Table B.1.
Summary of results from our optical spectroscopic campaign.
| Fermi-LAT | Fermi-LAT | Associated | WISE | RA (J2000) | Dec (J2000) | Class | z | Refs. | Telescope | Literature |
|---|---|---|---|---|---|---|---|---|---|---|
| name | class | source | counterpart | hh:mm:ss | dd:mm:ss | |||||
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) | (10) | (11) |
| 4FGL J0003.9-1149 | bll | PMN J0004-1148 | J000404.91-114858.3 | 00:04:04.91 | −11:48:58.33 | bzb | ... | d | 6dF | |
| 4FGL J0009.7-3217 | rdg | IC 1531 | J000935.55-321636.8 | 00:09:35.56 | −32:16:36.85 | bzg | 0.0254 | d | 6dF | |
| 4FGL J0015.6+5551 | bll | GB6 J0015+5551 | J001540.13+555144.7 | 00:15:40.14 | +55:51:44.77 | bzb | ... | b | KPNO | |
| 4FGL J0015.9+2440 | bcu | GB6 J0016+2440 | J001603.62+244014.7 | 00:16:03.62 | +24:40:14.77 | bzb | ... | l | OAN-SPM | |
| FL8Y J0024.1+2401 | ugs | ... | J002406.10+240438.6 | 00:24:06.10 | +24:04:38.67 | bzb | 0.062? | o | SDSS | |
| 4FGL J0023.7-6820 | bcu | PKS 0021-686 | J002406.72-682054.5 | 00:24:06.72 | −68:20:54.50 | qso | 0.354 | f | SOAR | |
| 4FGL J0028.4+2001 | fsrq | TXS 0025+197 | J002829.81+200026.7 | 00:28:29.82 | +20:00:26.77 | bzq | 1.5517 | d | SDSS DR12 | |
| 4FGL J0037.9+2612 | bll | MG3 J003720+2613 | J003719.15+261312.6 | 00:37:19.15 | +26:13:12.60 | bzg | 0.1477 | k | SDSS | |
| 4FGL J0038.7-0204 | rdg | 3C 17 | J003820.53-020740.5 | 00:38:20.53 | −02:07:40.50 | bzq | 0.2204 | k | SDSS | |
| 4FGL J0040.4-2340 | bll | PMN J0040-2340 | J004024.90-234000.7 | 00:40:24.90 | −23:40:00.70 | bzg | 0.213 | f | SOAR | |
| 4FGL J0043.5-0442 | bll | 1RXS J004333.7-044257 | J004334.12-044300.6 | 00:43:34.12 | −04:43:00.67 | bzb | ... | d | 6dF | |
| 4FGL J0043.7-1116 | bcu | 1RXS J004349.3-111612 | J004348.66-111607.2 | 00:43:48.66 | −11:16:07.23 | bzb | 0.264 | c | SOAR, NOT | h |
Notes. Column descriptions: (1) Fermi-LAT name; (2) Fermi-LAT classification; (3) Fermi-LAT low-energy counterpart association name; (4) WISE counterpart name; (5) J2000 right ascension; (6) J2000 declination; (7) spectroscopic class; (8) redshift; (10) telescope. References. (9) References to our campaign papers: a: Cowperthwaite et al. (2013); b: Álvarez Crespo et al. (2016a); c: Álvarez Crespo et al. (2016b); d: Álvarez-Crespo et al. (2016c); e: Landoni et al. (2015b); f: Marchesini et al. (2019); g: Massaro et al. (2014); h: Massaro et al. (2015d); i: Massaro et al. (2015b); j: Massaro et al. (2016); k: de Menezes et al. (2019); l: de Menezes et al. (2020b); m: Paggi et al. (2014); n: Peña-Herazo et al. (2017); o: Peña-Herazo et al. (2019); p: this work; q: Ricci et al. (2015). (11) References to spectra that were also reported in the literature: a: Desai et al. (2019); b: Falco et al. (1998); c: Jones et al. (2009); d: Hewitt & Burbidge (1980); e: Klindt et al. (2017); f: La Mura et al. (2017); g: Marchesi et al. (2018); h: Marchesini et al. (2016); i: Marlow et al. (2000); j: Martí et al. (2004); k: Masetti et al. (2013); l: Paiano et al. (2017a); m: Paiano et al. (2017b); n: Shaw et al. (2013); o: Titov et al. (2013); p: Tsarevsky et al. (2005); q: Vermeulen & Taylor (1995); r: Paiano et al. (2019).
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.