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
1 A 3376 90.5561 -39.9584 90.148808 -39.956705 90.960808 -63.398292 246.50686261 -25.98989573 107.6124 53649.6153703704 2005-10-06 14:46:08 53653.4495833333 2005-10-10 10:47:24 100034010 118.7792 150 118.7792 121.7373 118.8498 119.3357 2 2 2 2 1 0 0 100.5401 100.5401 331.2537 3 PROCESSED 57527.6218171296 2016-05-19 14:55:25 54247 2007-05-27 00:00:00 54109.6396990741 2007-01-09 15:21:10 3.0.22.43 5 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 000034 Abell 3376 (z=0.046) is a merging cluster with a T=4 keV (*3) hosting a pair of strong radio halos (see figure). It is one of the few clusters from which BeppoSAX positively detected excess hard X-rays (Nevalainen et al. ApJ 608, 166, 2004). Because of the relatively low temperature, the HXD-PIN energy band is expected to be relatively free from thermal emission, making this object ideal to the search for non-thermal signals. We expect the non-thermal flux to be 4-5% of the PIN background at 20 keV, and a 150 ksec on-source exposure would be needed to securely detect this. To know the current background over the full COR range, an off-source exposure for one day or a ~40 ksec exposure onto a very soft source, would be required immediately before or after the on-source data acquisition. CALIBRATION 1 A SWG JAP 0 SWG Diffuse Hard X-rays from Clusters N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100034010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '100034010'

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