The Second Data Release of the Survey of the MAgellanic Stellar History (SMASH)

Publikation: Bidrag til tidsskrift › Tidsskriftartikel › Forskning › fagfællebedømt

Standard

The Second Data Release of the Survey of the MAgellanic Stellar History (SMASH). / Nidever, David L.; Olsen, Knut; Choi, Yumi; Ruiz-Lara, Tomas; Miller, Amy E.; Johnson, L. Clifton; Bell, Cameron P. M.; Blum, Robert D.; Cioni, Maria-Rosa L.; Gallart, Carme; Majewski, Steven R.; Martin, Nicolas F.; Massana, Pol; Monachesi, Antonela; Noel, Noelia E. D.; Sakowska, Joanna D.; van der Marel, Roeland P.; Walker, Alistair R.; Zaritsky, Dennis; Bell, Eric F.; Conn, Blair C.; de Boer, Thomas J. L.; Gruendl, Robert A.; Monelli, Matteo; Munoz, Ricardo R.; Saha, Abhijit; Katherina Vivas, A.; Bernard, Edouard; Besla, Gurtina; Carballo-Bello, Julio A.; Dorta, Antonio; Martinez-Delgado, David; Goater, Alex; Rusakov, Vadim; Stringfellow, Guy S.

I: Astronomical Journal, Bind 161, Nr. 2, 74, 01.02.2021.

Publikation: Bidrag til tidsskrift › Tidsskriftartikel › Forskning › fagfællebedømt

Harvard

Nidever, DL, Olsen, K, Choi, Y, Ruiz-Lara, T, Miller, AE, Johnson, LC, Bell, CPM, Blum, RD, Cioni, M-RL, Gallart, C, Majewski, SR, Martin, NF, Massana, P, Monachesi, A, Noel, NED, Sakowska, JD, van der Marel, RP, Walker, AR, Zaritsky, D, Bell, EF, Conn, BC, de Boer, TJL, Gruendl, RA, Monelli, M, Munoz, RR, Saha, A, Katherina Vivas, A, Bernard, E, Besla, G, Carballo-Bello, JA, Dorta, A, Martinez-Delgado, D, Goater, A, Rusakov, V & Stringfellow, GS 2021, 'The Second Data Release of the Survey of the MAgellanic Stellar History (SMASH)', Astronomical Journal, bind 161, nr. 2, 74. https://doi.org/10.3847/1538-3881/abceb7

APA

Nidever, D. L., Olsen, K., Choi, Y., Ruiz-Lara, T., Miller, A. E., Johnson, L. C., Bell, C. P. M., Blum, R. D., Cioni, M-R. L., Gallart, C., Majewski, S. R., Martin, N. F., Massana, P., Monachesi, A., Noel, N. E. D., Sakowska, J. D., van der Marel, R. P., Walker, A. R., Zaritsky, D., ... Stringfellow, G. S. (2021). The Second Data Release of the Survey of the MAgellanic Stellar History (SMASH). Astronomical Journal, 161(2), [74]. https://doi.org/10.3847/1538-3881/abceb7

Vancouver

Nidever DL, Olsen K, Choi Y, Ruiz-Lara T, Miller AE, Johnson LC o.a. The Second Data Release of the Survey of the MAgellanic Stellar History (SMASH). Astronomical Journal. 2021 feb. 1;161(2). 74. https://doi.org/10.3847/1538-3881/abceb7

Author

Nidever, David L. ; Olsen, Knut ; Choi, Yumi ; Ruiz-Lara, Tomas ; Miller, Amy E. ; Johnson, L. Clifton ; Bell, Cameron P. M. ; Blum, Robert D. ; Cioni, Maria-Rosa L. ; Gallart, Carme ; Majewski, Steven R. ; Martin, Nicolas F. ; Massana, Pol ; Monachesi, Antonela ; Noel, Noelia E. D. ; Sakowska, Joanna D. ; van der Marel, Roeland P. ; Walker, Alistair R. ; Zaritsky, Dennis ; Bell, Eric F. ; Conn, Blair C. ; de Boer, Thomas J. L. ; Gruendl, Robert A. ; Monelli, Matteo ; Munoz, Ricardo R. ; Saha, Abhijit ; Katherina Vivas, A. ; Bernard, Edouard ; Besla, Gurtina ; Carballo-Bello, Julio A. ; Dorta, Antonio ; Martinez-Delgado, David ; Goater, Alex ; Rusakov, Vadim ; Stringfellow, Guy S. / The Second Data Release of the Survey of the MAgellanic Stellar History (SMASH). I: Astronomical Journal. 2021 ; Bind 161, Nr. 2.

