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
1 NGC741MOSAICS_P1 29.0595 4.7357 28.408059 4.491575 28.699079 -6.708921 151.53660126 -54.49712787 71.6617 55052.4780671296 2009-08-09 11:28:25 55052.6946643518 2009-08-09 16:40:19 804054010 9.3222 10 9.3302 9.3222 0 9.3302 1 1 0 1 1 0 0 8.003 8.003 18.6719 1 PROCESSED 57548.0801967593 2016-06-09 01:55:29 55451 2010-09-12 00:00:00 55084.9869212963 2009-09-10 23:41:10 3.0.22.43 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 041515 Galaxies have a baryon fraction only 1/3 of the cosmological value, so powerful galactic winds must have driven the gas out. In galaxy groups, the sites of most galaxies, the baryon fraction is also 1/3-1/2 of the cosmological value within half the virial radius, so the gas has been pushed further outward, probably from the heating of the same galactic superwinds. Studies with other telescopes do not go beyond half of the virial radius due to background limitations. With Suzaku, we can observe to the virial radius by using the low background XIS and choosing a galaxy group in a region of low Galactic XRB. We will discover whether the missing baryons reside in the outer parts of the group or if they have been expelled beyond the virial radius. EXTRAGALACTIC DIFFUSE SOURCES 8 B JOEL BREGMAN USA 4 AO4 THE MISSING BARYONS IN GALAXY GROUPS XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/804054010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '804054010'

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