Overview of the SDSS-IV MaNGA Survey: Mapping nearby Galaxies at Apache Point Observatory. Bundy, K., Bershady, M. A., Law, D. R., Yan, R., Drory, N., MacDonald, N., Wake, D. A., Cherinka, B., Sánchez-Gallego, J. R., Weijmans, A., Thomas, D., Tremonti, C., Masters, K., Coccato, L., Diamond-Stanic, A. M., Aragón-Salamanca, A., Avila-Reese, V., Badenes, C., Falcón-Barroso, J., Belfiore, F., Bizyaev, D., Blanc, G. A., Bland-Hawthorn, J., Blanton, M. R., Brownstein, J. R., Byler, N., Cappellari, M., Conroy, C., Dutton, A. A., Emsellem, E., Etherington, J., Frinchaboy, P. M., Fu, H., Gunn, J. E., Harding, P., Johnston, E. J., Kauffmann, G., Kinemuchi, K., Klaene, M. A., Knapen, J. H., Leauthaud, A., Li, C., Lin, L., Maiolino, R., Malanushenko, V., Malanushenko, E., Mao, S., Maraston, C., McDermid, R. M., Merrifield, M. R., Nichol, R. C., Oravetz, D., Pan, K., Parejko, J. K., Sanchez, S. F., Schlegel, D., Simmons, A., Steele, O., Steinmetz, M., Thanjavur, K., Thompson, B. A., Tinker, J. L., van den Bosch, R. C. E., Westfall, K. B., Wilkinson, D., Wright, S., Xiao, T., & Zhang, K. The Astrophysical Journal, 798:7, January, 2015. ![Overview of the SDSS-IV MaNGA Survey: Mapping nearby Galaxies at Apache Point Observatory [link]](https://bibbase.org/img/filetypes/link.svg "link")
Paper doi abstract bibtex We present an overview of a new integral field spectroscopic survey called MaNGA (Mapping Nearby Galaxies at Apache Point Observatory), one of three core programs in the fourth-generation Sloan Digital Sky Survey (SDSS-IV) that began on 2014 July 1. MaNGA will investigate the internal kinematic structure and composition of gas and stars in an unprecedented sample of 10,000 nearby galaxies. We summarize essential characteristics of the instrument and survey design in the context of MaNGA's key science goals and present prototype observations to demonstrate MaNGA's scientific potential. MaNGA employs dithered observations with 17 fiber-bundle integral field units that vary in diameter from 12'' (19 fibers) to 32'' (127 fibers). Two dual-channel spectrographs provide simultaneous wavelength coverage over 3600-10300 Å at R \textasciitilde 2000. With a typical integration time of 3 hr, MaNGA reaches a target r-band signal-to-noise ratio of 4-8 (Å-1 per 2'' fiber) at 23 AB mag arcsec-2, which is typical for the outskirts of MaNGA galaxies. Targets are selected with M * \textgreater\textasciitilde 109 M ⊙ using SDSS-I redshifts and i-band luminosity to achieve uniform radial coverage in terms of the effective radius, an approximately flat distribution in stellar mass, and a sample spanning a wide range of environments. Analysis of our prototype observations demonstrates MaNGA's ability to probe gas ionization, shed light on recent star formation and quenching, enable dynamical modeling, decompose constituent components, and map the composition of stellar populations. MaNGA's spatially resolved spectra will enable an unprecedented study of the astrophysics of nearby galaxies in the coming 6 yr.
@article{bundy_overview_2015,
title = {Overview of the {SDSS}-{IV} {MaNGA} {Survey}: {Mapping} nearby {Galaxies} at {Apache} {Point} {Observatory}},
volume = {798},
issn = {0004-637X},
shorttitle = {Overview of the {SDSS}-{IV} {MaNGA} {Survey}},
url = {http://adsabs.harvard.edu/abs/2015ApJ...798....7B},
doi = {10.1088/0004-637X/798/1/7},
abstract = {We present an overview of a new integral field spectroscopic survey
called MaNGA (Mapping Nearby Galaxies at Apache Point Observatory), one
of three core programs in the fourth-generation Sloan Digital Sky Survey
(SDSS-IV) that began on 2014 July 1. MaNGA will investigate the internal
kinematic structure and composition of gas and stars in an unprecedented
sample of 10,000 nearby galaxies. We summarize essential characteristics
of the instrument and survey design in the context of MaNGA's key
science goals and present prototype observations to demonstrate MaNGA's
scientific potential. MaNGA employs dithered observations with 17
fiber-bundle integral field units that vary in diameter from 12'' (19
fibers) to 32'' (127 fibers). Two dual-channel spectrographs provide
simultaneous wavelength coverage over 3600-10300 Å at R {\textasciitilde} 2000.
