Pith. sign in

REVIEW 3 cited by

Overdensity of Lyman-Break Galaxy Candidates Around Hot Dust-Obscured Galaxies

Not yet reviewed by Pith; the record is open.

Re-run · record.json Download PDF Read on arXiv ↗

This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.

SPECIMEN: schema-true, not a live event

T0 review · schema-true

One-sentence machine reading of the paper's core claim.

pith:XXXXXXXX · record.json · timestamp

arxiv 2412.04436 v1 pith:BYAUMHR6 submitted 2024-12-05 astro-ph.GA

Dejene Zewdie , Roberto J. Assef , Trystan Lambert , Chiara Mazzucchelli , S. Ilani Loubser , Manuel Aravena , Jorge González-López , Hyunsung D. Jun
show 10 more authors
Chao-Wei Tsai Daniel Stern Guodong Li Román Fernández Aranda Tanio Díaz-Santos Peter R. M. Eisenhardt Andrey Vayner Lee R. Martin Andrew W. Blain Jingwen Wu
This is my paper · ORCID
classification astro-ph.GA
keywords deltadogsaroundcandidatesgalaxyoverdensitieswisecatalog
verification ladder T0 review T1 audit T2 compute T3 formal

Signed reviews

No signed human review yet.

0 comments
abstract

Hot dust-obscured galaxies (Hot DOGs), are a family of hyper-luminous, heavily obscured quasars. A number of studies have shown that these objects reside in significantly overdense regions of the Universe based on the identification of companions at optical through far-IR wavelengths. Here we present further characterization of their environments by studying the surface density of Lyman break galaxy (LBG) candidates in the vicinity of three Hot DOGs. For two of them, WISE J041010.60-091305.2 at z=3.631 and WISE J083153.25+014010.8 at z=3.912, we identify the candidate LBG companions using deep observations obtained with Baade/IMACS. For the third, WISE J224607.56-052634.9 at z=4.601, we re-analyse previously published data obtained with Gemini-S/GMOS-S. We optimise the LBG photometric selection criteria at the redshift of each target using the COSMOS2020 catalog. When comparing the density of LBG candidates found in the vicinity of these Hot DOGs with that in the COSMOS2020 catalog, we find overdensities of $\delta=1.83\pm 0.08$ ($\delta' = 7.49\pm 0.68$), $\delta=4.67\pm 0.21$ ($\delta' = 29.17\pm 2.21$), and $\delta = 2.36\pm 0.25$ ($\delta' = 11.60\pm 1.96$) around W0410-0913, W0831+0140, and W2246-0526, respectively, without (with) contamination correction. Additionally, we find that the overdensities are centrally concentrated around each Hot DOG. Our analysis also reveals that the overdensity of the fields surrounding W0410-0913 and W0831+0140 declines steeply beyond physical scales of $\sim$2 Mpc. If these overdensities evolve to clusters by z=0, these results suggest that the Hot DOG may correspond to the early formation stages of the brightest cluster galaxy. We were unable to determine if this is also the case for W2246-0526 due to the smaller field of view of the GMOS-S observations. Our results imply that Hot DOGs may be excellent tracers of protoclusters.

Discussion (0). Continue with ORCID to comment.

Forward citations

Cited by 3 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Evidence for universal gas depletion in a sample of 41 luminous Type 1 quasars at z $\sim$ 2

    astro-ph.GA 2025-05 conditional novelty 6.0 of 10

    Luminous unobscured quasars at z~2 have molecular gas fractions of 2-32 percent, generally lower than those of inactive galaxies and obscured quasars, supporting an obscured-to-unobscured evolutionary sequence.

  2. Multi-Component Ionized Gas Outflows in a Hot Dust-Obscured Galaxy W2026+0716 with Keck/OSIRIS

    astro-ph.GA 2025-04 conditional novelty 6.0 of 10

    W2026+0716 hosts a multi-component, likely biconical ionized gas outflow in which [O III] and H-alpha trace separated spatial regions with deprojected outflow velocities near 3210 and 2310 km/s.

  3. Powerful nuclear outflows and circumgalactic medium shocks driven by the most luminous known obscured quasar in the Universe

    astro-ph.GA 2024-12 conditional novelty 6.0 of 10

    JWST observations of the most luminous obscured quasar at z=4.6 reveal a 10 kpc shock-excited nebula and a 13,000 km/s nuclear outflow whose energy budget can account for the large-scale turbulence and shocks.

