DARTS/Astro Query System - SQL Search -
All the tables available for SQL Search and information on each table are listed in the Available Data page. Please see the User Guide for the usage of "SQL Search".
total 1
No. |
object_name
|
center_ra
|
center_dec
|
center_ra_b1950
|
center_dec_b1950
|
center_ecliptic_lon
|
center_ecliptic_lat
|
center_galactic_lon
|
center_galactic_lat
|
roll_angle
|
observation_start_time_mjd
|
observation_start_time
|
observation_end_time_mjd
|
observation_end_time
|
observation_id
|
exposure
|
awarded_exposure
|
xis0_exposure
|
xis1_exposure
|
xis2_exposure
|
xis3_exposure
|
xis0_observation_mode
|
xis1_observation_mode
|
xis2_observation_mode
|
xis3_observation_mode
|
hxd_observation_mode
|
hxd_coarse_clock_rate_exposure
|
hxd_first_clock_rate_exposure
|
hxd_normal_clock_rate_exposure
|
hxd_all_clock_rate_exposure
|
hxd_wam_exposure
|
quantity_of_hxd_burst
|
processing_status
|
processing_date_mjd
|
processing_date
|
public_date_mjd
|
public_date
|
distribution_date_mjd
|
distribution_date
|
processing_version
|
processing_count
|
processing_software
|
proposal_id
|
proposal_abstract
|
proposal_category
|
proposal_category_code
|
proposal_priority
|
pi_name
|
co_pi_name
|
proposal_affiliated_country
|
proposal_cycle
|
observation_type
|
proposal_title
|
main_instrument
|
has_xis_injection
|
data_access_url
|
ql_access_url
|
ql_image_url
|
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1 | A399/401 FILAMENT | 44.7475 | 13.2485 | 44.061375 | 13.049612 | 46.15841 | -3.573964 | 164.45015039 | -39.12843885 | 74.1756 | 53966.1736921296 | 2006-08-19 04:10:07 | 53969.4641666667 | 2006-08-22 11:08:24 | 801020010 | 151.0601 | 150 | 151.0601 | 151.0681 | 151.0681 | 151.0681 | 2 | 2 | 2 | 2 | 1 | 0 | 0 | 142.2036 | 142.2036 | 284.2738 | 5 | PROCESSED | 57535.3984837963 | 2016-05-27 09:33:49 | 54526 | 2008-03-01 00:00:00 | 54021.1056944444 | 2006-10-13 02:32:12 | 3.0.22.43 | 3 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 010063 | Although warm-hot intergalactic medium (WHIM) is supposed to account for most of the baryon in the Universe, its detection is extremely difficult. Here, we propose to observe the cosmological filament between clusters A399 and A401 with Suzaku. We try to detect the OVII emission line and confirm the existence of WHIM in the filament. We expect that the density of the WHIM in the filament is high, and that the detection will be easier than that in other regions in the Universe. Moreover, since the redshift of the filament is relatively high, we can discriminate between the OVII mission from the WHIM and that from our Galaxy by studying the redshift of the line. | EXTRAGALACTIC DIFFUSE SOURCES | 8 | A | YUTAKA FUJITA | JAP | 1 | AO1 | THE DETECTION OF WHIM IN THE A399/401 FILAMENT | XIS | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/801020010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '801020010'
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