With a typical integration time of 3 hr, MaNGA reaches a target r-band
signal-to-noise ratio of 4-8 (Å-1 per 2'' fiber) at 23
AB mag arcsec-2, which is typical for the outskirts of MaNGA
galaxies. Targets are selected with M * {\textgreater}{\textasciitilde} 109
M ⊙ using SDSS-I redshifts and i-band luminosity to
achieve uniform radial coverage in terms of the effective radius, an
approximately flat distribution in stellar mass, and a sample spanning a
wide range of environments. Analysis of our prototype observations
demonstrates MaNGA's ability to probe gas ionization, shed light on
recent star formation and quenching, enable dynamical modeling,
decompose constituent components, and map the composition of stellar
populations. MaNGA's spatially resolved spectra will enable an
unprecedented study of the astrophysics of nearby galaxies in the coming
6 yr.},
urldate = {2018-06-26},
journal = {The Astrophysical Journal},
author = {Bundy, Kevin and Bershady, Matthew A. and Law, David R. and Yan, Renbin and Drory, Niv and MacDonald, Nicholas and Wake, David A. and Cherinka, Brian and Sánchez-Gallego, José R. and Weijmans, Anne-Marie and Thomas, Daniel and Tremonti, Christy and Masters, Karen and Coccato, Lodovico and Diamond-Stanic, Aleksandar M. and Aragón-Salamanca, Alfonso and Avila-Reese, Vladimir and Badenes, Carles and Falcón-Barroso, Jésus and Belfiore, Francesco and Bizyaev, Dmitry and Blanc, Guillermo A. and Bland-Hawthorn, Joss and Blanton, Michael R. and Brownstein, Joel R. and Byler, Nell and Cappellari, Michele and Conroy, Charlie and Dutton, Aaron A. and Emsellem, Eric and Etherington, James and Frinchaboy, Peter M. and Fu, Hai and Gunn, James E. and Harding, Paul and Johnston, Evelyn J. and Kauffmann, Guinevere and Kinemuchi, Karen and Klaene, Mark A. and Knapen, Johan H. and Leauthaud, Alexie and Li, Cheng and Lin, Lihwai and Maiolino, Roberto and Malanushenko, Viktor and Malanushenko, Elena and Mao, Shude and Maraston, Claudia and McDermid, Richard M. and Merrifield, Michael R. and Nichol, Robert C. and Oravetz, Daniel and Pan, Kaike and Parejko, John K. and Sanchez, Sebastian F. and Schlegel, David and Simmons, Audrey and Steele, Oliver and Steinmetz, Matthias and Thanjavur, Karun and Thompson, Benjamin A. and Tinker, Jeremy L. and van den Bosch, Remco C. E. and Westfall, Kyle B. and Wilkinson, David and Wright, Shelley and Xiao, Ting and Zhang, Kai},
month = jan,
year = {2015},
keywords = {galaxies: evolution, galaxies: general, surveys, techniques: imaging spectroscopy},
pages = {7},
}
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C.","Oravetz, D.","Pan, K.","Parejko, J. K.","Sanchez, S. F.","Schlegel, D.","Simmons, A.","Steele, O.","Steinmetz, M.","Thanjavur, K.","Thompson, B. A.","Tinker, J. L.","van den Bosch, R. C. E.","Westfall, K. B.","Wilkinson, D.","Wright, S.","Xiao, T.","Zhang, K."],"bibdata":{"bibtype":"article","type":"article","title":"Overview of the SDSS-IV MaNGA Survey: Mapping nearby Galaxies at Apache Point Observatory","volume":"798","issn":"0004-637X","shorttitle":"Overview of the SDSS-IV MaNGA Survey","url":"http://adsabs.harvard.edu/abs/2015ApJ...798....7B","doi":"10.1088/0004-637X/798/1/7","abstract":"We present an overview of a new integral field spectroscopic survey called MaNGA (Mapping Nearby Galaxies at Apache Point Observatory), one of three core programs in the fourth-generation Sloan Digital Sky Survey (SDSS-IV) that began on 2014 July 1. MaNGA will investigate the internal kinematic structure and composition of gas and stars in an unprecedented sample of 10,000 nearby galaxies. We summarize essential characteristics of the instrument and survey design in the context of MaNGA's key