Bibtex

@article{07b82f155f10499f853e2267ab39c553,
title = "The Second Data Release of the Survey of the MAgellanic Stellar History (SMASH)",
abstract = "The Large and Small Magellanic Clouds (LMC and SMC) are the largest satellite galaxies of the Milky Way and close enough to allow for a detailed exploration of their structure and formation history. The Survey of the MAgellanic Stellar History (SMASH) is a community Dark Energy Camera (DECam) survey of the Magellanic Clouds using similar to 50 nights to sample over similar to 2400 deg(2) centered on the Clouds at similar to 20% filling factor (but with contiguous coverage in the central regions) and to depths of similar to 24th mag in ugriz. The primary goals of SMASH are to map out the extended stellar peripheries of the Clouds and uncover their complicated interaction and accretion history as well as to derive spatially resolved star formation histories of the central regions and create a {"}movie{"} of their past star formation. Here we announce the second SMASH public data release (DR2), which contains all 197 fully calibrated DECam fields including the main body fields in the central regions. The DR2 data are available through the Astro Data Lab hosted by the NSF's National Optical-Infrared Astronomy Research Laboratory. We highlight three science cases that make use of the SMASH DR2 data and will be published in the future: (1) preliminary star formation histories of the LMC, (2) the search for Magellanic star clusters using citizen scientists, and, (3) photometric metallicities of Magellanic Cloud stars using the DECam u-band.",
keywords = "Magellanic Clouds, Local Group, Milky Way Galaxy, Dwarf galaxies, Dwarf irregular galaxies, Surveys, Large Magellanic Cloud, Small Magellanic Cloud, Photometry, CCD photometry, STAR-FORMATION HISTORY, COLOR-MAGNITUDE DIAGRAMS, BACKGROUND GALAXIES, HST OBSERVATIONS, CLOUD CLUSTERS, VMC SURVEY, POPULATION, EVOLUTION, LMC, CATALOG",
author = "Nidever, {David L.} and Knut Olsen and Yumi Choi and Tomas Ruiz-Lara and Miller, {Amy E.} and Johnson, {L. Clifton} and Bell, {Cameron P. M.} and Blum, {Robert D.} and Cioni, {Maria-Rosa L.} and Carme Gallart and Majewski, {Steven R.} and Martin, {Nicolas F.} and Pol Massana and Antonela Monachesi and Noel, {Noelia E. D.} and Sakowska, {Joanna D.} and {van der Marel}, {Roeland P.} and Walker, {Alistair R.} and Dennis Zaritsky and Bell, {Eric F.} and Conn, {Blair C.} and {de Boer}, {Thomas J. L.} and Gruendl, {Robert A.} and Matteo Monelli and Munoz, {Ricardo R.} and Abhijit Saha and {Katherina Vivas}, A. and Edouard Bernard and Gurtina Besla and Carballo-Bello, {Julio A.} and Antonio Dorta and David Martinez-Delgado and Alex Goater and Vadim Rusakov and Stringfellow, {Guy S.}",
year = "2021",
month = feb,
day = "1",
doi = "10.3847/1538-3881/abceb7",
language = "English",
volume = "161",
journal = "The Astronomical Journal",
issn = "0004-6256",
publisher = "Institute of Physics Publishing, Inc",
number = "2",

}

RIS

TY - JOUR

T1 - The Second Data Release of the Survey of the MAgellanic Stellar History (SMASH)

AU - Nidever, David L.

AU - Olsen, Knut

AU - Choi, Yumi

AU - Ruiz-Lara, Tomas

AU - Miller, Amy E.

AU - Johnson, L. Clifton

AU - Bell, Cameron P. M.

AU - Blum, Robert D.

AU - Cioni, Maria-Rosa L.

AU - Gallart, Carme

AU - Majewski, Steven R.

AU - Martin, Nicolas F.

