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 | AWM7 | 43.631 | 41.5933 | 42.82175 | 41.390486 | 53.723626 | 23.815753 | 146.34082925 | -15.61629549 | 90.4997 | 53954.2348842593 | 2006-08-07 05:38:14 | 53954.71625 | 2006-08-07 17:11:24 | 801035010 | 18.9858 | 20 | 18.9858 | 18.9858 | 18.9858 | 18.9858 | 2 | 2 | 2 | 2 | 1 | 0 | 0 | 17.5542 | 17.5542 | 41.588 | 0 | PROCESSED | 57535.2434953704 | 2016-05-27 05:50:38 | 54422 | 2007-11-18 00:00:00 | 54020.7471759259 | 2006-10-12 17:55:56 | 3.0.22.43 | 3 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 010076 | The bright elongated cluster AWM7 is likely to be the place of gas infall along the large-scale filament of the Pisces-Perseus supercluster. We propose to probe the gas motion by measuring the energy shift and line broadening of Fe-K line based on the good energy resolution and low background of the XIS instrument. The motion of 1000 km/s is a reliably detectable level and we can directly measure the cluster formation process and its relation with the large-scale filament for the first time. If no gas motion is found, then secular asymmetric structure of the dark matter halo is implied. | EXTRAGALACTIC DIFFUSE SOURCES | 8 | B | TAKAYA OHASHI | JAP | 1 | AO1 | SIGNATURE OF LARGE-SCALE GAS MOTION IN AWM7 | XIS | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/801035010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '801035010'
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