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 | NGC 253 OFFSET | 12.0926 | -25.0475 | 11.478671 | -25.320084 | 0.364314 | -27.643554 | 104.44696227 | -87.8082396 | 247.2843 | 54829.0152430556 | 2008-12-29 00:21:57 | 54830.2502430556 | 2008-12-30 06:00:21 | 803004010 | 56.7104 | 50 | 56.7104 | 56.7104 | 0 | 56.7104 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 51.3026 | 51.3026 | 106.6718 | 1 | PROCESSED | 57545.0814351852 | 2016-06-06 01:57:16 | 55213 | 2010-01-17 00:00:00 | 54847.4571296296 | 2009-01-16 10:58:16 | 3.0.22.43 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 030027 | Suzaku observations of a hot halo of nearby, edge-on starburst galaxy NGC 253 are proposed. The low background and high energy resolution of Suzaku XIS is the best tool to study the low surface brightness emission like halo emission around galaxies. In addition, we will eliminate the contamination from the the point source by XMM-Newton and the Galactic hot emission by an offset observation. The temperature and pressure structure and the chemical composition in the bright halo will reveal the physical condition and the dynamics of the galaxy outflow to the intergalactic space. | EXTRAGALACTIC DIFFUSE SOURCES | 8 | C | NORIKO YAMASAKI | JAP | 3 | AO3 | SUZAKU OBSERVATION OF A BRIGHTEST STARBURST GALAXY NGC 253 | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/803004010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '803004010'
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