Table 2.
Open in new tab

Galactic Plane surveys used in this study: survey name, wavelength and beam size, 1σ sensitivity, longitude (ℓ) and latitude (b) coverage, and reference.

SurveyWavelengths |$\&$| BeamSensitivityℓ coverageb coverageReference
(mJy beam−1)°°
CORNISH5 |$\rm GHz$||$\&$| 1.5″0.4 (1σ)10< l < 65°|b|< 1°1
MAGPIS20|$\, \rm cm$||$\&$| 6|$^{^{\prime \prime }}$|∼0.3 (1σ)10<l<32°|b| < 0.8°2
THOR1 − 2 |$\rm GHz$||$\&$| 10 − 25″0.3 − 1 (1σ)14.0|$\lt \,$|l|$\, \lt$|37.9°|$\&$| 47.1< l <51.2°|b| ≤ 1°3
White200520 |$\rm cm$||$\&$| 6|$^{^{\prime \prime }}$|∼0.9 (1σ)10< l < 39°|b| < 1°4
39≤ l < 65°|b| < 0.8°
Total overlapping sky regionl  = 10 − 39°,47.1 − 51.2°|$\&$||b| < 1°
l  = 39.0 − 65°|$\&$||b| < 0.8°
Hi-GAL250 |${\mu{\rm m}}$||$\&$| 18″∼ 12.8 (1σ)|l| ≤ 60°|b| ≤ 1°5
ATLASGAL|$870\, {\mu} {\rm m}$||$\&$| 19″∼50 − 70 (1σ)-60< l < 60°|b| < 1.5°6
SurveyWavelengths |$\&$| BeamSensitivityℓ coverageb coverageReference
(mJy beam−1)°°
CORNISH5 |$\rm GHz$||$\&$| 1.5″0.4 (1σ)10< l < 65°|b|< 1°1
MAGPIS20|$\, \rm cm$||$\&$| 6|$^{^{\prime \prime }}$|∼0.3 (1σ)10<l<32°|b| < 0.8°2
THOR1 − 2 |$\rm GHz$||$\&$| 10 − 25″0.3 − 1 (1σ)14.0|$\lt \,$|l|$\, \lt$|37.9°|$\&$| 47.1< l <51.2°|b| ≤ 1°3
White200520 |$\rm cm$||$\&$| 6|$^{^{\prime \prime }}$|∼0.9 (1σ)10< l < 39°|b| < 1°4
39≤ l < 65°|b| < 0.8°
Total overlapping sky regionl  = 10 − 39°,47.1 − 51.2°|$\&$||b| < 1°
l  = 39.0 − 65°|$\&$||b| < 0.8°
Hi-GAL250 |${\mu{\rm m}}$||$\&$| 18″∼ 12.8 (1σ)|l| ≤ 60°|b| ≤ 1°5
ATLASGAL|$870\, {\mu} {\rm m}$||$\&$| 19″∼50 − 70 (1σ)-60< l < 60°|b| < 1.5°6

Note. Reference: 1, Hoare et al. (2012); Purcell et al. (2013); 2, Helfand et al. (2006); 3, Bihr et al. (2016); Beuther et al. (2016); 4, White et al. (2005); 5, Molinari et al. (2010); 6, Schuller et al. (2009).

Table 2.
Open in new tab

Galactic Plane surveys used in this study: survey name, wavelength and beam size, 1σ sensitivity, longitude (ℓ) and latitude (b) coverage, and reference.

SurveyWavelengths |$\&$| BeamSensitivityℓ coverageb coverageReference
(mJy beam−1)°°
CORNISH5 |$\rm GHz$||$\&$| 1.5″0.4 (1σ)10< l < 65°|b|< 1°1
MAGPIS20|$\, \rm cm$||$\&$| 6|$^{^{\prime \prime }}$|∼0.3 (1σ)10<l<32°|b| < 0.8°2
THOR1 − 2 |$\rm GHz$||$\&$| 10 − 25″0.3 − 1 (1σ)14.0|$\lt \,$|l|$\, \lt$|37.9°|$\&$| 47.1< l <51.2°|b| ≤ 1°3
White200520 |$\rm cm$||$\&$| 6|$^{^{\prime \prime }}$|∼0.9 (1σ)10< l < 39°|b| < 1°4
39≤ l < 65°|b| < 0.8°
Total overlapping sky regionl  = 10 − 39°,47.1 − 51.2°|$\&$||b| < 1°
l  = 39.0 − 65°|$\&$||b| < 0.8°
Hi-GAL250 |${\mu{\rm m}}$||$\&$| 18″∼ 12.8 (1σ)|l| ≤ 60°|b| ≤ 1°5
ATLASGAL|$870\, {\mu} {\rm m}$||$\&$| 19″∼50 − 70 (1σ)-60< l < 60°|b| < 1.5°6
SurveyWavelengths |$\&$| BeamSensitivityℓ coverageb coverageReference
(mJy beam−1)°°
CORNISH5 |$\rm GHz$||$\&$| 1.5″0.4 (1σ)10< l < 65°|b|< 1°1
MAGPIS20|$\, \rm cm$||$\&$| 6|$^{^{\prime \prime }}$|∼0.3 (1σ)10<l<32°|b| < 0.8°2
THOR1 − 2 |$\rm GHz$||$\&$| 10 − 25″0.3 − 1 (1σ)14.0|$\lt \,$|l|$\, \lt$|37.9°|$\&$| 47.1< l <51.2°|b| ≤ 1°3
White200520 |$\rm cm$||$\&$| 6|$^{^{\prime \prime }}$|∼0.9 (1σ)10< l < 39°|b| < 1°4
39≤ l < 65°|b| < 0.8°
Total overlapping sky regionl  = 10 − 39°,47.1 − 51.2°|$\&$||b| < 1°
l  = 39.0 − 65°|$\&$||b| < 0.8°
Hi-GAL250 |${\mu{\rm m}}$||$\&$| 18″∼ 12.8 (1σ)|l| ≤ 60°|b| ≤ 1°5
ATLASGAL|$870\, {\mu} {\rm m}$||$\&$| 19″∼50 − 70 (1σ)-60< l < 60°|b| < 1.5°6

Note. Reference: 1, Hoare et al. (2012); Purcell et al. (2013); 2, Helfand et al. (2006); 3, Bihr et al. (2016); Beuther et al. (2016); 4, White et al. (2005); 5, Molinari et al. (2010); 6, Schuller et al. (2009).

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