The Taurus Boundary of Stellar/Substellar (TBOSS) Survey - I. Far-IR disk emission measured with Herschel

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Volume 570 (October 2014)

A&A, 570 (2014) A29

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Issue		A&A Volume 570, October 2014


Article Number		A29
Number of page(s)		34
Section		Interstellar and circumstellar matter
DOI		https://doi.org/10.1051/0004-6361/201323088
Published online		10 October 2014

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8. Compilation of literature flux densities

The compilation of flux densities from optical-millimeter wavelength of the known 154 M4-L0 Taurus members is given in Tables A.1–A.4. Table A.1 lists the R_C, I_C, and 2MASS JHK_S flux densities. Table A.2 lists the Spitzer IRAC, MIPS-1, and WISE All-Sky Data release flux densities. Table A.3 lists the Herschel PACS, and Spitzer MIPS-2 flux densities. Table A.4 lists the submillimeter and millimeter (350 μm–2.6 mm) flux densities. The tables are only available at the CDS.

Appendix A: Herschel PACS maps

The Herschel PACS maps of the detected targets observed under this program shown in Figs. A.1–A.7, and are displayed in order of spectral class and type. Target name and spectral type are labeled in the top left-hand corner of each map. Both the blue channel (70 μm) and red channel (160 μm) maps are 60″ in size along each axis. In each map the black star indicates the 2MASS position of the target. The 2MASS positions of known multiple companions are indicted by yellow triangles in the blue channel maps, and green triangles in the red channel maps. The scale bar shows the intensity of each map in units of mJy/pixel. Contour levels begin at 3σ in all maps and are plotted at intervals depending on the source brightness. The PACS beam size is represented by the blue circle in the lower, right-hand corner of each map.

	Fig. A.1 Class I objects with PACS blue and red channel detections.
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	Fig. A.2 Class II objects with PACS blue and red channel detections.
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	Fig. A.3 Class II objects with PACS blue and red channel detections.
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	Fig. A.4 Class II objects with PACS blue and red channel detections.
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	Fig. A.5 Class II objects with PACS blue and red channel detections.
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	Fig. A.6 Class II objects with PACS blue channel detections only.
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	Fig. A.7 Class III objects with PACS blue and/or red channel detections.
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Appendix B: SEDs of the TBOSS sample – Class I objects

The SEDs for Class I objects of the TBOSS sample are shown in Fig. B.1. As IRAS 04191+1523 B is unresolved from IRAS 04191+1523 A with Herschel PACS, the SED(s) for this category of system(s) is shown in Fig. C.1.

Fig. B.1

SEDs of the TBOSS of the Class I objects. The target name, spectral type, and spectral class are labeled in each SED. The observed broadband photometry is compiled from optical (R_C, I_C), and near-IR (2MASS; JHK_S) wavelengths (black points), the mid-IR (IRAC and WISE; green and purple open circles respectively), the far-IR (MIPS, PACS blue and red channels; green open circles, blue and red points respectively) and submm-mm wavelengths (black points). 3σ upper limits are represented by the downwards triangles. The best-fit atmospheric model are displayed for each target.

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Appendix C: SEDs of the TBOSS sample – Class II objects

The additional SEDs for the Class II objects of the TBOSS sample are shown in Figs. C.1–C.4. Figure C.1 shows the targets that are in multiple systems of which are unresolved with Herschel PACS. Figures C.2 and C.3 shows the SEDs the Class II objects that are detected with Herschel PACS. Finally, Fig. C.4 shows the SEDs of the Class II objects that were undetected with Herschel PACS.

Fig. C.1

SEDs of the four known TBOSS Class I and/or Class II multiple systems for which the system broadband photometry and the combined atmospheric models of each system component are shown. The system name, component spectral types, and spectral classes are labeled in each SED. The observed broadband photometry is compiled from optical (R_C, I_C), and near-IR (2MASS; JHK_S) wavelengths (black points), the mid-IR (IRAC and WISE; green and purple open circles respectively), the far-IR (MIPS, PACS blue and red channels; green open circles, blue and red points respectively) and submm-mm wavelengths (black points). 3σ upper limits are represented by the downwards triangles. The best-fit atmospheric model are displayed for each target.

