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 1550-OFFSET1 | 65.1493 | 2.6086 | 64.497489 | 2.490158 | 63.709607 | -18.593747 | 190.9426677 | -31.53770965 | 265.5852 | 54901.8171875 | 2009-03-11 19:36:45 | 54903.699525463 | 2009-03-13 16:47:19 | 803046010 | 66.8274 | 62 | 66.8274 | 66.8274 | 0 | 66.8274 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 60.9307 | 60.9307 | 162.6001 | 2 | PROCESSED | 57545.8588541667 | 2016-06-06 20:36:45 | 55329 | 2010-05-13 00:00:00 | 54917.3952314815 | 2009-03-27 09:29:08 | 3.0.22.43 | 3 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 031422 | We propose a set of two 19 arcmin offset observations of the galaxy groups NGC 1550 and MKW 4 to measure spatially resolved densities, temperatures and iron abundances out to r_500. These measurements are crucial for an accurate determination of the gas mass profile and gas fraction, for probing the entropy profile near the region where the accretion shocks start to be important, and for exploring the chemical enrichment at a spatial scale which retains information of early SNII and SNIa enrichment. Due to their brightness, regularity and low temperature, the two objects are ideal candidates for an offset observation of their peripheral gas by Suzaku, making an excellent use of its low background and soft X-ray sensitivity. | EXTRAGALACTIC DIFFUSE SOURCES | 8 | C | FABIO GASTALDELLO | USA | 3 | AO3 | THE OUTSKIRTS OF NGC 1550 AND MKW 4 | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/803046010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '803046010'
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