Reference graph

Works this paper leans on

75 extracted references · 36 canonical work pages · cited by 3 Pith papers

  1. [1]

    E., Springel, V ., White, S

    Angulo, R. E., Springel, V ., White, S. D. M., et al. 2012, MNRAS, 425, 2722

    work page 2012

  2. [2]

    2002, MNRAS, 329, 355

    Arnouts, S., Moscardini, L., Vanzella, E., et al. 2002, MNRAS, 329, 355

    2002

  3. [3]

    J., Bauer, F

    Assef, R. J., Bauer, F. E., Blain, A. W., et al. 2022, ApJ, 934, 101

    work page 2022

  4. [4]

    J., Brightman, M., Walton, D

    Assef, R. J., Brightman, M., Walton, D. J., et al. 2020, ApJ, 897, 112

    work page 2020

  5. [5]

    J., Eisenhardt, P

    Assef, R. J., Eisenhardt, P. R. M., Stern, D., et al. 2015, ApJ, 804, 27

    work page 2015

  6. [6]

    J., Walton, D

    Assef, R. J., Walton, D. J., Brightman, M., et al. 2016, ApJ, 819, 111 Bañados, E., Venemans, B., Walter, F., et al. 2013, ApJ, 773, 178 Bañados, E., Venemans, B. P., Mazzucchelli, C., et al. 2018, Nature, 553, 473

    work page 2016

  7. [7]

    2017, A&A, 606, A23

    Balmaverde, B., Gilli, R., Mignoli, M., et al. 2017, A&A, 606, A23

    work page 2017

  8. [8]

    & Arnouts, S

    Bertin, E. & Arnouts, S. 1996, A&AS, 117, 393

    1996

Show all 75 references
  1. [9]

    2002, in Astronomical Society of the Pacific Conference Series, V ol

    Bertin, E., Mellier, Y ., Radovich, M., et al. 2002, in Astronomical Society of the Pacific Conference Series, V ol. 281, Astronomical Data Analysis Software and Systems XI, ed. D. A. Bohlender, D. Durand, & T. H. Handley, 228

    2002

  2. [10]

    Bosman, S. E. I., Kakiichi, K., Meyer, R. A., et al. 2020, ApJ, 896, 49

    2020

  3. [11]

    B., van Dokkum, P

    Brammer, G. B., van Dokkum, P. G., & Coppi, P. 2008, ApJ, 686, 1503

    2008

  4. [12]

    Burgasser, A. J. 2014, in Astronomical Society of India Conference Series, V ol. 11, Astronomical Society of India Conference Series, 7–16 Article number, page 13 of 14 A&A proofs: manuscript no. IMACS_V olume2

    2014

  5. [13]

    & Kurucz, R

    Castelli, F. & Kurucz, R. L. 2004, A&A, 419, 725

    2004

  6. [14]

    B., Casey, C

    Champagne, J. B., Casey, C. M., Finkelstein, S. L., et al. 2023, ApJ, 952, 99

    2023

  7. [15]

    D., Wu, C

    Coleman, G. D., Wu, C. C., & Weedman, D. W. 1980, ApJS, 43, 393

    1980

  8. [16]

    M., Boyle, B

    Croom, S. M., Boyle, B. J., Shanks, T., et al. 2005, MNRAS, 356, 415

    2005

  9. [17]

    M., Shiralilou, B., et al

    Dayal, P., Rossi, E. M., Shiralilou, B., et al. 2019, MNRAS, 486, 2336 Díaz-Santos, T., Assef, R. J., Blain, A. W., et al. 2018, Science, 362, 1034 Díaz-Santos, T., Assef, R. J., Blain, A. W., et al. 2016, ApJ, 816, L6

    2019

  10. [18]

    Eisenhardt, P. R. M., Wu, J., Tsai, C.-W., et al. 2012, ApJ, 755, 173

    2012

  11. [19]

    P., et al

    Erben, T., Schirmer, M., Dietrich, J. P., et al. 2005, Astronomische Nachrichten, 326, 432

    2005

  12. [20]

    F., Han, Y ., & Knudsen, K

    Fan, L., Jones, S. F., Han, Y ., & Knudsen, K. K. 2017, PASP, 129, 124101

    2017

  13. [21]

    Fan, X., Bañados, E., & Simcoe, R. A. 2023, ARA&A, 61, 373

    2023

  14. [22]

    T., et al

    Finnerty, L., Larson, K., Soifer, B. T., et al. 2020, ApJ, 905, 16 Gaia Collaboration, Vallenari, A., Brown, A. G. A., et al. 2023, A&A, 674, A1 García-Vergara, C., Hennawi, J. F., Barrientos, L. F., & Arrigoni Battaia, F. 2019, ApJ, 886, 79 García-Vergara, C., Hennawi, J. F.,...

