# Proposal: KPGT_pandre_1 "Probing the origin of the stellar initial mass function: A wide-field Herschel photometric survey of nearby star-forming cloud complexes" Short name: Herschel Gould Belt survey (HGBS) # Download location: These products can also be downloaded from http://gouldbelt-herschel.cea.fr/archives. # References: + Andre, Ph., Menshchikov, A., Bontemps, S., et al. 2010, A&A, 518, L102 + Konyves, V., Andre, Ph., Men'shchikov, A., et al. 2015, A&A, 584, 91 + Marsh, K. A., Kirk, J. M., Andre, Ph., et al. 2016, MNRAS, 459, 342 + Bresnahan, D., Ward-Thompson, D., Kirk, J.M. et al. 2018, A&A, 615, A125 + Benedettini, M., Pezzuto, S., Schisano, E. et al. 2018, A&A, 619, A52 + Ladjelate, B., Andre, Ph, Konyves, V. et al. 2020, A&A, 638, A74 + Konyves, V., Andre, Ph, Arzoumanian, D. et al. 2020, 635, A34 + Di Francesco, J., Keown, J., Fallscheer, C. et al. 2020, ApJ, 904, 172 + Pezzuto, S., Benedettini, M., Di Francesco, J. et al. 2021, A&A, 645, A55 + Fiorellino, E., Elia, D., Andre, Ph. et al. 2021, MNRAS, 500, 4257 + Kirk, J. M., Ward-Thompson, D., Di Francesco, J. et al. 2024, MNRAS # Acknowledgements Every work using Herschel Gould Belt survey data should include the following acknowledgement text: This research has made use of data from the Herschel Gould Belt survey (HGBS) project (http://gouldbelt-herschel.cea.fr). The HGBS is a Herschel Key Programme jointly carried out by SPIRE Specialist Astronomy Group 3 (SAG 3), scientists of several institutes in the PACS Consortium (CEA Saclay, INAF-IFSI Rome and INAF-Arcetri, KU Leuven, MPIA Heidelberg), and scientists of the Herschel Science Center (HSC). and cite the introductory paper of the Herschel Gould Belt survey by Andre et al. (2010, A&A, 518, L102). # Description of data Several data products are provided for nine regions in the following formats: ./HGBS_Aquila - *_070.fits.gz, ... *_500.fits.gz: PACS (070, 160 um) and SPIRE (250, 350, 500 um) maps in fits format. The data reduction tools/ versions can be found in the headers. For a detailed description of the data treatment, see Konyves et al. (2015, A&A, 584, A91). - Postcard: konyves2015_aa25861-15-fig1.jpg - HGBS_aquilaM2_observed_core_catalog.txt: ASCII table of HGBS dense cores for the Aquila region, with verbose header. - HGBS_aquilaM2_derived_core_catalog.txt: ASCII table of derived core properties for the Aquila region, with verbose header. - HGBS_aquilaM2_core_blowups.pdf: Blow-up maps of all HGBS dense cores in Aquila at 70, 160, 250, 350, & 500 um, and H_2 column density. - HGBS_aquilaM2_core_SEDs.pdf: Spectral energy distributions of all HGBS dense cores in Aquila at Herschel wavelengths. - HGBS_aquilaM2_column_density_map.fits.gz and HGBS_aquilaM2_dust_temperature_map.fits.gz: H_2 column density and dust temperature maps of the Aquila region, as derived from HGBS data at nominal 500 um (36.3'') resolution (see Roy et al. 2014, A&A, 562, A138 for dust opacity assumptions). - HGBS_aquilaM2_hires_column_density_map.fits.gz: H_2 column density map of the Aquila region, as derived from HGBS data at 18.2'' resolution using the multi-resolution decomposition technique described in Appendix A of Palmeirim et al. 2013 (A&A, 550, A38). ./HGBS_TaurusL1495 - *_070.fits.gz, ... *_500.fits.gz: PACS (070, 160 um) and SPIRE (250, 350, 500 um) maps in fits format. The data reduction tools/ versions can be found in the headers. For a detailed description of the data treatment, see Marsh et al. (2016, MNRAS, 459, 342). - Postcard: marsh2016_MNRAS20162016.jpg - HGBS_taurusL1495_observed_core_catalog.txt: ASCII table of HGBS dense cores for the Taurus/L1495 region, with verbose header. - HGBS_taurusL1495_derived_core_catalog.txt: ASCII table of derived core properties for the Taurus/L1495 region, with verbose header. - HGBS_taurusL1495_core_blowups_and_SEDs.pdf: Spectral energy distributions and blow-up