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Table 1.

Sources not detected at 86 GHz.

ID MSX ID rms Obs. date
(K) (ddmmyy)
531 G020.4122−00.0703 0.010 031003
532 G020.7490−00.1120 0.008 031003
533 G022.3430+00.1438 0.010 101003
534* a G022.0265−00.2741 0.011 101003
535* a G024.6265+00.2856 0.009 121003
536 G024.8993+00.1493 0.009 121003
537 G024.4084−00.4077 0.013 121003
538 G025.1373−00.4375 0.012 121003
539 G027.0540−00.3708 0.011 211003/231003
540 G028.7480+00.2394 0.013 221003
541 G028.4568−00.1409 0.013 211003/031103
542 G028.5241−00.3361 0.013 221003
543 G029.1718−00.1392 0.011 221003
544 G029.9008+00.2034 0.014 231003
545 G030.3701+00.4129 0.013 231003
546 G029.3767−00.1393 0.013 231003
547 G029.2366−00.3039 0.013 221003
548 G031.0465+00.1522 0.012 231003
549 G031.6255+00.1417 0.012 231003
550 G033.9410+00.3822 0.013 301003
551 G033.3780−00.3974 0.014 301003
552 G034.3524+00.0414 0.014 301003
553 G034.4886+00.0030 0.014 301003
554* d G035.1766−00.1296 0.012 021103
555 G035.8117+00.1731 0.011 021103
556 G036.6828+00.4850 0.009 021103
557 G035.3035−00.3060 0.012 021103
558 G036.5733+00.2658 0.011 021103
559 G035.7171−00.3353 0.009 021103
560 G038.9702+00.2921 0.012 021103
561 G039.0025+00.0971 0.012 021103
562 G040.3720+00.0615 0.011 021103
563 G040.8270−00.4366 0.011 021103
564 G042.6920−00.0883 0.015 031103
565 G042.8776−00.1158 0.015 031103
566 G043.3079−00.1290 0.015 031103
567 G043.3686−00.3254 0.015 031103
568* a G045.0643−00.1249 0.014 031103
569 G048.1911+00.4459 0.017 031103
570 G048.1018+00.3077 0.017 031103
571 G048.1924−00.0121 0.017 031103
441* G029.5298+00.0110 0.013 231003
444* c G029.6750-00.3521 0.013 231003

Notes. (*) Alias: 534 = ISOGAL − PJ183220.6 − 094910; 535 = [NGM2010] S13; 441 = [MHS2002]441; 444 = [MHS2002] 444/[MZM2016]68; 554 = IRAS 18534+0152; 568 = ISOGAL − PJ191416.8 − 104318.

(a)

Stars #534 and #568 (non-detections) are reported as candidate YSOs by Felli et al. (2002).

(b)

Star #535 is a candidate RSG ([NGM2010]S13) in the cluster Alicante 8 (Negueruela et al. 2010).

(c)

Star #444 corresponds to MZM2016-68, an M2I (Messineo et al. 2016).

(d)

For star #554 (IRAS 18534+0152) there is an IRAS low resolution spectrum (LRS, featureless (F), Kwok et al. 1997).

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