    2020

  15. [23]

    2022, Nature Communications, 13, 4574

    Ginolfi, M., Piconcelli, E., Zappacosta, L., et al. 2022, Nature Communications, 13, 4574

    2022

  16. [24]

    2016, ApJ, 821, 123

    Harikane, Y ., Ouchi, M., Ono, Y ., et al. 2016, ApJ, 821, 123

    2016

  17. [25]

    C., Mosteller, F., & Tukey, J

    Hoaglin, D. C., Mosteller, F., & Tukey, J. W. 1983, Understanding robust and exploratory data anlysis

    1983

  18. [26]

    N., Stanway, E

    Husband, K., Bremer, M. N., Stanway, E. R., et al. 2013, MNRAS, 432, 2869

    2013

  19. [27]

    J., et al

    Ilbert, O., Arnouts, S., McCracken, H. J., et al. 2006, A&A, 457, 841

    2006

  20. [28]

    2020, ARA&A, 58, 27

    Inayoshi, K., Visbal, E., & Haiman, Z. 2020, ARA&A, 58, 27

    2020

  21. [29]

    T., Venemans, B

    Intema, H. T., Venemans, B. P., Kurk, J. D., et al. 2006, A&A, 456, 433

    2006

  22. [30]

    F., Blain, A

    Jones, S. F., Blain, A. W., Assef, R. J., et al. 2017, MNRAS, 469, 4565

    2017

  23. [31]

    F., Blain, A

    Jones, S. F., Blain, A. W., Stern, D., et al. 2014, MNRAS, 443, 146

    2014

  24. [32]

    D., Assef, R

    Jun, H. D., Assef, R. J., Bauer, F. E., et al. 2020, ApJ, 888, 110

    2020

  25. [33]

    2007, ApJ, 663, 765

    Kashikawa, N., Kitayama, T., Doi, M., et al. 2007, ApJ, 663, 765

    2007

  26. [34]

    2009, ApJ, 695, 809

    Kim, S., Stiavelli, M., Trenti, M., et al. 2009, ApJ, 695, 809

    2009

  27. [35]

    S., Assef, R

    Lambert, T. S., Assef, R. J., Mazzucchelli, C., et al. 2024, arXiv e-prints, arXiv:2402.06870

    2024 arXiv

  28. [36]

    Landy, S. D. & Szalay, A. S. 1993, ApJ, 412, 64

    1993

  29. [37]

    Y ., et al

    Lee, K.-S., Giavalisco, M., Gnedin, O. Y ., et al. 2006, ApJ, 642, 63

    2006

  30. [38]

    J., Tsai, C.-W., et al

    Li, G., Assef, R. J., Tsai, C.-W., et al. 2024, arXiv e-prints, arXiv:2405.20479

    2024 arXiv

  31. [39]

    2007, ApJ, 665, 187

    Li, Y ., Hernquist, L., Robertson, B., et al. 2007, ApJ, 665, 187

    2007

  32. [40]

    2022, ApJ, 935, 80

    Luo, Y ., Fan, L., Zou, H., et al. 2022, ApJ, 935, 80

    2022

  33. [41]

    H., Vernet, J., De Breuck, C., et al

    Mayo, J. H., Vernet, J., De Breuck, C., et al. 2012, A&A, 539, A33

    2012

  34. [42]

    2017, ApJ, 834, 83

    Mazzucchelli, C., Bañados, E., Decarli, R., et al. 2017, ApJ, 834, 83

    2017

  35. [43]

    2020, A&A, 642, L1

    Mignoli, M., Gilli, R., Decarli, R., et al. 2020, A&A, 642, L1

    2020

  36. [44]

    K., Overzier, R

    Miley, G. K., Overzier, R. A., Tsvetanov, Z. I., et al. 2004, Nature, 427, 47

    2004

  37. [45]

    2014, A&A, 568, A1

    Morselli, L., Mignoli, M., Gilli, R., et al. 2014, A&A, 568, A1

    2014

  38. [46]

    2018, ApJ, 859, 38

    Noirot, G., Stern, D., Mei, S., et al. 2018, ApJ, 859, 38

    2018

  39. [47]

    P., Taniguchi, Y ., et al

    Ota, K., Venemans, B. P., Taniguchi, Y ., et al. 2018, ApJ, 856, 109

    2018

  40. [48]

    2001, ApJ, 558, L83

    Ouchi, M., Shimasaku, K., Okamura, S., et al. 2001, ApJ, 558, L83

    2001

  41. [49]

