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Title: Constraining the Milky Way’s ultraviolet-to-infrared SED with Gaussian process regression

Abstract

ABSTRACT Improving our knowledge of global Milky Way (MW) properties is critical for connecting the detailed measurements only possible from within our Galaxy to our understanding of the broader galaxy population. We here train Gaussian process regression (GPR) models on SDSS (Sloan Digital Sky Survey) galaxies to map from galaxy properties (stellar mass, apparent axial ratio, star formation rate, bulge-to-total ratio, disc scale length, and bar vote fraction) to ultraviolet (UV; GALEX FUV/NUV), optical (SDSS ugriz), and infrared (IR; 2MASS JHKs and WISE W1/W2/W3/W4) fluxes and uncertainties. With these models, we estimate the photometric properties of the MW, resulting in a full UV-to-IR spectral energy distribution (SED) as it would be measured externally, viewed face-on. We confirm that the MW lies in the green valley in optical diagnostic diagrams, but show for the first time that the MW is in the star-forming region in standard UV and IR diagnostics – characteristic of the population of red spiral galaxies. Although our GPR method predicts one band at a time, the resulting MW UV–IR SED is consistent with SEDs of local spirals with characteristics broadly similar to the MW, suggesting that these independent predictions can be combined reliably. Our UV–IR SED willmore » be invaluable for reconstructing the MW’s star formation history using the same tools employed for external galaxies, allowing comparisons of results from in situ measurements to those from the methods used for extragalactic objects.« less

Authors:
ORCiD logo; ; ; ; ; ; ORCiD logo;
Publication Date:
Research Org.:
Lawrence Berkeley National Laboratory (LBNL), Berkeley, CA (United States). National Energy Research Scientific Computing Center (NERSC)
Sponsoring Org.:
USDOE Office of Science (SC), High Energy Physics (HEP); National Aeronautics Space Administration (NASA); Chinese Academy of Sciences (CAS); National Natural Science Foundation of China (NSFC); National Science Foundation (NSF)
OSTI Identifier:
1827472
Alternate Identifier(s):
OSTI ID: 1982536
Grant/Contract Number:  
AC02-05CH1123; AC02-05CH11231; 80NSSC19K0588; NAS5-98034; XDB09000000; 114A11KYSB20160057; 11433005; AST-0950945
Resource Type:
Published Article
Journal Name:
Monthly Notices of the Royal Astronomical Society
Additional Journal Information:
Journal Name: Monthly Notices of the Royal Astronomical Society Journal Volume: 508 Journal Issue: 3; Journal ID: ISSN 0035-8711
Publisher:
Oxford University Press
Country of Publication:
United Kingdom
Language:
English
Subject:
79 ASTRONOMY AND ASTROPHYSICS; Astronomy; Astrophysics; Galaxy; Fundamental parameters; Structure

Citation Formats

Fielder, Catherine E., Newman, Jeffrey A., Andrews, Brett H., Zasowski, Gail, Boardman, Nicholas F., Licquia, Tim, Masters, Karen L., and Salim, Samir. Constraining the Milky Way’s ultraviolet-to-infrared SED with Gaussian process regression. United Kingdom: N. p., 2021. Web. doi:10.1093/mnras/stab2618.
Fielder, Catherine E., Newman, Jeffrey A., Andrews, Brett H., Zasowski, Gail, Boardman, Nicholas F., Licquia, Tim, Masters, Karen L., & Salim, Samir. Constraining the Milky Way’s ultraviolet-to-infrared SED with Gaussian process regression. United Kingdom. https://doi.org/10.1093/mnras/stab2618
Fielder, Catherine E., Newman, Jeffrey A., Andrews, Brett H., Zasowski, Gail, Boardman, Nicholas F., Licquia, Tim, Masters, Karen L., and Salim, Samir. Wed . "Constraining the Milky Way’s ultraviolet-to-infrared SED with Gaussian process regression". United Kingdom. https://doi.org/10.1093/mnras/stab2618.
@article{osti_1827472,
title = {Constraining the Milky Way’s ultraviolet-to-infrared SED with Gaussian process regression},
author = {Fielder, Catherine E. and Newman, Jeffrey A. and Andrews, Brett H. and Zasowski, Gail and Boardman, Nicholas F. and Licquia, Tim and Masters, Karen L. and Salim, Samir},
abstractNote = {ABSTRACT Improving our knowledge of global Milky Way (MW) properties is critical for connecting the detailed measurements only possible from within our Galaxy to our understanding of the broader galaxy population. We here train Gaussian process regression (GPR) models on SDSS (Sloan Digital Sky Survey) galaxies to map from galaxy properties (stellar mass, apparent axial ratio, star formation rate, bulge-to-total ratio, disc scale length, and bar vote fraction) to ultraviolet (UV; GALEX FUV/NUV), optical (SDSS ugriz), and infrared (IR; 2MASS JHKs and WISE W1/W2/W3/W4) fluxes and uncertainties. With these models, we estimate the photometric properties of the MW, resulting in a full UV-to-IR spectral energy distribution (SED) as it would be measured externally, viewed face-on. We confirm that the MW lies in the green valley in optical diagnostic diagrams, but show for the first time that the MW is in the star-forming region in standard UV and IR diagnostics – characteristic of the population of red spiral galaxies. Although our GPR method predicts one band at a time, the resulting MW UV–IR SED is consistent with SEDs of local spirals with characteristics broadly similar to the MW, suggesting that these independent predictions can be combined reliably. Our UV–IR SED will be invaluable for reconstructing the MW’s star formation history using the same tools employed for external galaxies, allowing comparisons of results from in situ measurements to those from the methods used for extragalactic objects.},
doi = {10.1093/mnras/stab2618},
journal = {Monthly Notices of the Royal Astronomical Society},
number = 3,
volume = 508,
place = {United Kingdom},
year = {Wed Sep 15 00:00:00 EDT 2021},
month = {Wed Sep 15 00:00:00 EDT 2021}
}

