community will be optimizing detector performance for a variety of astrophysical sources that make competing demands on the detector sensitivity in different frequency bands. In this paper we…

General Relativity and Quantum Cosmology · Physics 2015-03-31 John Miller , Lisa Barsotti , Salvatore Vitale , Peter Fritschel , Daniel Sigg , Matthew Evans

ALMA's high-cadence imaging capabilities for solar observations

The Atacama Large Millimeter/submillimeter Array offers an unprecedented view of our Sun at sub-/millimeter wavelengths. The high spatial, temporal, and spectral resolution facilitates the measurement of gas temperatures and magnetic fields…

Solar and Stellar Astrophysics · Physics 2015-02-18 Sven Wedemeyer , Asbjorn Parmer

Evolution of the Milky Way in Semi-Analytic Models: Detecting Cold Gas at z=3 with ALMA and SKA

We forecast the abilities of the Atacama Large Millimeter/submillimeter Array (ALMA) and the Square Kilometer Array (SKA) to detect CO and HI emission lines in galaxies at redshift z=3. A particular focus is set on Milky Way (MW)…

Cosmology and Nongalactic Astrophysics · Physics 2015-03-19 Danail Obreschkow , Ian Heywood , Steve Rawlings

Future mmVLBI Research with ALMA: A European vision

Very long baseline interferometry at millimetre/submillimetre wavelengths (mmVLBI) offers the highest achievable spatial resolution at any wavelength in astronomy. The anticipated inclusion of ALMA as a phased array into a global VLBI…

Instrumentation and Methods for Astrophysics · Physics 2014-07-02 R. P. J. Tilanus , T. P. Krichbaum , J. A. Zensus , A. Baudry , M. Bremer , H. Falcke , G. Giovannini , R. Laing , H. J. van Langevelde , W. Vlemmings , Z. Abraham , J. Afonso , I. Agudo , A. Alberdi , J. Alcolea , D. Altamirano , S. Asadi , K. Assaf , P. Augusto , A-K. Baczko , M. Boeck , T. Boller , M. Bondi , F. Boone , G. Bourda , R. Brajsa , J. Brand , S. Britzen , V. Bujarrabal , S. Cales , C. Casadio , V. Casasola , P. Castangia , J. Cernicharo , P. Charlot , L. Chemin , Y. Clenet , F. Colomer , F. Combes , J. Cordes , M. Coriat , N. Cross , F. D'Ammando , D. Dallacasa , J-F. Desmurs , R. Eatough , A. Eckart , D. Eisenacher , S. Etoka , M. Felix , R. Fender , M. Ferreira , E. Freeland , S. Frey , C. Fromm , L. Fuhrmann , K. Gabanyi , R. Galvan-Madrid , M. Giroletti , C. Goddi , J. Gomez , E. Gourgoulhon , M. Gray , I. di Gregorio , R. Greimel , N. Grosso , J. Guirado , K. Hada , A. Hanslmeier , C. Henkel , F. Herpin , P. Hess , J. Hodgson , D. Horns , E. Humphreys , B. Hutawarakorn Kramer , V. Ilyushin , V. Impellizzeri , V. Ivanov , M. Julião , M. Kadler , E. Kerins , P. Klaassen , K. van 't Klooster , E. Kording , M. Kozlov , M. Kramer , A. Kreikenbohm , O. Kurtanidze , J. Lazio , A. Leite , M. Leitzinger , J. Lepine , S. Levshakov , R. Lico , M. Lindqvist , E. Liuzzo , A. Lobanov , P. Lucas , K. Mannheim , J. Marcaide , S. Markoff , I. Martí-Vidal , C. Martins , N. Masetti , M. Massardi , K. Menten , H. Messias , S. Migliari , A. Mignano , J. Miller-Jones , D. Minniti , P. Molaro , S. Molina , A. Monteiro , L. Moscadelli , C. Mueller , A. Müller , S. Muller , F. Niederhofer , P. Odert , H. Olofsson , M. Orienti , R. Paladino , F. Panessa , Z. Paragi , T. Paumard , P. Pedrosa , M. Pérez-Torres , G. Perrin , M. Perucho , D. Porquet , I. Prandoni , S. Ransom , D. Reimers , M. Rejkuba , L. Rezzolla , A. Richards , E. Ros , A. Roy , A. Rushton , T. Savolainen , R. Schulz , M. Silva , G. Sivakoff , R. Soria-Ruiz , R. Soria , M. Spaans , R. Spencer , B. Stappers , G. Surcis , A. Tarchi , M. Temmer , M. Thompson , J. Torrelles , J. Truestedt , V. Tudose , T. Venturi , J. Verbiest , J. Vieira , P. Vielzeuf , F. Vincent , N. Wex , K. Wiik , T. Wiklind , J. Wilms , E. Zackrisson , H. Zechlin

