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 2403 | 114.2007 | 65.5918 | 112.996594 | 65.703234 | 103.458828 | 43.277316 | 150.58117971 | 29.1798975 | 310.3004 | 53810.5896875 | 2006-03-16 14:09:09 | 53811.5884143518 | 2006-03-17 14:07:19 | 800021010 | 72.3687 | 70 | 72.3767 | 72.3687 | 72.3767 | 72.3767 | 2 | 2 | 2 | 2 | 1 | 0 | 0 | 59.3591 | 59.3591 | 86.2779 | 0 | PROCESSED | 57533.2480439815 | 2016-05-25 05:57:11 | 54247 | 2007-05-27 00:00:00 | 54042.0667708333 | 2006-11-03 01:36:09 | 3.0.22.43 | 3 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 001101 | We propose to observe NGC 2403, which is a nearby luminous normal spiral. Our main objective is to search and investigation of diffuse emission components. These include both rather soft (kT = 0.1 - 1 keV) ones already detected from a fair number of spirals, and hot (kT = a few keV) emission which, if established, may become an analogue to the Galactic ridge emission. | EXTRAGALACTIC DIFFUSE SOURCES | 8 | A | KAZUO MAKISHIMA | JAP | 0 | SWG | A PROPOSAL FOR A 70 KSEC SUZAKU OBSERVATION OF THE NORMAL SPIRAL GALAXY NGC 2403 | XIS | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/800021010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '800021010'
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