The ALMA Spectroscopic Survey in the Hubble Ultra Deep Field: constraining the molecular content at log (M[ast]/M[symbol sun]) [approximately] 9.5 with CO stacking of MUSE-detected z [approximately] 1.5 galaxies
We report molecular gas mass estimates obtained from a stacking analysis of CO line emission in the ALMA Spectroscopic Survey (ASPECS) using the spectroscopic redshifts from the optical integral field spectroscopic survey by the Multi Unit Spectroscopic Explorer (MUSE) of the Hubble Ultra Deep Field...
Saved in:
| Main Authors: | , , , , , , , , , , , , , , , , , , , , , |
|---|---|
| Format: | Article (Journal) |
| Language: | English |
| Published: |
2020 October 19
|
| In: |
The astrophysical journal
Year: 2020, Volume: 902, Issue: 2 |
| ISSN: | 1538-4357 |
| DOI: | 10.3847/1538-4357/abba2f |
| Online Access: | Verlag, lizenzpflichtig, Volltext: https://doi.org/10.3847/1538-4357/abba2f
|
| Author Notes: | Hanae Inami, Roberto Decarli, Fabian Walter, Axel Weiss, Chris Carilli, Manuel Aravena, Leindert Boogaard, Jorge Gonzaĺez-López, Gergö Popping, Elisabete da Cunha, Roland Bacon, Franz Bauer, Thierry Contini, Paulo C. Cortes, Pierre Cox, Emanuele Daddi, Tanio Díaz-Santos, Melanie Kaasinen, Dominik A. Riechers, Jeff Wagg, Paul van der Werf, and Lutz Wisotzki |
MARC
| LEADER | 00000caa a2200000 c 4500 | ||
|---|---|---|---|
| 001 | 1744866716 | ||
| 003 | DE-627 | ||
| 005 | 20230123155124.0 | ||
| 007 | cr uuu---uuuuu | ||
| 008 | 210118s2020 xx |||||o 00| ||eng c | ||
| 024 | 7 | |a 10.3847/1538-4357/abba2f |2 doi | |
| 035 | |a (DE-627)1744866716 | ||
| 035 | |a (DE-599)KXP1744866716 | ||
| 035 | |a (OCoLC)1341388912 | ||
| 040 | |a DE-627 |b ger |c DE-627 |e rda | ||
| 041 | |a eng | ||
| 084 | |a 29 |2 sdnb | ||
| 100 | 1 | |a Inami, Hanae |e VerfasserIn |0 (DE-588)1225305934 |0 (DE-627)1744870640 |4 aut | |
| 245 | 1 | 4 | |a The ALMA Spectroscopic Survey in the Hubble Ultra Deep Field |b constraining the molecular content at log (M[ast]/M[symbol sun]) [approximately] 9.5 with CO stacking of MUSE-detected z [approximately] 1.5 galaxies |c Hanae Inami, Roberto Decarli, Fabian Walter, Axel Weiss, Chris Carilli, Manuel Aravena, Leindert Boogaard, Jorge Gonzaĺez-López, Gergö Popping, Elisabete da Cunha, Roland Bacon, Franz Bauer, Thierry Contini, Paulo C. Cortes, Pierre Cox, Emanuele Daddi, Tanio Díaz-Santos, Melanie Kaasinen, Dominik A. Riechers, Jeff Wagg, Paul van der Werf, and Lutz Wisotzki |
| 246 | 3 | 0 | |a ~, Tilde, M⊙ Sonnenmasse Symbol Sonne, M* |
| 264 | 1 | |c 2020 October 19 | |
| 300 | |a 18 | ||
| 336 | |a Text |b txt |2 rdacontent | ||
| 337 | |a Computermedien |b c |2 rdamedia | ||
| 338 | |a Online-Ressource |b cr |2 rdacarrier | ||
| 500 | |a Gesehen am 18.01.2021 | ||
| 500 | |a Im Titel wird die Tilde als Zeichen dargestellt | ||
| 500 | |a Im Titel ist M[ast] als Tropfensternchen (englisch: teardrop-spoked asterisk) dargestellt und tiefgestellt | ||
| 500 | |a Im Titel ist M[symbol sun] als Abkürzung für die astronomische Maßeinheit Sonnenmasse dargestellt und tiefgestellt | ||