AU - Massana, Pol

AU - Monachesi, Antonela

AU - Noel, Noelia E. D.

AU - Sakowska, Joanna D.

AU - van der Marel, Roeland P.

AU - Walker, Alistair R.

AU - Zaritsky, Dennis

AU - Bell, Eric F.

AU - Conn, Blair C.

AU - de Boer, Thomas J. L.

AU - Gruendl, Robert A.

AU - Monelli, Matteo

AU - Munoz, Ricardo R.

AU - Saha, Abhijit

AU - Katherina Vivas, A.

AU - Bernard, Edouard

AU - Besla, Gurtina

AU - Carballo-Bello, Julio A.

AU - Dorta, Antonio

AU - Martinez-Delgado, David

AU - Goater, Alex

AU - Rusakov, Vadim

AU - Stringfellow, Guy S.

PY - 2021/2/1

Y1 - 2021/2/1

N2 - The Large and Small Magellanic Clouds (LMC and SMC) are the largest satellite galaxies of the Milky Way and close enough to allow for a detailed exploration of their structure and formation history. The Survey of the MAgellanic Stellar History (SMASH) is a community Dark Energy Camera (DECam) survey of the Magellanic Clouds using similar to 50 nights to sample over similar to 2400 deg(2) centered on the Clouds at similar to 20% filling factor (but with contiguous coverage in the central regions) and to depths of similar to 24th mag in ugriz. The primary goals of SMASH are to map out the extended stellar peripheries of the Clouds and uncover their complicated interaction and accretion history as well as to derive spatially resolved star formation histories of the central regions and create a "movie" of their past star formation. Here we announce the second SMASH public data release (DR2), which contains all 197 fully calibrated DECam fields including the main body fields in the central regions. The DR2 data are available through the Astro Data Lab hosted by the NSF's National Optical-Infrared Astronomy Research Laboratory. We highlight three science cases that make use of the SMASH DR2 data and will be published in the future: (1) preliminary star formation histories of the LMC, (2) the search for Magellanic star clusters using citizen scientists, and, (3) photometric metallicities of Magellanic Cloud stars using the DECam u-band.

AB - The Large and Small Magellanic Clouds (LMC and SMC) are the largest satellite galaxies of the Milky Way and close enough to allow for a detailed exploration of their structure and formation history. The Survey of the MAgellanic Stellar History (SMASH) is a community Dark Energy Camera (DECam) survey of the Magellanic Clouds using similar to 50 nights to sample over similar to 2400 deg(2) centered on the Clouds at similar to 20% filling factor (but with contiguous coverage in the central regions) and to depths of similar to 24th mag in ugriz. The primary goals of SMASH are to map out the extended stellar peripheries of the Clouds and uncover their complicated interaction and accretion history as well as to derive spatially resolved star formation histories of the central regions and create a "movie" of their past star formation. Here we announce the second SMASH public data release (DR2), which contains all 197 fully calibrated DECam fields including the main body fields in the central regions. The DR2 data are available through the Astro Data Lab hosted by the NSF's National Optical-Infrared Astronomy Research Laboratory. We highlight three science cases that make use of the SMASH DR2 data and will be published in the future: (1) preliminary star formation histories of the LMC, (2) the search for Magellanic star clusters using citizen scientists, and, (3) photometric metallicities of Magellanic Cloud stars using the DECam u-band.

KW - Magellanic Clouds

KW - Local Group

KW - Milky Way Galaxy

KW - Dwarf galaxies

KW - Dwarf irregular galaxies

KW - Surveys

KW - Large Magellanic Cloud

KW - Small Magellanic Cloud

KW - Photometry

KW - CCD photometry

KW - STAR-FORMATION HISTORY

KW - COLOR-MAGNITUDE DIAGRAMS

KW - BACKGROUND GALAXIES

KW - HST OBSERVATIONS

KW - CLOUD CLUSTERS

KW - VMC SURVEY

KW - POPULATION

KW - EVOLUTION

KW - LMC

KW - CATALOG

U2 - 10.3847/1538-3881/abceb7

DO - 10.3847/1538-3881/abceb7

M3 - Journal article

VL - 161

JO - The Astronomical Journal

JF - The Astronomical Journal

SN - 0004-6256

IS - 2

M1 - 74

ER -

ID: 256676528