Journal Article:
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https://doi.org/10.1093/mnras/stab2618

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Inclination‐dependent Luminosity Function of Spiral Galaxies in the Sloan Digital Sky Survey: Implications for Dust Extinction
journal, April 2007

  • Shao, Zhengyi; Xiao, Quanbao; Shen, Shiyin
  • The Astrophysical Journal, Vol. 659, Issue 2
  • DOI: 10.1086/511131

SciPy 1.0: fundamental algorithms for scientific computing in Python
journal, February 2020


The spatial distribution of 10 micron luminosity in spiral galaxies
journal, December 1987

  • Devereux, Nicholas
  • The Astrophysical Journal, Vol. 323
  • DOI: 10.1086/165809

The inhibition of star formation in barred spiral galaxies
journal, April 1982

  • Tubbs, A. D.
  • The Astrophysical Journal, Vol. 255
  • DOI: 10.1086/159846

Kinematic classification of non-interacting spiral galaxies
journal, January 2014


Spectroscopic Target Selection in the Sloan Digital Sky Survey: The Main Galaxy Sample
journal, September 2002

  • Strauss, Michael A.; Weinberg, David H.; Lupton, Robert H.
  • The Astronomical Journal, Vol. 124, Issue 3
  • DOI: 10.1086/342343

Galaxy Zoo: the effect of bar-driven fuelling on the presence of an active galactic nucleus in disc galaxies
journal, March 2015

  • Galloway, Melanie A.; Willett, Kyle W.; Fortson, Lucy F.
  • Monthly Notices of the Royal Astronomical Society, Vol. 448, Issue 4
  • DOI: 10.1093/mnras/stv235

Galactic‐Field Initial Mass Functions of Massive Stars
journal, December 2003

  • Kroupa, Pavel; Weidner, Carsten
  • The Astrophysical Journal, Vol. 598, Issue 2
  • DOI: 10.1086/379105

Towards a physical picture of star formation quenching: the photometric properties of recently quenched galaxies in the Sloan Digital Sky Survey
journal, January 2013

  • Mendel, J. Trevor; Simard, Luc; Ellison, Sara L.
  • Monthly Notices of the Royal Astronomical Society, Vol. 429, Issue 3
  • DOI: 10.1093/mnras/sts489

Specific Star Formation Rate Profiles in Nearby Spiral Galaxies: Quantifying the Inside‐Out Formation of Disks
journal, April 2007

  • Munoz‐Mateos, J. C.; Gil de Paz, A.; Boissier, S.
  • The Astrophysical Journal, Vol. 658, Issue 2
  • DOI: 10.1086/511812

KINGFISH—Key Insights on Nearby Galaxies: A Far-Infrared Survey with Herschel : Survey Description and Image Atlas1
journal, December 2011

  • Kennicutt, R. C.; Calzetti, D.; Aniano, G.
  • Publications of the Astronomical Society of the Pacific, Vol. 123, Issue 910
  • DOI: 10.1086/663818

The Dependence on Environment of the Color-Magnitude Relation of Galaxies
journal, January 2004

  • Hogg, David W.; Blanton, Michael R.; Brinchmann, Jarle
  • The Astrophysical Journal, Vol. 601, Issue 1
  • DOI: 10.1086/381749

A geometric distance measurement to the Galactic center black hole with 0.3% uncertainty
journal, May 2019


The physical properties of star-forming galaxies in the low-redshift Universe
journal, July 2004


When the Milky Way turned off the lights: APOGEE provides evidence of star formation quenching in our Galaxy
journal, April 2016


