Data

PHANGS-ALMA arcsecond CO(2-1) imaging of galaxies : J/ApJS/257/43

University of Southern Queensland
Leroy, Adam K. ; Schinnerer, Eva ; Hughes, Annie ; Rosolowsky, E. ; Pety, Jérôme ; Schruba, Andreas ; Usero, Antonio ; Blanc, Guillermo A. ; Chevance, Mélanie ; Emsellem, E. ; Faesi, Christopher M. ; Herrera, Cinthya N. ; Liu, Daizhong ; Meidt, Sharon ; Querejeta, Miguel ; Saito, Toshiki ; Sandstrom, Karin M. ; Sun, Jiayi ; Williams, Thomas ; Anand, Gagandeep ; Barnes, Ashley ; Behrens, Erica ; Belfiore, Francesco ; Benincasa, Samantha ; Bešlić, Ivana ; Bigiel, Frank ; Bolatto, Alberto ; den Brok, Jakob ; Cao, Yixian ; Chandar, Rupali ; Chastenet, Jérémy ; Chiang, I-Da ; Congiu, Enrico ; Dale, Daniel A. ; Deger, Sinan ; Eibensteiner, Cosima ; Egorov, Oleg ; García-Rodríguez, Axel ; Glover, Simon C. O. ; Grasha, Kathryn ; Henshaw, Jonathan ; Ho, I. Ting ; Kepley, Amanda A. ; Kim, Jaeyeon ; Klessen, Ralf ; Kreckel, K. ; Koch, Eric ; Kruijssen, J. M. Diederik ; Larson, Kirsten ; Lee, Janice ; Lopez , Laura A. ; Machado, Josh ; Mayker, Ness ; McElroy, Rebecca ; Murphy, Eric ; Ostriker, E. ; Pan, Hsi-An ; Pessa, Ismael ; Puschnig, Johannes ; Razza, Alessandro ; Sanchez-Blazquez, Patricia ; Francesco, Francesco ; Sardone, Amy ; Scheuermann, Fabian ; Sliwa, Kazimierz ; Sormani, Mattia ; Stuber, Sophia ; Thilker, David ; Turner, Jordan ; Utomo, Dyas ; Watkins, Elizabeth ; Whitmore, Bradley
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ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Adc&rfr_id=info%3Asid%2FANDS&rft_id=info:doi10.26093/cds/vizier.22570043&rft.title=PHANGS-ALMA arcsecond CO(2-1) imaging of galaxies : J/ApJS/257/43 &rft.identifier=http://doi.org/10.26093/cds/vizier.22570043&rft.description=PHANGS-ALMA is a key component of the multiwavelength observational campaign conducted by the Physics at High Angular resolution in Nearby Galaxies (PHANGS) project. Combining a Cycle 5 ALMA Large Program (PI: E. Schinnerer), a suite of smaller programs, and data from the ALMA archive, PHANGS-ALMA mapped the CO J=2->1 emission, hereafter CO(2-1), from a cleanly selected sample of 90 of the nearest, ALMA-accessible, massive, star-forming galaxies. We used the ALMA main array of 12m dishes in a compact configuration, which yields ~1 resolution at Band 6 ({nu}~230GHz), corresponding to ~100 pc linear resolution, or about the size of a massive giant molecular cloud at the typical distance to our targets. We covered the area of active star formation in each target using large mosaics that consisted of ~100-450 12m pointings per galaxy. Including all pilots and extensions, observations for PHANGS-ALMA spanned six years, from early 2013 until the end of&rft.creator=Leroy, Adam K. &rft.creator=Schinnerer, Eva &rft.creator=Hughes, Annie &rft.creator=Rosolowsky, E. &rft.creator=Pety, Jérôme &rft.creator=Schruba, Andreas &rft.creator=Usero, Antonio &rft.creator=Blanc, Guillermo A. &rft.creator=Chevance, Mélanie &rft.creator=Emsellem, E. &rft.creator=Faesi, Christopher M. &rft.creator=Herrera, Cinthya N. &rft.creator=Liu, Daizhong &rft.creator=Meidt, Sharon &rft.creator=Querejeta, Miguel &rft.creator=Saito, Toshiki &rft.creator=Sandstrom, Karin M. &rft.creator=Sun, Jiayi &rft.creator=Williams, Thomas &rft.creator=Anand, Gagandeep &rft.creator=Barnes, Ashley &rft.creator=Behrens, Erica &rft.creator=Belfiore, Francesco &rft.creator=Benincasa, Samantha &rft.creator=Bešlić, Ivana &rft.creator=Bigiel, Frank &rft.creator=Bolatto, Alberto &rft.creator=den Brok, Jakob &rft.creator=Cao, Yixian &rft.creator=Chandar, Rupali &rft.creator=Chastenet, Jérémy &rft.creator=Chiang, I-Da &rft.creator=Congiu, Enrico &rft.creator=Dale, Daniel A. &rft.creator=Deger, Sinan &rft.creator=Eibensteiner, Cosima &rft.creator=Egorov, Oleg &rft.creator=García-Rodríguez, Axel &rft.creator=Glover, Simon C. O. &rft.creator=Grasha, Kathryn &rft.creator=Henshaw, Jonathan &rft.creator=Ho, I. Ting &rft.creator=Kepley, Amanda A. &rft.creator=Kim, Jaeyeon &rft.creator=Klessen, Ralf &rft.creator=Kreckel, K. &rft.creator=Koch, Eric &rft.creator=Kruijssen, J. M. Diederik &rft.creator=Larson, Kirsten &rft.creator=Lee, Janice &rft.creator=Lopez , Laura A. &rft.creator=Machado, Josh &rft.creator=Mayker, Ness &rft.creator=McElroy, Rebecca &rft.creator=Murphy, Eric &rft.creator=Ostriker, E. &rft.creator=Pan, Hsi-An &rft.creator=Pessa, Ismael &rft.creator=Puschnig, Johannes &rft.creator=Razza, Alessandro &rft.creator=Sanchez-Blazquez, Patricia &rft.creator=Francesco, Francesco &rft.creator=Sardone, Amy &rft.creator=Scheuermann, Fabian &rft.creator=Sliwa, Kazimierz &rft.creator=Sormani, Mattia &rft.creator=Stuber, Sophia &rft.creator=Thilker, David &rft.creator=Turner, Jordan &rft.creator=Utomo, Dyas &rft.creator=Watkins, Elizabeth &rft.creator=Whitmore, Bradley &rft.date=2022&rft_subject=Carbon monoxide; Galaxies: nearby; Millimetric/submm sources;&rft.type=dataset&rft.language=English Access the data
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PHANGS-ALMA is a key component of the multiwavelength observational campaign conducted by the Physics at High Angular resolution in Nearby Galaxies (PHANGS) project. Combining a Cycle 5 ALMA Large Program (PI: E. Schinnerer), a suite of smaller programs, and data from the ALMA archive, PHANGS-ALMA mapped the CO J=2->1 emission, hereafter CO(2-1), from a cleanly selected sample of 90 of the nearest, ALMA-accessible, massive, star-forming galaxies. We used the ALMA main array of 12m dishes in a compact configuration, which yields ~1" resolution at Band 6 ({nu}~230GHz), corresponding to ~100 pc linear resolution, or about the size of a massive giant molecular cloud at the typical distance to our targets. We covered the area of active star formation in each target using large mosaics that consisted of ~100-450 12m pointings per galaxy. Including all pilots and extensions, observations for PHANGS-ALMA spanned six years, from early 2013 until the end of

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Carbon monoxide; Galaxies: nearby; Millimetric/submm sources; |

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uri : https://iopscience.iop.org/article/10.3847/1538-4365/ac17f3

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