views of all HGBS dense cores in Taurus/L1495 at Herschel wavelengths (and in H_2 column density as well for the blow-ups). - HGBS_taurus_L1495_column_density_map.fits.gz and HGBS_taurus_L1495_dust_temperature_map.fits.gz: H_2 column density and dust temperature maps of the Taurus L1495 region, as derived from HGBS data at nominal 500 um (36.3'') resolution (see Roy et al. 2014, A&A, 562, A138 for dust opacity assumptions). - HGBS_taurus_L1495_hires_column_density_map.fits.gz: H_2 column density map of the Taurus L1495 region, as derived from HGBS data at 18.2'' resolution using the multi-resolution decomposition technique described in Appendix A of Palmeirim et al. 2013 (A&A, 550, A38). ./HGBS_CrA - *_070.fits.gz, ... *_500.fits.gz: PACS (070, 160 um) and SPIRE (250, 350, 500 um) maps in fits format. The data reduction tools/ versions can be found in the headers. For a detailed description of the data treatment, see Bresnahan et al. (2018, A&A, 615, A125). - Postcard: bresnahan2018_aa30515-17-fig2.jpg - HGBS_craNS_observed_core_catalog.txt: ASCII table of HGBS dense cores for the Corona Australis region, with verbose header. - HGBS_craNS_derived_core_catalog.txt: ASCII table of derived core properties for the Corona Australis region, with verbose header. - HGBS_craNS_core_blowups.pdf: Blow-up maps of all HGBS dense cores in Corona Australis at 70, 160, 250, 350, & 500 um, and H_2 column density. - HGBS_craNS_core_SEDs.pdf: Spectral energy distributions of all HGBS dense cores in Corona Australis at Herschel wavelengths. - HGBS_craNS_column_density_map.fits.gz and HGBS_craNS_dust_temperature_map.fits.gz: H_2 column density and dust temperature maps of the Corona Australis region, as derived from HGBS data at nominal 500 um (36.3'') resolution (see Roy et al. 2014, A&A, 562, A138 for dust opacity assumptions). - HGBS_craNS_hires_column_density_map.fits.gz: H_2 column density map of th Corona Australis region, as derived from HGBS data at 18.2'' resolution using the multi-resolution decomposition technique described in Appendix A of Palmeirim et al. 2013 (A&A, 550, A38). ./HGBS_Lupus - *_070.fits.gz, ... *_500.fits.gz: PACS (070, 160 um) and SPIRE (250, 350, 500 um) maps in fits format. The data reduction tools/ versions can be found in the headers. For a detailed description of the data treatment, see Benedettini et al. (2018, A&A, 619, A52). - Postcards: benedettini2018_aa33364-18-fig1.jpg, benedettini2018_aa33364-18-fig2.jpg, benedettini2018_aa33364-18-fig3.jpg - HGBS_lupus*_observed_core_catalog.txt: ASCII tables of HGBS dense cores for the Lupus I, III, IV regions, with verbose header. - HGBS_lupus*_derived_core_catalog.txt: ASCII tables of derived core properties for the Lupus I, III, IV regions, with verbose header. - HGBS_lupus*_core_blowups.pdf: Blow-up maps of all HGBS dense cores in the Lupus I, III, IV regions at 70, 160, 250, 350, & 500 um, and H_2 column density. - HGBS_lupus*_core_SEDs.pdf: Spectral energy distributions of all HGBS dense cores in the Lupus I, III, IV regions at Herschel wavelengths. - HGBS_lupus*_column_density_map.fits.gz and HGBS_lupus*_dust_temperature_map.fits.gz: H_2 column density and dust temperature maps of the Lupus I, III, IV regions, as derived from HGBS data at nominal 500 um (36.3'') resolution (see Roy et al. 2014, A&A, 562, A138 for dust opacity assumptions). - HGBS_lupus*_hires_column_density_map.fits.gz: H_2 column density map of the Lupus I, III, IV regions, as derived from HGBS data at 18.2'' resolution using the multi-resolution decomposition technique described in Appendix A of Palmeirim et al. 2013 (A&A, 550, A38). ./HGBS_Ophiuchus - *_070.fits.gz, ... *_500.fits.gz: PACS (070, 160 um) and SPIRE (250, 350, 500 um) maps in fits format. The data reduction tools/ versions can be found in the headers. For a detailed description of the data treatment, see Ladjelate