| 520 | |a We report molecular gas mass estimates obtained from a stacking analysis of CO line emission in the ALMA Spectroscopic Survey (ASPECS) using the spectroscopic redshifts from the optical integral field spectroscopic survey by the Multi Unit Spectroscopic Explorer (MUSE) of the Hubble Ultra Deep Field (HUDF). Stacking was performed on subsets of the sample of galaxies classified by their stellar mass and position relative to the main-sequence relation (on, above, below). Among all the CO emission lines, from CO(2-1) to CO(6-5), with redshifts accessible via the ASPECS Band 3 and the MUSE data, CO(2-1) provides the strongest constraints on the molecular gas content. We detect CO(2-1) emission in galaxies down to stellar masses of . Below this stellar mass, we present a new constraint on the molecular gas content of main-sequence galaxies by stacking based on the MUSE detections. We find that the molecular gas mass of main-sequence galaxies continuously decreases with stellar mass down to . Assuming a metallicity-based CO-to-H 2 conversion factor, the molecular gas-to-stellar mass ratio from to ∼10.0 does not seem to decrease as fast as for , which is in line with simulations and studies at lower redshift. The inferred molecular gas density of MUSE-selected galaxies at is comparable with the one derived in the HUDF with a different CO selection. Using the MUSE data we recover most of the CO emission in our deep ALMA observations through stacking, demonstrating the synergy between volumetric surveys obtained at different wave bands. | ||
| 700 | 1 | |a Decarli, Roberto |e VerfasserIn |4 aut | |
| 700 | 1 | |a Walter, Fabian |e VerfasserIn |4 aut | |
| 700 | 1 | |a Weiss, Axel |e VerfasserIn |4 aut | |
| 700 | 1 | |a Carilli, Chris |e VerfasserIn |4 aut | |
| 700 | 1 | |a Aravena, Manuel |e VerfasserIn |4 aut | |
| 700 | 1 | |a Boogaard, Leindert |e VerfasserIn |4 aut | |
| 700 | 1 | |a Gonzaĺez-López, Jorge |e VerfasserIn |4 aut | |
| 700 | 1 | |a Popping, Gergö |e VerfasserIn |4 aut | |
| 700 | 1 | |a Cunha, Elisabete da |e VerfasserIn |4 aut | |
| 700 | 1 | |a Bacon, Roland |e VerfasserIn |4 aut | |
| 700 | 1 | |a Bauer, Franz |e VerfasserIn |4 aut | |
| 700 | 1 | |a Contini, Thierry |e VerfasserIn |4 aut | |
| 700 | 1 | |a Cortes, Paulo C. |e VerfasserIn |4 aut | |
| 700 | 1 | |a Cox, Pierre |e VerfasserIn |4 aut | |
| 700 | 1 | |a Daddi, Emanuele |e VerfasserIn |4 aut | |
| 700 | 1 | |a Díaz-Santos, Tanio |e VerfasserIn |4 aut | |
| 700 | 1 | |a Kaasinen, Melanie |d 1994- |e VerfasserIn |0 (DE-588)1198901357 |0 (DE-627)1681083140 |4 aut | |
| 700 | 1 | |a Riechers, Dominik A. |d 1978- |e VerfasserIn |0 (DE-588)133664767 |0 (DE-627)550677615 |0 (DE-576)300009178 |4 aut | |
| 700 | 1 | |a Wagg, Jeff |e VerfasserIn |4 aut | |
| 700 | 1 | |a Werf, Paul van der |e VerfasserIn |4 aut | |
| 700 | 1 | |a Wisotzki, Lutz |e VerfasserIn |4 aut | |
