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 | A3112E | 49.9177 | -44.1055 | 49.483567 | -44.285626 | 26.168536 | -58.996914 | 252.54334877 | -55.82694751 | 25.0007 | 56829.3656134259 | 2014-06-21 08:46:29 | 56830.3266435185 | 2014-06-22 07:50:22 | 809024010 | 33.435 | 45 | 33.435 | 34.195 | 0 | 34.219 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 30.293 | 30.293 | 82.9918 | 1 | PROCESSED | 57615.3104398148 | 2016-08-15 07:27:02 | 57239 | 2015-08-05 00:00:00 | 56873.1925 | 2014-08-04 04:37:12 | 3.0.22.44 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 090061 | We propose to confirm the difference of the entropy profiles to the virial radius derived from Suzaku and Planck by 255 ksec Suzaku observations. Combination of X-ray and the Sunyuaev-Zel'dvitch effect observations play key roles for investigating not only cluster evolutions but also determining cosmological parameters because those observations are important complementary probe. While Suzaku observations found the flatter entropy slope than that expected from the numerical simulation in the outer region of the clusters, the entropy profile from the Planck observations agreed with the expected one well. This proposed observations would give hints in investigating the difference between the Suzaku and Planck results. | EXTRAGALACTIC DIFFUSE SOURCES | 8 | B | KOSUKE SATO | JAP | 9 | AO9 | ENTROPY PROFILE OF ABELL 3112 TO THE VIRIAL RADIUS FOR COMPARING TO PLANCK RESULTS | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/809024010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '809024010'
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