J/A+A/688/A159ivo://CDS.VizieR/J/A+A/688/A159doi:10.26093/cds/vizier.36880159CDSKouroumpatzakis K.Svoboda J.Zezas A.Borkar A.Kyritsis E.,Boorman P.G.Daoutis C.Adamcova B.Grossova R.2024-11-21T20:02:34Z2024-08-14T07:12:31ZCDS support team

CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France

cds-question@unistra.frgalaxiesvisible-astronomyinfrared-sourcesline-intensitiesDwarf highly star-forming galaxies dominated the early Universe and are considered the main driver of its reionization. Direct observations of these very distant galaxies are limited mainly to rest-frame ultraviolet and visible wavelengths, and as a result, some of their properties are out of reach. Therefore, the study of their local analogs, the Green Pea (GP) and Blueberry (BB) galaxies is still of paramount importance. This work aims to expand the number of known BBs to smaller distances and the south equatorial sky. In addition to the already known, this new sample of BBs allows for a statistically significant study of their properties probed by visible and infrared (IR) light. We utilize HECATE, a catalog of galaxies up to 200Mpc, which provides optical/IR photometry and characterization of the sources. To select and analyze the sample, we adopt the Pan-STARSS and SDSS optical photometries, and MPA-JHU analysis for sources having spectroscopic observations. Benefited by the multiwavelength coverage, we perform spectral energy distribution fitting to provide homogeneous star-formation rates and stellar masses. The selected BBs are compared with GPs and other dwarf star- forming galaxies (SFGs). This work has identified 48 BBs out of which 40 are newly discovered. The nearest BB lies at 19Mpc while 14 BBs are in the south equatorial sky. The BBs tend to be extremely IR red in both WISE W1-W2 and W2-W3 colors, located in different positions in this diagram compared to typical SFGs. Overall, dwarf SFGs with higher specific star-formation rates tend to have redder IR colors. Although GPs and BBs share many similarities, the latter are the most intensively star-forming sources of the local Universe among dwarf galaxies. Overall BBs are intrinsically bluer in visible light, redder in the IR, less massive, have higher specific star-formation rates and equivalent widths, lower metallicities, and have the most strongly ionized interstellar medium compared to typical SFGs and GPs.2024A&A...688A.159Khttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/688/A159CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicehttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/688/A159https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/688/A159http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/688/A159https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/688/A159https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/688/A159http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/688/A159GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/A+A/688/A159/table23 (Observed g-r, and r-i colors from the different photometries, redshift, distances, sizes, stellar masses, sSFR, metallicities, EWs of the proposed Blueberry galaxies (BBs))https://vizier.cds.unistra.fr/viz-bin/conesearch/J/A+A/688/A159/table23?https://vizier.iucaa.in/viz-bin/conesearch/J/A+A/688/A159/table23?