The Imacs Cluster Building Survey. iv. the Log-Normal star Formation History of Galaxies
journal, May 2013

  • Gladders, Michael D.; Oemler, Augustus; Dressler, Alan
  • The Astrophysical Journal, Vol. 770, Issue 1
  • DOI: 10.1088/0004-637X/770/1/64

Astrophysically motivated bulge-disc decompositions of Sloan Digital Sky Survey galaxies: Bulge-disc decomposition of SDSS galaxies
journal, February 2012


The Apache Point Observatory Galactic Evolution Experiment (APOGEE)
journal, August 2017

  • Majewski, Steven R.; Schiavon, Ricardo P.; Frinchaboy, Peter M.
  • The Astronomical Journal, Vol. 154, Issue 3
  • DOI: 10.3847/1538-3881/aa784d

Galaxy Zoo: passive red spirals
journal, March 2010


The importance of satellite quenching for the build-up of the red sequence of present-day galaxies
journal, June 2008

  • van den Bosch, Frank C.; Aquino, Daniel; Yang, Xiaohu
  • Monthly Notices of the Royal Astronomical Society, Vol. 387, Issue 1
  • DOI: 10.1111/j.1365-2966.2008.13230.x

Modeling the Panchromatic Spectral Energy Distributions of Galaxies
journal, August 2013


Improved Estimates of the Milky Way’S Stellar mass and star Formation rate from Hierarchical Bayesian Meta-Analysis
journal, June 2015


Distribution of star formation in galactic bars as seen with H α and stacked GALEX UV imaging
journal, November 2020


Galaxy properties in different environments up to z∼ 3 in the GOODS NICMOS Survey: Galaxy properties in different environments
journal, January 2011

  • Grützbauch, Ruth; Chuter, Robert W.; Conselice, Christopher J.
  • Monthly Notices of the Royal Astronomical Society, Vol. 412, Issue 4
  • DOI: 10.1111/j.1365-2966.2010.18060.x

Green valley galaxies
journal, January 2014


AN ACCURATE NEW METHOD OF CALCULATING ABSOLUTE MAGNITUDES AND K -CORRECTIONS APPLIED TO THE SLOAN FILTER SET
journal, December 2014


The ages and metallicities of galaxies in the local universe
journal, September 2005

  • Gallazzi, Anna; Charlot, Stéphane; Brinchmann, Jarle
  • Monthly Notices of the Royal Astronomical Society, Vol. 362, Issue 1
  • DOI: 10.1111/j.1365-2966.2005.09321.x

The star Formation Efficiency in Nearby Galaxies: Measuring Where gas Forms Stars Effectively
journal, November 2008


Colors and magnitudes predicted for high redshift galaxies
journal, July 1980

  • Coleman, G. D.; Wu, C. -C.; Weedman, D. W.
  • The Astrophysical Journal Supplement Series, Vol. 43
  • DOI: 10.1086/190674

The Mira-Titan Universe. III. Emulation of the Halo Mass Function
journal, September 2020

  • Bocquet, Sebastian; Heitmann, Katrin; Habib, Salman
  • The Astrophysical Journal, Vol. 901, Issue 1
  • DOI: 10.3847/1538-4357/abac5c

Does the Milky way obey Spiral Galaxy Scaling Relations?
journal, December 2016

  • Licquia, Timothy C.; Newman, Jeffrey A.; Bershady, Matthew A.
  • The Astrophysical Journal, Vol. 833, Issue 2
  • DOI: 10.3847/1538-4357/833/2/220

The merging history of the Milky Way
journal, February 1996

  • Unavane, M.; Wyse, R. F. G.; Gilmore, G.
  • Monthly Notices of the Royal Astronomical Society, Vol. 278, Issue 3
  • DOI: 10.1093/mnras/278.3.727

The Gaia-ESO Survey: a quiescent Milky Way with no significant dark/stellar accreted disc★
journal, May 2015

  • Ruchti, G. R.; Read, J. I.; Feltzing, S.
  • Monthly Notices of the Royal Astronomical Society, Vol. 450, Issue 3
  • DOI: 10.1093/mnras/stv807

On the spiral structure of the Milky Way Galaxy
journal, February 2011


Galaxy Zoo: bars in disc galaxies★: Galaxy Zoo: bars in disc galaxies
journal, November 2010


Galaxy Zoo 2: detailed morphological classifications for 304 122 galaxies from the Sloan Digital Sky Survey
journal, September 2013

  • Willett, Kyle W.; Lintott, Chris J.; Bamford, Steven P.
  • Monthly Notices of the Royal Astronomical Society, Vol. 435, Issue 4
  • DOI: 10.1093/mnras/stt1458

The Wide-Field Infrared Survey Explorer (Wise): Mission Description and Initial On-Orbit Performance
journal, November 2010