et al. (2020, A&A, 638, A74). - Postcard: ladjelate2020_aa36442-19-fig2.jpg - HGBS_oph_L1688_observed_core_catalog.txt: ASCII table of HGBS dense cores for the Ophiuchus L1688 region, with verbose header. - HGBS_oph_L1688_derived_core_catalog.txt: ASCII table of derived core properties for the Ophiuchus L1688 region, with verbose header. - HGBS_oph_L1688_column_density_map.fits.gz and HGBS_oph_L1688_dust_temperature_map.fits.gz: H_2 column density and dust temperature maps of the Ophiuchus L1688 region, as derived from HGBS data at nominal 500 um (36.3'') resolution (see Roy et al. 2014, A&A, 562, A138 for dust opacity assumptions). - HGBS_oph_L1688_hires_column_density_map.fits.gz: H_2 column density map of the Ophiuchus L1688 region, as derived from HGBS data at 18.2'' resolution using the multi-resolution decomposition technique described in Appendix A of Palmeirim et al. 2013 (A&A, 550, A38). ./HGBS_OrionB - *_070.fits.gz, ... *_500.fits.gz: PACS (070, 160 um) and SPIRE (250, 350, 500 um) maps in fits format. The data reduction tools/ versions can be found in the headers. For a detailed description of the data treatment, see Konyves et al. (2020, A&A, 635, A34). - Postcard: konyves2020_aa34753-18-fig5.jpg - HGBS_OrionB_observed_core_catalog.txt: ASCII table of HGBS dense cores for the OrionB region, with verbose header. - HGBS_OrionB_derived_core_catalog.txt: ASCII table of derived core properties for the OrionB region, with verbose header. - HGBS_OrionB_core_blowups.pdf: Blow-up maps of all HGBS dense cores in OrionB at 70, 160, 250, 350, & 500 um, and H_2 column density. - HGBS_OrionB_core_SEDs.pdf: Spectral energy distributions of all HGBS dense cores in OrionB at Herschel wavelengths. - HGBS_OrionB_column_density_map.fits.gz and HGBS_OrionB_dust_temperature_map.fits.gz: H_2 column density and dust temperature maps of the OrionB region, as derived from HGBS data at nominal 500 um (36.3'') resolution (see Roy et al. 2014, A&A, 562, A138 for dust opacity assumptions). - HGBS_OrionB_hires_column_density_map.fits.gz: H_2 column density map of the OrionB region, as derived from HGBS data at 18.2'' resolution using the multi-resolution decomposition technique described in Appendix A of Palmeirim et al. 2013 (A&A, 550, A38). ./HGBS_Cepheus - *_070.fits.gz, ... *_500.fits.gz: PACS (070, 160 um) and SPIRE (250, 350, 500 um) maps in fits format. The data reduction tools/ versions can be found in the headers. For a detailed description of the data treatment, see Di Francesco et al. (2020, ApJ, 904, 172). - Postcards: difrancesco2020_apjabc016f1_hr.jpg, difrancesco2020_apjabc016f2_hr.jpg, difrancesco2020_apjabc016f3_hr.jpg, difrancesco2020_apjabc016f4_hr.jpg, difrancesco2020_apjabc016f5_hr.jpg - HGBS_Cep*_observed_core_catalog.txt: ASCII tables of HGBS dense cores for the Cepheus L1157, L1172, L1228, L1241, L1251 regions, with verbose header. - HGBS_Cep*_derived_core_catalog.txt: ASCII tables of derived core properties for the Cepheus L1157, L1172, L1228, L1241, L1251 regions, with verbose header. - HGBS_Cep*_core_blowups.pdf: Blow-up maps of all HGBS dense cores in the Cepheus L1157, L1172, L1228, L1241, L1251 regions at 70, 160, 250, 350, & 500 um, and H_2 column density. - HGBS_Cep*_core_SEDs.pdf: Spectral energy distributions of all HGBS dense cores in the Cepheus L1157, L1172, L1228, L1241, L1251 regions at Herschel wavelengths. - HGBS_Cep*_column_density_map.fits.gz and HGBS_Cep*_dust_temperature_map.fits.gz: H_2 column density and dust temperature maps of the Cepheus L1157, L1172, L1228, L1241, L1251 regions, as derived from HGBS data at nominal 500 um (36.3'') resolution (see Roy et al. 2014, A&A, 562, A138 for dust opacity assumptions). - HGBS_Cep*_hires_column_density_map.fits.gz: H_2 column density map of the Cepheus L1157, L1172, L1228, L1241, L1251 regions, as derived from HGBS data at 18.2'' resolution