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/688/A159/table23?GETtext/xml+votable180.050000true2.41562.57180.0055555555555555560/2.85864675833786e-19 3.5010283109654867e-19https://cdsarc.cds.unistra.fr/viz-bin/moc/J/A+A/688/A159?format=asciiOpticalInfrareddefaultJ/A+A/688/A159/table23Observed g-r, and r-i colors from the different photometries, redshift, distances, sizes, stellar masses, sSFR, metallicities, EWs of the proposed Blueberry galaxies (BBs)PGCPGC ID (PGC)meta.id;meta.mainintz? Redshift SDSS MPA-JHU (z)src.redshiftdoublenullablerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintBB[1/48] In-text identification (ID)meta.idintRAJ2000Right ascension (J2000) (RAdeg)degpos.eq.ra;meta.maine_g-rPetro? SDSS MPA-JHU Petro g-r colour error (Petro_(g-r)_e)magstat.errorfloatnullableg-rKron? Pan-STARRS Kron g-r colour (Kron_(g-r))magphot.color;em.opt.B;em.opt.Rfloatnullablee_g-rKron? Pan-STARRS Kron g-r colour error (Kron_(g-r)_e)magstat.errorfloatnullableg-rPSF? Pan-STARRS PSF g-r colour (PSF_(g-r))magphot.color;em.opt.B;em.opt.Rfloatnullablee_g-rPSF? Pan-STARRS PSF g-r colour error (PSF_(g-r)_e)magstat.errorfloatnullabler-icMod? SDSS MPA-JHU model r-i colour (cModelMag_(r-i))magphot.color;em.opt.R;em.opt.Ifloatnullablee_r-icMod? SDSS MPA-JHU model r-i colour error (cModelMag_(r-i)_e)magstat.errorfloatnullabler-iPetro? SDSS MPA-JHU Petro r-i colour (Petro_(r-i))magphot.color;em.opt.R;em.opt.Idoublenullablee_r-iPetro? SDSS MPA-JHU Petro r-i colour error (Petro_(r-i)_e)magstat.errorfloatnullabler-iKron? Pan-STARRS Kron r-i colour (Kron_(r-i))magphot.color;em.opt.R;em.opt.Ifloatnullablee_r-iKron? Pan-STARRS Kron r-i colour error (Kron_(r-i)_e)magstat.errorfloatnullabler-iPSF? Pan-STARRS PSF r-i colour (PSF_(r-i))magphot.color;em.opt.R;em.opt.Ifloatnullablee_r-iPSF? Pan-STARRS PSF r-i colour error (PSF_(r-i)_e)magstat.errorfloatnullableDist? Distance based on redshift or HECATE (Dist)Mpcpos.distancefloatnullableSize? Size based on distance and major axis size (Size)kpcpos.distancefloatnullablelogMstarSED? SED fitting stellar mass (log_Mstar_SED)log(solMass)phys.massfloatnullablee_logMstarSED? SED fitting stellar mass lower error (log_Mstar_SED_el)log(solMass)stat.errorfloatnullableE_logMstarSED? SED fitting stellar mass upper error (log_Mstar_SED_eu)log(solMass)stat.error;stat.maxfloatnullablelogMstarHEC? HECATE stellar mass (log_Mstar_HEC)log(solMass)phys.massfloatnullablelogMstarMPA-JHU? SDSS MPA-JHU stellar mass (log_Mstar_MPA-JHU)log(solMass)phys.massdoublenullablee_logMstarMPA-JHU? SDSS MPA-JHU stellar mass error (log_Mstar_MPA-JHU_e)log(solMass)stat.errorfloatnullablelogSFRSED? SED fitting star formation rate (log_SFR_SED)log(solMass.yr**-1)phys.SFRfloatnullablee_logSFRSED? SED fitting star formation rate lower error (log_SFR_SED_el)log(solMass.yr**-1)stat.errorfloatnullableE_logSFRSED? SED fitting star formation rate upper error (log_SFR_SED_eu)log(solMass.yr**-1)stat.error;stat.maxfloatnullablelogSFRHEC? HECATE star formation rate (log_SFR_HEC)log(solMass.yr**-1)meta.idfloatnullablelogSFRMPA-JHU? SDSS MPA-JHU star formation rate (log_SFR_MPA-JHU)log(solMass.yr**-1)phys.SFRdoublenullablee_logSFRMPA-JHU? SDSS MPA-JHU star formation rate error (log_SFR_MPA-JHU_e)log(solMass.yr**-1)stat.errorfloatnullable12+log(O/H)? SDSS MPA-JHU 12+log(O/H) abundance (12+log(O/H))phys.abunddoublenullablee_12+log(O/H)? SDSS MPA-JHU 12+log(O/H) abundance error (12+log(O/H)_e)stat.errorfloatnullableEWOII? SDSS MPA-JHU OII_3726 equivalent width (OII_3726_EQW)0.1nmspect.line.eqWidthdoublenullablee_EWOII? SDSS MPA-JHU OII_3726 equivalent width error (OII_3726_EQW_e)0.1nmstat.errordoublenullableEWHb? SDSS MPA-JHU H{beta} equivalent width (H_BETA_EQW)0.1nmspect.line.eqWidthdoublenullablee_EWHb? SDSS MPA-JHU H{beta} equivalent width error ( e_H_BETA_EQW_e)0.1nmstat.errordoublenullableEWOIII? SDSS MPA-JHU OIII_5007 equivalent width (OIII_5007_EQW)0.1nmspect.line.eqWidthdoublenullablee_EWOIII? SDSS MPA-JHU OIII_5007 equivalent width error (OIII_5007_EQW_e)0.1nmstat.errordoublenullableEWHa? SDSS MPA-JHU H{alpha} equivalent width (H_ALPHA_EQW)0.1nmspect.line.eqWidthdoublenullablee_EWHa? SDSS MPA-JHU H{alpha} equivalent width error (H_ALPHA_EQW_e)0.1nmstat.errordoublenullablelogFHeIIFADO? FADO HeII_4686 flux (FADO_log_HeII_4686_f)log(mW.m**-2)phot.fluxfloatnullablee_logFHeIIFADO? FADO HeII_4686 flux error (FADO_log_HeII_4686_f_e)log(mW.m**-2)stat.errorfloatnullableEWHeIIFADO? FADO HeII_4686 equivalent width (FADO_HeII_4686_EW)0.1nmspect.line.eqWidthfloatnullablee_EWHeIIFADO? FADO HeII_4686 equivalent width error (FADO_HeII_4686_EW_e)0.1nmstat.errorfloatnullablee_logFOIII1FADO? FADO OIII_4959 flux error (FADO_log_OIII_4959_f_e)log(mW.m**-2)stat.errorfloatnullableEWOIII1FADO? FADO OIII_4959 equivalent width (FADO_OIII_4959_EW)0.1nmspect.line.eqWidthfloatnullablee_EWOIII1FADO? FADO OIII_4959 equivalent width error (FADO_OIII_4959_EW_e)0.1nmstat.errorfloatnullablelogFOIII2FADO? FADO OIII_5007 flux (FADO_log_OIII_5007_f)log(mW.m**-2)phot.fluxfloatnullablee_logFOIII2FADO? FADO OIII_5007 flux error (FADO_log_OIII_5007_f_e)log(mW.m**-2)stat.errorfloatnullableEWOIII2FADO? FADO OIII_5007 equivalent width (FADO_OIII_5007_EW)0.1nmspect.line.eqWidthfloatnullablee_EWOIII2FADO? FADO OIII_5007 equivalent width error (FADO_OIII_5007_EW_e)0.1nmstat.errorfloatnullablelogFOIFADO? FADO OI_6300 flux (FADO_log_OI_6300_f)log(mW.m**-2)phot.fluxfloatnullablee_logFOIFADO? FADO OI_6300 flux error (FADO_log_OI_6300_f_e)log(mW.m**-2)stat.errorfloatnullableEWOIFADO? FADO OI_6300 equivalent width (FADO_OI_6300_EW)0.1nmspect.line.eqWidthfloatnullablee_EWOIFADO? FADO OI_6300 equivalent width error (FADO_OI_6300_EW_e)0.1nmstat.errorfloatnullablelogFNII1FADO? FADO NII_6548 flux (FADO_log_NII_6548_f)log(mW.m**-2)phot.fluxfloatnullablee_logFNII1FADO? FADO NII_6548 flux error (FADO_log_NII_6548_f_e)log(mW.m**-2)stat.errordoublenullablee_EWHaFADO? FADO H{alpha} equivalent width error (FADO_H_ALPHA_EW_e)0.1nmstat.errorfloatnullablelogFNII2FADO? FADO NII_6583 flux (FADO_log_NII_6583_f)log(mW.m**-2)phot.fluxfloatnullablee_logFNII2FADO? FADO NII_6583 flux error (FADO_log_NII_6583_f_e)log(mW.m**-2)stat.errorfloatnullableEWNII2FADO? FADO NII_6583 equivalent width (FADO_NII_6583_EW)0.1nmspect.line.eqWidthfloatnullablee_EWNII2FADO? FADO NII_6583 equivalent width error (FADO_NII_6583_EW_e)0.1nmstat.errorfloatnullablelogFSII1FADO? FADO SII_6716 flux (FADO_log_SII_6716_f)log(mW.m**-2)phot.fluxfloatnullablee_logFSII1FADO? FADO SII_6716 flux error (FADO_log_SII_6716_f_e)log(mW.m**-2)stat.errorfloatnullableEWSII1FADO? FADO SII_6716 equivalent width (FADO_SII_6716_EW)0.1nmspect.line.eqWidthfloatnullablee_EWSII1FADO? FADO II_6716 equivalent width error (FADO_SII_6716_EW_e)0.1nmstat.errorfloatnullablelogFSII2FADO? FADO SII_6731 flux (FADO_log_SII_6731_f)log(mW.m**-2)phot.fluxfloatnullablee_logFSII2FADO? FADO SII_6731 flux error (FADO_log_SII_6731_f_e)log(mW.m**-2)stat.errorfloatnullableEWSII2FADO? FADO SII_6731 equivalent width (FADO_SII_6731_EW)0.1nmspect.line.eqWidthfloatnullablee_EWSII2FADO? FADO SII_6731 equivalent width error (FADO_SII_6731_EW_e)0.1nmstat.errorfloatnullableCompact[0/1] Compact? No (0) or Yes (1) by visual inspection (Compact)meta.notefloatDEJ2000Declination (J2000) (DEdeg)degpos.eq.dec;meta.mainrmagcModSDSS MPA-JHU r magnitude (cModelMag_r)magphot.mag;em.opt.Rfloate_rmagcModSDSS MPA-JHU model r magnitude error (cModelMag_r_e)magstat.errorfloatg-rcMod? SDSS MPA-JHU model g-r colour (cModelMag_(g-r))magphot.color;em.opt.B;em.opt.Rfloatnullablee_g-rcMod? SDSS MPA-JHU g-r colour error (cModelMag_(g-r)_e)magstat.errorfloatnullableg-rPetro? SDSS MPA-JHU Petro g-r colour (Petro_(g-r))magphot.color;em.opt.B;em.opt.RdoublenullablelogFHbFADO? FADO H{beta} flux (FADO_log_H_BETA_f)log(mW.m**-2)phot.fluxfloatnullablee_logFHbFADO? FADO H{beta} flux error (FADO_log_H_BETA_f_e)log(mW.m**-2)stat.errorfloatnullableEWHbFADO? FADO H{beta} flux equivalent width (FADO_H_BETA_EW)0.1nmspect.line.eqWidthfloatnullablee_EWHbFADO? FADO H{beta} flux equivalent width error (FADO_H_BETA_EW_e)0.1nmstat.errorfloatnullablelogFOIII1FADO? FADO OIII_4959 flux (FADO_log_OIII_4959_f)log(mW.m**-2)phot.fluxfloatnullableEWNII1FADO? FADO NII_6548 equivalent width (FADO_NII_6548_EW)0.1nmspect.line.eqWidthfloatnullablee_EWNII1FADO? FADO NII_6548 equivalent width error (FADO_NII_6548_EW_e)0.1nmstat.errorfloatnullablelogFHaFADO? FADO H{alpha} flux (FADO_log_H_ALPHA_f)log(mW.m**-2)phot.fluxfloatnullablee_logFHaFADO? FADO H{alpha} flux error (FADO_log_H_ALPHA_f_e)log(mW.m**-2)stat.errorfloatnullableEWHaFADO? FADO H{alpha} equivalent width (FADO_H_ALPHA_EW)0.1nmspect.line.eqWidthfloatnullable