| 773 | 0 | 8 | |i Enthalten in |t The astrophysical journal |d London : Institute of Physics Publ., 1995 |g 902(2020,2) Artikel-Nummer 113, 18 Seiten |h Online-Ressource |w (DE-627)269019219 |w (DE-600)1473835-1 |w (DE-576)077662733 |x 1538-4357 |7 nnas |a The ALMA Spectroscopic Survey in the Hubble Ultra Deep Field constraining the molecular content at log (M[ast]/M[symbol sun]) [approximately] 9.5 with CO stacking of MUSE-detected z [approximately] 1.5 galaxies |
| 773 | 1 | 8 | |g volume:902 |g year:2020 |g number:2 |g extent:18 |a The ALMA Spectroscopic Survey in the Hubble Ultra Deep Field constraining the molecular content at log (M[ast]/M[symbol sun]) [approximately] 9.5 with CO stacking of MUSE-detected z [approximately] 1.5 galaxies |
| 856 | 4 | 0 | |u https://doi.org/10.3847/1538-4357/abba2f |x Verlag |x Resolving-System |z lizenzpflichtig |3 Volltext |
| 951 | |a AR | ||
| 992 | |a 20210118 | ||
| 993 | |a Article | ||
| 994 | |a 2020 | ||
| 998 | |g 1198901357 |a Kaasinen, Melanie |m 1198901357:Kaasinen, Melanie |d 130000 |e 130000PK1198901357 |k 0/130000/ |p 18 | ||
| 999 | |a KXP-PPN1744866716 |e 3838725336 | ||
| BIB | |a Y | ||
| SER | |a journal | ||
| JSO | |a {"recId":"1744866716","language":["eng"],"type":{"bibl":"article-journal","media":"Online-Ressource"},"note":["Gesehen am 18.01.2021","Im Titel wird die Tilde als Zeichen dargestellt","Im Titel ist M[ast] als Tropfensternchen (englisch: teardrop-spoked asterisk) dargestellt und tiefgestellt","Im Titel ist M[symbol sun] als Abkürzung für die astronomische Maßeinheit Sonnenmasse dargestellt und tiefgestellt"],"person":[{"role":"aut","roleDisplay":"VerfasserIn","display":"Inami, Hanae","given":"Hanae","family":"Inami"},{"given":"Roberto","family":"Decarli","role":"aut","display":"Decarli, Roberto","roleDisplay":"VerfasserIn"},{"display":"Walter, Fabian","roleDisplay":"VerfasserIn","role":"aut","family":"Walter","given":"Fabian"},{"display":"Weiss, Axel","roleDisplay":"VerfasserIn","role":"aut","family":"Weiss","given":"Axel"},{"given":"Chris","family":"Carilli","role":"aut","roleDisplay":"VerfasserIn","display":"Carilli, Chris"},{"role":"aut","roleDisplay":"VerfasserIn","display":"Aravena, Manuel","given":"Manuel","family":"Aravena"},{"family":"Boogaard","given":"Leindert","display":"Boogaard, Leindert","roleDisplay":"VerfasserIn","role":"aut"},{"family":"Gonzaĺez-López","given":"Jorge","roleDisplay":"VerfasserIn","display":"Gonzaĺez-López, Jorge","role":"aut"},{"given":"Gergö","family":"Popping","role":"aut","roleDisplay":"VerfasserIn","display":"Popping, Gergö"},{"given":"Elisabete da","family":"Cunha","role":"aut","roleDisplay":"VerfasserIn","display":"Cunha, Elisabete da"},{"family":"Bacon","given":"Roland","display":"Bacon, Roland","roleDisplay":"VerfasserIn","role":"aut"},{"given":"Franz","family":"Bauer","role":"aut","roleDisplay":"VerfasserIn","display":"Bauer, Franz"},{"given":"Thierry","family":"Contini","role":"aut","roleDisplay":"VerfasserIn","display":"Contini, Thierry"},{"family":"Cortes","given":"Paulo C.","display":"Cortes, Paulo