    2004, ApJ, 611, 660

    Ouchi, M., Shimasaku, K., Okamura, S., et al. 2004, ApJ, 611, 660

    2004

  42. [50]

    A., Bouwens, R

    Overzier, R. A., Bouwens, R. J., Cross, N. J. G., et al. 2008, ApJ, 673, 143

    2008

  43. [51]

    A., Guo, Q., Kauffmann, G., et al

    Overzier, R. A., Guo, Q., Kauffmann, G., et al. 2009, MNRAS, 394, 577

    2009

  44. [52]

    & Eales, S

    Roche, N. & Eales, S. A. 1999, MNRAS, 307, 703

    1999

  45. [53]

    2013, ApJS, 209, 21

    Schirmer, M. 2013, ApJS, 209, 21

    2013

  46. [54]

    2007, ApJS, 172, 1

    Scoville, N., Aussel, H., Brusa, M., et al. 2007, ApJS, 172, 1

    2007

  47. [55]

    E., Steidel, C

    Shapley, A. E., Steidel, C. C., Pettini, M., & Adelberger, K. L. 2003, ApJ, 588, 65

    2003

  48. [56]

    1982, MNRAS, 200, 115

    Soltan, A. 1982, MNRAS, 200, 115

    1982

  49. [57]

    C., Adelberger, K

    Steidel, C. C., Adelberger, K. L., Shapley, A. E., et al. 2003, ApJ, 592, 728

    2003

  50. [58]

    B., Assef, R

    Stern, D., Lansbury, G. B., Assef, R. J., et al. 2014, ApJ, 794, 102

    2014

  51. [59]

    & Miller, A

    Tachibana, Y . & Miller, A. A. 2018, PASP, 130, 128001

    2018

  52. [60]

    L., Stubbs, C

    Tonry, J. L., Stubbs, C. W., Lykke, K. R., et al. 2012, ApJ, 750, 99

    2012

  53. [61]

    Tsai, C.-W., Eisenhardt, P. R. M., Jun, H. D., et al. 2018, ApJ, 868, 15

    2018

  54. [62]

    Tsai, C.-W., Eisenhardt, P. R. M., Wu, J., et al. 2015, ApJ, 805, 90

    2015

  55. [63]

    2018, PASJ, 70, S32

    Uchiyama, H., Toshikawa, J., Kashikawa, N., et al. 2018, PASJ, 70, S32

    2018

  56. [64]

    2010, ApJ, 721, 1680

    Utsumi, Y ., Goto, T., Kashikawa, N., et al. 2010, ApJ, 721, 1680

    2010

  57. [65]

    P., Kurk, J

    Venemans, B. P., Kurk, J. D., Miley, G. K., et al. 2002, ApJ, 569, L11

    2002

  58. [66]

    P., Röttgering, H

    Venemans, B. P., Röttgering, H. J. A., Miley, G. K., et al. 2007, A&A, 461, 823

    2007

  59. [67]

    P., Röttgering, H

    Venemans, B. P., Röttgering, H. J. A., Overzier, R. A., et al. 2004, A&A, 424, L17

    2004

  60. [68]

    2021, ApJ, 907, L1

    Wang, F., Yang, J., Fan, X., et al. 2021, ApJ, 907, L1

    2021

  61. [69]

    R., Kauffmann, O

    Weaver, J. R., Kauffmann, O. B., Ilbert, O., et al. 2022, ApJS, 258, 11

    2022

  62. [70]

    L., Eisenhardt, P

    Wright, E. L., Eisenhardt, P. R. M., Mainzer, A. K., et al. 2010, AJ, 140, 1868

    2010

  63. [71]

    2012, ApJ, 756, 96

    Wu, J., Tsai, C.-W., Sayers, J., et al. 2012, ApJ, 756, 96

    2012

  64. [72]

    2013, ApJ, 769, 79

    Wylezalek, D., Galametz, A., Stern, D., et al. 2013, ApJ, 769, 79

    2013

  65. [73]

    2006, ApJ, 653, 988

    Yoshida, M., Shimasaku, K., Kashikawa, N., et al. 2006, ApJ, 653, 988

    2006

  66. [74]

    J., Mazzucchelli, C., et al

    Zewdie, D., Assef, R. J., Mazzucchelli, C., et al. 2023, A&A, 677, A54

    2023

  67. [75]

    A., Bouwens, R

    Zheng, W., Overzier, R. A., Bouwens, R. J., et al. 2006, ApJ, 640, 574 Article number, page 14 of 14

    2006

Pith tools