Evolution of Cold Gas at 2 < z < 5: A Blind Search for H i and OH Absorption Lines toward Mid-infrared Color-selected Radio-loud AGN

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Evolution of Cold Gas at 2 < z < 5 : A Blind Search for H i and OH Absorption Lines toward Mid-infrared Color-selected Radio-loud AGN. / Gupta, N.; Srianand, R.; Shukla, G.; Krogager, J-K; Noterdaeme, P.; Combes, F.; Dutta, R.; Fynbo, J. P. U.; Hilton, M.; Momjian, E.; Moodley, K.; Petitjean, P.

In: Astrophysical Journal Supplement Series, Vol. 255, No. 2, 28, 08.2021.

Research output: Contribution to journalJournal articleResearchpeer-review

Harvard

Gupta, N, Srianand, R, Shukla, G, Krogager, J-K, Noterdaeme, P, Combes, F, Dutta, R, Fynbo, JPU, Hilton, M, Momjian, E, Moodley, K & Petitjean, P 2021, 'Evolution of Cold Gas at 2 < z < 5: A Blind Search for H i and OH Absorption Lines toward Mid-infrared Color-selected Radio-loud AGN', Astrophysical Journal Supplement Series, vol. 255, no. 2, 28. https://doi.org/10.3847/1538-4365/ac03b5

APA

Gupta, N., Srianand, R., Shukla, G., Krogager, J-K., Noterdaeme, P., Combes, F., Dutta, R., Fynbo, J. P. U., Hilton, M., Momjian, E., Moodley, K., & Petitjean, P. (2021). Evolution of Cold Gas at 2 < z < 5: A Blind Search for H i and OH Absorption Lines toward Mid-infrared Color-selected Radio-loud AGN. Astrophysical Journal Supplement Series, 255(2), [28]. https://doi.org/10.3847/1538-4365/ac03b5

Vancouver

Gupta N, Srianand R, Shukla G, Krogager J-K, Noterdaeme P, Combes F et al. Evolution of Cold Gas at 2 < z < 5: A Blind Search for H i and OH Absorption Lines toward Mid-infrared Color-selected Radio-loud AGN. Astrophysical Journal Supplement Series. 2021 Aug;255(2). 28. https://doi.org/10.3847/1538-4365/ac03b5

Author

Gupta, N. ; Srianand, R. ; Shukla, G. ; Krogager, J-K ; Noterdaeme, P. ; Combes, F. ; Dutta, R. ; Fynbo, J. P. U. ; Hilton, M. ; Momjian, E. ; Moodley, K. ; Petitjean, P. / Evolution of Cold Gas at 2 < z < 5 : A Blind Search for H i and OH Absorption Lines toward Mid-infrared Color-selected Radio-loud AGN. In: Astrophysical Journal Supplement Series. 2021 ; Vol. 255, No. 2.

Bibtex

@article{79970a80532648af8662223eaaf41979,
title = "Evolution of Cold Gas at 2 < z < 5: A Blind Search for H i and OH Absorption Lines toward Mid-infrared Color-selected Radio-loud AGN",
abstract = "We present results from a spectroscopically blind search for associated and intervening H i 21 cm and OH 18 cm absorption lines toward 88 active galactic nuclei (AGN) at 2 2. The detection rate ( 1.6(-1.4)(+3.8) %) suggests a low covering factor of the cold neutral medium (CNM; T similar to 100 K) associated with these powerful AGN. The intervening absorption line search, with a sensitivity to detect the CNM in damped Ly alpha systems (DLAs), has comoving absorption path lengths of Delta X = 130.1 and 167.7 for HI and OH, respectively. The corresponding number of absorbers per unit comoving path length are 2. Our AGN sample is optically fainter compared to the quasars used to search for DLAs in the past. In our optical spectra obtained using SALT and NOT, we detect five intervening (redshift path similar to 9.3) and two proximate DLAs. This is slightly excessive compared to the statistics based on optically selected quasars. The nondetection of H I 21 cm absorption from these DLAs suggests a small CNM covering fraction around galaxies at z > 2.",
keywords = "FOCUS IMAGING SPECTROGRAPH, AFRICAN LARGE TELESCOPE, LYMAN-ALPHA SYSTEMS, QUASAR-GALAXY PAIRS, DIGITAL SKY SURVEY, 21-CM ABSORPTION, CM ABSORPTION, NEUTRAL HYDROGEN, CENTIMETER ABSORPTION, INTERSTELLAR-MEDIUM",
author = "N. Gupta and R. Srianand and G. Shukla and J-K Krogager and P. Noterdaeme and F. Combes and R. Dutta and Fynbo, {J. P. U.} and M. Hilton and E. Momjian and K. Moodley and P. Petitjean",
year = "2021",
month = aug,
doi = "10.3847/1538-4365/ac03b5",
language = "English",
volume = "255",
journal = "Astrophysical Journal",
issn = "0067-0049",
publisher = "Institute of Physics Publishing, Inc",
number = "2",