C.","roleDisplay":"VerfasserIn","role":"aut"},{"family":"Cox","given":"Pierre","roleDisplay":"VerfasserIn","display":"Cox, Pierre","role":"aut"},{"role":"aut","display":"Daddi, Emanuele","roleDisplay":"VerfasserIn","given":"Emanuele","family":"Daddi"},{"given":"Tanio","family":"Díaz-Santos","role":"aut","display":"Díaz-Santos, Tanio","roleDisplay":"VerfasserIn"},{"given":"Melanie","family":"Kaasinen","role":"aut","display":"Kaasinen, Melanie","roleDisplay":"VerfasserIn"},{"family":"Riechers","given":"Dominik A.","display":"Riechers, Dominik A.","roleDisplay":"VerfasserIn","role":"aut"},{"given":"Jeff","family":"Wagg","role":"aut","display":"Wagg, Jeff","roleDisplay":"VerfasserIn"},{"given":"Paul van der","family":"Werf","role":"aut","roleDisplay":"VerfasserIn","display":"Werf, Paul van der"},{"role":"aut","display":"Wisotzki, Lutz","roleDisplay":"VerfasserIn","given":"Lutz","family":"Wisotzki"}],"title":[{"title_sort":"ALMA Spectroscopic Survey in the Hubble Ultra Deep Field","title":"The ALMA Spectroscopic Survey in the Hubble Ultra Deep Field","subtitle":"constraining the molecular content at log (M[ast]/M[symbol sun]) [approximately] 9.5 with CO stacking of MUSE-detected z [approximately] 1.5 galaxies"}],"relHost":[{"title":[{"subtitle":"an international review of spectroscopy and astronomical physics","title":"The astrophysical journal","title_sort":"astrophysical journal"}],"titleAlt":[{"title":"The astrophysical journal / 1"},{"title":"ApJ"}],"part":{"issue":"2","year":"2020","extent":"18","volume":"902","text":"902(2020,2) Artikel-Nummer 113, 18 Seiten"},"pubHistory":["Vol. 447 (1995) [?]-"],"recId":"269019219","language":["eng"],"disp":"The ALMA Spectroscopic Survey in the Hubble Ultra Deep Field constraining the molecular content at log (M[ast]/M[symbol sun]) [approximately] 9.5 with CO stacking of MUSE-detected z [approximately] 1.5 galaxiesThe astrophysical journal","type":{"bibl":"periodical","media":"Online-Ressource"},"note":["Gesehen am 18.01.2022","Fortsetzung der Druck-Ausgabe"],"id":{"zdb":["1473835-1"],"eki":["269019219"],"issn":["1538-4357"]},"origin":[{"publisherPlace":"London ; Chicago, Ill. [u.a.]","dateIssuedDisp":"[1995?]-","publisher":"Institute of Physics Publ. ; Univ. of Chicago Press"}],"name":{"displayForm":["publ. in coll. with the American Astronomical Society. S. Chandrasekhar, managing ed"]},"physDesc":[{"extent":"Online-Ressource"}]}],"physDesc":[{"extent":"18 S."}],"name":{"displayForm":["Hanae Inami, Roberto Decarli, Fabian Walter, Axel Weiss, Chris Carilli, Manuel Aravena, Leindert Boogaard, Jorge Gonzaĺez-López, Gergö Popping, Elisabete da Cunha, Roland Bacon, Franz Bauer, Thierry Contini, Paulo C. Cortes, Pierre Cox, Emanuele Daddi, Tanio Díaz-Santos, Melanie Kaasinen, Dominik A. Riechers, Jeff Wagg, Paul van der Werf, and Lutz Wisotzki"]},"id":{"doi":["10.3847/1538-4357/abba2f"],"eki":["1744866716"]},"origin":[{"dateIssuedKey":"2020","dateIssuedDisp":"2020 October 19"}]} | ||
| SRT | |a INAMIHANAEALMASPECTR2020 | ||