using the multi-resolution decomposition technique described in Appendix A of Palmeirim et al. 2013 (A&A, 550, A38). ./HGBS_Perseus - *_070.fits.gz, ... *_500.fits.gz: PACS (070, 160 um) and SPIRE (250, 350, 500 um) maps in fits format. The data reduction tools/ versions can be found in the headers. For a detailed description of the data treatment, see Pezzuto et al. (2021, A&A, 645, A55). - Postcard: pezzuto2021_aa36534-19-fig23.jpg - HGBS_Perseus_observed_core_catalog.txt: ASCII table of HGBS dense cores for the Perseus region, with verbose header. - HGBS_Perseus_derived_core_catalog.txt: ASCII table of derived core properties for the Perseus region, with verbose header. - HGBS_Perseus_core_blowups_and_seds.pdf: Blow-up maps of all HGBS dense cores in Perseus at 70, 160, 250, 350, & 500 um, and H_2 column density, along with their spectral energy distributions. - HGBS_Perseus_column_density_map.fits.gz and HGBS_Perseus_dust_temperature_map.fits.gz: H_2 column density and dust temperature maps of the Perseus region, as derived from HGBS data at nominal 500 um (36.3'') resolution (see Roy et al. 2014, A&A, 562, A138 for dust opacity assumptions). - HGBS_Perseus_hires_column_density_map.fits.gz: H_2 column density map of the Perseus region, as derived from HGBS data at 18.2'' resolution using the multi-resolution decomposition technique described in Appendix A of Palmeirim et al. 2013 (A&A, 550, A38). ./HGBS_Serpens - *_070.fits.gz, ... *_500.fits.gz: PACS (070, 160 um) and SPIRE (250, 350, 500 um) maps in fits format. The data reduction tools/ versions can be found in the headers. For a detailed description of the data treatment, see Fiorellino et al. (2021, MNRAS, 500, 4257). - Postcard: fiorellino2021_mnras_staa3420fig1.jpg - HGBS_Serpens_observed_core_catalog.txt: ASCII table of HGBS dense cores for the Serpens region, with verbose header. - HGBS_Serpens_derived_core_catalog.txt: ASCII table of derived core properties for the Serpens region, with verbose header. - HGBS_Serpens_column_density_map.fits.gz and HGBS_Serpens_dust_temperature_map.fits.gz: H_2 column density and dust temperature maps of the Serpens region, as derived from HGBS data at nominal 500 um (36.3'') resolution (see Roy et al. 2014, A&A, 562, A138 for dust opacity assumptions). - HGBS_Serpens_hires_column_density_map.fits.gz: H_2 column density map of the Serpens region, as derived from HGBS data at 18.2'' resolution using the multi-resolution decomposition technique described in Appendix A of Palmeirim et al. 2013 (A&A, 550, A38). ./HGBS_TaurusTMC1 - *_070.fits.gz, ... *_500.fits.gz: PACS (070, 160 um) and SPIRE (250, 350, 500 um) maps in fits format. The data reduction tools/ versions can be found in the headers. For a detailed description of the data treatment, see Kirk et al. (2024, MNRAS). - Postcard: kirk2024_mnras_fig12.jpg - HGBS_taurusTMC1_observed_core_catalog.txt: ASCII table of HGBS dense cores for the Taurus TMC1 region, with verbose header. - HGBS_taurusTMC1_derived_core_catalog.txt: ASCII table of derived core properties for the Taurus TMC1 region, with verbose header. - HGBS_taurusTMC1_core_blowups_and_SEDs.pdf: Spectral energy distributions and blow-up views of all HGBS dense cores in Taurus TMC1 at Herschel wavelengths (and in H_2 column density as well for the blow-ups). - HGBS_taurusTMC1_column_density_map.fits.gz and HGBS_taurusTMC1_dust_temperature_map.fits.gz: H_2 column density and dust temperature maps of the Taurus TMC1 region, as derived from HGBS data at nominal 500 um (36.3'') resolution (see Roy et al. 2014, A&A, 562, A138 for dust opacity assumptions). - HGBS_taurusTMC1_hires_column_density_map.fits.gz: H_2 column density map of the Taurus TMC1 region, as derived from HGBS data at 18.2'' resolution using the multi-resolution decomposition technique described in Appendix A of Palmeirim et al. 2013 (A&A, 550, A38).