}

RIS

TY - JOUR

T1 - Evolution of Cold Gas at 2 < z < 5

T2 - A Blind Search for H i and OH Absorption Lines toward Mid-infrared Color-selected Radio-loud AGN

AU - Gupta, N.

AU - Srianand, R.

AU - Shukla, G.

AU - Krogager, J-K

AU - Noterdaeme, P.

AU - Combes, F.

AU - Dutta, R.

AU - Fynbo, J. P. U.

AU - Hilton, M.

AU - Momjian, E.

AU - Moodley, K.

AU - Petitjean, P.

PY - 2021/8

Y1 - 2021/8

N2 - We present results from a spectroscopically blind search for associated and intervening H i 21 cm and OH 18 cm absorption lines toward 88 active galactic nuclei (AGN) at 2 2. The detection rate ( 1.6(-1.4)(+3.8) %) suggests a low covering factor of the cold neutral medium (CNM; T similar to 100 K) associated with these powerful AGN. The intervening absorption line search, with a sensitivity to detect the CNM in damped Ly alpha systems (DLAs), has comoving absorption path lengths of Delta X = 130.1 and 167.7 for HI and OH, respectively. The corresponding number of absorbers per unit comoving path length are 2. Our AGN sample is optically fainter compared to the quasars used to search for DLAs in the past. In our optical spectra obtained using SALT and NOT, we detect five intervening (redshift path similar to 9.3) and two proximate DLAs. This is slightly excessive compared to the statistics based on optically selected quasars. The nondetection of H I 21 cm absorption from these DLAs suggests a small CNM covering fraction around galaxies at z > 2.

AB - We present results from a spectroscopically blind search for associated and intervening H i 21 cm and OH 18 cm absorption lines toward 88 active galactic nuclei (AGN) at 2 2. The detection rate ( 1.6(-1.4)(+3.8) %) suggests a low covering factor of the cold neutral medium (CNM; T similar to 100 K) associated with these powerful AGN. The intervening absorption line search, with a sensitivity to detect the CNM in damped Ly alpha systems (DLAs), has comoving absorption path lengths of Delta X = 130.1 and 167.7 for HI and OH, respectively. The corresponding number of absorbers per unit comoving path length are 2. Our AGN sample is optically fainter compared to the quasars used to search for DLAs in the past. In our optical spectra obtained using SALT and NOT, we detect five intervening (redshift path similar to 9.3) and two proximate DLAs. This is slightly excessive compared to the statistics based on optically selected quasars. The nondetection of H I 21 cm absorption from these DLAs suggests a small CNM covering fraction around galaxies at z > 2.

KW - FOCUS IMAGING SPECTROGRAPH

KW - AFRICAN LARGE TELESCOPE

KW - LYMAN-ALPHA SYSTEMS

KW - QUASAR-GALAXY PAIRS

KW - DIGITAL SKY SURVEY

KW - 21-CM ABSORPTION

KW - CM ABSORPTION

KW - NEUTRAL HYDROGEN

KW - CENTIMETER ABSORPTION

KW - INTERSTELLAR-MEDIUM

U2 - 10.3847/1538-4365/ac03b5

DO - 10.3847/1538-4365/ac03b5

M3 - Journal article

VL - 255

JO - Astrophysical Journal

JF - Astrophysical Journal

SN - 0067-0049

IS - 2

M1 - 28

ER -

ID: 276215239