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 | FILAMENT OF GALAXIES | 238.2847 | 27.6247 | 237.767937 | 27.772087 | 227.420415 | 46.484967 | 44.49442625 | 49.89393343 | 305.997 | 55408.8620833333 | 2010-07-31 20:41:24 | 55410.6883101852 | 2010-08-02 16:31:10 | 805030010 | 61.7703 | 80 | 61.7703 | 61.7703 | 0 | 61.7703 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 55.5833 | 55.5833 | 157.7518 | 0 | PROCESSED | 57552.8205671296 | 2016-06-13 19:41:37 | 55793 | 2011-08-20 00:00:00 | 55427.2133449074 | 2010-08-19 05:07:13 | 3.0.22.43 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 050032 | Warm Hot Intergalactic Medium (WHIM) is the most promising candidate for the cosmic missing baryons. Nevertheless, no concrete evidence of the presence of the WHIM has been unveiled yet. We propose a SUZAKU observation of a filament discovered through a systematic analysis of the SDSS galaxy catalogue. The observation toward a 10 Mpc long section of this filament aligned with the line of sight will provide the redshifted OVII and OVIII emission lines from the WHIM or much stronger constraint on the overdensity of the WHIM. | EXTRAGALACTIC DIFFUSE SOURCES | 8 | B | HAJIME KAWAHARA | JAP | 5 | AO5 | SEARCHING FOR MISSING BARYONS ALONG A FILAMENT OF GALAXIES | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/805030010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '805030010'
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