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Fig. C.2

SEDs of the detected Class II objects with spectral types M4-M5.5. The target name, spectral type, and spectral class are labeled in each SED. The observed broadband photometry is compiled from optical (R_C, I_C), and near-IR (2MASS; JHK_S) wavelengths (black points), the mid-IR (IRAC and WISE; green and purple open circles respectively), the far-IR (MIPS, PACS blue and red channels; green open circles, blue and red points respectively) and submm-mm wavelengths (black points). 3σ upper limits are represented by the downwards triangles. The best-fit atmospheric model are displayed for each target.

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Fig. C.3

SEDs of the detected Class II objects with spectral types M5.6-M9. The target name, spectral type, and spectral class are labeled in each SED. The observed broadband photometry is compiled from optical (R_C, I_C), and near-IR (2MASS; JHK_S) wavelengths (black points), the mid-IR (IRAC and WISE; green and purple open circles respectively), the far-IR (MIPS, PACS blue and red channels; green open circles, blue and red points respectively) and submm-mm wavelengths (black points). 3σ upper limits are represented by the downwards triangles. The best-fit atmospheric model are displayed for each target.

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Fig. C.4

SEDs of the undetected Class II objects with spectral types spanning M4.25-M9. The target name, spectral type, and spectral class are labeled in each SED. The observed broadband photometry is compiled from optical (R_C, I_C), and near-IR (2MASS; JHK_S) wavelengths (black points), the mid-IR (IRAC and WISE; green and purple open circles respectively), the far-IR (MIPS, PACS blue and red channels; green open circles, blue and red points respectively) and submm-mm wavelengths (black points). 3σ upper limits are represented by the downwards triangles. The best-fit atmospheric model are displayed for each target. The gray cross shows level of the artificial detection generated from combined Class II (70 μm) upper limit maps, and similarly the gray downward arrow shows the 160 μm upper limit from the combined maps.

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Appendix D: SEDs of the TBOSS sample – Class III objects

The SEDs for the Class III objects of the TBOSS sample that are undetected with Herschel PACS are shown in Figs. D.1–D.4.

Fig. D.1

SEDs of the undetected Class III objects with spectral types spanning M4-M5. Additionally, the known M4.5 member – XEST 26-052 – for which no far-IR observations exist, is also included within the panel. The target name, spectral type, and spectral class are labeled in each SED. The observed broadband photometry is compiled from optical (R_C, I_C), and near-IR (2MASS; JHK_S) wavelengths (black points), the mid-IR (IRAC and WISE; green and purple open circles respectively), the far-IR (MIPS, PACS blue and red channels; green open circles, blue and red points respectively) and submm-mm wavelengths (black points). 3σ upper limits are represented by the downwards triangles. The best-fit atmospheric model are displayed for each target.

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Fig. D.2

SEDs of the undetected Class III objects with spectral types spanning M5-M6.25. The target name, spectral type, and spectral class are labeled in each SED. The observed broadband photometry is compiled from optical (R_C, I_C), and near-IR (2MASS; JHK_S) wavelengths (black points), the mid-IR (IRAC and WISE; green and purple open circles respectively), the far-IR (MIPS, PACS blue and red channels; green open circles, blue and red points respectively) and submm-mm wavelengths (black points). 3σ upper limits are represented by the downwards triangles. The best-fit atmospheric model are displayed for each target.

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Fig. D.3

SEDs of the undetected Class III objects with spectral types spanning M6.25-M7.75. The target name, spectral type, and spectral class are labeled in each SED. The observed broadband photometry is compiled from optical (R_C, I_C), and near-IR (2MASS; JHK_S) wavelengths (black points), the mid-IR (IRAC and WISE; green and purple open circles respectively), the far-IR (MIPS, PACS blue and red channels; green open circles, blue and red points respectively) and submm-mm wavelengths (black points). 3σ upper limits are represented by the downwards triangles. The best-fit atmospheric model are displayed for each target.

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Fig. D.4

SEDs of the undetected Class III objects with spectral types spanning M7.75-L0. The target name, spectral type, and spectral class are labeled in each SED. The observed broadband photometry is compiled from optical (R_C, I_C), and near-IR (2MASS; JHK_S) wavelengths (black points), the mid-IR (IRAC and WISE; green and purple open circles respectively), the far-IR (MIPS, PACS blue and red channels; green open circles, blue and red points respectively) and submm-mm wavelengths (black points). 3σ upper limits are represented by the downwards triangles. The best-fit atmospheric model are displayed for each target.

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© ESO, 2014

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