science goals and present prototype observations to demonstrate MaNGA's scientific potential. MaNGA employs dithered observations with 17 fiber-bundle integral field units that vary in diameter from 12'' (19 fibers) to 32'' (127 fibers). Two dual-channel spectrographs provide simultaneous wavelength coverage over 3600-10300 Å at R \\textasciitilde 2000. With a typical integration time of 3 hr, MaNGA reaches a target r-band signal-to-noise ratio of 4-8 (Å-1 per 2'' fiber) at 23 AB mag arcsec-2, which is typical for the outskirts of MaNGA galaxies. Targets are selected with M * \\textgreater\\textasciitilde 109 M ⊙ using SDSS-I redshifts and i-band luminosity to achieve uniform radial coverage in terms of the effective radius, an approximately flat distribution in stellar mass, and a sample spanning a wide range of environments. Analysis of our prototype observations demonstrates MaNGA's ability to probe gas ionization, shed light on recent star formation and quenching, enable dynamical modeling, decompose constituent components, and map the composition of stellar populations. 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evolution, galaxies: general, surveys, techniques: imaging spectroscopy","pages":"7","bibtex":"@article{bundy_overview_2015,\n\ttitle = {Overview of the {SDSS}-{IV} {MaNGA} {Survey}: {Mapping} nearby {Galaxies} at {Apache} {Point} {Observatory}},\n\tvolume = {798},\n\tissn = {0004-637X},\n\tshorttitle = {Overview of the {SDSS}-{IV} {MaNGA} {Survey}},\n\turl = {http://adsabs.harvard.edu/abs/2015ApJ...798....7B},\n\tdoi = {10.1088/0004-637X/798/1/7},\n\tabstract = {We present an overview of a new integral field spectroscopic survey \ncalled MaNGA (Mapping Nearby Galaxies at Apache Point Observatory), one\nof three core programs in the fourth-generation Sloan Digital Sky Survey\n(SDSS-IV) that began on 2014 July 1. MaNGA will investigate the internal\nkinematic structure and composition of gas and stars in an unprecedented\nsample of 10,000 nearby galaxies. We summarize essential characteristics\nof the instrument and survey design in the context of MaNGA's key\nscience goals and present prototype observations to demonstrate MaNGA's\nscientific potential. MaNGA employs dithered observations with 17\nfiber-bundle integral field units that vary in diameter from 12'' (19\nfibers) to 32'' (127 fibers). Two dual-channel spectrographs provide\nsimultaneous wavelength coverage over 3600-10300 Å at R {\\textasciitilde} 2000.\nWith a typical integration time of 3 hr, MaNGA reaches a target r-band\nsignal-to-noise ratio of 4-8 (Å-1 per 2'' fiber) at 23\nAB mag arcsec-2, which is typical for the outskirts of MaNGA\ngalaxies. Targets are selected with M * {\\textgreater}{\\textasciitilde} 109\nM ⊙ using SDSS-I redshifts and i-band luminosity to\nachieve uniform radial coverage in terms of the effective radius, an\napproximately flat distribution in stellar mass, and a sample spanning a\nwide range of environments. Analysis of our prototype observations\ndemonstrates MaNGA's ability to probe gas ionization, shed light on\nrecent star formation and quenching, enable dynamical modeling,\ndecompose constituent components, and map the composition of stellar\npopulations. MaNGA's spatially resolved spectra will enable an\nunprecedented study of the astrophysics of nearby galaxies in the coming\n6 yr.