ALMA High-frequency Long-baseline Campaign in 2017: A Comparison of the Band-to-band and In-band Phase Calibration Techniques and Phase-calibrator Separation Angles

The Atacama Large millimeter/submillimeter Array (ALMA) obtains spatial resolutions of 15 to 5 milli-arcsecond (mas) at 275-950GHz (0.87-0.32mm) with 16km baselines. Calibration at higher-frequencies is challenging as ALMA sensitivity and…

Instrumentation and Methods for Astrophysics · Physics 2020-09-15 Luke T. Maud , Yoshiharu Asaki , Edward B. Fomalont , William R. F. Dent , Akihiko Hirota , Satoki Matsushita , Neil M. Phillips , John M. Carpenter , Satoko Takahashi , Eric Villard , Tsuyoshi Sawada , Stuartt Corder

Report by the ESA-ESO Working Group on "The Herschel-ALMA Synergies"

The Herschel Satellite and the Atacama Large Millimeter Array (ALMA) are two very large sub-mm and far infrared (FIR) astronomy projects that are expected to come into operation in this decade. This report contains descriptions of these…

Astrophysics · Physics 2007-05-23 T. L. Wilson , D. Elbaz , eds

ALMA Band 2 line survey of a $z = 3.44$ clumpy strongly-lensed submillimetre galaxy

I present the first molecular line survey of the strongly lensed submillimetre galaxy SPT-S J002706-5007.4 ($z = 3.44$) using the new Atacama Large Millimeter/submillimeter Array (ALMA) Band~2 receivers (67 - 116 GHz), whose commissioning…

Astrophysics of Galaxies · Physics 2026-05-18 Tom J. L. C. Bakx

ALMA Resolves 30 Doradus: Sub-parsec Molecular Cloud Structure Near the Closest Super-Star Cluster

We present ALMA observations of 30 Doradus -- the highest resolution view of molecular gas in an extragalactic star formation region to date (~0.4pc x 0.6pc). The 30Dor-10 cloud north of R136 was mapped in 12CO 2-1, 13CO 2-1, C18O 2-1,…

Astrophysics of Galaxies · Physics 2015-06-16 Remy Indebetouw , Crystal Brogan , C. -H. Rosie Chen , Adam Leroy , Kelsey Johnson , Erik Muller , Suzanne Madden , Diane Cormier , Frederic Galliano , Annie Hughes , Todd Hunter , Akiko Kawamura , Amanda Kepley , Vianney Lebouteiller , Margaret Meixner , Joana M. Oliveira , Toshikazu Onishi , Tatiana Vasyunina

Exciting Maser Science with New Instruments - the Promise of the EVLA

In the near future, the Expanded Very Large Array (EVLA) will allow surveys for maser sources with unprecedented sensitivity, spectral coverage and spectroscopic capabilities. In particular, comprehensive surveys for many maser species with…

Astrophysics · Physics 2009-11-13 Karl M. Menten

ALMA Observation of a $z\gtrsim10$ Galaxy Candidate Discovered with JWST

We report the ALMA observation of a $z\gtrsim10$ galaxy candidate (GHZ1) discovered from the GLASS-JWST Early Release Science Program. Our ALMA program aims to detect the [OIII] emission line at the rest-frame 3393.0062 GHz ($88.36\mu$m)…

Astrophysics of Galaxies · Physics 2023-06-28 Ilsang Yoon , Christopher L. Carilli , Seiji Fujimoto , Marco Castellano , Emiliano Merlin , Paola Santini , Min S. Yun , Eric J. Murphy , Intae Jung , Caitlin M. Casey , Steven L. Finkelstein , Casey Papovich , Adriano Fontana , Tommaso Treu , Jonathan Letai

ALMA observations of alpha Centauri: First detection of main-sequence stars at 3mm wavelength

The precise mechanisms that provide the non-radiative energy for heating the chromosphere and the corona of the Sun and those of other stars constitute an active field of research. By studying stellar chromospheres one aims at identifying…

Solar and Stellar Astrophysics · Physics 2014-12-24 R. Liseau , W. Vlemmings , A. Bayo , E. Bertone , J. H. Black , C. del Burgo , M. Chavez , W. Danchi , V. De la Luz , C. Eiroa , S. Ertel , M. C. W. Fridlund , K. Justtanont , A. Krivov , J. P. Marshall , A. Mora , B. Montesinos , L. -A. Nyman , G. Olofsson , J. Sanz-Forcada , P. Thebault , G. J. White