},\n\turldate = {2018-06-26},\n\tjournal = {The Astrophysical Journal},\n\tauthor = {Bundy, Kevin and Bershady, Matthew A. and Law, David R. and Yan, Renbin and Drory, Niv and MacDonald, Nicholas and Wake, David A. and Cherinka, Brian and Sánchez-Gallego, José R. and Weijmans, Anne-Marie and Thomas, Daniel and Tremonti, Christy and Masters, Karen and Coccato, Lodovico and Diamond-Stanic, Aleksandar M. and Aragón-Salamanca, Alfonso and Avila-Reese, Vladimir and Badenes, Carles and Falcón-Barroso, Jésus and Belfiore, Francesco and Bizyaev, Dmitry and Blanc, Guillermo A. and Bland-Hawthorn, Joss and Blanton, Michael R. and Brownstein, Joel R. and Byler, Nell and Cappellari, Michele and Conroy, Charlie and Dutton, Aaron A. and Emsellem, Eric and Etherington, James and Frinchaboy, Peter M. and Fu, Hai and Gunn, James E. and Harding, Paul and Johnston, Evelyn J. and Kauffmann, Guinevere and Kinemuchi, Karen and Klaene, Mark A. and Knapen, Johan H. and Leauthaud, Alexie and Li, Cheng and Lin, Lihwai and Maiolino, Roberto and Malanushenko, Viktor and Malanushenko, Elena and Mao, Shude and Maraston, Claudia and McDermid, Richard M. and Merrifield, Michael R. and Nichol, Robert C. and Oravetz, Daniel and Pan, Kaike and Parejko, John K. and Sanchez, Sebastian F. and Schlegel, David and Simmons, Audrey and Steele, Oliver and Steinmetz, Matthias and Thanjavur, Karun and Thompson, Benjamin A. and Tinker, Jeremy L. and van den Bosch, Remco C. E. and Westfall, Kyle B. and Wilkinson, David and Wright, Shelley and Xiao, Ting and Zhang, Kai},\n\tmonth = jan,\n\tyear = {2015},\n\tkeywords = {galaxies: evolution, galaxies: general, surveys, techniques: imaging spectroscopy},\n\tpages = {7},\n}\n\n","author_short":["Bundy, K.","Bershady, M. A.","Law, D. R.","Yan, R.","Drory, N.","MacDonald, N.","Wake, D. A.","Cherinka, B.","Sánchez-Gallego, J. R.","Weijmans, A.","Thomas, D.","Tremonti, C.","Masters, K.","Coccato, L.","Diamond-Stanic, A. M.","Aragón-Salamanca, A.","Avila-Reese, V.","Badenes, C.","Falcón-Barroso, J.","Belfiore, F.","Bizyaev, D.","Blanc, G. A.","Bland-Hawthorn, J.","Blanton, M. R.","Brownstein, J. R.","Byler, N.","Cappellari, M.","Conroy, C.","Dutton, A. A.","Emsellem, E.","Etherington, J.","Frinchaboy, P. M.","Fu, H.","Gunn, J. E.","Harding, P.","Johnston, E. J.","Kauffmann, G.","Kinemuchi, K.","Klaene, M. A.","Knapen, J. 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B.","Wilkinson, D.","Wright, S.","Xiao, T.","Zhang, K."],"key":"bundy_overview_2015","id":"bundy_overview_2015","bibbaseid":"bundy-bershady-law-yan-drory-macdonald-wake-cherinka-etal-overviewofthesdssivmangasurveymappingnearbygalaxiesatapachepointobservatory-2015","role":"author","urls":{"Paper":"http://adsabs.harvard.edu/abs/2015ApJ...798....7B"},"keyword":["galaxies: evolution","galaxies: general","surveys","techniques: imaging spectroscopy"],"metadata":{"authorlinks":{}}},"bibtype":"article","biburl":"https://bibbase.org/zotero/polyphant","dataSources":["7gvjSdWrEu7z5vjjj"],"keywords":["galaxies: evolution","galaxies: general","surveys","techniques: imaging spectroscopy"],"search_terms":["overview","sdss","manga","survey","mapping","nearby","galaxies","apache","point","observatory","bundy","bershady","law","yan","drory","macdonald","wake","cherinka","sánchez-gallego","weijmans","thomas","tremonti","masters","coccato","diamond-stanic","aragón-salamanca","avila-reese","badenes","falcón-barroso","belfiore","bizyaev","blanc","bland-hawthorn","blanton","brownstein","byler","cappellari","conroy","dutton","emsellem","etherington","frinchaboy","fu","gunn","harding","johnston","kauffmann","kinemuchi","klaene","knapen","leauthaud","li","lin","maiolino","malanushenko","malanushenko","mao","maraston","mcdermid","merrifield","nichol","oravetz","pan","parejko","sanchez","schlegel","simmons","steele","steinmetz","thanjavur","thompson","tinker","van den bosch","westfall","wilkinson","wright","xiao","zhang"],"title":"Overview of the SDSS-IV MaNGA Survey: Mapping nearby Galaxies at Apache Point Observatory","year":2015}